1 00:00:07,900 --> 00:00:02,960 so thank you very much for coming for 2 00:00:12,169 --> 00:00:10,280 you're here to the bitter end and we're 3 00:00:15,410 --> 00:00:12,179 glad to have you here 4 00:00:16,760 --> 00:00:15,420 we're very we're very excited and I 5 00:00:18,830 --> 00:00:16,770 think the whole community should be 6 00:00:21,980 --> 00:00:18,840 excited that this marvellous telescope 7 00:00:25,790 --> 00:00:21,990 has lasted through to this year and this 8 00:00:29,359 --> 00:00:25,800 begins the 25th year of Hubble Space 9 00:00:31,939 --> 00:00:29,369 Telescope operations who knew it's done 10 00:00:33,889 --> 00:00:31,949 an amazing amount of science it's really 11 00:00:35,840 --> 00:00:33,899 transformed a lot of the way we do 12 00:00:39,979 --> 00:00:35,850 science as well as our thinking on many 13 00:00:42,500 --> 00:00:39,989 topics and so today as part of the 14 00:00:44,900 --> 00:00:42,510 anniversary here at the kick-off 15 00:00:47,869 --> 00:00:44,910 proceedings at the double-a s we started 16 00:00:50,930 --> 00:00:47,879 with some great press releases 17 00:00:53,720 --> 00:00:50,940 beautifully beautiful imagery and now 18 00:00:57,319 --> 00:00:53,730 with the Town Hall which is being 19 00:01:00,920 --> 00:00:57,329 recorded for posterity and also if you 20 00:01:03,470 --> 00:01:00,930 like to share with your friends that we 21 00:01:05,479 --> 00:01:03,480 did record this and we will put it on 22 00:01:07,789 --> 00:01:05,489 YouTube so it can be viewed later by 23 00:01:10,850 --> 00:01:07,799 those who were not fortunate enough to 24 00:01:14,149 --> 00:01:10,860 be here in this town hall we're going to 25 00:01:17,780 --> 00:01:14,159 have three speakers first can Sam Bach 26 00:01:21,320 --> 00:01:17,790 from Space Telescope who is the Hubble 27 00:01:23,749 --> 00:01:21,330 Space Telescope mission had that and 28 00:01:26,810 --> 00:01:23,759 he's going to review a little bit about 29 00:01:30,710 --> 00:01:26,820 where we are with HST and it's bright 30 00:01:33,230 --> 00:01:30,720 future then we're going to have Jennifer 31 00:01:35,660 --> 00:01:33,240 lots who's from Space Telescope who's 32 00:01:39,590 --> 00:01:35,670 going to talk to us about our major 33 00:01:42,980 --> 00:01:39,600 effort of large observation for the 34 00:01:45,830 --> 00:01:42,990 frontier fields and she's the PI of that 35 00:01:48,170 --> 00:01:45,840 program and some really beautiful data 36 00:01:52,580 --> 00:01:48,180 and fantastic results have come out of 37 00:01:55,280 --> 00:01:52,590 that program and then amber straw from 38 00:01:57,620 --> 00:01:55,290 NASA headquarters is going to talk to 39 00:02:00,649 --> 00:01:57,630 you about the 25th anniversary 40 00:02:03,859 --> 00:02:00,659 celebration the year of activities that 41 00:02:06,289 --> 00:02:03,869 are ongoing and how you can participate 42 00:02:08,240 --> 00:02:06,299 and I will let each speaker handoff to 43 00:02:11,500 --> 00:02:08,250 the next and then at the end we will 44 00:02:13,020 --> 00:02:11,510 have ample time for your questions and 45 00:02:15,000 --> 00:02:13,030 discussion 46 00:02:22,020 --> 00:02:15,010 thank you so first off we'll be ken-san 47 00:02:26,760 --> 00:02:22,030 Bach on what about HST today and Thank 48 00:02:27,809 --> 00:02:26,770 You Carol so yeah today I'm going to 49 00:02:29,520 --> 00:02:27,819 tell you a little bit about where we 50 00:02:31,470 --> 00:02:29,530 stand with the observatory today and 51 00:02:34,440 --> 00:02:31,480 where we're heading and heading in the 52 00:02:37,229 --> 00:02:34,450 next few years and punchline is this 53 00:02:38,309 --> 00:02:37,239 Hubble is just doing beautifully it's as 54 00:02:41,070 --> 00:02:38,319 powerful as ever 55 00:02:44,370 --> 00:02:41,080 we have excellent imaging and 56 00:02:46,710 --> 00:02:44,380 spectroscopy capabilities we're still 57 00:02:49,199 --> 00:02:46,720 doing choreography and Strama tree with 58 00:02:53,340 --> 00:02:49,209 the telescope and the observing program 59 00:02:54,900 --> 00:02:53,350 is addressing everything from exoplanet 60 00:02:58,050 --> 00:02:54,910 science to the architecture of the 61 00:03:00,540 --> 00:02:58,060 universe the science that Hubble does 62 00:03:03,750 --> 00:03:00,550 cuts across NASA's main science themes 63 00:03:07,199 --> 00:03:03,760 and as always Hubble remains a great 64 00:03:10,710 --> 00:03:07,209 Observatory multi-purpose and in my 65 00:03:12,630 --> 00:03:10,720 demand by the observing community you 66 00:03:15,600 --> 00:03:12,640 probably saw this beautiful image on 67 00:03:17,670 --> 00:03:15,610 Monday when it was released this 68 00:03:20,789 --> 00:03:17,680 original image of the Eagle Nebula was 69 00:03:24,509 --> 00:03:20,799 taken 20 years ago now our Wide Field 70 00:03:27,300 --> 00:03:24,519 Camera 3 has reimaged that field both at 71 00:03:30,509 --> 00:03:27,310 visible and at near-infrared wavelengths 72 00:03:33,600 --> 00:03:30,519 and you can see how remarkable that 73 00:03:36,270 --> 00:03:33,610 field looks both in the visible with a 74 00:03:39,090 --> 00:03:36,280 wider field of view and in the infrared 75 00:03:42,660 --> 00:03:39,100 where you can see deep into some of 76 00:03:44,340 --> 00:03:42,670 these pillars of star formation many of 77 00:03:47,759 --> 00:03:44,350 you have probably also seen the 78 00:03:52,740 --> 00:03:47,769 tremendous m31 mosaic that's outside the 79 00:03:55,710 --> 00:03:52,750 other hall that we have conference talks 80 00:03:57,750 --> 00:03:55,720 in that image is the largest image ever 81 00:04:01,440 --> 00:03:57,760 produced by the observatory both 82 00:04:03,240 --> 00:04:01,450 physically printed by the observatory as 83 00:04:04,890 --> 00:04:03,250 well as the largest mosaic we've ever 84 00:04:07,259 --> 00:04:04,900 made on the sky and that was done by 85 00:04:08,729 --> 00:04:07,269 julian del canton and heard folks here 86 00:04:10,590 --> 00:04:08,739 at the university of washington so it 87 00:04:14,670 --> 00:04:10,600 was very fitting that we were able to 88 00:04:16,289 --> 00:04:14,680 bring that mosaic here to Seattle take a 89 00:04:18,630 --> 00:04:16,299 look at that get your nose up close to 90 00:04:21,620 --> 00:04:18,640 that particular image 100 million stars 91 00:04:24,270 --> 00:04:21,630 and that image resolved it's amazing 92 00:04:26,060 --> 00:04:24,280 hobo science output continues to be 93 00:04:28,220 --> 00:04:26,070 extremely good 94 00:04:30,470 --> 00:04:28,230 past year was another excellent year 95 00:04:33,590 --> 00:04:30,480 with more than 800 papers published 96 00:04:35,750 --> 00:04:33,600 based on HST data we're running right 97 00:04:38,390 --> 00:04:35,760 around 800 papers a year or so for the 98 00:04:40,910 --> 00:04:38,400 last four or five years there have now 99 00:04:44,450 --> 00:04:40,920 been almost 13,000 papers published to 100 00:04:46,970 --> 00:04:44,460 date based on HST data and an even more 101 00:04:50,210 --> 00:04:46,980 remarkable number is that almost 13,000 102 00:04:53,990 --> 00:04:50,220 700 different people have published or 103 00:04:55,700 --> 00:04:54,000 had their names on HST papers think 104 00:04:57,830 --> 00:04:55,710 about that for a minute that's that's 105 00:05:00,290 --> 00:04:57,840 bigger than the size of the SS for sure 106 00:05:02,200 --> 00:05:00,300 and so you know Hubble is definitely 107 00:05:05,180 --> 00:05:02,210 touching generations of astronomers 108 00:05:07,220 --> 00:05:05,190 there have been more than 500 PhD theses 109 00:05:09,640 --> 00:05:07,230 based on Hubble data and right now 110 00:05:13,940 --> 00:05:09,650 approximately 40 or 50 people a year 111 00:05:18,260 --> 00:05:13,950 have PhD theses published that are based 112 00:05:20,720 --> 00:05:18,270 on Hubble data overall the observatory 113 00:05:22,310 --> 00:05:20,730 is doing extremely well the science 114 00:05:24,620 --> 00:05:22,320 instruments are all healthy and 115 00:05:26,810 --> 00:05:24,630 operating the advanced camera for 116 00:05:29,510 --> 00:05:26,820 surveys is and the Wide Field Camera 3 117 00:05:32,390 --> 00:05:29,520 both have charge transfer Corrections in 118 00:05:33,740 --> 00:05:32,400 place for their CCD cameras which is 119 00:05:36,050 --> 00:05:33,750 great because it means that we're 120 00:05:39,140 --> 00:05:36,060 actually able to rollback the aging 121 00:05:41,810 --> 00:05:39,150 clocks a bit on those cameras the cosmic 122 00:05:45,200 --> 00:05:41,820 origins spectrograph sensitivity is 123 00:05:47,030 --> 00:05:45,210 still very very good we now have very 124 00:05:50,480 --> 00:05:47,040 blue modes that get down well below 125 00:05:52,100 --> 00:05:50,490 lyman-alpha the Space Telescope imaging 126 00:05:53,330 --> 00:05:52,110 spectrograph is operating well and as I 127 00:05:56,090 --> 00:05:53,340 said before it's being used for 128 00:05:58,550 --> 00:05:56,100 choreography as well as spectroscopy and 129 00:06:00,880 --> 00:05:58,560 imaging on the main systems of the 130 00:06:03,770 --> 00:06:00,890 observatory those are also working well 131 00:06:05,840 --> 00:06:03,780 five of the six gyros are available for 132 00:06:09,050 --> 00:06:05,850 use we lost one gyro back in March of 133 00:06:10,550 --> 00:06:09,060 last year not a surprise gyros are not a 134 00:06:12,200 --> 00:06:10,560 life limiting factor for this 135 00:06:16,340 --> 00:06:12,210 Observatory we know how to run in a 136 00:06:20,750 --> 00:06:18,440 overall the thermal control the data 137 00:06:24,760 --> 00:06:20,760 management systems and so on are all in 138 00:06:26,990 --> 00:06:24,770 excellent health one interesting tidbit 139 00:06:28,850 --> 00:06:27,000 two instruments were repaired during 140 00:06:31,040 --> 00:06:28,860 servicing mission five and a half years 141 00:06:33,580 --> 00:06:31,050 ago that advanced camera for surveys and 142 00:06:36,470 --> 00:06:33,590 Space Telescope imaging spectrograph 143 00:06:39,439 --> 00:06:36,480 those failures that originally occurred 144 00:06:41,689 --> 00:06:39,449 were electronic in nature the 145 00:06:45,350 --> 00:06:41,699 astronauts installed new electronics in 146 00:06:47,689 --> 00:06:45,360 both instruments those two new 147 00:06:49,519 --> 00:06:47,699 instruments have run now on those newly 148 00:06:52,640 --> 00:06:49,529 installed electronics longer than they 149 00:06:54,379 --> 00:06:52,650 ran on the original electronics that's 150 00:06:56,659 --> 00:06:54,389 very encouraging because it suggests 151 00:06:59,209 --> 00:06:56,669 that the instruments have outlived their 152 00:07:01,279 --> 00:06:59,219 infant mortality period so it's quite 153 00:07:02,929 --> 00:07:01,289 possible even though we originally 154 00:07:04,700 --> 00:07:02,939 thought those two instruments might not 155 00:07:06,350 --> 00:07:04,710 last more than five years they may 156 00:07:11,029 --> 00:07:06,360 actually last considerably longer than 157 00:07:12,860 --> 00:07:11,039 that we'll see in looking forward the 158 00:07:15,019 --> 00:07:12,870 mission has put together what it calls a 159 00:07:16,939 --> 00:07:15,029 20/20 vision for the observatory and 160 00:07:19,339 --> 00:07:16,949 that 20/20 vision is very 161 00:07:22,459 --> 00:07:19,349 straightforward and simple is to operate 162 00:07:23,809 --> 00:07:22,469 the observatory out