Coordinated Observation Report

sunit_id  PC            Plan_Window_start - Plan_Window_end      USC(s) and Visit_Comments
-------  -----------    -----------------   -----------------    --------------------------...
1409201   JANUSZEWSKI   2015.306:04:55:00 - 2015.306:05:45:00    USC='Visit is coord with New Horizons'  

1407613   ARMSTRONG     2016.007:00:00:00 - 2016.015:17:55:30    VISIT_COMMENT='This is a close white dwarf + white dwarf binary, with a projected orbital separation of ~0.7", and a period of ~19 years. This binary is monitored with HST/FGS for more than a decade (PI Howard Bond). The aim of this visit should be observe both white dwarfs simultanesoulsy by acquiring the binary along the cross-dispersion direction on the 52x2 slit. 12 Sep 2015: J. Farihi has updated the roll angle so that there is a good chance to get both stars on the STIS slit; Ed Nelan and Gail Schaefer have provided a detailed, month by month ephemeris for the binary over cycle 23. The only viable scheduling period is during a 10 day window in January(). ORIENT required to avoid diffraction spikes of primary. Target is expected at PA=335.9 deg on 2016 Jan 12 (middle of 10-day window), and thus optimal slit alignment is 335.9 deg, and U3 axis at 20.9 deg or 200.9 deg 11 Nov 2015: Removed "on hold" flag, as Jay already implemented the PA constraints.'  

1419306   PERRIELLO     2016.023:05:17:33 - 2016.023:05:17:35    USC='Coordinated with ground-based.'  

1419307   PERRIELLO     2016.025:04:55:28 - 2016.025:04:55:30    USC='coordinated with ground based'  

1419308   PERRIELLO     2016.027:02:57:33 - 2016.027:02:57:35    USC='coordinated with ground based'  

1419309   PERRIELLO     2016.029:02:37:30 - 2016.029:02:37:32    USC='coordinated with ground based'  

1419310   PERRIELLO     2016.071:04:44:13 - 2016.071:04:44:15    USC='coordinated with ground based.'  

1445311   VICK          2016.086:04:12:19 - 2016.086:04:12:21    USC='keep to spring, loosely coord with Spitzer'  

1445321   VICK          2016.091:08:12:22 - 2016.091:08:12:24    USC='keep to spring, loosely coord with Spitzer'  

1445331   VICK          2016.098:16:40:05 - 2016.098:16:40:07    USC='keep to spring, loosely coord with Spitzer'  

1445341   VICK          2016.104:14:08:44 - 2016.104:14:08:46    USC='keep to spring, loosely coord with Spitzer'  

1448001   TAYLOR        2016.121:03:00:00 - 2016.122:12:59:59    USC='Two-day window covers XMM availability. Will tweak closer to scheduling time.'  

1419301   PERRIELLO     2016.135:19:45:00 - 2016.135:20:29:59    USC='Coordinated with Swift, Spitzer, and ground-based.'  

1419302   PERRIELLO     2016.138:01:45:00 - 2016.138:02:19:59    USC='Coordinated with Swift, Spitzer, and ground-based.'  

1419303   PERRIELLO     2016.139:17:20:00 - 2016.139:17:59:59    USC='Coordinated with Swift, Spitzer, and Ground-based.'  

1410505   JANUSZEWSKI   2016.139:22:59:08 - 2016.139:23:44:59    USC='Force where it works, coord with Chandra, XMM.'  

1410506   JANUSZEWSKI   2016.140:00:00:00 - 2016.140:01:14:59    USC='Force where it can work. Coord with Chandra and XMM.'  

1410507   JANUSZEWSKI   2016.140:02:00:00 - 2016.140:02:59:59    USC='Force where it can work.  Coord with Chandra, XMM.'  

1419304   PERRIELLO     2016.141:21:45:00 - 2016.141:22:29:59    USC='Coordinated with Swift, Spitzer, and ground-based.'  

1447901   ROYLE         2016.142:00:00:00 - 2016.177:23:59:59    USC='Semi-Coordinated with two other observatories.'     VISIT_COMMENT='Should be simultaneous with the coordinated XMM-Newton observation. To achieve a 4-fold diversity of grating settings for each grating, instead of using 4 FPPOS positions for each grating, we use multiple central wavelengths for G130M and G160M to make sure we span the gap between segments A and B, and we use different FPPOS positions for each of those.'  

1410513   JANUSZEWSKI   2016.145:17:24:04 - 2016.145:17:59:59    USC='Force where it can work. Coord with Chardra and XMM.'  

1410514   JANUSZEWSKI   2016.145:18:30:00 - 2016.145:19:29:59    USC='Forced where it can work.  Coord with Chandra and XMM.'  

1410515   JANUSZEWSKI   2016.145:20:15:00 - 2016.145:21:14:59    USC='Forced where it can work. Coord with Chandra and XMM.'  

