! File: 3848C.PROP ! Database: PEPDB ! Date: 19-FEB-1994:21:37:07 coverpage: title_1: SEPARATE LIGHTCURVES OF PLUTO AND CHARON sci_cat: SOLAR SYSTEM sci_subcat: MINOR PLANETS proposal_for: GO longterm: 1 pi_title: DR. pi_fname: MARC pi_mi: W. pi_lname: BUIE pi_inst: LOWELL OBSERVATORY pi_country: USA pi_phone: 602-774-3358 hours_pri: 12.14 num_pri: 1 wf_pc: Y time_crit: Y funds_amount: 306000 funds_length: 24 funds_date: JUN-92 off_fname: ROBERT off_mi: L. off_lname: MILLIS off_title: DIRECTOR off_inst: LOWELL OBSERVATORY off_addr_1: MARS HILL RD., 1400 WEST off_city: FLAGSTAFF off_state: AZ off_zip: 86001 off_country: USA off_phone: (602)774-3358 ! end of coverpage abstract: line_1: With this program we will begin a systematic effort to collect separate line_2: lightcurve data on the Pluto and Charon system. Such observations will line_3: continue to improve the albedo mapping of their surfaces by splitting the line_4: present ground-based ambiguity in the combined lightcurve. The observations line_5: must be done at the such times when it is within 25 arcseconds of a star of line_6: similar brightness. Such data will provide both the lightcurves and the line_7: phase angle behavior of each object. In addition to the photometry, line_8: astrometric measurements of Pluto and Charon relative to each of the background line_9: field stars can be made from the imaging data. In sufficient quantity, these line_10: data will further refine our knowledge of the sizes and relative masses of line_11: Pluto and Charon. Continued work on the photometry will allow us to watch the line_12: lightcurve evolution as Pluto moves away from the sun and as the Sun progresses line_13: to higher and higher latitudes. ! ! end of abstract general_form_proposers: lname: BUIE fname: MARC title: PI mi: W. inst: LOWELL OBSERVATORY country: USA ! lname: THOLEN fname: DAVID mi: J. inst: UNIVERSITY OF HAWAII country: USA ! lname: WASSERMAN fname: LARRY mi: H. inst: LOWELL OBSERVATORY country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: All observations are blind-pointed PC exposures of the Pluto-Charon line_2: system while in the same PC6 field of view with a star similar in line_3: brightness to Pluto. For each appulse, we take two sets of exposures line_4: separated by at least 6 hours to get distinct lightcurve points. line_5: During 10 of the 12 appulses, we will take exposures only in F555W. line_6: During the other 2 appulses we will take exposures in F439W and F555W. line_7: The target pointing is constructed so that the telescope is pointed to line_8: and tracks the mid-point between the Pluto-Charon barycenter and the line_9: appulse star. The window on the target specification is defined to line_10: include only the time the star and Pluto can appear on PC6 for nominal line_11: roll. The window is conservative at a level of 3" on each side to line_12: allow for pointing errors from the guide stars and for slight line_13: off-nominal roll conditions. If off-nominal roll is required to line_14: schedule the observations, the PI can provide verification on whether line_15: the pointing will work or not. The only hard and fast rule for line_16: checking this is to see if Pluto and the star are on PC6 for the given line_17: time and roll angle. The PI is willing to provide additional line_18: information if off-nominal roll is required to schedule the line_19: observations. line_21: Tracking the mid-point between Pluto and the appulse star will cause line_22: some slight trailing for the F555W exposures and more noticeable line_23: trailing for the F439W exposures. Both Pluto and the star will be ! question: 3 section: 2 line_1: trailed by nearly equal amounts. To allow us to remove the effects of line_2: the trailing, we require full pointing (V1 and V3 on the line_3: plane-of-the-sky) reconstructions with each observation. We would also line_4: appreciate a FHST update immediately before each visit to provide the line_5: best possible information on roll angle. The default tracking mode of line_6: fine-lock is preferred for all