to 2020 or beyond so 163 00:07:26,360 --> 00:07:23,819 that there's at least a year of 164 00:07:29,209 --> 00:07:26,370 overlapping science observations with 165 00:07:30,800 --> 00:07:29,219 JWST and that's going to be performed in 166 00:07:33,230 --> 00:07:30,810 a manner that maximizes the science 167 00:07:36,829 --> 00:07:33,240 return of both observatories takes full 168 00:07:39,369 --> 00:07:36,839 advantages of HST unique capabilities 169 00:07:42,290 --> 00:07:39,379 and really addresses the community's 170 00:07:45,559 --> 00:07:42,300 scientific curiosity and engages the 171 00:07:47,869 --> 00:07:45,569 public in scientific discovery let's 172 00:07:49,489 --> 00:07:47,879 think about that for a minute if we 173 00:07:52,459 --> 00:07:49,499 operate out through the end of fiscal 174 00:07:54,829 --> 00:07:52,469 year twenty one which is cycle 28 we're 175 00:07:58,159 --> 00:07:54,839 currently in cycle 22 right now that's 176 00:08:00,850 --> 00:07:58,169 about seven cycles of observations at 177 00:08:03,589 --> 00:08:00,860 about 4,000 science orbits per cycle 178 00:08:06,050 --> 00:08:03,599 4,000 hours per cycle roughly that's 179 00:08:08,389 --> 00:08:06,060 28,000 orbits of science remaining and 180 00:08:12,260 --> 00:08:08,399 for comparison we typically have about 181 00:08:15,110 --> 00:08:12,270 20,000 hours or orbits requested each 182 00:08:16,760 --> 00:08:15,120 cycle there's clearly no loss of things 183 00:08:18,679 --> 00:08:16,770 or lack of things to do with this 184 00:08:21,529 --> 00:08:18,689 Observatory in its remaining years the 185 00:08:24,559 --> 00:08:21,539 question is what do we do and so we've 186 00:08:29,300 --> 00:08:24,569 put out a call for HST 2020 as an extra 187 00:08:34,160 --> 00:08:32,120 you never know we put out a call for 188 00:08:36,890 --> 00:08:34,170 vision white paper short white papers 189 00:08:38,180 --> 00:08:36,900 from the community just asking what is 190 00:08:39,740 --> 00:08:38,190 it that we should be doing with the 191 00:08:41,660 --> 00:08:39,750 observatory over the next five or six 192 00:08:45,110 --> 00:08:41,670 years that would enhance the scientific 193 00:08:48,020 --> 00:08:45,120 legacy those are due February 20th and 194 00:08:50,000 --> 00:08:48,030 the submission details are there those 195 00:08:51,770 --> 00:08:50,010 papers can address any aspect of a 196 00:08:54,410 --> 00:08:51,780 Hubble program so I'll put forward a 197 00:08:55,970 --> 00:08:54,420 couple of questions to you are there 198 00:08:58,520 --> 00:08:55,980 specific programs we should be 199 00:08:59,930 --> 00:08:58,530 undertaking now in preparation for JWST 200 00:09:02,780 --> 00:08:59,940 or during the period of overlapping 201 00:09:04,130 --> 00:09:02,790 observations what types of synergies 202 00:09:05,110 --> 00:09:04,140 might be available we'd like to hear 203 00:09:07,820 --> 00:09:05,120 your thoughts on that 204 00:09:10,310 --> 00:09:07,830 are there other observations from ground 205 00:09:11,900 --> 00:09:10,320 or space-based observatories that should 206 00:09:13,700 --> 00:09:11,910 be more closely linked to HST 207 00:09:15,230 --> 00:09:13,710 observations over the next few years 208 00:09:17,180 --> 00:09:15,240 should we have some kind of a reciprocal 209 00:09:21,590 --> 00:09:17,190 observing agreement like we do with nao 210 00:09:22,970 --> 00:09:21,600 nao or NRAO for example are there 211 00:09:24,680 --> 00:09:22,980 science questions that should receive 212 00:09:26,480 --> 00:09:24,690 greater emphasis over the next five 213 00:09:28,130 --> 00:09:26,490 years that's kind of a loaded question 214 00:09:31,370 --> 00:09:28,140 but we'd like to hear your thoughts on 215 00:09:35,090 --> 00:09:31,380 that and of course your rationale for 216 00:09:37,190 --> 00:09:35,100 why that should be should we devote a 217 00:09:41,210 --> 00:09:37,200 greater proportion of observing time to 218 00:09:43,010 --> 00:09:41,220 specific purposes and one that I 219 00:09:45,530 --> 00:09:43,020 mentioned earlier should we be putting 220 00:09:47,450 --> 00:09:45,540 more emphasis on making sure that 221 00:09:49,790 --> 00:09:47,460 students can finish their PhDs or use 222 00:09:50,990 --> 00:09:49,800 Hubble for their PhD thesis I think 223 00:09:53,720 --> 00:09:51,000 that's a great question to ask the 224 00:09:55,520 --> 00:09:53,730 community should we make a special 225 00:09:57,440 --> 00:09:55,530 effort to optimize the observing 226 00:10:00,620 --> 00:09:57,450 programme for transient phenomena in the 227 00:10:04,520 --> 00:10:00,630 area of pan-starrs LSST transient 228 00:10:05,900 --> 00:10:04,530 phenomena are going to be leading to all 229 00:10:09,380 --> 00:10:05,910 kinds of discoveries should we be doing 230 00:10:10,730 --> 00:10:09,390 something with Hubble to optimize their 231 00:10:13,190 --> 00:10:10,740 science return from those kinds of 232 00:10:15,770 --> 00:10:13,200 observations and given that Hubble's 233 00:10:17,570 --> 00:10:15,780 feit lifetime is finite are there 234 00:10:19,760 --> 00:10:17,580 changes the time allocation committee 235 00:10:22,670 --> 00:10:19,770 that maybe we should make not that it 236 00:10:24,140 --> 00:10:22,680 needs to be made it runs well but maybe 237 00:10:25,730 --> 00:10:24,150 there's something that we could do to 238 00:10:27,170 --> 00:10:25,740 enable quicker responses to new 239 00:10:31,640 --> 00:10:27,180 discoveries is there something that we 240 00:10:34,190 --> 00:10:31,650 should be doing let us know so we have a 241 00:10:37,210 --> 00:10:34,200 call for proposals out now that was 242 00:10:41,450 --> 00:10:37,220 released yesterday the proposals are due 243 00:10:43,280 --> 00:10:41,460 April 10th there are key features remain 244 00:10:45,079 --> 00:10:43,290 from previous 245 00:10:47,600 --> 00:10:45,089 so the ultraviolet observing initiative 246 00:10:49,940 --> 00:10:47,610 continues the medium proposal category 247 00:10:51,230 --> 00:10:49,950 continues the frontier fields which 248 00:10:53,750 --> 00:10:51,240 you'll hear about in just a moment from 249 00:10:55,670 --> 00:10:53,760 Jennifer continue and we encourage 250 00:10:58,160 --> 00:10:55,680 people to submit archival in theory in 251 00:10:59,630 --> 00:10:58,170 general observer proposals specifically 252 00:11:02,960 --> 00:10:59,640 that develops not the scientific 253 00:11:05,380 --> 00:11:02,970 landscape for JWST and help maximize its 254 00:11:07,850 --> 00:11:05,390 scientific return or can exploit 255 00:11:11,000 --> 00:11:07,860 potential of those frontier field 256 00:11:12,590 --> 00:11:11,010 programs we'll be talking with the 257 00:11:15,220 --> 00:11:12,600 community some more about this at our 258 00:11:18,980 --> 00:11:15,230 May symposium at the Institute in April 259 00:11:21,290 --> 00:11:18,990 that's the symposium devoted to looking 260 00:11:24,019 --> 00:11:21,300 not only back at the extraordinary 261 00:11:26,540 --> 00:11:24,029 impact that Hubble has had on science 262 00:11:29,449 --> 00:11:26,550 culture and society but also looking at 263 00:11:32,329 --> 00:11:29,459 how we can craft a real scientific 264 00:11:33,560 --> 00:11:32,339 legacy for the mission and to focus on 265 00:11:36,590 --> 00:11:33,570 what we should be doing in the coming 266 00:11:38,949 --> 00:11:36,600 years so in addition to the white papers 267 00:11:41,329 --> 00:11:38,959 this will be another place for people to 268 00:11:46,400 --> 00:11:41,339 convey their thoughts to us that which 269 00:11:49,150 --> 00:11:46,410 would be great now each year we do about 270 00:11:51,740 --> 00:11:49,160 40 press releases or so this is just a 271 00:11:54,590 --> 00:11:51,750 kind of an eye chart and you just look 272 00:11:58,639 --> 00:11:54,600 at the bars that on the chart and notice 273 00:12:00,949 --> 00:11:58,649 that the y-axis is millions and this is 274 00:12:03,560 --> 00:12:00,959 the potential circulation of the media 275 00:12:05,090 --> 00:12:03,570 outlets that pick up Hubble results so 276 00:12:06,710 --> 00:12:05,100 we typically measure those in hundreds 277 00:12:08,449 --> 00:12:06,720 of millions and you can see that some 278 00:12:10,910 --> 00:12:08,459 things really capture the imagination of 279 00:12:14,269 --> 00:12:10,920 the public I understand from our press 280 00:12:17,600 --> 00:12:14,279 people yesterday that the Eagle Nebula 281 00:12:19,519 --> 00:12:17,610 and m31 images that were released at the 282 00:12:21,980 --> 00:12:19,529 SS this week will probably be somewhere 283 00:12:24,980 --> 00:12:21,990 up around the 500 or 600 million mark on 284 00:12:27,490 --> 00:12:24,990 this particular kind of plot so with 285 00:12:29,980 --> 00:12:27,500 that being said let us help you 286 00:12:32,389 --> 00:12:29,990 communicate your science to the public 287 00:12:34,970 --> 00:12:32,399 alert us to the newsworthy science 288 00:12:37,250 --> 00:12:34,980 results that you have and let's get your 289 00:12:42,500 --> 00:12:37,260 let's get your science results up on to 290 00:12:46,490 --> 00:12:42,510 that chart I have one final slide and 291 00:12:50,630 --> 00:12:46,500 that is the HST budget here's the budget 292 00:12:52,699 --> 00:12:50,640 breakdown between grants and operations 293 00:12:55,540 --> 00:12:52,709 both at the Institute and at Goddard you 294 00:12:58,890 --> 00:12:55,550 can see it's roughly a third third of 295 00:13:02,080 --> 00:12:58,900 I show this for one reason and that's to 296 00:13:04,420 --> 00:13:02,090 let you know that a fair fraction of the 297 00:13:05,620 --> 00:13:04,430 money that's spent on Hubble actually 298 00:13:08,260 --> 00:13:05,630 goes out to the scientific community 299 00:13:09,970 --> 00:13:08,270 directly in the form of grants and we're 300 00:13:12,850 --> 00:13:09,980 committed as a mission to make sure that 301 00:13:14,380 --> 00:13:12,860 that continues we very much like to see 302 00:13:16,750 --> 00:13:14,390 something on the order of twenty eight 303 00:13:18,970 --> 00:13:16,760 to thirty million dollars a year from 304 00:13:21,010 --> 00:13:18,980 the mission budget being put out to the 305 00:13:23,830 --> 00:13:21,020 community directly in the form of a 306 00:13:26,170 --> 00:13:23,840 grants that help support getting the 307 00:13:29,590 --> 00:13:26,180 science out to the public and to our 308 00:13:31,030 --> 00:13:29,600 scientific colleagues so I'll leave you 309 00:13:32,050 --> 00:13:31,040 with one final slide and the thought 310 00:13:35,620 --> 00:13:32,060 from John Bacall 311 00:13:36,730 --> 00:13:35,630 Blake John Bacall we often frame our 312 00:13:38,800 --> 00:13:36,740 understanding what the Space Telescope 313 00:13:40,720 --> 00:13:38,810 will do in terms of what we expect to 314 00:13:43,090 --> 00:13:40,730 find and actually it would be terribly 315 00:13:45,460 --> 00:13:43,100 anticlimactic if in fact we find what we 316 00:13:47,050 --> 00:13:45,470 expect to find the most important 317 00:13:48,730 --> 00:13:47,060 discoveries will provide answers to 318 00:13:51,130 --> 00:13:48,740 questions that we do not yet know how to 319 00:13:53,650 --> 00:13:51,140 ask and will concern objects we have not 320 00:13:55,600 --> 00:13:53,660 yet imagined I suspect that will remain 321 00:13:57,790 --> 00:13:55,610 true throughout Hubble's lifetime and 322 