1448201   VICK          2016.160:00:00:00 - 2016.212:00:00:00    USC='rough spot.  Tighter coordination to come.'     VISIT_COMMENT='Should be simultaneous with the coordinated XMM-Newton observation. To achieve a 4-fold diversity of grating settings for each grating, instead of using 4 FPPOS positions for each grating, we use multiple central wavelengths for G130M and G160M to make sure we span the gap between segments A and B, and we use different FPPOS positions for each of those.'  

1426701   VICK          2016.181:04:00:00 - 2016.181:06:21:59    USC='coord with Cassini'  

1426702   VICK          2016.181:04:00:00 - 2016.181:06:21:59    USC='coord with Cassini'  

1426703   VICK          2016.181:04:00:00 - 2016.181:06:22:04    USC='coord with Cassini'  

1419305   PERRIELLO     2016.188:00:45:00 - 2016.188:01:19:59    USC='Coordinated with Swift, Spitzer, and Ground-based.'  

1407204   ARMSTRONG     2016.191:00:00:00 - 2016.247:00:00:00    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407201   ARMSTRONG     2016.193:00:00:00 - 2016.249:00:00:00    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407202   ARMSTRONG     2016.193:00:00:00 - 2016.249:00:00:00    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407205   ARMSTRONG     2016.193:00:00:00 - 2016.249:00:00:00    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407206   ARMSTRONG     2016.193:00:00:00 - 2016.249:00:00:00    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1433101   MEYETT        2016.201:14:00:00 - 2016.201:14:22:45    VISIT_COMMENT='We have do not have yet the XMM schedule.'  

1426704   VICK          2016.232:18:49:44 - 2016.232:23:17:29    USC='coord with Cassini'  

1426705   VICK          2016.232:18:49:44 - 2016.232:23:17:29    USC='coord with Cassini'  

1426706   VICK          2016.232:18:49:44 - 2016.232:23:17:29    USC='coord with Cassini'  

1434701   JANUSZEWSKI   2016.242:00:00:00 - 2016.263:00:00:00    USC='Visits loosly coord w/NRAO.'  

1434702   JANUSZEWSKI   2016.242:00:00:00 - 2016.263:00:00:00    USC='Visits loosly coord w/NRAO.'  

1407203   ARMSTRONG     2016.243:00:00:00 - 2016.256:23:59:59    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407207   ARMSTRONG     2016.243:00:00:00 - 2016.256:23:59:59    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407208   ARMSTRONG     2016.243:00:00:00 - 2016.256:23:59:59    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407209   ARMSTRONG     2016.243:00:00:00 - 2016.256:23:59:59    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407210   ARMSTRONG     2016.243:00:00:00 - 2016.294:23:59:59    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407213   ARMSTRONG     2016.243:00:00:00 - 2016.291:00:00:00    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407215   ARMSTRONG     2016.247:00:00:00 - 2016.302:23:59:59    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407211   ARMSTRONG     2016.250:00:00:00 - 2016.305:00:00:00    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1418801   PERRIELLO     2016.250:11:43:35 - 2016.254:00:00:00    USC='Coordinated with Spitzer'     VISIT_COMMENT='This 5-orbit visit should be coordinated with simultaneous Spitzer observations (17.6 Spitzer hours awarded, so there is a fairly long range of overlap).'  

1447601   MEYETT        2016.265:11:26:00 - 2016.266:04:27:59    USC='This is an XMM/HST coordinated observation.  Although the XXM and HST observation do not need to overlap, it is best to get them to schedule as close as possible.  The PI would prefer the 16.265 scheduling window as her first option and 16.266 scheduling'  

1407217   ARMSTRONG     2016.291:00:00:00 - 2016.347:00:00:00    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407214   ARMSTRONG     2016.339:00:00:00 - 2017.006:23:59:59    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407216   ARMSTRONG     2016.340:00:00:00 - 2017.030:00:00:00    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407218   ARMSTRONG     2016.340:00:00:00 - 2017.030:00:00:00    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407212   ARMSTRONG     2016.348:00:00:00 - 2017.030:00:00:00    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407219   ARMSTRONG     2016.351:00:00:00 - 2017.030:00:00:00    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

1407220   ARMSTRONG     2017.040:00:00:00 - 2017.060:23:59:59    VISIT_COMMENT='Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy allows for maximum exposure lengths with ACS in parallel, mitigating latency due to buffer dumps. Orientation requirements set to ensure that the parallel falls within the PHAT coverage & to maximize coverage of star-forming regions. These restrictions can be loosened if schedulability becomes an issue.'  

-------  -----------    -----------------   -----------------    --------------------------...
sunit_id  PC            Plan_Window_start - Plan_Window_end      USC(s) and Visit_Comments

Generated on  Sun Apr 10 18:45:44 2016