observations but coarse-track is line_7: acceptable if there aren't enough stars to support fine-lock. line_9: We have chosen 12 appulses from the full set of 24. This set of 12 line_10: maximizes the scientific return for the allotted spacecraft time. line_11: However, some of these appulses may be unobservable due to SAA passages line_12: or lunar avoidance. The other 12 appulses are provided as backup line_13: observations if any of the original 12 cannot be scheduled. The PI line_14: must be contacted for the replacement observation since it depends on line_15: the coverage lost by the unschedulable observation. line_17: The primary set of observations from the SELECT SET are EXP LOG LINEs line_18: 10, 30, 50, 70, 90, 100, 130, 150, 170, 190, 210, and 220. ! question: 4 section: 1 line_1: Separating the individual lightcurves of Pluto and Charon is a very difficult line_2: task from ground-based observatories. At best, their separation is 1 line_3: arc-sec. Under the best conditions from the best site at the best telescope line_4: (often considered to be CFHT on Mauna Kea), it is possible to get separate line_5: magnitudes for Pluto and Charon, near elongation, under conditions of line_6: excellent seeing. However, collecting a complete lightcurve becomes line_7: extremely difficult when conditions of telescope scheduling and weather are line_8: confronted. In this case, weather includes losing a night to bad seeing, not line_9: just poor photometric conditions. The telescope scheduling difficulties are line_10: not to be understated. Due to the slow rotation period of Pluto, photometric line_11: measurements are spread out over a large number of nights. These line_12: observations do not take very much time but at present scheduling practices line_13: at most telescopes preclude using a large number of partial nights. Also, line_14: resolved images near minimum separation cannot be obtained from the ground. line_16: The Hubble Space Telescope counters both of these difficulties. The enhanced line_17: spatial resolution of HST can easily separate the two bodies, even fairly line_18: close to minimum separation (about 0.2 arcsec). The image degradation caused line_19: by the spherical aberration may actually be beneficial to this project because line_20: more source photons can be collected per image. Given the low efficiency of line_21: this program, the photometric signal-to-noise ratio of the observations as a line_22: function of spacecraft time is greatly increased by the aberration. Also, line_23: the larger image size to pixel size ratio will permit a more accurate ! question: 4 section: 2 line_1: determination of the image centroid, thereby improving the relative line_2: astrometry of the two bodies. line_4: An additional advantage of HST is the way it is scheduled and run. An line_5: observation of this nature requiring periodic, short obseravations can line_6: be accomodated much more easily than with most ground-based observatories. ! question: 5 section: 1 line_1: This proposal will require special scheduling to ensure that Pluto is line_2: always seen in a field with another similarly bright star. All the line_3: special scheduling is provided as time windows on the target list. line_4: The initial set of observations chosen from the candiate SELECT set line_5: provides optimum lightcurve and solar phase angle coverage. ! question: 6 section: 1 line_1: For accurate image deconvolutions and positional measurements we require line_2: full pointing reconstructions (RA and DEC vs. time) during each exposure. line_3: This will allow us to create numerical PSFs that match the actual jitter line_4: and tracking that occurs during each exposure. We also need the best line_5: possible knowledge of the roll angle of the spacecraft. If possible, line_6: please schedule an FHST update immediately prior to each observation. ! question: 7 section: 1 line_1: The data reduction and analysis will be carried out by the proposers on their line_2: currently available computers. We expect additional work to be carried out line_3: by a post-doc for whom we wish to procure a new workstation. line_5: The data reductions will require PSF fitting to establish the magnitudes and line_6: relative positions of Pluto, Charon, and the field star. These data must be line_7: cross referenced with the nearly simultaneous ground-based observations of the line_8: combined magnitudes to complete the photometric reductions prior to modeling. line_9: Ground-based astrometry must also be collected so that the astrometric net line_10: provided by the appulse star can be calibrated. We plan to try conventional line_11: Schmidt astrometry on this field but if this proved inadequate we will do line_12: the astrometry using wide-field plates to be taken at CFHT on Mauna Kea. line_13: Our goal is to obtain astrometry at the 0.001" level. This may prove infeasible line_14: but is required to advance our knowledge of the individual densities of line_15: Pluto and Charon. line_17: Once the astrometric and lightcurve reductions are complete, the observations line_18: will be added to existing orbit and albedo models. ! question: 8 section: 1 line_1: Ground-based observations will be required to establish a high-precision line_2: astrometric net which will tie together all the individual HST line_3: observations. This net of stars will cover all of the appulse stars in line_4: our candiate list. Without these supporting observations, we will be unable line_5: to provide any information about the barycentric motion of Pluto and Charon. line_7: We also must continue to provide ground-based combined lightcurve line_8: measurements. The photometric accuracy of HST and the PC are insufficient line_9: for our models. By combining extremely accurate low spatial resolution line_10: ground-based observations with lower accuracy high spatial resolution data, line_11: we can achieve significant improvements in our model of the surface of Pluto line_12: and Charon. The ground-based observations are essential for maximizing the line_13: return from the HST data. ! question: 10 section: 1 line_1: The PI and Co-I's already have most of the computer facilities and line_2: the necessary access to ground-based telescopes to support this project. line_3: The PI will also work to secure computing time from supercomputer centers line_4: such as NCSA or SDSC to support the albedo modeling efforts. ! !end of general form text general_form_address: lname: BUIE fname: MARC mi: W. category: PI inst: LOWELL OBSERVATORY addr_1: MARS HILL ROAD, 1400 WEST city: FLAGSTAFF state: AZ zip: 86001 country: USA phone: (602)774-3358 ! ! end of general_form_address records ! No fixed target records found solar_system_targets: targnum: 1 name_1: PL-CH-1 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 31M 44.455S, lev1_3: DEC1 = -03D 21' 50.69", lev1_4: RA2 = 15H 31M 42.039S, lev1_5: DEC2 = -03D 21' 44.79", lev1_6: EPOCH1=20-MAY-92:20:50, lev1_7: EPOCH2=21-MAY-92:15:10, lev1_8: EQUINOX=J2000,RANGE=28.7325180 wind_1: WND1=20-MAY-92:20:50 TO 21-MAY-92:15:10 comment_1: PLUTO NEAR TARGET 101, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.164+/-0.042 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 2 name_1: PL-CH-2 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 31M 31.214S, lev1_3: DEC1 = -03D 21' 23.46", lev1_4: RA2 = 15H 31M 29.575S, lev1_5: DEC2 = -03D 21' 19.76", lev1_6: EPOCH1=23-MAY-92:00:30, lev1_7: EPOCH2=23-MAY-92:13:00, lev1_8: EQUINOX=J2000,RANGE=28.7381043 wind_1: WND1=23-MAY-92:00:30 TO 23-MAY-92:13:00 comment_1: PLUTO NEAR TARGET 102, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.090+/-0.018 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 3 name_1: PL-CH-3 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 30M 52.263S, lev1_3: DEC1 = -03D 19' 51.45", lev1_4: RA2 = 15H 30M 50.921S, lev1_5: DEC2 = -03D 19' 49.21", lev1_6: EPOCH1=29-MAY-92:07:30, lev1_7: EPOCH2=29-MAY-92:18:00, lev1_8: EQUINOX=J2000,RANGE=28.7625066 wind_1: WND1=29-MAY-92:07:30 TO 29-MAY-92:18:00 comment_1: PLUTO NEAR TARGET 103, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.107+/-0.012 