00:14:18,519 --> 00:13:57,800 will almost certainly be the case in the 323 00:14:24,489 --> 00:14:22,539 okay so it's my pleasure to talk to you 324 00:14:27,039 --> 00:14:24,499 this afternoon about the frontier fields 325 00:14:29,919 --> 00:14:27,049 a major initiative using directors 326 00:14:31,659 --> 00:14:29,929 discretionary time to try to peer deeper 327 00:14:32,349 --> 00:14:31,669 into the universe than we ever have 328 00:14:34,929 --> 00:14:32,359 before 329 00:14:37,269 --> 00:14:34,939 so I'm acting as the PI of this program 330 00:14:39,039 --> 00:14:37,279 on behalf of Mount Mountain and I'm very 331 00:14:40,719 --> 00:14:39,049 privileged to work with a dedicated and 332 00:14:45,119 --> 00:14:40,729 talents a team of people at Space 333 00:14:48,999 --> 00:14:47,529 so the image in the background here is 334 00:14:52,059 --> 00:14:49,009 one that we all know and love and has 335 00:14:53,739 --> 00:14:52,069 become iconic but more than being a 336 00:14:55,979 --> 00:14:53,749 beautiful image the Hubble ultra-deep 337 00:14:57,789 --> 00:14:55,989 field has really transformed our 338 00:15:00,579 --> 00:14:57,799 understanding of the history of the 339 00:15:04,269 --> 00:15:00,589 universe and in fact it represents a 340 00:15:06,939 --> 00:15:04,279 huge investment of Hubble time so as 341 00:15:08,499 --> 00:15:06,949 this version of the observations the 342 00:15:10,779 --> 00:15:08,509 infrared observations of the Hubble 343 00:15:12,309 --> 00:15:10,789 ultra-deep field were wrapping up the 344 00:15:14,979 --> 00:15:12,319 director of Space Telescope mount 345 00:15:16,509 --> 00:15:14,989 Mountain asked the question could we top 346 00:15:18,989 --> 00:15:16,519 the Hubble ultra-deep field 347 00:15:21,609 --> 00:15:18,999 can we appear deeper into the universe 348 00:15:23,979 --> 00:15:21,619 with Hubble before the launch of the 349 00:15:26,349 --> 00:15:23,989 James Webb Space Telescope is there 350 00:15:29,589 --> 00:15:26,359 exciting D field science left to be done 351 00:15:31,119 --> 00:15:29,599 with Hubble in its remaining years so he 352 00:15:33,279 --> 00:15:31,129 posed this question to a group of 353 00:15:34,839 --> 00:15:33,289 astronomers and of course when you ask 354 00:15:36,729 --> 00:15:34,849 them could they do interesting things 355 00:15:40,689 --> 00:15:36,739 with lots of Hubble time the answer is 356 00:15:42,849 --> 00:15:40,699 usually yes and the answer they came 357 00:15:45,549 --> 00:15:42,859 back with was to use a trick you use 358 00:15:48,879 --> 00:15:45,559 gravitational lensing that is nature's 359 00:15:50,649 --> 00:15:48,889 telescopes strong lensing clusters plus 360 00:15:53,649 --> 00:15:50,659 Hubble to peer deeper into the universe 361 00:15:57,249 --> 00:15:53,659 than we have before using less exposure 362 00:15:59,949 --> 00:15:57,259 time and they propose not just looking 363 00:16:02,829 --> 00:15:59,959 at one strong lensing cluster but to 364 00:16:04,899 --> 00:16:02,839 look at six and to put turn on both of 365 00:16:06,939 --> 00:16:04,909 Hubble's primary workhorse cameras and 366 00:16:10,689 --> 00:16:06,949 use those in parallel so that you will 367 00:16:12,999 --> 00:16:10,699 get six lens fields in addition to six 368 00:16:15,099 --> 00:16:13,009 blank fields and this would add up to an 369 00:16:19,629 --> 00:16:15,109 exciting new parameter space for 370 00:16:21,909 --> 00:16:19,639 exploring the distant universe so the 371 00:16:23,829 --> 00:16:21,919 primary science goals of this program as 372 00:16:25,719 --> 00:16:23,839 outlined by that science working group 373 00:16:27,789 --> 00:16:25,729 are firstly 374 00:16:29,379 --> 00:16:27,799 simply to see deeper than we have before 375 00:16:31,540 --> 00:16:29,389 and to probe those galaxies that are 376 00:16:34,060 --> 00:16:31,550 intrinsically fainter 377 00:16:37,600 --> 00:16:34,070 anything we've seen and those galaxies 378 00:16:39,070 --> 00:16:37,610 that are that we can see at times before 379 00:16:42,040 --> 00:16:39,080 and during the epoch of reorganization 380 00:16:44,019 --> 00:16:42,050 and by going this deep we would be able 381 00:16:46,090 --> 00:16:44,029 to trace the early star formation 382 00:16:48,460 --> 00:16:46,100 histories of those galaxies small enough 383 00:16:51,759 --> 00:16:48,470 faint enough to be the early progenitors 384 00:16:53,470 --> 00:16:51,769 of our own Milky Way of course 385 00:16:55,120 --> 00:16:53,480 gravitational lensing not only makes 386 00:16:56,710 --> 00:16:55,130 things appear brighter but it stretches 387 00:16:59,110 --> 00:16:56,720 them out and so we would have the 388 00:17:01,240 --> 00:16:59,120 opportunity to study these galaxies and 389 00:17:03,730 --> 00:17:01,250 greater spatial with greater spatial 390 00:17:06,220 --> 00:17:03,740 resolution than possible with Hubble 391 00:17:08,949 --> 00:17:06,230 alone looking at their resolved 392 00:17:11,110 --> 00:17:08,959 structures their colors their sizes and 393 00:17:12,549 --> 00:17:11,120 some of these galaxies may be boosted 394 00:17:16,569 --> 00:17:12,559 enough for ground-based spectroscopic 395 00:17:18,220 --> 00:17:16,579 follow-up finally with six lens fields 396 00:17:20,650 --> 00:17:18,230 and six parallel fields we could build 397 00:17:25,179 --> 00:17:20,660 up a better statistical picture of 398 00:17:27,100 --> 00:17:25,189 galaxy formation at early times so this 399 00:17:29,500 --> 00:17:27,110 slide is my one slide summary of our 400 00:17:31,030 --> 00:17:29,510 observing program all of these 401 00:17:33,010 --> 00:17:31,040 observations with Hubble are beyond 402 00:17:35,680 --> 00:17:33,020 being done with directors discretionary 403 00:17:38,919 --> 00:17:35,690 time and so for each cluster parallel 404 00:17:43,390 --> 00:17:38,929 pointing we are dedicating 140 HST 405 00:17:46,000 --> 00:17:43,400 orbits using both the ACS optical imager 406 00:17:49,169 --> 00:17:46,010 and the wide field Infrared channel in 407 00:17:52,180 --> 00:17:49,179 parallel obtaining optical and infrared 408 00:17:55,360 --> 00:17:52,190 images and seven bands going down to 409 00:17:57,130 --> 00:17:55,370 27th magnitude and our observing plan is 410 00:17:58,960 --> 00:17:57,140 such that we're looking at two of these 411 00:18:01,890 --> 00:17:58,970 clusters per year spread out over three 412 00:18:04,659 --> 00:18:01,900 years for a total of 840 orbits a 413 00:18:06,880 --> 00:18:04,669 spitzer has also dedicated a major chunk 414 00:18:09,310 --> 00:18:06,890 of its directors discretionary time and 415 00:18:11,140 --> 00:18:09,320 so for every cluster and blank field 416 00:18:13,659 --> 00:18:11,150 pointing they will be exceptionally deep 417 00:18:16,210 --> 00:18:13,669 Iraq channel 1 and channel 2 imaging and 418 00:18:17,980 --> 00:18:16,220 all of this data is public the raw data 419 00:18:20,890 --> 00:18:17,990 is public and we're working very hard at 420 00:18:25,630 --> 00:18:20,900 Space Telescope to produce high quality 421 00:18:28,720 --> 00:18:25,640 science images as well so these are our 422 00:18:31,510 --> 00:18:28,730 six frontier fields the clusters and 423 00:18:33,880 --> 00:18:31,520 these were selected in consultation with 424 00:18:36,430 --> 00:18:33,890 the community primarily based on the 425 00:18:37,870 --> 00:18:36,440 known lensing strength at the time but 426 00:18:40,060 --> 00:18:37,880 also on their locate based on their 427 00:18:42,130 --> 00:18:40,070 location in the sky how dark was the 428 00:18:45,420 --> 00:18:42,140 background and whether or not there was 429 00:18:46,890 --> 00:18:45,430 any ancillary data available 430 00:18:49,460 --> 00:18:46,900 and I'll just highlight our last two 431 00:18:51,600 --> 00:18:49,470 clusters recently these were approved 432 00:18:54,570 --> 00:18:51,610 and we'll be going forward with the 433 00:18:56,370 --> 00:18:54,580 observations for these in cycle 23 and I 434 00:18:57,930 --> 00:18:56,380 recommend you take a look at at the call 435 00:19:00,150 --> 00:18:57,940 for proposals that went out yesterday 436 00:19:04,470 --> 00:19:00,160 for more details about how to use these 437 00:19:06,420 --> 00:19:04,480 for your science so this is a beautiful 438 00:19:08,370 --> 00:19:06,430 image which may be familiar to you it's 439 00:19:10,920 --> 00:19:08,380 been shown a few times around at the 440 00:19:14,670 --> 00:19:10,930 double-a s meeting this year this is our 441 00:19:16,440 --> 00:19:14,680 first cluster Abell 2744 all of the data 442 00:19:18,390 --> 00:19:16,450 is in hand for this cluster you can go 443 00:19:20,040 --> 00:19:18,400 to our website get the raw data get to 444 00:19:23,220 --> 00:19:20,050 the reduced data get lots of beautiful 445 00:19:25,980 --> 00:19:23,230 images but I also like to show an 446 00:19:30,420 --> 00:19:25,990 amped-up version of this image so this 447 00:19:33,150 --> 00:19:30,430 is the infrared version of a bell 27:44 448 00:19:35,100 --> 00:19:33,160 with the stretch maximized to show just 449 00:19:37,200 --> 00:19:35,110 how deep we're really going when we look 450 00:19:38,970 --> 00:19:37,210 at this cluster so if you're a cluster 451 00:19:40,650 --> 00:19:38,980 scientist you'll see we've got lots of 452 00:19:43,110 --> 00:19:40,660 inter cluster light you can see the 453 00:19:45,540 --> 00:19:43,120 tidal features of cluster galaxies that 454 00:19:47,130 --> 00:19:45,550 are interacting with each other and if 455 00:19:48,660 --> 00:19:47,140 you were to zoom in very close in this 456 00:19:51,330 --> 00:19:48,670 image you'll see we'll are also finding 457 00:19:53,130 --> 00:19:51,340 lots of little faint red galaxies in the 458 00:19:59,700 --> 00:19:53,140 background which of course is one of the 459 00:20:02,160 --> 00:19:59,710 primary goals of this program to 460 00:20:03,780 --> 00:20:02,170 interpret this image you need to have an 461 00:20:07,170 --> 00:20:03,790 understanding of the optics of the 462 00:20:08,910 --> 00:20:07,180 cluster so we've gotten a number of 463 00:20:10,830 --> 00:20:08,920 modelers from the community to provide 464 00:20:13,290 --> 00:20:10,840 us their best models for the maps of the 465 00:20:15,810 --> 00:20:13,300 dark matter and the lensing strengths of 466 00:20:18,000 --> 00:20:15,820 these clusters so shown in blue overlaid 467 00:20:19,710 --> 00:20:18,010 in blue is that blue is an estimate of 468 00:20:23,220 --> 00:20:19,720 the Dark Matter mass distribution in the 469 00:20:25,490 --> 00:20:23,230 cluster and in red is the critical curve 470 00:20:28,410 --> 00:20:25,500 so those areas of highest magnification 471 00:20:31,290 --> 00:20:28,420 so background galaxies that that are 472 00:20:33,810 --> 00:20:31,300 fall behind those critical lines can be 473 00:20:36,930 --> 00:20:33,820 magnified by factors up to a 10 or even 474 00:20:39,090 --> 00:20:36,940 100 and it's along those let those red 475 00:20:44,070 --> 00:20:39,100 regions where we are getting the deepest 476 00:20:46,530 --> 00:20:44,080 ever views into the universe so we've 477 00:20:48,480 --> 00:20:46,540 been going along here for over a year 478 00:20:51,330 --> 00:20:48,490 now and I'm pleased to say we have some 479 00:20:53,400 --> 00:20:51,340 very exciting science results we have in 480 00:20:55,920 --> 00:20:53,410 fact detected one of the most distant 