Page 1 PROPOSAL FOR HUBBLE SPACE TELESCOPE OBSERVATIONS ST ScI Use Only ID 5378 Report Date: 18-Jul-95:17:16 Version: ********** Check-in Date: ********** 1.Proposal Title: MORPHOLOGICAL EVOLUTION OF GALAXIES IN CLUSTERS AT Z = 0.5 ------------------------------------------------------------------------------------ 2. Scientific Category 3. Proposal For 4. Proposal Type 5. Continuation ID GALAXIES & CLUSTERS GO Sub Category DISTANT GALAXIES ------------------------------------------------------------------------------------ 6. Principal Investigator Institution Country Telephone Alan Dressler 3030 USA 818-304-0245 ------------------------------------------------------------------------------------ 7. Abstract Our program is intended to study galaxy evolution through the investigation of galaxy morphology and spectrophotometry as a function of lookback time. Cycle 1 and 2 observations made by two teams represented in this proposal have demonstrated HST's unique potential for providing detailed morphological information for galaxies in clusters at z = 0.5. Such data are applicable to basic questions such as the development of disks and bulges, and the role mergers and interactions, and other environmental influences on the evolution of structure and stellar populations. Both teams made Cycle 1 and 2 observations that are described here. However, the combination of the SA problem and reduced time allocations severely limited the scope of both programs; thus, we request consideration under the Precedents Policy for originally approved Cycle 1 programs. We use our earlier results to demonstrate the feasibility of our program, pointing out the interesting but ambiguous nature of what has been learned to this point. In order to better understand the processes at work and and their range, we propose a more extensive program which includes a wider representation of cluster environments, adds color information, and reaches to higher redshifts. ------------------------------------------------------------------------------------ ------------------------------------------------------------------------------------ 9. Est obs time (hours) pri: 41.42 par: 0 10. Num targs pri: 8 par: 0 ------------------------------------------------------------------------------------ 11. Instruments requested: WF/PC ------------------------------------------------------------------------------------ ------------------------------------------------------------------------------------ Page 2 I. GENERAL FORM Proposal 5378 PI: Alan Dressler Proposal Title: MORPHOLOGICAL EVOLUTION OF GALAXIES IN CLUSTERS AT Z = 0.5 ------------------------------------------------------------------------------------ 1. Proposers: Proposers Institution Country ESA ------------------------------------------------------------------------------------ Alan Dressler 3030 USA Harvey Butcher 6880 NETHERLANDS X Warrick Couch 4145 AUSTRALIA Richard Ellis 8014 UK X Augustus, Jr. Oemler 3900 USA Ray Sharples 8018 UK X ------------------------------------------------------------------------------------ 3. Description of proposed observations. We will observe 8 fields in rich clusters of galaxies covering the redshift range 0.37 < z < 0.55. These fields contain a range of environments and properties. We will image these fields with WFC-2 multiple-orbit exposures that will later be coadded to achieve sufficient signal-to-noise ratio for morphological classification. Field centers and boundaries are chosen with to ground-based spectroscopic and photometric studies of galaxies over the entire field. HST-WFC-2 observations will be 4-7 coadded single-orbit exposures of of 2000-2200 s, in a broad-band color roughly corresponding to rest-frame V, and, for some fields, additional exposures in a band corresponding to rest-frame U. The range in exposure time will (partially) compensate for the degradation in signal-to-noise ratio due to increasing redshift. Color maps will be constructed to study the distribution of star formation. Morphological classifications will be done primarily from the rest-frame V images (this corresponds closely with the traditional bandpass used for low-redshift galaxy classifications) but we will attempt adding both bands to see if