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 4 name_1: PL-CH-4 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 30M 24.201S, lev1_3: DEC1 = -03D 19' 13.03", lev1_4: RA2 = 15H 30M 22.526S, lev1_5: DEC2 = -03D 19' 11.03", lev1_6: EPOCH1=02-JUN-92:21:32, lev1_7: EPOCH2=03-JUN-92:11:02, lev1_8: EQUINOX=J2000,RANGE=28.7875598 wind_1: WND1=02-JUN-92:21:32 TO 03-JUN-92:11:02 comment_1: PLUTO NEAR TARGET 104, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.160+/-0.027 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 5 name_1: PL-CH-5 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 27M 12.364S, lev1_3: DEC1 = -03D 45' 48.74", lev1_4: RA2 = 15H 27M 13.104S, lev1_5: DEC2 = -03D 46' 02.60", lev1_6: EPOCH1=21-AUG-92:21:30, lev1_7: EPOCH2=22-AUG-92:13:00, lev1_8: EQUINOX=J2000,RANGE=29.8440529 wind_1: WND1=21-AUG-92:21:30 TO 22-AUG-92:13:00 comment_1: PLUTO NEAR TARGET 105, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.157+/-0.026 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 6 name_1: PL-CH-6 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 27M 52.758S, lev1_3: DEC1 = -03D 56' 01.62", lev1_4: RA2 = 15H 27M 54.154S, lev1_5: DEC2 = -03D 56' 18.28", lev1_6: EPOCH1=04-SEP-92:04:22, lev1_7: EPOCH2=04-SEP-92:21:22, lev1_8: EQUINOX=J2000,RANGE=30.0542900 wind_1: WND1=04-SEP-92:04:22 TO 04-SEP-92:21:22 comment_1: PLUTO NEAR TARGET 106, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.257+/-0.085 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 7 name_1: PL-CH-7 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 28M 59.920S, lev1_3: DEC1 = -04D 07' 32.19", lev1_4: RA2 = 15H 29M 01.033S, lev1_5: DEC2 = -04D 07' 42.14", lev1_6: EPOCH1=18-SEP-92:11:15, lev1_7: EPOCH2=18-SEP-92:20:55, lev1_8: EQUINOX=J2000,RANGE=30.2576415 wind_1: WND1=18-SEP-92:11:15 TO 18-SEP-92:20:55 comment_1: PLUTO NEAR TARGET 107, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.432+/-0.019 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 8 name_1: PL-CH-8 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 43M 35.643S, lev1_3: DEC1 = -05D 10' 00.60", lev1_4: RA2 = 15H 43M 37.405S, lev1_5: DEC2 = -05D 10' 01.87", lev1_6: EPOCH1=05-JAN-93:05:20, lev1_7: EPOCH2=05-JAN-93:17:50, lev1_8: EQUINOX=J2000,RANGE=30.3169860 wind_1: WND1=05-JAN-93:05:20 TO 05-JAN-93:17:50 comment_1: PLUTO NEAR TARGET 108, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.401+/-0.036 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 9 name_1: PL-CH-9 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 44M 20.064S, lev1_3: DEC1 = -05D 10' 37.06", lev1_4: RA2 = 15H 44M 21.648S, lev1_5: DEC2 = -05D 10' 37.12", lev1_6: EPOCH1=12-JAN-93:02:54, lev1_7: EPOCH2=12-JAN-93:15:24, lev1_8: EQUINOX=J2000,RANGE=30.2241384 wind_1: WND1=12-JAN-93:02:54 TO 12-JAN-93:15:24 comment_1: PLUTO NEAR TARGET 109, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.333+/-0.032 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 10 name_1: PL-CH-10 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 45M 26.406S, lev1_3: DEC1 = -05D 09' 48.74", lev1_4: RA2 = 15H 45M 28.268S, lev1_5: DEC2 = -05D 09' 45.63", lev1_6: EPOCH1=24-JAN-93:05:54, lev1_7: EPOCH2=25-JAN-93:00:54, lev1_8: EQUINOX=J2000,RANGE=30.0417849 wind_1: WND1=24-JAN-93:05:54 TO 25-JAN-93:00:54 comment_1: PLUTO NEAR TARGET 110, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.388+/-0.051 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 11 name_1: PL-CH-11 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 46M 46.228S, lev1_3: DEC1 = -05D 02' 57.66", lev1_4: RA2 = 15H 46M 47.679S, lev1_5: DEC2 = -05D 02' 30.94", lev1_6: EPOCH1=19-FEB-93:02:38, lev1_7: EPOCH2=21-FEB-93:11:38, lev1_8: EQUINOX=J2000,RANGE=29.6055087 wind_1: WND1=19-FEB-93:02:38 TO 21-FEB-93:11:38 comment_1: PLUTO NEAR TARGET 111, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.305+/-0.077 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 12 name_1: PL-CH-12 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 46M 37.544S, lev1_3: DEC1 = -04D 52' 09.90", lev1_4: RA2 = 15H 46M 36.408S, lev1_5: DEC2 = -04D 51' 52.63", lev1_6: EPOCH1=15-MAR-93:22:15, lev1_7: EPOCH2=17-MAR-93:01:45, lev1_8: EQUINOX=J2000,RANGE=29.2260982 wind_1: WND1=15-MAR-93:22:15 TO 17-MAR-93:01:45 comment_1: PLUTO NEAR TARGET 112, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.321+/-0.040 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 13 name_1: PL-CH-13 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 45M 31.008S, lev1_3: DEC1 = -04D 41' 21.44", lev1_4: RA2 = 15H 45M 29.694S, lev1_5: DEC2 = -04D 41' 11.95", lev1_6: EPOCH1=06-APR-93:01:40, lev1_7: EPOCH2=06-APR-93:16:20, lev1_8: EQUINOX=J2000,RANGE=28.9650902 wind_1: WND1=06-APR-93:01:40 TO 06-APR-93:16:20 comment_1: PLUTO NEAR TARGET 113, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.162+/-0.000 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 14 name_1: PL-CH-14 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 44M 21.939S, lev1_3: DEC1 = -04D 34' 12.57", lev1_4: RA2 = 15H 44M 20.093S, lev1_5: DEC2 = -04D 34' 02.88", lev1_6: EPOCH1=20-APR-93:05:00, lev1_7: EPOCH2=20-APR-93:21:15, lev1_8: EQUINOX=J2000,RANGE=28.8419223 wind_1: WND1=20-APR-93:05:00 TO 20-APR-93:21:15 comment_1: PLUTO NEAR TARGET 114, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.096+/-0.028 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 15 name_1: PL-CH-15 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 42M 56.629S, lev1_3: DEC1 = -04D 27' 37.40", lev1_4: RA2 = 15H 42M 54.830S, lev1_5: DEC2 = -04D 27' 30.52", lev1_6: EPOCH1=04-MAY-93:20:30, lev1_7: EPOCH2=05-MAY-93:10:30, lev1_8: EQUINOX=J2000,RANGE=28.7700941 wind_1: WND1=04-MAY-93:20:30 TO 05-MAY-93:10:30 comment_1: PLUTO NEAR TARGET 115, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.098+/-0.065 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 16 name_1: PL-CH-16 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 41M 42.716S, lev1_3: DEC1 = -04D 23' 25.77", lev1_4: RA2 = 15H 41M 41.220S, lev1_5: DEC2 = -04D 23' 21.55", lev1_6: EPOCH1=16-MAY-93:14:45, lev1_7: EPOCH2=17-MAY-93:02:00, lev1_8: EQUINOX=J2000,RANGE=28.7556572 wind_1: WND1=16-MAY-93:14:45 TO 17-MAY-93:02:00 comment_1: PLUTO NEAR TARGET 116, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.015+/-0.014 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 17 name_1: PL-CH-17 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 41M 01.852S, lev1_3: DEC1 = -04D 21' 53.70", lev1_4: RA2 = 15H 40M 59.501S, lev1_5: DEC2 = -04D 21' 48.38", lev1_6: EPOCH1=22-MAY-93:22:25, lev1_7: EPOCH2=23-MAY-93:16:10, lev1_8: EQUINOX=J2000,RANGE=28.7644454 wind_1: WND1=22-MAY-93:22:25 TO 23-MAY-93:16:10 comment_1: PLUTO NEAR TARGET 117, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.022+/-0.016 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 18 name_1: PL-CH-18 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 40M 53.604S, lev1_3: DEC1 = -04D 21' 31.52", lev1_4: RA2 = 15H 40M 51.253S, lev1_5: DEC2 = -04D 21' 26.46", lev1_6: EPOCH1=24-MAY-93:05:30, lev1_7: EPOCH2=24-MAY-93:23:18, lev1_8: EQUINOX=J2000,RANGE=28.7676374 wind_1: WND1=24-MAY-93:05:30 TO 24-MAY-93:23:18 comment_1: PLUTO NEAR TARGET 118, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.160+/-0.092 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 19 name_1: PL-CH-19 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 40M 08.917S, lev1_3: DEC1 = -04D 20' 21.40", lev1_4: RA2 = 15H 40M 07.568S, lev1_5: DEC2 = -04D 20' 19.36", lev1_6: EPOCH1=31-MAY-93:10:15, lev1_7: EPOCH2=31-MAY-93:20:45, lev1_8: EQUINOX=J2000,RANGE=28.7931819 wind_1: WND1=31-MAY-93:10:15 TO 31-MAY-93:20:45 comment_1: PLUTO NEAR TARGET 119, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.290+/-0.019 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 20 name_1: PL-CH-20 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 39M 31.550S, lev1_3: DEC1 = -04D 19' 13.59", lev1_4: RA2 = 15H 39M 29.665S, lev1_5: DEC2 = -04D 19' 11.89", lev1_6: EPOCH1=06-JUN-93:13:23, lev1_7: EPOCH2=07-JUN-93:04:40, lev1_8: EQUINOX=J2000,RANGE=28.8270085 wind_1: WND1=06-JUN-93:13:23 TO 07-JUN-93:04:40 comment_1: PLUTO NEAR TARGET 120, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.271+/-0.046 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 21 name_1: PL-CH-21 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 38M 34.880S, lev1_3: DEC1 = -04D 18' 58.45", lev1_4: RA2 = 15H 38M 32.984S, lev1_5: DEC2 = -04D 18' 58.95", lev1_6: EPOCH1=16-JUN-93:13:10, lev1_7: EPOCH2=17-JUN-93:06:10, lev1_8: EQUINOX=J2000,RANGE=28.9024568 wind_1: WND1=16-JUN-93:13:10 TO 17-JUN-93:06:10 comment_1: PLUTO NEAR TARGET 121, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.120+/-0.025 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 22 name_1: PL-CH-22 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 37M 06.647S, lev1_3: DEC1 = -04D 21' 39.94", lev1_4: RA2 = 15H 37M 04.777S, lev1_5: DEC2 = -04D 21' 47.31", lev1_6: EPOCH1=05-JUL-93:15:40, lev1_7: EPOCH2=06-JUL-93:15:51, lev1_8: EQUINOX=J2000,RANGE=29.1118267 wind_1: WND1=05-JUL-93:15:40 TO 06-JUL-93:15:51 comment_1: PLUTO NEAR TARGET 122, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.141+/-0.038 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 23 name_1: PL-CH-23 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 37M 23.221S, lev1_3: DEC1 = -04D 58' 50.18", lev1_4: RA2 = 15H 37M 25.095S, lev1_5: DEC2 = -04D 59' 09.82", lev1_6: EPOCH1=10-SEP-93:19:15, lev1_7: EPOCH2=11-SEP-93:15:32, lev1_8: EQUINOX=J2000,RANGE=30.1513996 wind_1: WND1=10-SEP-93:19:15 TO 11-SEP-93:15:32 comment_1: PLUTO NEAR TARGET 123, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.417+/-0.021 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 24 name_1: PL-CH-24 descr_1: PLANET PLUTO lev1_1: TYPE=G_CIRCLE, lev1_2: RA1 = 15H 38M 20.637S, lev1_3: DEC1 = -05D 07' 29.84", lev1_4: RA2 = 15H 38M 21.702S, lev1_5: DEC2 = -05D 07' 38.81", lev1_6: EPOCH1=22-SEP-93:04:47, lev1_7: EPOCH2=22-SEP-93:13:47, lev1_8: EQUINOX=J2000,RANGE=30.3094320 wind_1: WND1=22-SEP-93:04:47 TO 22-SEP-93:13:47 comment_1: PLUTO NEAR TARGET 124, MUST POINT AND comment_2: TRACK ON THE MID-POINT BETWEEN PLUTO comment_3: AND THE STAR fluxnum_1: 1 fluxval_1: V=14.192+/-0.026 fluxnum_2: 2 fluxval_2: B-V=0.842+/-0.001 ! targnum: 101 name_1: GSC-5020-0294 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 31M 43.240S, lev1_3: DEC = -03D 21' 47.85", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 1. fluxnum_1: 1 fluxval_1: V=14.15+/-0.5 ! targnum: 102 name_1: GSC-5020-0259 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 31M 30.353S, lev1_3: DEC = -03D 21' 25.73", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 2. fluxnum_1: 1 fluxval_1: V=12.81+/-0.5 ! targnum: 103 name_1: GSC-5020-0272 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 30M 51.640S, lev1_3: DEC = -03D 19' 39.65", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 3. fluxnum_1: 1 fluxval_1: V=13.75+/-0.5 ! targnum: 104 name_1: GSC-5020-0583 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 30M 23.302S, lev1_3: DEC = -03D 19' 03.32", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 4. fluxnum_1: 1 fluxval_1: V=15.29+/-0.5 ! targnum: 105 name_1: GSC-5011-0479 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 27M 13.340S, lev1_3: DEC = -03D 45' 48.41", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 5. fluxnum_1: 1 fluxval_1: V=15.56+/-0.5 ! targnum: 106 name_1: GSC-5011-0520 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 27M 53.179S, lev1_3: DEC = -03D 56' 15.93", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 6. fluxnum_1: 1 fluxval_1: V=13.23+/-0.5 ! targnum: 107 name_1: GSC-5011-0069 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 29M 00.089S, lev1_3: DEC = -04D 07' 46.51", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 7. fluxnum_1: 1 fluxval_1: V=14.96+/-0.5 ! targnum: 108 name_1: GSC-5025-0319 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 43M 36.457S, lev1_3: DEC = -05D 09' 51.79", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 8. fluxnum_1: 1 fluxval_1: V=13.57+/-0.5 ! targnum: 109 name_1: GSC-5025-0889 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 44M 20.749S, lev1_3: DEC = -05D 10' 