481 00:20:57,600 --> 00:20:55,930 and intrinsically faintest objects so 482 00:21:00,420 --> 00:20:57,610 this is a redshift 10 483 00:21:03,330 --> 00:21:00,430 galaxy candidate which is triply imaged 484 00:21:04,590 --> 00:21:03,340 by this cluster and so one of the 485 00:21:07,170 --> 00:21:04,600 reasons why we think this is such a 486 00:21:09,240 --> 00:21:07,180 secure candidate for a redshift n object 487 00:21:11,880 --> 00:21:09,250 is not just the fact that has extremely 488 00:21:14,310 --> 00:21:11,890 red colors but where it lies relative to 489 00:21:16,530 --> 00:21:14,320 those critical curves its position it 490 00:21:19,020 --> 00:21:16,540 positions in this image provide further 491 00:21:23,400 --> 00:21:19,030 evidence of it being at an exceptionally 492 00:21:25,800 --> 00:21:23,410 high redshift so this is our second 493 00:21:27,630 --> 00:21:25,810 cluster Maxima for 1/6 all of the data 494 00:21:31,050 --> 00:21:27,640 for this cluster is also in hand 495 00:21:33,840 --> 00:21:31,060 unavailable and available online and 496 00:21:36,000 --> 00:21:33,850 these first two HST frontier fields and 497 00:21:37,770 --> 00:21:36,010 their parallels have have really been a 498 00:21:39,450 --> 00:21:37,780 success they've dramatically increased 499 00:21:43,290 --> 00:21:39,460 the number of intrinsically faint 500 00:21:46,950 --> 00:21:43,300 galaxies known to be in the first 501 00:21:49,740 --> 00:21:46,960 billion years of the universe why is 502 00:21:51,960 --> 00:21:49,750 this important well this is a result 503 00:21:55,290 --> 00:21:51,970 from a very recent paper looking just at 504 00:21:58,500 --> 00:21:55,300 the first cluster Abell 2744 this is a 505 00:22:01,230 --> 00:21:58,510 redshift 7 UV luminosity function I show 506 00:22:03,030 --> 00:22:01,240 with a black arrow the limit for the 507 00:22:04,620 --> 00:22:03,040 Hubble ultra-deep field and you can see 508 00:22:07,500 --> 00:22:04,630 we're going several magnitudes fainter 509 00:22:09,150 --> 00:22:07,510 than that one of the reasons why you 510 00:22:10,890 --> 00:22:09,160 know we're not just posted we're not 511 00:22:12,840 --> 00:22:10,900 just collecting little faint galaxies 512 00:22:15,360 --> 00:22:12,850 this is actually quite important because 513 00:22:17,730 --> 00:22:15,370 understanding how many faint galaxies 514 00:22:20,250 --> 00:22:17,740 they are can help us count up the number 515 00:22:21,870 --> 00:22:20,260 of photons that could contribute to the 516 00:22:24,540 --> 00:22:21,880 reionization of the universe at this 517 00:22:26,250 --> 00:22:24,550 epoch so as we go forward and we collect 518 00:22:28,140 --> 00:22:26,260 the rest of the clusters we'll be able 519 00:22:29,550 --> 00:22:28,150 to place incredibly good constraints on 520 00:22:31,950 --> 00:22:29,560 the slope of the faint end of the 521 00:22:35,880 --> 00:22:31,960 luminosity function during the era of 522 00:22:37,500 --> 00:22:35,890 reionisation of course there's lots and 523 00:22:39,180 --> 00:22:37,510 lots of other science that can be done 524 00:22:40,830 --> 00:22:39,190 with these images and I think that's one 525 00:22:43,710 --> 00:22:40,840 of the more exciting aspects of the 526 00:22:45,060 --> 00:22:43,720 program you know it's not just redshift 527 00:22:47,040 --> 00:22:45,070 10 galaxies that are interesting 528 00:22:49,260 --> 00:22:47,050 galaxies at cosmic high noon at rest 529 00:22:50,580 --> 00:22:49,270 just one to four will also be magnified 530 00:22:52,830 --> 00:22:50,590 and stretched and we can do 531 00:22:56,040 --> 00:22:52,840 groundbreaking science with those images 532 00:22:57,690 --> 00:22:56,050 on the clusters themselves will be you 533 00:22:59,850 --> 00:22:57,700 know can be studied in great detail 534 00:23:01,350 --> 00:22:59,860 we'll be able to map out the dark matter 535 00:23:04,500 --> 00:23:01,360 and the substructure within those 536 00:23:06,750 --> 00:23:04,510 clusters to unprecedented levels study 537 00:23:09,030 --> 00:23:06,760 the cluster galaxies the dwarfs and 538 00:23:10,840 --> 00:23:09,040 inter cluster light and some of the most 539 00:23:12,730 --> 00:23:10,850 exciting science is coming out of the 540 00:23:14,590 --> 00:23:12,740 franzine science looking for supernovae 541 00:23:17,560 --> 00:23:14,600 in these fields and there are lots of 542 00:23:20,950 --> 00:23:17,570 other things on going i'll just note 543 00:23:23,190 --> 00:23:20,960 that we have three geo programs that are 544 00:23:27,340 --> 00:23:23,200 getting ancillary data on these these 545 00:23:29,830 --> 00:23:27,350 clusters in the UV with the wif c3i are 546 00:23:32,080 --> 00:23:29,840 grism and then Steve Rodney's program 547 00:23:33,940 --> 00:23:32,090 which is a t oo program to follow up any 548 00:23:36,700 --> 00:23:33,950 exciting transients and there's 549 00:23:39,100 --> 00:23:36,710 something like 10 or 11 HST archival and 550 00:23:41,560 --> 00:23:39,110 theory programs from cycle 21 and 22 551 00:23:44,140 --> 00:23:41,570 that are dedicated to doing science with 552 00:23:46,030 --> 00:23:44,150 these data and so I encourage you to 553 00:23:47,530 --> 00:23:46,040 look again at the call for proposals and 554 00:23:52,000 --> 00:23:47,540 think about what you might want to do 555 00:23:55,270 --> 00:23:52,010 for cycle 23 I mentioned Dark Matter as 556 00:23:57,310 --> 00:23:55,280 one of the things that you can do and 557 00:23:59,140 --> 00:23:57,320 these data are also going to be 558 00:24:00,550 --> 00:23:59,150 transformative in our understanding of 559 00:24:02,890 --> 00:24:00,560 the Dark Matter distribution and 560 00:24:05,350 --> 00:24:02,900 clusters the fact that we are going so 561 00:24:08,440 --> 00:24:05,360 deep provides many multiplied image 562 00:24:10,050 --> 00:24:08,450 galaxies which provides allows us to map 563 00:24:13,120 --> 00:24:10,060 out the dark matter to unprecedented 564 00:24:14,710 --> 00:24:13,130 resolution and precision and so this is 565 00:24:18,070 --> 00:24:14,720 a map of the Dark Matter distribution 566 00:24:22,360 --> 00:24:18,080 made by Mathilde jazak earlier or last 567 00:24:24,310 --> 00:24:22,370 year this is our third cluster max oh 568 00:24:26,710 --> 00:24:24,320 seven one seven we're about halfway done 569 00:24:29,500 --> 00:24:26,720 with this cluster this image is of the 570 00:24:33,220 --> 00:24:29,510 ACS optical we're going to start getting 571 00:24:35,140 --> 00:24:33,230 the whiff c3 IR in a few weeks here we 572 00:24:36,820 --> 00:24:35,150 as of yesterday we're officially halfway 573 00:24:39,190 --> 00:24:36,830 complete with our frontier field 574 00:24:40,900 --> 00:24:39,200 observations and as I said those last 575 00:24:44,050 --> 00:24:40,910 two clusters and parallels are approved 576 00:24:46,810 --> 00:24:44,060 for next year's observations so this is 577 00:24:50,740 --> 00:24:46,820 the cluster that we were getting data 578 00:24:52,870 --> 00:24:50,750 for yesterday max 11:49 we completed the 579 00:24:55,930 --> 00:24:52,880 whiff c3 our observations will start 580 00:24:57,700 --> 00:24:55,940 again in April with ACS the background 581 00:25:00,100 --> 00:24:57,710 image here is beautiful but not quite as 582 00:25:02,050 --> 00:25:00,110 deep as our frontier fields will be this 583 00:25:04,930 --> 00:25:02,060 is taken from The Clash survey of a few 584 00:25:06,910 --> 00:25:04,940 years ago and I'm just going to zoom in 585 00:25:09,760 --> 00:25:06,920 here on the center of this cluster and 586 00:25:12,400 --> 00:25:09,770 sort of highlight this spiral galaxy in 587 00:25:14,230 --> 00:25:12,410 the middle so this is a spiral galaxy 588 00:25:17,170 --> 00:25:14,240 that's a background galaxy behind the 589 00:25:18,159 --> 00:25:17,180 cluster one of its arms as being lens by 590 00:25:20,409 --> 00:25:18,169 that one of the 591 00:25:23,950 --> 00:25:20,419 little red cluster galaxies in the 592 00:25:26,379 --> 00:25:23,960 middle and this object has been a source 593 00:25:27,789 --> 00:25:26,389 of one of the most unexpected things I 594 00:25:29,619 --> 00:25:27,799 think is coming out of the frontier 595 00:25:31,629 --> 00:25:29,629 fields so for any of the press in the 596 00:25:34,539 --> 00:25:31,639 audience this is embargoed but I just 597 00:25:36,669 --> 00:25:34,549 had to share these images see Rodney 598 00:25:40,180 --> 00:25:36,679 talked about this yesterday at the 599 00:25:42,430 --> 00:25:40,190 frontier fields hyperwall so the so this 600 00:25:44,560 --> 00:25:42,440 an object I said the this cluster was 601 00:25:47,619 --> 00:25:44,570 observed in 2011 as part of the clash 602 00:25:50,919 --> 00:25:47,629 program glass which is the grism program 603 00:25:52,690 --> 00:25:50,929 went back in November and the supernova 604 00:25:54,460 --> 00:25:52,700 team including Patrick Kelly and Steve 605 00:25:57,909 --> 00:25:54,470 Rodney were looking at these images and 606 00:26:02,349 --> 00:25:57,919 bam a pop not one not two not three but 607 00:26:04,450 --> 00:26:02,359 four images and they were incredibly 608 00:26:06,970 --> 00:26:04,460 lucky because we were about to start our 609 00:26:09,729 --> 00:26:06,980 seven week observing campaign getting 610 00:26:12,430 --> 00:26:09,739 seventy orbits on this cluster shortly 611 00:26:14,259 --> 00:26:12,440 thereafter so this object is actually 612 00:26:16,210 --> 00:26:14,269 the first detected multiply image 613 00:26:19,840 --> 00:26:16,220 supernova if christened its supernova 614 00:26:23,710 --> 00:26:19,850 ref stall after a seminal paper but 615 00:26:25,810 --> 00:26:23,720 that's not all so the arm of this spiral 616 00:26:27,879 --> 00:26:25,820 is being multiplied imaged by that 617 00:26:31,239 --> 00:26:27,889 little red galaxy but the spiral galaxy 618 00:26:33,340 --> 00:26:31,249 itself appears multiple times as well so 619 00:26:37,629 --> 00:26:33,350 there are three more images of that 620 00:26:39,489 --> 00:26:37,639 spiral arm in the in this cluster and we 621 00:26:41,799 --> 00:26:39,499 think that that super manova may have 622 00:26:44,320 --> 00:26:41,809 appeared several times before and will 623 00:26:46,629 --> 00:26:44,330 appear again so the light from this 624 00:26:48,580 --> 00:26:46,639 supernova has traveled seven has 625 00:26:51,700 --> 00:26:48,590 traveled or will travel seven separate 626 00:26:56,769 --> 00:26:51,710 paths around max 11:49 on its way to 627 00:26:59,919 --> 00:26:56,779 earth so just to summarize here with the 628 00:27:01,779 --> 00:26:59,929 ways that you can use this data as I 629 00:27:03,759 --> 00:27:01,789 said we had the raw data the science 630 00:27:07,119 --> 00:27:03,769 quality data and lensing maps are all 631 00:27:08,919 --> 00:27:07,129 public on mast and on our website we're 632 00:27:10,960 --> 00:27:08,929 done with the first two clusters we're 633 00:27:12,519 --> 00:27:10,970 halfway through with the second two 634 00:27:14,979 --> 00:27:12,529 clusters and they're breaking new 635 00:27:17,320 --> 00:27:14,989 frontiers left and right we had a 636 00:27:18,789 --> 00:27:17,330 successful midterm review and we're 637 00:27:21,759 --> 00:27:18,799 going forward with those last two 638 00:27:23,529 --> 00:27:21,769 clusters in cycle 23 and we're also 639 00:27:25,509 --> 00:27:23,539 thinking about providing