! $Id: 1070,v 10.1 1994/10/13 15:02:26 pepsa Exp $ ! coverpage: title_1: HIGH RESOLUTION IMAGING OF RADIO GALAXIES AT LARGE REDSHIFT sci_cat: GALAXIES & CLUSTERS proposal_for: GTO/OS pi_title: PROF. pi_fname: MALCOLM pi_mi: S. pi_lname: LONGAIR pi_inst: CAVENDISH LABORATORY, CAMBRIDGE pi_country: UNITED KINGDOM pi_phone: 44-223-337083 keywords_1: RADIO GALAXIES, LARGE REDSHIFTS, ACTIVE GALAXIES, keywords_2: COSMOLOGY hours_pri: 43.00 num_pri: 28 pi_position: PROFESSOR off_fname: MALCOLM off_mi: S. off_lname: LONGAIR off_title: DR. off_addr_1: CAVENDISH LABORATORY off_addr_2: MADINGLEY ROAD off_addr_3: CAMBRIDGE CB3 0HE off_country: UNITED KINGDOM off_phone: 44-223-337083 ! end of coverpage abstract: line_1: Recent ground-based observations of the colours and magnitudes of 3C line_2: radio galaxies at z ~ 1 have enabled a picture of the evolution of the line_3: stellar populations of these galaxies to be constructed. Some galaxies line_4: show only the effects of the passive evolution of the main sequence line_5: turn-off point, while a substantial fraction show evidence of addition- line_6: al susbtantial populations of young stars in an actively evolving line_7: stellar population. Ground based observations indicate that this range line_8: of evolutionary behavior is maintained at least to z ~ 2, but little line_9: progress has been possible in understanding the star-formation activity line_10: seen in a fraction of these galaxies at all redshifts z >/~ 0.7. line_12: It is proposed to take two-colour deep high-resolution images of a line_13: well-defined sample of 22 3C galaxies with 0.6 < z < 1.30 and single- line_14: colour exposures of an additional 6 galaxies at z > 1.3, using the line_15: WFPC2. These will allow the morphologies and structures of both act- line_16: ively and passively evolving galaxies to be determined, allow the line_17: distribution of star-forming regions in the galaxies to be mapped and line_18: the cause of this activity to be understood. The data will also line_19: allow the nearby cluster environments of the galaxies to be studied. ! ! end of abstract general_form_proposers: lname: LONGAIR fname: MALCOLM mi: S inst: CAVENDISH LABORATORY, CAMBRIDGE country: ENGLAND, U.K. esa: Y ! lname: LILLY fname: SIMON mi: J. inst: DEPARTMENT OF ASTRONOMY, UNIVERSITY OF TORONTO country: CANADA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: For each of the 22 radio galaxies with 0.6 /~ 1.3, a 30 min exposure will be made line_11: through the 'broad I' filter. This will be repeated for the 3 line_12: galaxies that have only been marginally detected optically wavelengths line_14: to give a total integration of 5400 seconds. The absolute pointing and line_15: the accuracy of the coordinates of the radio galaxies is not critical line_16: to these wide field images. ! question: 4 section: 1 line_1: The Space Telescope is absolutely essential in achieving the required line_2: spatial resolution on these faint extended objects. This experiment line_3: cannot be satisfactorily carried out from the ground. Existing ground- line_4: based observations have indicated the presence of evolution in the line_5: stellar populations of these galaxies and has indicated that active line_6: star-formation is occurring in many of the galaxies, but the form of line_7: the star-formation regions, and the nature of the immediate line_8: environments of the galaxies remains unknown. ! question: 6 section: 1 line_1: Only standard flat-field and photometric calibration of WFPC2 line_2: camera images is required. The exposure should be line_3: uninterupted to minimize cosmic ray degradation of the images ! ! question: 10 section: 1 line_1: Data analysis will be carried out on a Sparc2 SUN workstation at line_2: Cambridge. ! question: 13 section: 1 line_1: Deep high resolution two colour images will be taken of the fields of line_2: twenty-two 3C radio galaxies in the redshift interval 0.6 < z < 1.30 line_3: and single colour images of an additional 6 at z > 1.3. These data line_4: will be used to study their structure, the distribution of the active line_5: star-forming regions in them, and the nature of their cluster line_6: environments. ! !end of general form text general_form_address: lname: LONGAIR fname: MALCOLM mi: S. title: PROF. category: PI inst: CAVENDISH LABORATORY, UNIVERSITY OF CAMBRIDGE addr_1: MADINGLEY ROAD city: CAMBRIDGE CB3 0HE country: ENGLAND, U.K. ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: 3C266 descr_1: E,315 pos_1: RA = 11H 43M 04.27S +/- 0.01S, pos_2: DEC = +50D 02' 47.0" +/- 0.1S equinox: 1950 rv_or_z: Z=1.28 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=22 ! targnum: 2 name_1: 3C324 descr_1: E,315 pos_1: RA = 15H 47M 37.10S +/- 0.01S, pos_2: DEC = +21D 34' 40.1" +/- 0.1S equinox: 1950 rv_or_z: Z=1.21 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=21.5 ! targnum: 3 name_1: 3C65 descr_1: E,315 pos_1: RA = 02H 20M 37.24S +/- 0.01S, pos_2: DEC = +39D 47' 17.1" +/- 0.1S equinox: 1950 rv_or_z: Z=1.17 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=23 ! targnum: 4 name_1: 3C267 descr_1: E,315 pos_1: RA = 11H 47M 22.11S +/- 0.01S, pos_2: DEC = +13D 04' 00.2" +/- 0.1S equinox: 1950 rv_or_z: Z=1.14 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=22.5 ! targnum: 5 name_1: 3C368 descr_1: E,315 pos_1: RA = 18H 02M 45.60S +/- 0.01S, pos_2: DEC = +11D 01' 13.8" +/- 