the increased signal-to-noise and bluer color aids in the determination of galaxy type. According to the convention for WFPC- 2, coordinates as given in the FIXED TARGETS positions are shifted by POS TARG +10,+10 to bring the center to the apex of the pyramid. Exposures for a given field and a given color are split into two groups with a shift introduced of +2,+2 arcseconds, in order to displace objects situated on CCD defects or on the seams of the pyramid. Thus, POS TARG +12,+12 corresponds to the second group. CR-SPLIT=NO for all observations with more than 5 orbits, since in those cases there are sufficient multiple exposures to perform cosmic ray rejection. Orient angles are generally not critical, but some attempt has been made to maximize the number of "active" galaxies covered by the WFPC-2 field, and to take some advantage of the PC chip, and to minimize the disadvantage of its smaller field. The most important factor is to keep the ORIENT ANGLE the *SAME* for all observations of a target, so that the same objects are sampled in all exposures and to simplify coadding of the images. Page 3 ------------------------------------------------------------------------------------ 4. Justification of need for HST observations. Typical morphological classifications for galaxies at low redshift have better than 1 kiloparsec resolution. In his study of 55 rich cluster, Dressler (1980 ApJS 42) was able to achieve reliable classifications for approximately 6000 galaxies in rich clusters, out to a redshift of z = 0.05, at which point the resolution with 1.0 arcsecond seeing was slightly better than a kiloparsec. The best ground-based imaging for faint objects, R > 19, has achieved 0.4 arcseconds FWHM with image stabilization, but this amounts to approximately 3 kpc at z = 0.5, too crude for reliable classification. The HST is the only instrument that can provide the ~= 0.1 arcsecond FWHM imaging that can achieve sub-kiloparsec resolution for galaxies at z = 0.5 to allow comparable morphological classifications to low-redshift galaxies. The Wide-Field Camera, by virtue of its comparatively large field, makes feasible a study of clusters of galaxies which contain many galaxies, allowing statistical samples to be assembled. The time requested reflects the need for a substantial number of fields (8) and the need for long exposures to achieve sufficient signal-to- noise ratios for morphological classification. The case for 8 different fields is justified by the need to sample a range of cluster types and environments, as explained in Section 2. Exposures of between 140 to 245 minutes are necessary to accumulate sufficient signal-to-noise ratios for accurate morphological classification of galaxies in clusters at 0.35 < z < 0.55. These correspond to 4-7 orbit (typically 2100 s per orbit) exposures, depending on the redshift. The range of 4 to 7 orbits reflects an attempt to partially compensate for the decrease in signal-to-noise ratio with increasing redshift, again based on simulations. In summary, then, the Cycle 1 and 2 observations confirmed our original estimates of 4-6 orbit exposures for WFC-1, slightly augmented to account for the loss of efficiency in WFC-2. The above calculations refer to our F702W and F814W exposures. We are also imaging some of the cluster fields in F555W as well, to acquire color information. Because of the lower efficiency in F555W and the generally lower fluxes in the ultraviolet for cluster galaxies, we expect that these exposures will go much less deep in an equivalent time. ------------------------------------------------------------------------------------ 5. Description of special scheduling requirements. To allow for timely data reduction & analysis, we request the following: Do all exposures PER TARGET in this program within 7 days. ( This limit may be relaxed if necessary so long as the essential goal of having all exposures of the science target, made at the SAME ORIENT, is met, and that the preferable ORIENT angle is used. We chose these angles pretty carefully to minimize the effect of the smaller PC FOV.) The maintenance of the same ORIENT is important for field coverage and frame coadding. Exposures of 2000-2200 s are made in two groups, one or, in