additional 640 00:27:28,479 --> 00:27:25,519 funding opportunities for updating and 641 00:27:30,249 --> 00:27:28,489 improving the lensing models I didn't 642 00:27:31,300 --> 00:27:30,259 have any time to talk about Spitzer and 643 00:27:33,340 --> 00:27:31,310 Chandra but this 644 00:27:34,630 --> 00:27:33,350 Iraq observations for those last two 645 00:27:37,330 --> 00:27:34,640 clusters are underway 646 00:27:39,490 --> 00:27:37,340 Chandra there's lots of observations 647 00:27:42,820 --> 00:27:39,500 being done by Steve Murray and by 648 00:27:44,680 --> 00:27:42,830 Christine Jones foreman and in August at 649 00:27:46,750 --> 00:27:44,690 the IU there will be a several day 650 00:28:22,500 --> 00:27:46,760 workshop highlighting the frontier 651 00:28:28,470 --> 00:28:25,230 okay well the 25th anniversary of Hubble 652 00:28:31,230 --> 00:28:28,480 is obviously a huge milestone and we 653 00:28:34,110 --> 00:28:31,240 have an entire year of activities and 654 00:28:36,780 --> 00:28:34,120 events and programs planned starting 655 00:28:38,970 --> 00:28:36,790 really here at this meeting you've all 656 00:28:41,940 --> 00:28:38,980 seen all the great press that's come out 657 00:28:43,890 --> 00:28:41,950 all the the hype on social media from 658 00:28:46,230 --> 00:28:43,900 the release of the images this week so 659 00:28:48,330 --> 00:28:46,240 things are really kicking off this week 660 00:28:50,760 --> 00:28:48,340 for this year of celebration so I just 661 00:28:52,590 --> 00:28:50,770 wanted to highlight some of the our 662 00:28:55,440 --> 00:28:52,600 high-level plans and some of the the 663 00:28:57,000 --> 00:28:55,450 specifics that we have going on in the 664 00:29:01,380 --> 00:28:57,010 next year to celebrate Hubble's 25th 665 00:29:04,110 --> 00:29:01,390 anniversary so in a high level and we're 666 00:29:07,020 --> 00:29:04,120 sort of going on the the broad basic 667 00:29:09,360 --> 00:29:07,030 themes of celebrating this past quarter 668 00:29:12,120 --> 00:29:09,370 century of discovery and inspiration and 669 00:29:15,180 --> 00:29:12,130 really the effect on culture that Hubble 670 00:29:17,909 --> 00:29:15,190 has had and we want to not only look to 671 00:29:20,250 --> 00:29:17,919 the past but we want to also emphasize 672 00:29:22,140 --> 00:29:20,260 that the Hubble is going strong we 673 00:29:24,840 --> 00:29:22,150 expect it to last out till 2020 maybe 674 00:29:29,400 --> 00:29:24,850 longer and then of course emphasized 675 00:29:31,620 --> 00:29:29,410 Hubble's successor JWST and again sort 676 00:29:33,539 --> 00:29:31,630 of taking taking advantage of the fact 677 00:29:35,970 --> 00:29:33,549 that the Hubble is really infiltrated 678 00:29:38,250 --> 00:29:35,980 our culture in all these different 679 00:29:41,010 --> 00:29:38,260 realms we want to get out that message 680 00:29:42,570 --> 00:29:41,020 and be be really promoting the the idea 681 00:29:44,610 --> 00:29:42,580 that Hubble is the people's telescope 682 00:29:47,400 --> 00:29:44,620 it's not just a tool for astronomers 683 00:29:49,590 --> 00:29:47,410 that it's something that the public that 684 00:29:51,570 --> 00:29:49,600 our society can can celebrate and we 685 00:29:54,840 --> 00:29:51,580 also want to talk about how Hubble is a 686 00:29:57,330 --> 00:29:54,850 human story you know the the science 687 00:29:59,700 --> 00:29:57,340 that we do we people do the science and 688 00:30:01,650 --> 00:29:59,710 in addition to that of course Hubble has 689 00:30:03,480 --> 00:30:01,660 the great legacy of having had 690 00:30:05,730 --> 00:30:03,490 astronauts go to service it and that's a 691 00:30:06,960 --> 00:30:05,740 story that really resonates with the 692 00:30:09,180 --> 00:30:06,970 public and so we really want to 693 00:30:12,650 --> 00:30:09,190 emphasize the the human side of Hubble 694 00:30:14,610 --> 00:30:12,660 all along through the next year and so 695 00:30:18,450 --> 00:30:14,620 anytime we're doing these sort of 696 00:30:20,039 --> 00:30:18,460 outreach communications plans we take an 697 00:30:21,570 --> 00:30:20,049 audience based approach to make sure 698 00:30:23,330 --> 00:30:21,580 that what we're getting out is 699 00:30:25,950 --> 00:30:23,340 appropriate for the different audiences 700 00:30:27,720 --> 00:30:25,960 we really want to celebrate and engage 701 00:30:29,940 --> 00:30:27,730 what John Grunsfeld calls the Hubble 702 00:30:32,159 --> 00:30:29,950 generation so this generation of people 703 00:30:33,990 --> 00:30:32,169 25 and younger that have grown up with 704 00:30:34,799 --> 00:30:34,000 Hubble always having been in space and 705 00:30:37,710 --> 00:30:34,809 so 706 00:30:41,159 --> 00:30:37,720 we really want to emphasize on to that 707 00:30:42,930 --> 00:30:41,169 generation in our outreach events so we 708 00:30:46,440 --> 00:30:42,940 have a whole year of events and programs 709 00:30:48,960 --> 00:30:46,450 and products and we have of course along 710 00:30:50,669 --> 00:30:48,970 with the the specific discrete events we 711 00:30:52,980 --> 00:30:50,679 have a really robust social media and 712 00:30:54,720 --> 00:30:52,990 traditional media outreach plan which 713 00:30:57,480 --> 00:30:54,730 again has already started really in 714 00:31:00,330 --> 00:30:57,490 earnest this week our audience based 715 00:31:04,919 --> 00:31:00,340 approach is what you would expect of 716 00:31:07,889 --> 00:31:04,929 course we are celebrating and and really 717 00:31:09,930 --> 00:31:07,899 trying to to get the message out about 718 00:31:12,419 --> 00:31:09,940 that the team that built Hubble and the 719 00:31:15,450 --> 00:31:12,429 teams of scientists that have have used 720 00:31:17,399 --> 00:31:15,460 Hubble over the past 25 years and and of 721 00:31:19,710 --> 00:31:17,409 course the public is a big target of our 722 00:31:21,299 --> 00:31:19,720 outreach as always we really want to 723 00:31:24,299 --> 00:31:21,309 focus on on getting to non-traditional 724 00:31:25,950 --> 00:31:24,309 audiences you know there's a whole host 725 00:31:27,779 --> 00:31:25,960 of people out there that are already big 726 00:31:29,759 --> 00:31:27,789 NASA fans and we're glad about that 727 00:31:31,980 --> 00:31:29,769 we're happy about that we want to reach 728 00:31:35,430 --> 00:31:31,990 into some more audiences that might not 729 00:31:37,499 --> 00:31:35,440 already sort of be our fans and try to 730 00:31:40,289 --> 00:31:37,509 reach out to them and to get them 731 00:31:42,419 --> 00:31:40,299 engaged in the Hubble celebrations and 732 00:31:44,789 --> 00:31:42,429 then of course we have a very robust 733 00:31:47,100 --> 00:31:44,799 plan to reach out to teachers and 734 00:31:48,779 --> 00:31:47,110 students in the classroom which the 735 00:31:51,749 --> 00:31:48,789 Space Telescope Science Institute has a 736 00:31:53,489 --> 00:31:51,759 really great an excellent team that has 737 00:31:55,680 --> 00:31:53,499 been doing that for many years already 738 00:31:58,619 --> 00:31:55,690 and so we're just going to incorporate 739 00:32:00,600 --> 00:31:58,629 Hubble 25th into all of the great things 740 00:32:02,190 --> 00:32:00,610 that that Space Telescope does over the 741 00:32:04,289 --> 00:32:02,200 next year and then of course there's our 742 00:32:07,409 --> 00:32:04,299 external stakeholders or friends on 743 00:32:09,359 --> 00:32:07,419 Capitol Hill and our corporate partners 744 00:32:11,759 --> 00:32:09,369 that will be involved in a lot of these 745 00:32:14,999 --> 00:32:11,769 things as well this is all a big 746 00:32:16,169 --> 00:32:15,009 collaboration between NASA ISA obviously 747 00:32:19,230 --> 00:32:16,179 the Space Telescope Science Institute 748 00:32:22,049 --> 00:32:19,240 and then our external partners and also 749 00:32:24,330 --> 00:32:22,059 our have have a big role in a lot of our 750 00:32:25,950 --> 00:32:24,340 events as well so when I tell you about 751 00:32:27,210 --> 00:32:25,960 some of the specific things that we have 752 00:32:29,340 --> 00:32:27,220 planned and this is just going to 753 00:32:30,960 --> 00:32:29,350 scratch the surface of everything and 754 00:32:33,950 --> 00:32:30,970 just keep in mind again that everything 755 00:32:36,840 --> 00:32:33,960 that we do is going to be amplified by 756 00:32:38,759 --> 00:32:36,850 traditional and social media so the 757 00:32:40,889 --> 00:32:38,769 first big thing of course is a 758 00:32:43,889 --> 00:32:40,899 celebration event at the National Air 759 00:32:45,079 --> 00:32:43,899 and Space Museum in Washington DC so we 760 00:32:47,809 --> 00:32:45,089 have the 761 00:32:49,579 --> 00:32:47,819 the evenings secured on April 24th which 762 00:32:52,729 --> 00:32:49,589 is of course the launch anniversary and 763 00:32:55,729 --> 00:32:52,739 so that will be a large event to to 764 00:32:59,269 --> 00:32:55,739 celebrate to celebrate the launch and in 765 00:33:00,439 --> 00:32:59,279 addition to to that event IMAX has 766 00:33:02,689 --> 00:33:00,449 confirmed that they're going to 767 00:33:04,699 --> 00:33:02,699 re-release Hubble 3d in the month of 768 00:33:06,709 --> 00:33:04,709 April of this year so if you haven't 769 00:33:09,349 --> 00:33:06,719 seen that be sure to check out your 770 00:33:12,109 --> 00:33:09,359 local IMAX and it's a really great film 771 00:33:13,999 --> 00:33:12,119 so one of the things that we wanted to 772 00:33:16,069 --> 00:33:14,009 do for that event obviously only a 773 00:33:18,259 --> 00:33:16,079 certain number of people can attend it 774 00:33:21,919 --> 00:33:18,269 so we are planning to webcast that event 775 00:33:23,749 --> 00:33:21,929 and then have science centers planet 776 00:33:26,029 --> 00:33:23,759 area and all the NASA centers sort of 777 00:33:28,099 --> 00:33:26,039 host their own satellite sort of 778 00:33:29,869 --> 00:33:28,109 birthday parties for Hubble around the 779 00:33:32,749 --> 00:33:29,879 webcast and then kind of put their own 780 00:33:34,789 --> 00:33:32,759 Flair on whatever they want to do as to 781 00:33:37,219 --> 00:33:34,799 have their own localized event so we're 782 00:33:39,709 --> 00:33:37,229 envisioning you know a nationwide and 783 00:33:43,729 --> 00:33:39,719 even a worldwide celebration on that day 784 00:33:46,549 --> 00:33:43,739 of the launch anniversary so in addition 785 00:33:48,529 --> 00:33:46,559 to that all the NASA centers are engaged 786 00:33:50,089 --> 00:33:48,539 in the anniversary and they all have 787 00:33:52,759 --> 00:33:50,099 their again their different sort of spin 788 00:33:55,039 --> 00:33:52,769 that they'll put on on Hubble um a lot 789 00:33:57,889 --> 00:33:55,049 of the center's have besides Goddard 790 00:34:00,169 --> 00:33:57,899 obviously Goddard a big Center but many 791 00:34:01,759 --> 00:34:00,179 of the NASA centers had had parts in in 792 00:34:04,759 --> 00:34:01,769 the development of Hubble and the 793 00:34:06,919 --> 00:34:04,769 engineering especially so we're getting 794 00:34:09,019 --> 00:34:06,929 all the NASA centers engaged and they 795 00:34:11,329 --> 00:34:09,029 have their own sort of events plan in 796 00:34:15,529 --> 00:34:11,339 addition to the April 24th sort of 797 00:34:17,960 --> 00:34:15,539 Keystone event we're working on a big 798 00:34:21,139 --> 00:34:17,970 event the next day on April 25th that's 799 00:34:23,180 --> 00:34:21,149 Saturday at var hozy many of the 800 00:34:24,649 --> 00:34:23,190 astronauts the servicing mission and 801 00:34:26,779 --> 00:34:24,659 deployment astronauts will be in town 802 00:34:28,339 --> 00:34:26,789 for the event on the 24th so we wanted 803 00:34:30,680 --> 00:34:28,349 to take that great opportunity while we 804 00:34:33,319 --> 00:34:30,690 have all the astronauts in town to come 805 00:34:35,240 --> 00:34:33,329 up and have a big public event so we're 806 00:34:38,089 --> 00:34:35,250 working with the Smithsonian to to plan 807 00:34:40,549 --> 00:34:38,099 a big public event on that Saturday the 808 00:34:42,829 --> 00:34:40,559 25th attitude raha Zi with astronauts so 809 00:34:44,359 --> 00:34:42,839 that should be a lot of fun and we'll 810 00:34:48,710 --> 00:34:44,369 also look into the possibility of doing 811 00:34:52,190 --> 00:34:48,720 some webcast of that event as well New 812 00:34:54,200 --> 00:34:52,200 York City is very interested and already 813 00:34:56,659 --> 00:34:54,210 involved in many ways in celebrating 814 00:34:58,320 --> 00:34:56,669 Hubble and there's so many I mean 815 00:35:00,840 --> 00:34:58,330 there's several different 816 00:35:02,340 --> 00:35:00,850 museums which most of us familiar for 817 00:35:04,260 --> 00:35:02,350 and the American Museum of national 818 00:35:06,060 --> 00:35:04,270 history there's the intrepid museum the 819 00:35:07,890 --> 00:35:06,070 World Science Festival takes place every 820 00:35:09,450 --> 00:35:07,900 summer in New York City and so there's 821 00:35:11,250 --> 00:35:09,460 all these different groups that are all 822 00:35:14,190 --> 00:35:11,260 interested in have already started to 823 00:35:16,140 --> 00:35:14,200 contact us at NASA about how they can be 824 00:35:19,140 --> 00:35:16,150 involved in celebrating hubble's 25th 825 00:35:21,030 --> 00:35:19,150 anniversary so we're working on untying 826 00:35:23,460 --> 00:35:21,040 all those pieces together and really 827 00:35:26,940 --> 00:35:23,470 having a big celebration in the month of 828 00:35:28,440 --> 00:35:26,950 April in New York City so we did have 829 00:35:32,700 --> 00:35:28,450 something that has already happened in 830 00:35:34,680 --> 00:35:32,710 New York on New Year's Eve we had the 831 00:35:36,780 --> 00:35:34,690 Hubble video which I'll play for you in 832 00:35:39,900 --> 00:35:36,790 a few minutes it's a sort of a teaser 833 00:35:41,700 --> 00:35:39,910 video we had that played on a big 834 00:35:43,470 --> 00:35:41,710 Toshiba screen in Times Square on New 835 00:35:45,570 --> 00:35:43,480 Year's Eve where there were so many 836 00:35:48,870 --> 00:35:45,580 people gathered there and Mike Massimino 837 00:35:49,980 --> 00:35:48,880 gave a little a little short talk on the 838 00:35:52,470 --> 00:35:49,990 webcast of the New Year's Eve 839 00:35:55,320 --> 00:35:52,480 celebration so we've already had a 840 00:35:57,300 --> 00:35:55,330 really a really good a good event happen 841 00:35:59,940 --> 00:35:57,310 in New York City and we're looking 842 00:36:03,540 --> 00:35:59,950 forward to other events in the coming 843 00:36:05,820 --> 00:36:03,550 several months so in addition to New 844 00:36:12,300 --> 00:36:05,830 York there are of course museums 845 00:36:14,010 --> 00:36:12,310 planetary accretion events and in 846 00:36:16,380 --> 00:36:14,020 particular I mentioned the intrepid 847 00:36:18,900 --> 00:36:16,390 museum in New York City has already 848 00:36:22,320 --> 00:36:18,910 opened up in October an event dedicated 849 00:36:23,550 --> 00:36:22,330 to to the Hubble 25th anniversary so the 850 00:36:24,990 --> 00:36:23,560 next time you're in New York check that 851 00:36:27,810 --> 00:36:25,000 out it's a really beautiful exhibit 852 00:36:30,750 --> 00:36:27,820 it'll be up through next fall there was 853 00:36:33,060 --> 00:36:30,760 a panel there in October with the in 854 00:36:34,670 --> 00:36:33,070 November with the servicing mission for 855 00:36:37,470 --> 00:36:34,680 astronauts that was really well attended 856 00:36:42,450 --> 00:36:37,480 and that was also videoed and replayed 857 00:36:44,400 --> 00:36:42,460 on NASA TV and of course will work with 858 00:36:47,430 --> 00:36:44,410 NASA headquarters office of legislative 859 00:36:49,970 --> 00:36:47,440 and Inter government affairs and our 860 00:36:53,070 --> 00:36:49,980 industry partners to engage all our 861 00:36:54,720 --> 00:36:53,080 external stakeholders in in a lot of the 862 00:36:56,070 --> 00:36:54,730 events that they already do so the NASA 863 00:36:58,410 --> 00:36:56,080 day on the hill and those sorts of 864 00:37:01,110 --> 00:36:58,420 events so we have we're working with 865 00:37:05,280 --> 00:37:01,120 with them to to plan those things as 866 00:37:06,990 --> 00:37:05,290 well one really great way to reach out 867 00:37:09,420 --> 00:37:07,000 to some of the non-traditional audiences 868 00:37:10,300 --> 00:37:09,430 I mentioned is and these big public 869 00:37:11,770 --> 00:37:10,310 events that happen 870 00:37:14,290 --> 00:37:11,780 so one good example is South by 871 00:37:16,690 --> 00:37:14,300 Southwest down in Austin and that 872 00:37:18,490 --> 00:37:16,700 happens every March so the last few 873 00:37:20,200 --> 00:37:18,500 years NASA's had a very big presence at 874 00:37:22,240 --> 00:37:20,210 South by Southwest and this is an 875 00:37:24,490 --> 00:37:22,250 audience that is very tech interested 876 00:37:26,560 --> 00:37:24,500 but not necessarily space interested and 877 00:37:28,750 --> 00:37:26,570 so they love it when we show up with 878 00:37:30,910 --> 00:37:28,760 NASA stuff at South by Southwest and so 879 00:37:33,280 --> 00:37:30,920 we're going back again this year we have 880 00:37:35,950 --> 00:37:33,290 a panel in the interactive session on 881 00:37:39,370 --> 00:37:35,960 Hubble 25th and John Grunsfeld is on 882 00:37:41,140 --> 00:37:39,380 that panel and we have a big NASA 883 00:37:42,850 --> 00:37:41,150 exhibit that we're gonna have Hubble 884 00:37:46,090 --> 00:37:42,860 25th Clinton out we're going to take the 885 00:37:48,790 --> 00:37:46,100 big the Andromeda mosaic down to that so 886 00:37:50,320 --> 00:37:48,800 a lot of really exciting things for 887 00:37:51,730 --> 00:37:50,330 different large festivals that happen 888 00:37:53,320 --> 00:37:51,740 across the country and I already 889 00:37:55,750 --> 00:37:53,330 mentioned in World Science Festival and 890 00:37:57,040 --> 00:37:55,760 there are several other sort of events 891 00:38:01,230 --> 00:37:57,050 like that across the country that we're 892 00:38:05,020 --> 00:38:01,240 going to be doing over the next year 893 00:38:08,070 --> 00:38:05,030 we're excited to have secured exhibits 894 00:38:11,710 --> 00:38:08,080 in the Dulles and Reagan airports and 895 00:38:13,510 --> 00:38:11,720 this is just some some concepts of what 896 00:38:16,540 --> 00:38:13,520 that might look like and we're also 897 00:38:18,880 --> 00:38:16,550 reaching out to BWI and to some other 898 00:38:20,310 --> 00:38:18,890 airports across the country as well and 899 00:38:22,720 --> 00:38:20,320 Space Telescope is leading that effort 900 00:38:24,520 --> 00:38:22,730 but so when next time you fly through 901 00:38:27,190 --> 00:38:24,530 one of these major airports look out for 902 00:38:29,110 --> 00:38:27,200 Hubble cuz it'll be there there'll be a 903 00:38:31,180 --> 00:38:29,120 nationwide University lecture series 904 00:38:33,910 --> 00:38:31,190 going on I through the month of April 905 00:38:36,130 --> 00:38:33,920 and we're still working on that slide 906 00:38:38,920 --> 00:38:36,140 deck for that and so um get in touch 907 00:38:41,380 --> 00:38:38,930 with us to get to get slides to get 908 00:38:44,920 --> 00:38:41,390 support material for that of course the 909 00:38:47,560 --> 00:38:44,930 Hubble 2020 I'm symposium and that's 910 00:38:49,570 --> 00:38:47,570 coming up in April and then really just 911 00:38:51,430 --> 00:38:49,580 some other events of course double yes 912 00:38:53,880 --> 00:38:51,440 so we're at right now and other 913 00:38:57,010 --> 00:38:53,890 scientific meetings throughout the year 914 00:38:58,750 --> 00:38:57,020 Space Telescope again has a excellent 915 00:39:01,180 --> 00:38:58,760 team that's doing formal and informal 916 00:39:03,760 --> 00:39:01,190 education and so there's a whole host of 917 00:39:05,860 --> 00:39:03,770 education programs going on throughout 918 00:39:08,230 --> 00:39:05,870 the year that all focus on on Hubble 919 00:39:11,080 --> 00:39:08,240 25th I've already mentioned several 920 00:39:15,340 --> 00:39:11,090 times we have an extensive traditional 921 00:39:18,520 --> 00:39:15,350 and social media outreach plan we have a 922 00:39:19,960 --> 00:39:18,530 really a willing audience on social 923 00:39:22,690 --> 00:39:19,970 media and so we really hope to leverage 924 00:39:23,560 --> 00:39:22,700 all our different accounts the at NASA 925 00:39:25,330 --> 00:39:23,570 Twitter 926 00:39:28,470 --> 00:39:25,340 has eight and a half million followers 927 00:39:30,850 --> 00:39:28,480 just to give you an example and so we 928 00:39:33,190 --> 00:39:30,860 will work with all of the different 929 00:39:35,980 --> 00:39:33,200 partners and our corporate partners to 930 00:39:38,350 --> 00:39:35,990 just to really have a really consistent 931 00:39:40,090 --> 00:39:38,360 year-long presence on social media 932 00:39:42,700 --> 00:39:40,100 Twitter Facebook and all the other 933 00:39:44,920 --> 00:39:42,710 platforms and then the traditional media 934 00:39:48,670 --> 00:39:44,930 of course is also I'm a key part of this 935 00:39:50,680 --> 00:39:48,680 we there will be helpful 25th specials 936 00:39:52,750 --> 00:39:50,690 on National Geographic and Nova is also 937 00:39:54,760 --> 00:39:52,760 doing a documentary I already mentioned 938 00:39:58,900 --> 00:39:54,770 that um the Hubble 3d will be released 939 00:40:01,620 --> 00:39:58,910 on IMAX and then ISA is leading an 940 00:40:04,000 --> 00:40:01,630 effort to to get planetarium shorts 941 00:40:07,570 --> 00:40:04,010 distributed throughout throughout Europe 942 00:40:09,010 --> 00:40:07,580 and also throughout the US so that is 943 00:40:10,810 --> 00:40:09,020 another really exciting thing that will 944 00:40:13,300 --> 00:40:10,820 be happening across the planet area 945 00:40:15,760 --> 00:40:13,310 across the country and then Space 946 00:40:17,080 --> 00:40:15,770 Telescope is also doing three minute 947 00:40:18,490 --> 00:40:17,090 videos that they're going to be 948 00:40:20,740 --> 00:40:18,500 releasing every month and the preview 949 00:40:22,750 --> 00:40:20,750 for that sorry yacht so be looking for 950 00:40:24,580 --> 00:40:22,760 that one thing I haven't actually put in 951 00:40:26,620 --> 00:40:24,590 my slides but the place where you can go 952 00:40:29,200 --> 00:40:26,630 to find all of this information that 953 00:40:30,790 --> 00:40:29,210 will be constantly updated is a website 954 00:40:33,490 --> 00:40:30,800 that we have dedicated to the to the 955 00:40:36,520 --> 00:40:33,500 25th and that's Hubble 25th org so it's 956 00:40:39,250 --> 00:40:36,530 Hubble - 5 th org and so all of this 957 00:40:42,220 --> 00:40:39,260 information and ways to get involved for 958 00:40:44,560 --> 00:40:42,230 free