0.1S equinox: 1950 rv_or_z: Z=1.13 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=21.5 ! targnum: 6 name_1: 3C252 descr_1: E,315 pos_1: RA = 11H 08M 48.93S +/- 0.01S, pos_2: DEC = +35D 57' 00.1" +/- 0.1S equinox: 1950 rv_or_z: Z=1.11 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=22.0 ! targnum: 7 name_1: 3C356 descr_1: E,315 pos_1: RA = 17H 23M 06.66S +/- 0.01S, pos_2: DEC = +51D 00' 18.1" +/- 0.1S equinox: 1950 rv_or_z: Z=1.08 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=21.5 ! targnum: 8 name_1: 3C280 descr_1: E,315 pos_1: RA = 12H 54M 41.66S +/- 0.01S, pos_2: DEC = +47D 36' 32.7" +/- 0.1S equinox: 1950 rv_or_z: Z=1.00 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=22.0 ! targnum: 9 name_1: 3C22 descr_1: E,315 pos_1: RA = 00H 48M 04.71S +/- 0.01S, pos_2: DEC = +50D 55' 45.4" +/- 0.1S equinox: 1950 rv_or_z: Z=0.94 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=22.0 ! targnum: 10 name_1: 3C289 descr_1: E,315 pos_1: RA = 13H 43M 27.38S +/- 0.01S, pos_2: DEC = +50D 01' 32.0" +/- 0.1S equinox: 1950 rv_or_z: Z=0.97 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=23.0 ! targnum: 11 name_1: 3C217 descr_1: E,315 pos_1: RA = 09H 05M 41.42S +/- 0.01S, pos_2: DEC = +38D 00' 29.9" +/- 0.1S equinox: 1950 rv_or_z: Z=0.90 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=22 ! targnum: 12 name_1: 3C13 descr_1: E,315 pos_1: RA = 00H 31M 33.15S +/- 0.01S, pos_2: DEC = +39D 07' 41.8" +/- 0.1S equinox: 1950 rv_or_z: Z=1.35 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=22.5 ! targnum: 13 name_1: 3C241 descr_1: E,315 pos_1: RA = 10H 19M 09.44S +/- 0.01S, pos_2: DEC = +22D 14' 40.7" +/- 0.1S equinox: 1950 rv_or_z: Z=1.62 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=23.5 ! targnum: 14 name_1: 3C239 descr_1: E,315 pos_1: RA = 10H 08M 38.97S +/- 0.01S, pos_2: DEC = +46D 43' 08.4" +/- 0.1S equinox: 1950 rv_or_z: Z=1.78 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=22.5 ! targnum: 15 name_1: 3C68.2 descr_1: E,315 pos_1: RA = 02H 31M 24.75S +/- 0.01S, pos_2: DEC = +31D 21' 11.5" +/- 0.1S equinox: 1950 rv_or_z: Z = 1.58 comment_1: VERY FAINT GALAXY fluxnum_1: 1 fluxval_1: V=24 ! targnum: 16 name_1: 3C437 descr_1: E,315 pos_1: RA = 21H 45M 01.36S +/- 0.01S, pos_2: DEC = +15D 06' 37.85" +/- 0.1" equinox: 1950 rv_or_z: Z = 1.48 comment_1: VERY FAINT GALAXY fluxnum_1: 1 fluxval_1: V=23.0 ! targnum: 17 name_1: 3C470 descr_1: E,315 pos_1: RA = 23H 56M 02.98S +/- 0.01S, pos_2: DEC = +43D 48' 03.6" +/- 0.1" equinox: 1950 rv_or_z: Z = 1.65 comment_1: VERY FAINT GALAXY fluxnum_1: 1 fluxval_1: V=22.5 ! targnum: 18 name_1: 3C226 descr_1: E,315 pos_1: RA = 09H 41M 36.16S +/- 0.01S, pos_2: DEC = +10D 00' 05.1" +/- 0.1" equinox: 1950 rv_or_z: Z=0.82 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=19.5 ! targnum: 19 name_1: 3C265 descr_1: E,315 pos_1: RA = 11H 42M 52.39S +/- 0.01S, pos_2: DEC = +31D 50' 29.1" +/- 0.1" equinox: 1950 rv_or_z: Z=0.81 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=20.9 ! targnum: 20 name_1: 3C352 descr_1: E,315 pos_1: RA = 17H 09M 18.00S +/- 0.01S, pos_2: DEC = +46D 05' 06.0" +/- 0.1" equinox: 1950 rv_or_z: Z=0.81 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=22.8 ! targnum: 21 name_1: 3C41 descr_1: E,315 pos_1: RA = 01H 23M 54.74S +/- 0.01S, pos_2: DEC = +32D 57' 38.3" +/- 0.1" equinox: 1950 rv_or_z: Z=0.79 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=21.0 ! targnum: 22 name_1: 3C340 descr_1: E,315 pos_1: RA = 16H 27M 29.41S +/- 0.01S, pos_2: DEC = +23D 26' 42.6" +/- 0.1" equinox: 1950 rv_or_z: Z=0.78 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=22.0 ! targnum: 25 name_1: 3C441 descr_1: E,315 pos_1: RA = 22H 03M 49.27S +/- 0.01S, pos_2: DEC = +29D 14' 43.9" +/- 0.1" equinox: 1950 rv_or_z: Z=0.71 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=21.0 ! targnum: 26 name_1: 3C34 descr_1: E,315 pos_1: RA = 01H 07M 32.50S +/- 0.01S, pos_2: DEC = +31D 31' 22.5" +/- 0.1" equinox: 1950 rv_or_z: Z=0.69 comment_1: FAINT GALAXY fluxnum_1: 1 fluxval_1: V=21.0 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 targname: 3C266 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F702W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 comment_1: EACH EXPOSURE HAS BEEN SET NOMINALLY comment_2: TO 30 MINUTES. THE INTENTION IS THAT comment_3: EACH EXPOSURE SHOULD TAKE ONE HALF comment_4: ORBIT AND SO A SLIGHTLY LONGER comment_5: INTEGRATION TIME MAY BE POSSIBLE. ! linenum: 2.000 targname: 3C266 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F814W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 3.000 targname: 3C266 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F555W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 4.000 targname: 3C324 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F702W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 5.000 targname: 3C324 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F1042M num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 6.000 targname: 3C324 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F791W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 7.000 targname: 3C65 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F675W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 8.000 targname: 3C65 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F814W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 9.000 targname: 3C267 