some cases, two colors. For the first group the Fixed Target List coordinates are placed at the apex of the WFPC-2 pyramid by POS TARG +10,+10. For a second group POS TARG +12,+12 moves all objects +2,+2 arcseconds, so that objects are displaced from CCD defects and objects formerly on the seams of the pyramid are revealed. CR-SPLIT=NO is used when six or more orbits are taken, since this provides sufficient frames for cosmic ray rejection, but CR-SPLIT=0.5 is used when 5 or fewer frames are taken, along with CR-TOLERANCE=0.0 in order to keep the exposure times split evenly to facilitate the removal of cosmic rays, etc. Please contact the PI as soon as possible if any of the links in this program have been or are to be broken for purposes of implementation and/or scheduling, in case he has any alternative preferences, etc. ------------------------------------------------------------------------------------ 6. Description of special calibration exposures. ------------------------------------------------------------------------------------ 8. Additional comments or special requests. Page 4 ------------------------------------------------------------------------------------ 9. Description of previous HST work. No. 2373/3857/4719 "Morphology of Galaxies in Clusters at z = 0.5" Cycles 1 and 2; GO; Dressler, Butcher, Gunn, and Oemler No. 2600 "Cores of Early-Type Galaxies" Cycles 1 and 2; GO; Faber, Kormendy, Richstone, Tremaine, Lauer, and Dressler No. 2269 "Galaxy Populations in Intermediate Redshift Clusters Cycle 1; GO; Couch, Ellis, and Sharples No. 4072 "Star Formation Rates in Distant Cluster Galaxies" Cycle 2; GTO; Ellis, Couch, Sharples, and MacCay No. 4298 "Galaxy Populations in Intermediate Redshift Clusters" Cycle 3; GO; Couch, Ellis, Sharples, and Smail Observations from 2373/3857/4719 and N2269 are the only relevant proposals with data (no data for 4072 and 4298 as of this writing). The results of these two programs are covered in Section 2 of this proposal. ``The Spectra and Morphology of Galaxies in High-Redshift Clusters'', Dressler, A., in ``Observational Cosmology'', eds. G. Chincarini et al., ASP Conference Series, in press. ``A Cluster of Nascent Galaxies at z=2?'', Dressler, A, Oemler, A. Jr., Gunn, J. E., and Butcher, H., ApJ, 404, L45, 1993 ``Deep WFPC Imaging of the z=0.3 cluster AC114'' Sharples, R.M., Smail, I., Ellis, R.S., Couch, W.J., Fitchett, M. and Jorgensen, H. E. in ``Science with the Hubble Space Telescope'', eds. Benvenuti, P. \& Schreier, E., ESO Conference and Workshop Proceedings 44, 119-126 (1993). ``Morphological Studies of the Galaxy Populations in Distant Butcher-Oemler Clusters with HST'' Couch, W.J., Ellis, R.S., Sharples, R.M. and Smail, I. in ``Observational Cosmology'', eds. Chincarini, G. et al., ASP Conference Series, in press. ------------------------------------------------------------------------------------ 10. Resources to be supplied by investigator's institution(s). Extensive data-analysis capabilities, including systems and software support, are provided by each of the five institutions represented here, with good networking capabilities between these systems. Partial support for students will be provided by Yale, Cambridge, Durham, and New South Wales, where appropriate. ------------------------------------------------------------------------------------ 11. Address Information Name: ALAN DRESSLER Category: PI Institution: 3030 Address: THE OBSERVATORIES OF CIW 813 SANTA BARBARA ST. City: PASADENA State: CA Zip Code: 91101 Country: USA Telephone: 818-304-0245 Telex (or e-mail): DRESSLER@OCIW.CALTECH.EDU ------------------------------------------------------------------------------------ TARGET LIST a) Fixed Targets ID = 5378 [ 5] ------------------------------------------------------------------------------------------------------------------------------------ 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial |Acqui|FLX| Flux data No | Name | Description | Position |Eqnx | Vel. |Prblm|REF| | | | | | | | | ------------------------------------------------------------------------------------------------------------------------------------ 1 GAL-CLUS- F,404,406 RA = 00H 15M 58.4S +/- 0.1S, 1950.0 1 SURF(V) = 23.0 +/- 1.0 001558+1609 