for you you all to get involved in 959 00:40:45,580 --> 00:40:44,570 this will be available there and of 960 00:40:46,180 --> 00:40:45,590 course you can always get in touch with 961 00:40:50,440 --> 00:40:46,190 any of us 962 00:40:52,750 --> 00:40:50,450 to find out details as well so I'm gonna 963 00:40:54,850 --> 00:40:52,760 leave you with the the video that the 964 00:40:57,790 --> 00:40:54,860 NASA TV folks at headquarters um made 965 00:40:59,560 --> 00:40:57,800 for us just a couple months ago and I'm 966 00:42:16,840 --> 00:40:59,570 gonna go and play that now and finish 967 00:42:22,160 --> 00:42:19,790 thank you to our speakers for these 968 00:42:24,080 --> 00:42:22,170 great presentations and now if you we 969 00:42:26,810 --> 00:42:24,090 have a couple of minutes if you'd like 970 00:42:32,180 --> 00:42:26,820 to ask a question please make your way 971 00:42:33,800 --> 00:42:32,190 to a microphone and think not only of a 972 00:42:35,990 --> 00:42:33,810 question that you'd like to ask but 973 00:42:38,230 --> 00:42:36,000 maybe somebody out there in the 974 00:42:41,150 --> 00:42:38,240 community who'd like to ask a question 975 00:42:43,820 --> 00:42:41,160 and you can do that on behalf of them so 976 00:42:44,480 --> 00:42:43,830 that when we play this back they'll have 977 00:42:50,870 --> 00:42:44,490 the answer 978 00:42:53,480 --> 00:42:50,880 anybody don't be shy okay we've got a 979 00:42:56,180 --> 00:42:53,490 very shy audience okay great Martin 980 00:42:58,370 --> 00:42:56,190 thanks you Carol thanks oh is that the 981 00:42:59,600 --> 00:42:58,380 science right a meeting there was done 982 00:43:02,330 --> 00:42:59,610 yesterday and I was kind of curious 983 00:43:04,910 --> 00:43:02,340 there was a an omission and I'm kind of 984 00:43:07,160 --> 00:43:04,920 curious what is happening with cus 985 00:43:08,990 --> 00:43:07,170 that's such a powerful instrument 986 00:43:12,500 --> 00:43:09,000 there's a lot of science and interesting 987 00:43:14,270 --> 00:43:12,510 stories coming out could somebody tell 988 00:43:17,060 --> 00:43:14,280 us something about the cosmic origins 989 00:43:23,630 --> 00:43:17,070 spectrograph for for promote you know 990 00:43:24,890 --> 00:43:23,640 telling what Hubble is doing you'd like 991 00:43:26,540 --> 00:43:24,900 to hear about what kind of science is 992 00:43:29,600 --> 00:43:26,550 coming out is that the is that the 993 00:43:32,420 --> 00:43:29,610 question or is when was installed there 994 00:43:35,240 --> 00:43:32,430 was a lot of interest in what it was 995 00:43:38,570 --> 00:43:35,250 going to do but most of the public stuff 996 00:43:40,760 --> 00:43:38,580 that is out there is imagery right right 997 00:43:43,130 --> 00:43:40,770 but I'm wondering if there are stories 998 00:43:45,170 --> 00:43:43,140 in there for science writers or 999 00:43:46,640 --> 00:43:45,180 communicators like me and planetariums 1000 00:43:51,260 --> 00:43:46,650 and things that we can really highlight 1001 00:43:52,130 --> 00:43:51,270 yes the race person because advocate of 1002 00:43:54,860 --> 00:43:52,140 the conflict 1003 00:43:56,960 --> 00:43:54,870 yeah I'm spectroscopy is by training so 1004 00:43:59,020 --> 00:43:56,970 that's a it's an instrument that's near 1005 00:44:01,400 --> 00:43:59,030 and dear to my heart 1006 00:44:04,130 --> 00:44:01,410 cost is touching all kinds of 1007 00:44:07,060 --> 00:44:04,140 interesting subjects we've had several 1008 00:44:09,950 --> 00:44:07,070 large programs over the past few years 1009 00:44:12,680 --> 00:44:09,960 devoted to understanding 1010 00:44:14,150 --> 00:44:12,690 material out of which galaxies form the 1011 00:44:16,849 --> 00:44:14,160 circum Galactic medium and the 1012 00:44:20,060 --> 00:44:16,859 intergalactic medium and there's great 1013 00:44:22,250 --> 00:44:20,070 stories there about how you know this 1014 00:44:26,510 --> 00:44:22,260 the universe evolves and that structure 1015 00:44:29,210 --> 00:44:26,520 out of which galaxies forms on which 1016 00:44:32,960 --> 00:44:29,220 galaxies form evolves you've probably 1017 00:44:35,359 --> 00:44:32,970 seen some of that the the press update 1018 00:44:37,640 --> 00:44:35,369 that Andrew Fox gave on Monday was just 1019 00:44:39,800 --> 00:44:37,650 a little snippet of that and there's a 1020 00:44:42,290 --> 00:44:39,810 much bigger picture there much bigger 1021 00:44:45,829 --> 00:44:42,300 context cost is doing really great 1022 00:44:47,720 --> 00:44:45,839 things in the exoplanet area in the 1023 00:44:50,870 --> 00:44:47,730 looking at the atmospheres of exoplanets 1024 00:44:54,560 --> 00:44:50,880 and detecting heavy elements and 1025 00:44:58,099 --> 00:44:54,570 different kinds of species in the plan 1026 00:45:01,880 --> 00:44:58,109 planets that are essentially evaporating 1027 00:45:06,670 --> 00:45:01,890 these hot Jupiters there's lots of 1028 00:45:09,770 --> 00:45:06,680 interest in observations of hot stars 1029 00:45:12,800 --> 00:45:09,780 active galactic nuclei material 1030 00:45:16,010 --> 00:45:12,810 funneling into black holes just about 1031 00:45:18,680 --> 00:45:16,020 every area that you can think of causes 1032 00:45:21,290 --> 00:45:18,690 touching in some ways it's unfortunate 1033 00:45:24,710 --> 00:45:21,300 that oftentimes because of the 1034 00:45:27,500 --> 00:45:24,720 spectroscopic result it doesn't get put 1035 00:45:31,730 --> 00:45:27,510 into a context that's easy for the 1036 00:45:33,500 --> 00:45:31,740 public to understand and i'm carol knows 1037 00:45:34,940 --> 00:45:33,510 this i keep bugging her about this and 1038 00:45:37,339 --> 00:45:34,950 our other folks in our office of public 1039 00:45:40,579 --> 00:45:37,349 outreach to you know to try and make 1040 00:45:42,440 --> 00:45:40,589 that case better make it easier for you 1041 00:45:44,450 --> 00:45:42,450 and other science writers out there to 1042 00:45:46,910 --> 00:45:44,460 convey those interesting science results 1043 00:45:49,579 --> 00:45:46,920 so one of the things that we've started 1044 00:45:52,970 --> 00:45:49,589 doing is including some of the spectra 1045 00:45:54,710 --> 00:45:52,980 from costs and cysts in the material 1046 00:45:56,290 --> 00:45:54,720 that we release with press releases and 1047 00:45:58,520 --> 00:45:56,300 we're going to continue to do that 1048 00:46:01,760 --> 00:45:58,530 that's incredibly important because 1049 00:46:02,839 --> 00:46:01,770 James Webb is a spectroscopic machine 1050 00:46:04,160 --> 00:46:02,849 right 1051 00:46:05,990 --> 00:46:04,170 it will certainly produce beautiful 1052 00:46:08,870 --> 00:46:06,000 images but it's going to produce a 1053 00:46:10,160 --> 00:46:08,880 boatload of spectroscopy and most of its 1054 00:46:13,490 --> 00:46:10,170 science is going to be spectroscopy 1055 00:46:15,470 --> 00:46:13,500 related so thanks for asking that 1056 00:46:18,020 --> 00:46:15,480 question I'd be happy to talk with you 1057 00:46:21,079 --> 00:46:18,030 more individually one on one about some 1058 00:46:22,710 --> 00:46:21,089 specific suggestions and now that you've 1059 00:46:24,900 --> 00:46:22,720 asked that question I'm going 1060 00:46:28,050 --> 00:46:24,910 I'm gonna be emailing you and your 1061 00:46:30,420 --> 00:46:28,060 colleagues about how to help us convey 1062 00:46:31,859 --> 00:46:30,430 that information because you know we 1063 00:46:34,260 --> 00:46:31,869 often get these results and we're 1064 00:46:36,210 --> 00:46:34,270 working with the scientist to get their 1065 00:46:39,089 --> 00:46:36,220 results forward but we do need to be 1066 00:46:40,470 --> 00:46:39,099 able to convey that information to the 1067 00:46:45,810 --> 00:46:40,480 public so we have a question here and 1068 00:46:49,280 --> 00:46:45,820 then a question here so was launched I I 1069 00:46:51,780 --> 00:46:49,290 was about learning to read or write but 1070 00:46:53,520 --> 00:46:51,790 and I understand that I mean some 1071 00:46:57,000 --> 00:46:53,530 instruments and Hubble have been changed 1072 00:46:58,800 --> 00:46:57,010 but the things Hubble has Hubble has 1073 00:47:02,910 --> 00:46:58,810 apparently done very well in the past is 1074 00:47:05,609 --> 00:47:02,920 images but they'd say visit Gemini 1075 00:47:08,550 --> 00:47:05,619 planet image and so ground-based AO has 1076 00:47:11,070 --> 00:47:08,560 caught up almost called a plus Apple do 1077 00:47:13,830 --> 00:47:11,080 you see it trained to spectroscopy or 1078 00:47:15,300 --> 00:47:13,840 trained to UV in the proposals which are 1079 00:47:17,400 --> 00:47:15,310 areas where there's no ground-based 1080 00:47:22,109 --> 00:47:17,410 machine or no ground-based telescope 1081 00:47:29,130 --> 00:47:22,119 they'll ever be able to do that it's 1082 00:47:31,859 --> 00:47:29,140 it's certainly it's certainly good to 1083 00:47:33,390 --> 00:47:31,869 encourage things that you know people to 1084 00:47:35,460 --> 00:47:33,400 propose only things that Hubble can do 1085 00:47:36,990 --> 00:47:35,470 and like you said UV spectroscopy of 1086 00:47:38,280 --> 00:47:37,000 things of that nature is something that 1087 00:47:40,620 --> 00:47:38,290 only Hubble can do and when Hubble is 1088 00:47:42,530 --> 00:47:40,630 gone there won't be a resource at least 1089 00:47:44,820 --> 00:47:42,540 in the near term future to do that 1090 00:47:47,070 --> 00:47:44,830 Hubble is still extremely competitive 1091 00:47:49,160 --> 00:47:47,080 with even 8 and 10 meter telescopes on 1092 00:47:54,320 --> 00:47:49,170 the ground from an imaging standpoint 1093 00:47:57,839 --> 00:47:54,330 both from a resolution and sensitivity 1094 00:47:59,940 --> 00:47:57,849 standpoint but also from a grism 1095 00:48:02,480 --> 00:47:59,950 spectroscopy standpoint Wide Field 1096 00:48:05,070 --> 00:48:02,490 Camera 3 Grissom's 1097 00:48:06,839 --> 00:48:05,080 we can go deeper with those grism zan 1098 00:48:11,550 --> 00:48:06,849 you can possibly go from the ground now 1099 00:48:14,609 --> 00:48:11,560 that era to will end with the advent of 1100 00:48:16,410 --> 00:48:14,619 extremely large telescopes but for now 1101 00:48:18,660 --> 00:48:16,420 in at least the next couple years Hubble 1102 00:48:21,540 --> 00:48:18,670 should be very competitive with 1103 00:48:22,650 --> 00:48:21,550 ground-based observatories synergistic 1104 00:48:26,220 --> 00:48:22,660 certainly with some of the things that 1105 00:48:30,740 --> 00:48:26,230 Alma is doing and still have you know a 1106 00:48:34,290 --> 00:48:30,750 lot of discovery space available to it 1107 00:48:35,400 --> 00:48:34,300 yes your question thanks I'm Gregg 1108 00:48:36,049 --> 00:48:35,410 running from the University of Kansas 1109 00:48:37,999 --> 00:48:36,059 and 1110 00:48:39,289 --> 00:48:38,009 I want to ask a question about the 1111 00:48:41,299 --> 00:48:39,299 celebrations are at the 25th anniversary 1112 00:48:44,959 --> 00:48:41,309 I mean many of the activities are New 1113 00:48:47,209 --> 00:48:44,969 York City Washington area airports but 1114 00:48:50,420 --> 00:48:47,219 there is a distributed interest across 1115 00:48:52,099 --> 00:48:50,430 the entire country and so I was my 1116 00:48:53,779 --> 00:48:52,109 interest was piqued partly by your 1117 00:48:54,679 --> 00:48:53,789 University lecture series so I'd like to 1118 00:48:57,469 --> 