45.84", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 9. fluxnum_1: 1 fluxval_1: V=13.32+/-0.5 ! targnum: 110 name_1: GSC-5026-0736 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 45M 27.362S, lev1_3: DEC = -05D 09' 53.42", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 10. fluxnum_1: 1 fluxval_1: V=14.69+/-0.5 ! targnum: 111 name_1: GSC-5026-0697 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 46M 46.795S, lev1_3: DEC = -05D 02' 43.67", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 11. fluxnum_1: 1 fluxval_1: V=10.38+/-0.5 ! targnum: 112 name_1: GSC-5026-0751 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 46M 36.590S, lev1_3: DEC = -04D 52' 07.04", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 12. fluxnum_1: 1 fluxval_1: V=14.65+/-0.5 ! targnum: 113 name_1: GSC-5026-0848 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 45M 30.057S, lev1_3: DEC = -04D 41' 26.36", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 13. fluxnum_1: 1 fluxval_1: V=14.38+/-0.5 ! targnum: 114 name_1: GSC-5025-0779 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 44M 20.943S, lev1_3: DEC = -04D 34' 14.34", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 14. fluxnum_1: 1 fluxval_1: V=14.05+/-0.5 ! targnum: 115 name_1: GSC-5025-0011 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 42M 55.815S, lev1_3: DEC = -04D 27' 30.53", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 15. fluxnum_1: 1 fluxval_1: V=15.48+/-0.5 ! targnum: 116 name_1: GSC-5025-0433 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 41M 42.057S, lev1_3: DEC = -04D 23' 14.40", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 16. fluxnum_1: 1 fluxval_1: V=15.51+/-0.5 ! targnum: 117 name_1: GSC-5025-0987 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 41M 00.651S, lev1_3: DEC = -04D 21' 53.86", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 17. fluxnum_1: 1 fluxval_1: V=14.75+/-0.5 ! targnum: 118 name_1: GSC-5025-0931 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 40M 52.383S, lev1_3: DEC = -04D 21' 27.93", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 18. fluxnum_1: 1 fluxval_1: V=15.42+/-0.5 ! targnum: 119 name_1: GSC-5025-0132 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 40M 08.133S, lev1_3: DEC = -04D 20' 31.81", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 19. fluxnum_1: 1 fluxval_1: V=15.10+/-0.5 ! targnum: 120 name_1: GSC-5025-0321 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 39M 30.556S, lev1_3: DEC = -04D 19' 02.33", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 20. fluxnum_1: 1 fluxval_1: V=12.20+/-0.5 ! targnum: 121 name_1: GSC-5025-0391 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 38M 33.915S, lev1_3: DEC = -04D 18' 54.30", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 21. fluxnum_1: 1 fluxval_1: V=15.52+/-0.5 ! targnum: 122 name_1: GSC-5024-0627 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 37M 05.746S, lev1_3: DEC = -04D 21' 49.26", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 22. fluxnum_1: 1 fluxval_1: V=10.71+/-0.5 ! targnum: 123 name_1: GSC-5024-0705 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 37M 24.141S, lev1_3: DEC = -04D 59' 02.87", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 23. fluxnum_1: 1 fluxval_1: V=14.96+/-0.5 ! targnum: 124 name_1: GSC-5025-0794 descr_1: OTHER ASTROMETRIC REFERENCE STAR lev1_1: TYPE=STELLAR, lev1_2: RA = 15H 38M 21.596S, lev1_3: DEC = -05D 07' 23.77", lev1_4: M_RA=0.0, M_DEC=0.0, lev1_5: P=0.0,EPOCH=01-JAN-1950, lev1_6: EQUINOX = J2000 comment_1: ASTROMETRIC REFERENCE STAR TO BE comment_2: OBSERVED IN THE FIELD WITH TARGET comment_3: NUMBER 24. fluxnum_1: 1 fluxval_1: V=13.24+/-0.5 ! ! end of solar system targets ! No generic target records found exposure_logsheet: linenum: 1.000 sequence_1: DEFINE sequence_2: PLBV targname: # config: PC opmode: IMAGE aperture: PC6-FIX sp_element: F555W num_exp: 2 time_per_exp: 30S s_to_n: 100 fluxnum_1: 1 priority: 1 req_1: CYCLE 2; req_2: SEQ 1.0-2.0 WITHIN 50M; comment_1: LINES 1.0 AND 2.0 MUST FIT WITHIN comment_2: A SINGLE