DEC = +16D 9' 7.0" +/- 1.0" CL0016+16 Comments: THE FIELD CONTAINS MANY FAINT GALAXIES IN THE RANGE 21 < V < 25. ------------------------------------------------------------------------------------------------------------------------------------ 2 GAL-CLUS- F,404,406 RA = 00H 54M 29.3S +/- 0.1S, 1950.0 1 SURF(V) = 23.0 +/- 1.0 005431-2756 DEC = -27D 56' 44.0" +/- J1888.16CL 1.0" Comments: THE FIELD CONTAINS MANY FAINT GALAXIES IN THE RANGE 21 < V < 25. ------------------------------------------------------------------------------------------------------------------------------------ 3 GAL-CLUS- F,404,406 RA = 16H 01M 30.7S +/- 0.1S, 1950.0 1 SURF(V) = 23.0 +/- 1.0 160134+4254 DEC = +42D 53' 47.0" +/- HOG CLUSTER 1.0" 16H-BETA- BETA Comments: THE FIELD CONTAINS MANY FAINT GALAXIES IN THE RANGE 21 < V < 25. ------------------------------------------------------------------------------------------------------------------------------------ 4 GAL-CLUS- F,404,406 RA = 04H 12M 31.2S +/- 0.1S, 1950.0 1 SURF(V) = 23.0 +/- 1.0 041234-6558 DEC = -65D 57' 49.9" +/- F1557-19TC 1.0" Comments: THE FIELD CONTAINS MANY FAINT GALAXIES IN THE RANGE 21 < V < 25. ------------------------------------------------------------------------------------------------------------------------------------ 5 GAL-CLUS- F,404 RA = 14H 09M 32.3S +/- 0.1S, 1950.0 1 SURF(V) = 23.0 +/- 1.0 140933+5226 DEC = +52D 26' 25.0" +/- 3C295 1.0" CLUSTER Comments: THE FIELD CONTAINS MANY FAINT GALAXIES IN THE RANGE 21 < V < 25. ------------------------------------------------------------------------------------------------------------------------------------ 6 GAL-CLUS- F,404 RA = 03H 03M 27.2S +/- 0.1S, 1950.0 1 SURF(V) = 23.0 +/- 1.0 030330+1706 DEC = +17D 07' 44.0" +/- HOG CLUSTER 1.0" 3HCL2 Comments: THE FIELD CONTAINS MANY FAINT GALAXIES IN THE RANGE 21 < V < 25. ------------------------------------------------------------------------------------------------------------------------------------ 7 GAL-CLUS- F,404 RA = 09H 39M 48.0S +/- 0.1S, 1950.0 1 SURF(V) = 23.0 +/- 1.0 093942+4713- DEC = +47D 09' 51.0" +/- FLD2 ABELL 1.0" 851 Comments: THE FIELD CONTAINS MANY FAINT GALAXIES IN THE RANGE 21 < V < 25. ------------------------------------------------------------------------------------------------------------------------------------ 8 GAL-CLUS- F,404 RA = 02H 37M 28.6S +/- 0.1S, 1950.0 1 SURF(V) = 23.0 +/- 1.0 ABELL370- DEC = -01D 49' 36.0" +/- FLD2 1.0" Comments: THE FIELD CONTAINS MANY FAINT GALAXIES IN THE RANGE 21 < V < 25. TARGET LIST a) Fixed Targets ID = 5378 [ 6] ------------------------------------------------------------------------------------------------------------------------------------ 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial |Acqui|FLX| Flux data No | Name | Description | Position |Eqnx | Vel. |Prblm|REF| | | | | | | | | ------------------------------------------------------------------------------------------------------------------------------------ ------------------------------------------------------------------------------------------------------------------------------------ EXPOSURE LOGSHEET ID = 5378 [ 7] ------------------------------------------------------------------------------------------------------------------------------------ 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15 ------------------------------------------------------------------------------------------------------------------------------------ Line | Seq | Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | S/N |Flx|Pr| Special Number | Name | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| |Rel. Time|Ref| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1.1 GAL-CLUS- WFPC2 IMAGE WFALL- F814W CR-SPLIT=NO 4 2100S 1 CYCLE 4 / 1.1-1.4 001558+1609 FIX POS TARG +10,+10 GROUP 1.1-1.4 WITHIN 7D SAME ORIENT FOR 1.2-1.4 AS 1.1 Comments: POS TARG +10,+10 PLACES TARGET ORIENT 135D +/- COORDS ~AT APEX OF PYRAMID. 