00:48:54,689 hear a little bit more about what that 1119 00:48:59,449 --> 00:48:57,479 is but I also like to hear about what 1120 00:49:04,729 --> 00:48:59,459 kind of efforts are there to extend the 1121 00:49:06,620 --> 00:49:04,739 celebrations to institutions for example 1122 00:49:07,729 --> 00:49:06,630 all across the country for us so for 1123 00:49:10,099 --> 00:49:07,739 example one of the largest amateur 1124 00:49:12,829 --> 00:49:10,109 astronomy organizations in the country 1125 00:49:15,019 --> 00:49:12,839 is in Kansas City there are astronauts 1126 00:49:16,729 --> 00:49:15,029 spread all around the country we have a 1127 00:49:18,739 --> 00:49:16,739 few in Kansas Steve Hall is actually 1128 00:49:21,019 --> 00:49:18,749 offices next to mine so you know I'm 1129 00:49:22,910 --> 00:49:21,029 curious what efforts throw out to tap 1130 00:49:24,589 --> 00:49:22,920 into those resources or well all those 1131 00:49:27,079 --> 00:49:24,599 people be flying to DC I mean you know 1132 00:49:30,589 --> 00:49:27,089 for the anniversary and so we'll miss 1133 00:49:34,609 --> 00:49:30,599 that opportunity so I mentioned this one 1134 00:49:35,870 --> 00:49:34,619 yeah I mentioned the the event on April 1135 00:49:39,859 --> 00:49:35,880 24th that we're doing will be webcast 1136 00:49:42,709 --> 00:49:39,869 and we have someone that is going to be 1137 00:49:45,079 --> 00:49:42,719 like the point person for coordinating 1138 00:49:46,609 --> 00:49:45,089 and helping to distribute materials and 1139 00:49:50,390 --> 00:49:46,619 information to sort of host their own 1140 00:49:53,799 --> 00:49:50,400 celebrations that day so she has a list 1141 00:49:56,630 --> 00:49:53,809 of 200 you know science centers 1142 00:49:59,839 --> 00:49:56,640 planetary it's more focused on sort of 1143 00:50:02,029 --> 00:49:59,849 museums but also the University lecture 1144 00:50:03,949 --> 00:50:02,039 series is they'll be going on during 1145 00:50:05,719 --> 00:50:03,959 during that month that you mentioned 1146 00:50:08,660 --> 00:50:05,729 that's also a great way to get involved 1147 00:50:12,499 --> 00:50:08,670 so the the website that I mentioned will 1148 00:50:15,169 --> 00:50:12,509 will soon be hosting you know materials 1149 00:50:17,120 --> 00:50:15,179 that you can go and download or use and 1150 00:50:18,890 --> 00:50:17,130 then we'll also find ways to facilitate 1151 00:50:23,029 --> 00:50:18,900 you know sending materials to people who 1152 00:50:24,259 --> 00:50:23,039 want to do things so those those things 1153 00:50:27,829 --> 00:50:24,269 are definitely being planned 1154 00:50:31,489 --> 00:50:27,839 so anyone it can get in touch with us 1155 00:50:33,890 --> 00:50:31,499 for for help and for materials to to 1156 00:50:36,049 --> 00:50:33,900 sort of you know make your own sort of 1157 00:50:38,779 --> 00:50:36,059 celebration and we're working closely 1158 00:50:40,880 --> 00:50:38,789 with the astronaut office at NASA in 1159 00:50:42,890 --> 00:50:40,890 order to like you said to to sort of 1160 00:50:44,299 --> 00:50:42,900 take advantage of the fact that a lot of 1161 00:50:46,009 --> 00:50:44,309 the Hubble astronauts are sort of spread 1162 00:50:47,179 --> 00:50:46,019 out across the country so yeah we're 1163 00:50:48,890 --> 00:50:47,189 definitely we're definitely thinking 1164 00:50:49,400 --> 00:50:48,900 about those things but but yeah get in 1165 00:50:51,680 --> 00:50:49,410 touch 1166 00:50:55,039 --> 00:50:51,690 after the fact if you want more details 1167 00:50:57,289 --> 00:50:55,049 are to be you know to lead an event or 1168 00:51:00,859 --> 00:50:57,299 anything like that thanks very much 1169 00:51:03,769 --> 00:51:00,869 thank you question over here like your I 1170 00:51:05,479 --> 00:51:03,779 liked your slide on the status of Hubble 1171 00:51:07,339 --> 00:51:05,489 and in the fact that the gyro was 1172 00:51:09,620 --> 00:51:07,349 weren't going to be a foreseeable issue 1173 00:51:13,430 --> 00:51:09,630 but I heard from a friend of an engineer 1174 00:51:15,380 --> 00:51:13,440 that the the most critical component are 1175 00:51:17,299 --> 00:51:15,390 the one that that is they're most 1176 00:51:19,039 --> 00:51:17,309 concerned about is actually the solar 1177 00:51:21,349 --> 00:51:19,049 panels but I didn't see that on your 1178 00:51:24,019 --> 00:51:21,359 slide and that I'm hearing correctly 1179 00:51:27,019 --> 00:51:24,029 from my friend of the engineer or can 1180 00:51:29,960 --> 00:51:27,029 you give me an update on that at the 1181 00:51:31,430 --> 00:51:29,970 moment the electrical system on Hubble 1182 00:51:33,890 --> 00:51:31,440 is extremely good 1183 00:51:38,180 --> 00:51:33,900 I know of no issues with the solar 1184 00:51:41,059 --> 00:51:38,190 panels the solar panels do slowly 1185 00:51:43,609 --> 00:51:41,069 degrade with time we have not had any 1186 00:51:46,489 --> 00:51:43,619 issues with them in the last five years 1187 00:51:48,859 --> 00:51:46,499 or so the amount of power that they're 1188 00:51:52,009 --> 00:51:48,869 able to produce is declining with time 1189 00:51:53,690 --> 00:51:52,019 but it's not declining rapidly enough 1190 00:51:58,640 --> 00:51:53,700 that we would have to shut off an 1191 00:51:59,900 --> 00:51:58,650 instrument say honestly I think unless 1192 00:52:04,099 --> 00:51:59,910 there's some kind of a catastrophic 1193 00:52:06,140 --> 00:52:04,109 failure or meteorite hit or some kind of 1194 00:52:07,969 --> 00:52:06,150 catastrophic electrical failure that the 1195 00:52:10,609 --> 00:52:07,979 solar panels are not an issue it'd be 1196 00:52:24,140 --> 00:52:10,619 interesting to know exactly what your 1197 00:52:29,390 --> 00:52:24,150 engineer friend was thinking about very 1198 00:52:34,819 --> 00:52:29,400 same question Wow no problem with the 1199 00:52:35,630 --> 00:52:34,829 solar panels batteries batteries are in 1200 00:52:38,950 --> 00:52:35,640 really good shape 1201 00:52:41,900 --> 00:52:38,960 we've got about 500 amp hours a charge 1202 00:52:46,130 --> 00:52:41,910 capability with those now that's still 1203 00:52:48,319 --> 00:52:46,140 up well above what we need and so they 1204 00:52:49,640 --> 00:52:48,329 were they were replaced during the 1205 00:52:53,989 --> 00:52:49,650 servicing mission as well and they're 1206 00:52:55,969 --> 00:52:53,999 performing beautifully well let's thank 1207 00:52:58,309 --> 00:52:55,979 our speakers again and thank you for 1208 00:53:03,289 --> 00:52:58,319 coming to the town hall 1209 00:53:05,749 --> 00:53:03,299 oh we have one more question sorry so I 1210 00:53:08,170 --> 00:53:05,759 think it was a few months ago that a 1211 00:53:11,630 --> 00:53:08,180 very interesting paper by Neil Reed 1212 00:53:14,779 --> 00:53:11,640 appeared in a strop eh and I'm just 1213 00:53:16,969 --> 00:53:14,789 wondering if anything is being done to 1214 00:53:19,459 --> 00:53:16,979 mitigate the problem that he pointed out 1215 00:53:23,029 --> 00:53:19,469 exists statistically in the proposal 1216 00:53:25,910 --> 00:53:23,039 reviews sure I'll I'll take that I'm 1217 00:53:29,059 --> 00:53:25,920 part of the science mission office so 1218 00:53:31,969 --> 00:53:29,069 the the study that the speaker's is 1219 00:53:34,609 --> 00:53:31,979 referring to was an analysis of the 1220 00:53:38,239 --> 00:53:34,619 success rates of female and male PI's 1221 00:53:40,670 --> 00:53:38,249 over the history of HSTs tack process 1222 00:53:44,839 --> 00:53:40,680 and every year there is a very very 1223 00:53:46,959 --> 00:53:44,849 small but but really there difference in 1224 00:53:49,670 --> 00:53:46,969 that women pis are underrepresented 1225 00:53:52,339 --> 00:53:49,680 relative to the male PI's and when you 1226 00:53:54,140 --> 00:53:52,349 add that up over you know the 20 or so 1227 00:53:56,449 --> 00:53:54,150 tax it becomes apparent that this is a 1228 00:53:59,420 --> 00:53:56,459 real trend this happens every single 1229 00:54:01,699 --> 00:53:59,430 year so we're we're aware of the problem 1230 00:54:04,640 --> 00:54:01,709 we don't really know how to fix this 1231 00:54:10,609 --> 00:54:04,650 last year we tried an experiment where 1232 00:54:13,579 --> 00:54:10,619 we removed we took the names of the pis 1233 00:54:15,140 --> 00:54:13,589 we only included the first initial so 1234 00:54:17,569 --> 00:54:15,150 that people didn't necessarily know 1235 00:54:20,120 --> 00:54:17,579 whether it was a male or female PI we 1236 00:54:22,579 --> 00:54:20,130 also put the names on a second page and 1237 00:54:25,670 --> 00:54:22,589 we labeled the proposals by number not 1238 00:54:28,539 --> 00:54:25,680 name and we instructed people to discuss 1239 00:54:30,559 --> 00:54:28,549 the proposal and not who the PI's were 1240 00:54:32,809 --> 00:54:30,569 that didn't seem to make a big 1241 00:54:34,910 --> 00:54:32,819 difference so will we're going to 1242 00:54:37,549 --> 00:54:34,920 continue to investigate this problem the 1243 00:54:39,620 --> 00:54:37,559 other thing that we do during the at the 1244 00:54:41,900 --> 00:54:39,630 start of each attack during the 1245 00:54:44,749 --> 00:54:41,910 orientation that we remind people about 1246 00:54:46,640 --> 00:54:44,759 the issue of unconscious bias and make 1247 00:54:48,199 --> 00:54:46,650 sure that all the panelists and the takt 1248 00:54:50,979 --> 00:54:48,209 chairs are aware that this is a real 1249 00:54:54,199 --> 00:54:50,989 issue in when you're discussing 1250 00:54:57,499 --> 00:54:54,209 proposals and and female versus male pis 1251 00:55:04,459 --> 00:54:57,509 but you know we're aware we're doing the 1252 00:55:06,229 --> 00:55:04,469 best that we can I would say is there a 1253 00:55:10,130 --> 00:55:06,239 new study that's going to be done about 1254 00:55:12,050 --> 00:55:10,140 whether there's institutional bias you 1255 00:55:14,600 --> 00:55:12,060 mean at the level of 1256 00:55:16,640 --> 00:55:14,610 can you ask about can you clarify I can 1257 00:55:23,000 --> 00:55:16,650 clarify that because I was at an 1258 00:55:25,700 --> 00:55:23,010 institution 16 years ago and one year I 1259 00:55:27,920 --> 00:55:25,710 submitted three Hubble proposals and I 1260 00:55:30,050 --> 00:55:27,930 had three Hubble proposals accepted 1261 00:55:32,780 --> 00:55:30,060 which was excellent I then moved to a 1262 00:55:35,200 --> 00:55:32,790 much larger institution and since then 1263 00:55:38,330 --> 00:55:35,210 my success rate has gone down 1264 00:55:41,630 --> 00:55:38,340 significantly and I'm just you know it 1265 00:55:43,880 --> 00:55:41,640 just seemed very very peculiar that's 1266 00:55:46,070 --> 00:55:43,890 that's we can look into that we I don't 1267 00:55:47,960 --> 00:55:46,080 know that we have done that study of 1268 00:55:49,580 --> 00:55:47,970 large versus small institutions but 1269 00:55:53,030 --> 00:55:49,590 that's something that I think the idea 1270 00:55:54,860 --> 00:55:53,040 to look at okay thank you I will say 1271 00:55:58,460 --> 00:55:54,870 that I'm on a proposal studying 1272 00:56:01,430 --> 00:55:58,470 Westerlund too and it's all women sort 1273 00:56:04,670 --> 00:56:01,440 of not by accident but we did get the 1274 00:56:06,920 --> 00:56:04,680 time so and we're coming out pretty soon 1275 00:56:10,010 --> 00:56:06,930 with some pretty impressive results so