TARGET VISIBILITY WINDOW. ! linenum: 2.000 sequence_1: DEFINE sequence_2: PLBV targname: # config: PC opmode: IMAGE aperture: PC6-FIX sp_element: F439W num_exp: 2 time_per_exp: 180S s_to_n: 100 fluxnum_1: 1 priority: 1 req_1: CYCLE 2; ! linenum: 3.000 sequence_1: DEFINE sequence_2: PLBV targname: # config: PC opmode: IMAGE aperture: PC6-FIX sp_element: F439W num_exp: 2 time_per_exp: 180S s_to_n: 100 fluxnum_1: 1 priority: 1 req_1: CYCLE 2; req_2: SEQ 3.0-4.0 WITHIN 50M; req_3: AFTER 1.0 BY 6H; comment_1: LINES 3.0 AND 4.0 MUST FIT WITHIN comment_2: A SINGLE TARGET VISIBILITY WINDOW. ! linenum: 4.000 sequence_1: DEFINE sequence_2: PLBV targname: # config: PC opmode: IMAGE aperture: PC6-FIX sp_element: F555W num_exp: 2 time_per_exp: 30S s_to_n: 100 fluxnum_1: 1 priority: 1 req_1: CYCLE 2; ! linenum: 5.000 sequence_1: DEFINE sequence_2: PLV targname: # config: PC opmode: IMAGE aperture: PC6-FIX sp_element: F555W num_exp: 2 time_per_exp: 30S s_to_n: 100 fluxnum_1: 1 priority: 1 req_1: CYCLE 2; comment_1: THIS LINE MUST SCHEDULE WITHIN comment_2: A SINGLE TARGET VISIBILITY WINDOW. ! linenum: 6.000 sequence_1: DEFINE sequence_2: PLV targname: # config: PC opmode: IMAGE aperture: PC6-FIX sp_element: F555W num_exp: 2 time_per_exp: 30S s_to_n: 100 fluxnum_1: 1 priority: 1 req_1: CYCLE 2; req_2: AFTER 5.0 BY 6H; comment_1: THIS LINE MUST SCHEDULE WITHIN comment_2: A SINGLE TARGET VISIBILITY WINDOW. ! linenum: 10.000 sequence_1: USE PLV targname: PL-CH-1 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; COND IF CHOSEN BY PI / 10-240; ! linenum: 20.000 sequence_1: USE PLV targname: PL-CH-2 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 30.000 sequence_1: USE PLBV targname: PL-CH-3 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 40.000 sequence_1: USE PLV targname: PL-CH-4 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 50.000 sequence_1: USE PLV targname: PL-CH-5 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 60.000 sequence_1: USE PLV targname: PL-CH-6 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 70.000 sequence_1: USE PLV targname: PL-CH-7 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 80.000 sequence_1: USE PLV targname: PL-CH-8 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 90.000 sequence_1: USE PLV targname: PL-CH-9 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 100.000 sequence_1: USE PLV targname: PL-CH-10 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 110.000 sequence_1: USE PLV targname: PL-CH-11 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 120.000 sequence_1: USE PLV targname: PL-CH-12 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 130.000 sequence_1: USE PLV targname: PL-CH-13 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 140.000 sequence_1: USE PLV targname: PL-CH-14 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 150.000 sequence_1: USE PLV targname: PL-CH-15 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 160.000 sequence_1: USE PLV targname: PL-CH-16 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 170.000 sequence_1: USE PLV targname: PL-CH-17 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 180.000 sequence_1: USE PLV targname: PL-CH-18 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 190.000 sequence_1: USE PLBV targname: PL-CH-19 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 200.000 sequence_1: USE PLV targname: PL-CH-20 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 210.000 sequence_1: USE PLV targname: PL-CH-21 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 220.000 sequence_1: USE PLV targname: PL-CH-22 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 230.000 sequence_1: USE PLV targname: PL-CH-23 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! linenum: 240.000 sequence_1: USE PLV targname: PL-CH-24 req_1: SELECT 12 OF 10 OR 20 OR 30 OR 40 OR 50 req_2: OR 60 OR 70 OR 80 OR 90 OR 100 OR 110 OR req_3: 120 OR 130 OR 140 OR 150 OR 160 OR 170 OR req_4: 180 OR 190 OR 200 OR 210 OR 220 OR 230 OR req_5: 240; ! ! end of exposure logsheet ! No scan data records found