90D "GROUP WITHIN 7D" MAY BE RELAXED SO LONG AS BOTH "SAME ORIENT" AND "ABSOLUTE ORIENT" CONSTRAINTS CAN STILL BE MET VIA OFF-NOMINAL ROLL. ------------------------------------------------------------------------------------------------------------------------------------ 1.2 GAL-CLUS- WFPC2 IMAGE WFALL- F555W CR-SPLIT=NO 3 2100S 1 SAME POS FOR 1.2 001558+1609 FIX AS 1.1 ------------------------------------------------------------------------------------------------------------------------------------ 1.3 GAL-CLUS- WFPC2 IMAGE WFALL- F814W CR-SPLIT=NO 4 2100S 1 POS TARG +12,+12 001558+1609 FIX Comments: OFFSET 2 ARCSEC IN X AND 2 ARCSEC IN Y TO DISPLACE OBJECTS FROM PIXEL DEFECTS AND FROM SEAMS OF PYRAMID ------------------------------------------------------------------------------------------------------------------------------------ 1.4 GAL-CLUS- WFPC2 IMAGE WFALL- F555W CR-SPLIT=NO 3 2100S 1 SAME POS FOR 1.4 001558+1609 FIX AS 1.3 ------------------------------------------------------------------------------------------------------------------------------------ 2.1 GAL-CLUS- WFPC2 IMAGE WFALL- F814W CR-SPLIT=NO 4 2100S 1 CYCLE 4 / 2.1-2.4 005431-2756 FIX POS TARG +10,+10 GROUP 2.1-2.4 WITHIN 7D SAME ORIENT FOR 2.2-2.4 AS 2.1 Comments: POS TARG +10,+10 PLACES TARGET ORIENT 300D +/- COORDS ~AT APEX OF PYRAMID. 20D "GROUP WITHIN 7D" MAY BE RELAXED SO LONG AS BOTH "SAME ORIENT" AND "ABSOLUTE ORIENT" CONSTRAINTS CAN STILL BE MET VIA OFF-NOMINAL ROLL. ------------------------------------------------------------------------------------------------------------------------------------ 2.2 GAL-CLUS- WFPC2 IMAGE WFALL- F555W CR-SPLIT=NO 3 2100S 1 SAME POS FOR 2.2 005431-2756 FIX AS 2.1 ------------------------------------------------------------------------------------------------------------------------------------ 2.3 GAL-CLUS- WFPC2 IMAGE WFALL- F814W CR-SPLIT=NO 4 2100S 1 POS TARG +12,+12 005431-2756 FIX Comments: OFFSET 2 ARCSEC IN X AND 2 ARCSEC IN Y TO DISPLACE OBJECTS FROM PIXEL DEFECTS AND FROM SEAMS OF PYRAMID ------------------------------------------------------------------------------------------------------------------------------------ EXPOSURE LOGSHEET ID = 5378 [ 8] ------------------------------------------------------------------------------------------------------------------------------------ 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15 ------------------------------------------------------------------------------------------------------------------------------------ Line | Seq | Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | S/N |Flx|Pr| Special Number | Name | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| |Rel. Time|Ref| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2.4 GAL-CLUS- WFPC2 IMAGE WFALL- F555W CR-SPLIT=NO 3 2100S 1 SAME POS FOR 2.4 005431-2756 FIX AS 2.3 ------------------------------------------------------------------------------------------------------------------------------------ 3.1 GAL-CLUS- WFPC2 IMAGE WFALL- F702W CR-SPLIT=NO 4 2100S 1 CYCLE 4 / 3.1-3.2 160134+4254 FIX POS TARG +10,+10 GROUP 3.1-3.2 WITHIN 7D SAME ORIENT FOR 3.2 AS 3.1 Comments: POS TARG +10,+10 PLACES TARGET ORIENT 135D +/- COORDS ~AT APEX OF PYRAMID. 10D "GROUP WITHIN 7D" MAY BE RELAXED SO LONG AS BOTH "SAME ORIENT" AND "ABSOLUTE ORIENT" CONSTRAINTS CAN STILL BE MET VIA OFF-NOMINAL ROLL. ------------------------------------------------------------------------------------------------------------------------------------ 3.2 GAL-CLUS- WFPC2 IMAGE WFALL- F702W CR-SPLIT=NO 4 2100S 1 POS TARG +12,+12 160134+4254 FIX Comments: OFFSET 2 ARCSEC IN X AND 2 ARCSEC IN Y TO DISPLACE OBJECTS FROM PIXEL DEFECTS AND FROM SEAMS OF PYRAMID ------------------------------------------------------------------------------------------------------------------------------------ 4.1 GAL-CLUS- WFPC2 IMAGE WFALL- F814W CR-SPLIT=NO 4 2100S 1 CYCLE 4 / 4.1-4.4 041234-6558 FIX POS TARG +10,+10 GROUP 4.1-4.4 WITHIN 7D SAME ORIENT FOR 4.2-4.4 AS 4.1 Comments: POS TARG +10,+10 PLACES TARGET ORIENT 4D +/- 10D COORDS ~AT APEX OF PYRAMID. "GROUP WITHIN 7D" MAY BE RELAXED SO LONG AS BOTH "SAME ORIENT" AND "ABSOLUTE ORIENT" CONSTRAINTS CAN STILL BE MET VIA OFF-NOMINAL ROLL. ------------------------------------------------------------------------------------------------------------------------------------ 4.2 GAL-CLUS- WFPC2 IMAGE WFALL- F555W CR-SPLIT=NO 3 2100S 1 SAME POS FOR 4.2 041234-6558 FIX AS 4.1 ------------------------------------------------------------------------------------------------------------------------------------ 