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F702W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 10.000 targname: 3C267 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F1042M num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 11.000 targname: 3C267 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F791W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 12.000 targname: 3C368 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F702W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 13.000 targname: 3C368 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F1042M num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 14.000 targname: 3C368 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F791W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 15.000 targname: 3C252 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F622W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 16.000 targname: 3C252 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F814W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 17.000 targname: 3C356 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F622W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 18.000 targname: 3C356 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F814W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 19.000 targname: 3C280 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F622W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 20.000 targname: 3C280 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F1042M num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 21.000 targname: 3C22 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F622W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 22.000 targname: 3C22 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F1042M num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 23.000 targname: 3C289 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F622W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 24.000 targname: 3C289 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F814W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 25.000 targname: 3C217 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F622W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 26.000 targname: 3C217 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F814W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 27.000 targname: 3C13 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F785LP num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 28.000 targname: 3C241 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F785LP num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 29.000 targname: 3C239 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F785LP num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 30.000 targname: 3C68.2 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F785LP num_exp: 2 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 31.000 targname: 3C437 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F785LP num_exp: 2 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 32.000 targname: 3C470 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F785LP num_exp: 2 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 33.000 targname: 3C226 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F555W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 34.000 targname: 3C226 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F785LP num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 35.000 targname: 3C265 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F555W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 36.000 targname: 3C265 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F785LP num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 37.000 targname: 3C352 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F555W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 38.000 targname: 3C352 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F814W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4 ! linenum: 39.000 targname: 3C41 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F555W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4; ! linenum: 40.000 targname: 3C41 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F785LP num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4; ! linenum: 41.000 targname: 3C340 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F555W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4; ! linenum: 42.000 targname: 3C340 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F785LP num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4; ! linenum: 47.000 targname: 3C441 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F555W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4; ! linenum: 48.000 targname: 3C441 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F785LP num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4; ! linenum: 49.000 targname: 3C34 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F555W num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4; ! linenum: 50.000 targname: 3C34 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F785LP num_exp: 1 time_per_exp: 30M fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.3 req_1: CYCLE 4; ! ! ! end of exposure logsheet ! No scan data records found