4.3 GAL-CLUS- WFPC2 IMAGE WFALL- F814W CR-SPLIT=NO 3 2100S 1 POS TARG +12,+12 041234-6558 FIX Comments: OFFSET 2 ARCSEC IN X AND 2 ARCSEC IN Y TO DISPLACE OBJECTS FROM PIXEL DEFECTS AND FROM SEAMS OF PYRAMID ------------------------------------------------------------------------------------------------------------------------------------ 4.4 GAL-CLUS- WFPC2 IMAGE WFALL- F555W CR-SPLIT=NO 3 2100S 1 SAME POS FOR 4.4 041234-6558 FIX AS 4.3 ------------------------------------------------------------------------------------------------------------------------------------ EXPOSURE LOGSHEET ID = 5378 [ 9] ------------------------------------------------------------------------------------------------------------------------------------ 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15 ------------------------------------------------------------------------------------------------------------------------------------ Line | Seq | Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | S/N |Flx|Pr| Special Number | Name | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| |Rel. Time|Ref| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 5.1 GAL-CLUS- WFPC2 IMAGE WFALL- F702W CR-SPLIT=NO 3 2100S 1 CYCLE 4 / 5.1-5.2 140933+5226 FIX POS TARG +10,+10 GROUP 5.1-5.2 WITHIN 7D SAME ORIENT FOR 5.2 AS 5.1 Comments: POS TARG +10,+10 PLACES TARGET ORIENT 110D +/- COORDS ~AT APEX OF PYRAMID. 10D "GROUP WITHIN 7D" MAY BE RELAXED SO LONG AS BOTH "SAME ORIENT" AND "ABSOLUTE ORIENT" CONSTRAINTS CAN STILL BE MET VIA OFF-NOMINAL ROLL. ------------------------------------------------------------------------------------------------------------------------------------ 5.2 GAL-CLUS- WFPC2 IMAGE WFALL- F702W CR-SPLIT=NO 3 2100S 1 POS TARG +12,+12 140933+5226 FIX Comments: OFFSET 2 ARCSEC IN X AND 2 ARCSEC IN Y TO DISPLACE OBJECTS FROM PIXEL DEFECTS AND FROM SEAMS OF PYRAMID ------------------------------------------------------------------------------------------------------------------------------------ 6.1 GAL-CLUS- WFPC2 IMAGE WFALL- F702W CR-SPLIT=NO 3 2100S 1 CYCLE 4 / 6.1-6.2 030330+1706 FIX POS TARG +10,+10 GROUP 6.1-6.2 WITHIN 7D SAME ORIENT FOR 6.2 AS 6.1 Comments: POS TARG +10,+10 PLACES TARGET ORIENT 225D +/- COORDS ~AT APEX OF PYRAMID. 10D "GROUP WITHIN 7D" MAY BE RELAXED SO LONG AS BOTH "SAME ORIENT" AND "ABSOLUTE ORIENT" CONSTRAINTS CAN STILL BE MET VIA OFF-NOMINAL ROLL. ------------------------------------------------------------------------------------------------------------------------------------ 6.2 GAL-CLUS- WFPC2 IMAGE WFALL- F702W CR-SPLIT=NO 3 2100S 1 POS TARG +12,+12 030330+1706 FIX Comments: OFFSET 2 ARCSEC IN X AND 2 ARCSEC IN Y TO DISPLACE OBJECTS FROM PIXEL DEFECTS AND FROM SEAMS OF PYRAMID ------------------------------------------------------------------------------------------------------------------------------------ EXPOSURE LOGSHEET ID = 5378 [ 10] ------------------------------------------------------------------------------------------------------------------------------------ 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15 ------------------------------------------------------------------------------------------------------------------------------------ Line | Seq | Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | S/N |Flx|Pr| Special Number | Name | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| |Rel. Time|Ref| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 7.1 GAL-CLUS- WFPC2 IMAGE WFALL- F814W CR-SPLIT=NO 1 2100S 1 CYCLE 4 / 7.1-7.41 093942+4713 FIX POS TARG +10,+10 -FLD2 GROUP 7.1-7.41 WITHIN 7D SAME ORIENT FOR 7.11-7.41 AS 7.1 Comments: POS TARG +10,+10 PLACES TARGET ORIENT 135D +/- COORDS ~AT APEX OF PYRAMID. 90D "GROUP WITHIN 7D" MAY BE RELAXED SO LONG AS BOTH "SAME ORIENT" AND "ABSOLUTE ORIENT" CONSTRAINTS CAN STILL BE MET VIA OFF-NOMINAL ROLL. ------------------------------------------------------------------------------------------------------------------------------------ 7.11 GAL-CLUS- WFPC2 IMAGE WFALL- F814W CR-SPLIT=NO 1 2100S 1 SAME POS FOR 7.11 093942+4713 FIX - 7.21 AS 7.1 -FLD2 ------------------------------------------------------------------------------------------------------------------------------------ 7.12 GAL-CLUS- WFPC2 IMAGE WFALL- F814W CR-SPLIT=NO 1 2100S 1 093942+4713 FIX -FLD2 ------------------------------------------------------------------------------------------------------------------------------------ 7.2 GAL-CLUS- WFPC2 IMAGE WFALL- F555W CR-SPLIT=0.5 1 2100S 1 093942+4713 FIX CR- -FLD2 TOLERANCE=0.0 Comments: CR-SPLIT=0.5 BECAUSE LESS THAN 6 EXPOSURES FOR COSMIC RAY REJECTION. THIS WILL RESULT IN 4 X 1000S EXPOSURES SINCE EACH 2100S/2=1050S WILL BE ROUNDED DOWN TO THE NEXT LOWEST LEGAL WFPC2 EXP TIME OF 1000S. ------------------------------------------------------------------------------------------------------------------------------------ 7.21 GAL-CLUS- WFPC2 IMAGE WFALL- F555W CR-SPLIT=0.5 1 2100S 1 093942+4713 FIX CR- -FLD2 TOLERANCE=0.0 ------------------------------------------------------------------------------------------------------------------------------------ 7.3 GAL-CLUS- WFPC2 IMAGE WFALL- F814W CR-SPLIT=NO 1 2100S 1 POS TARG +12,+12 093942+4713 FIX -FLD2 Comments: OFFSET 2 ARCSEC IN X AND 2 ARCSEC IN Y TO DISPLACE OBJECTS FROM PIXEL DEFECTS AND FROM SEAMS OF PYRAMID ------------------------------------------------------------------------------------------------------------------------------------ 7.31 GAL-CLUS- WFPC2 IMAGE WFALL- F814W CR-SPLIT=NO 1 2100S 1 SAME POS FOR 7.31 093942+4713 FIX - 7.41 AS 7.3 -FLD2 ------------------------------------------------------------------------------------------------------------------------------------ 7.32 GAL-CLUS- WFPC2 IMAGE WFALL- F814W CR-SPLIT=NO 1 2100S 1 093942+4713 FIX -FLD2 ------------------------------------------------------------------------------------------------------------------------------------ EXPOSURE LOGSHEET ID = 5378 [ 11] ------------------------------------------------------------------------------------------------------------------------------------ 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15 ------------------------------------------------------------------------------------------------------------------------------------ Line | Seq | Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | S/N |Flx|Pr| Special Number | Name | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| |Rel. Time|Ref| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 7.4 GAL-CLUS- WFPC2 IMAGE WFALL- F555W CR-SPLIT=0.5 1 2100S 1 093942+4713 FIX CR- -FLD2 TOLERANCE=0.0 Comments: CR-SPLIT=0.5 BECAUSE LESS THAN 6 EXPOSURES FOR COSMIC RAY REJECTION. THIS WILL RESULT IN 4 X 1000S EXPOSURES SINCE EACH 2100S/2=1050S WILL BE ROUNDED DOWN TO THE NEXT LOWEST LEGAL WFPC2 EXP TIME OF 1000S. ------------------------------------------------------------------------------------------------------------------------------------ 7.41 GAL-CLUS- WFPC2 IMAGE WFALL- F555W CR-SPLIT=0.5 1 2100S 1 093942+4713 FIX CR- -FLD2 TOLERANCE=0.0 ------------------------------------------------------------------------------------------------------------------------------------ 8.1 GAL-CLUS- WFPC2 IMAGE WFALL- F814W CR-SPLIT=NO 3 2100S 1 CYCLE 4 / 8.1-8.4 ABELL370- FIX POS TARG +10,+10 FLD2 GROUP 8.1-8.4 WITHIN 7D SAME ORIENT FOR 8.2-8.4 AS 8.1 Comments: POS TARG +10,+10 PLACES TARGET ORIENT 135D +/- COORDS ~AT APEX OF PYRAMID. 90D "GROUP WITHIN 7D" MAY BE RELAXED SO LONG AS BOTH "SAME ORIENT" AND "ABSOLUTE ORIENT" CONSTRAINTS CAN STILL BE MET VIA OFF-NOMINAL ROLL. ------------------------------------------------------------------------------------------------------------------------------------ 8.2 GAL-CLUS- WFPC2 IMAGE WFALL- F555W CR-SPLIT=0.5 2 2100S 1 SAME POS FOR 8.2 ABELL370- FIX CR- AS 8.1 FLD2 TOLERANCE=0.0 Comments: CR-SPLIT=0.5 BECAUSE LESS THAN 6 EXPOSURES FOR COSMIC RAY REJECTION. THIS WILL RESULT IN 4 X 1000S EXPOSURES SINCE EACH 2100S/2=1050S WILL BE ROUNDED DOWN TO THE NEXT LOWEST LEGAL WFPC2 EXP TIME OF 1000S. ------------------------------------------------------------------------------------------------------------------------------------ 8.3 GAL-CLUS- WFPC2 IMAGE WFALL- F814W CR-SPLIT=NO 3 2100S 1 POS TARG +12,+12 ABELL370- FIX FLD2 Comments: OFFSET 2 ARCSEC IN X AND 2 ARCSEC IN Y TO DISPLACE OBJECTS FROM PIXEL DEFECTS AND FROM SEAMS OF PYRAMID ------------------------------------------------------------------------------------------------------------------------------------ EXPOSURE LOGSHEET ID = 5378 [ 12] ------------------------------------------------------------------------------------------------------------------------------------ 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15 ------------------------------------------------------------------------------------------------------------------------------------ Line | Seq | Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | S/N |Flx|Pr| Special Number | Name | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| |Rel. Time|Ref| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 8.4 GAL-CLUS- WFPC2 IMAGE WFALL- F555W CR-SPLIT=0.5 2 2100S 1 SAME POS FOR 8.4 ABELL370- FIX CR- AS 8.3 FLD2 TOLERANCE=0.0 Comments: CR-SPLIT=0.5 BECAUSE LESS THAN 6 EXPOSURES FOR COSMIC RAY REJECTION. THIS WILL RESULT IN 4 X 1000S EXPOSURES SINCE EACH 2100S/2=1050S WILL BE ROUNDED DOWN TO THE NEXT LOWEST LEGAL WFPC2 EXP TIME OF 1000S. ------------------------------------------------------------------------------------------------------------------------------------ Summary Form for Proposal 5378 [ 13] Item Used in this proposal ------------------------------------------------------------------------------------------------------------------------------------ Configurations WFPC2 ------------------------------------------------------------------------------------------------------------------------------------ Opmodes IMAGE ------------------------------------------------------------------------------------------------------------------------------------ Optional Parameters CR-SPLIT=NO CR-SPLIT=0.5 CR-TOLERANCE=0.0 ------------------------------------------------------------------------------------------------------------------------------------ Proposal for GO ------------------------------------------------------------------------------------------------------------------------------------ S/C Hours 41.42 ------------------------------------------------------------------------------------------------------------------------------------ Scientific Category GALAXIES & CLUSTERS ------------------------------------------------------------------------------------------------------------------------------------ Scientific Sub-category DISTANT GALAXIES ------------------------------------------------------------------------------------------------------------------------------------ Special Requirements CYCLE 4 / 1.1-1.4; POS TARG +10,+10; GROUP 1.1-1.4 WITHIN 7D; SAME ORIENT FOR 1.2-1.4 AS 1.1; ORIENT 135D +/- 90D; SAME POS FOR 1.2 AS 1.1 POS TARG +12,+12; SAME POS FOR 1.4 AS 1.3 CYCLE 4 / 2.1-2.4; GROUP 2.1-2.4 WITHIN 7D; SAME ORIENT FOR 2.2-2.4 AS 2.1; ORIENT 300D +/- 20D; SAME POS FOR 2.2 AS 2.1 SAME POS FOR 2.4 AS 2.3 CYCLE 4 / 3.1-3.2; GROUP 3.1-3.2 WITHIN 7D; SAME ORIENT FOR 3.2 AS 3.1; ORIENT 135D +/- 10D; CYCLE 4 / 4.1-4.4; GROUP 4.1-4.4 WITHIN 7D; SAME ORIENT FOR 4.2-4.4 AS 4.1; ORIENT 4D +/- 10D; SAME POS FOR 4.2 AS 4.1 SAME POS FOR 4.4 AS 4.3 CYCLE 4 / 5.1-5.2; GROUP 5.1-5.2 WITHIN 7D; SAME ORIENT FOR 5.2 AS 5.1; ORIENT 110D +/- 10D; CYCLE 4 / 6.1-6.2; GROUP 6.1-6.2 WITHIN 7D; SAME ORIENT FOR 6.2 AS 6.1; ORIENT 225D +/- 10D; CYCLE 4 / 7.1-7.41; GROUP 7.1-7.41 WITHIN 7D; SAME ORIENT FOR 7.11-7.41 AS 7.1; SAME POS FOR 7.11 - 7.21 AS 7.1 SAME POS FOR 7.31 - 7.41 AS 7.3 CYCLE 4 / 8.1-8.4; GROUP 8.1-8.4 WITHIN 7D; SAME ORIENT FOR 8.2-8.4 AS 8.1; SAME POS FOR 8.2 AS 8.1 SAME POS FOR 8.4 AS 8.3 ------------------------------------------------------------------------------------------------------------------------------------ Spectral Elements F814W F555W F702W ------------------------------------------------------------------------------------------------------------------------------------ Target Names GAL-CLUS-001558+1609 CL0016+16 GAL-CLUS-005431-2756 J1888.16CL GAL-CLUS-160134+4254 HOG CLUSTER 16H-BETA-BETA GAL-CLUS-041234-6558 F1557-19TC GAL-CLUS-140933+5226 3C295 CLUSTER GAL-CLUS-030330+1706 HOG CLUSTER 3HCL2 GAL-CLUS-093942+4713-FLD2 ABELL 851 GAL-CLUS-ABELL370-FLD2 ------------------------------------------------------------------------------------------------------------------------------------