! $Id: 5234,v 8.1 1994/11/18 20:40:25 pepsa Exp $ coverpage: title_1: FAINT CLUSTERS OF GALAXIES (WC09) CYCLE 4 sci_cat: GALAXIES & CLUSTERS proposal_for: GTO/WFC pi_title: PROF. pi_fname: JAMES pi_mi: A. pi_lname: WESTPHAL pi_inst: CALTECH pi_country: USA pi_phone: (818) 395-4900 keywords_1: BRIGHTEST GALAXY, COSMOLOGY, SPIRAL GALAXY, GALAXY keywords_2: EVOLUTION, GALAXY MORPHOLOGY, DISTANT GALAXY CLUSTER hours_pri: 31.03 num_pri: 4 wf_pc: Y pi_position: PROFESSOR OF PLANETA ! end of coverpage abstract: line_1: Two distant clusters of galaxies, with redshifts from 0.70 to 0.92, will line_2: be imaged in two colors corresponding to rest wavelengths of about 3400 and line_3: 4500 angstroms. The primary object of the study is to investigate the color line_4: and morphological evolution of cluster galaxies. Sufficient signal-to-noise line_5: will be obtained for all objects to see spiral structure, if present, and all line_6: fields contain starburst galaxies, whose morphology is of special interest. line_7: In addition, the data will yield structural parameters for the bright cluster line_8: galaxiess, which will aid in interpreting the classical Hubble diagram for line_9: the determination of the deceleration parameter. ! ! end of abstract general_form_proposers: lname: WESTPHAL fname: JAMES title: PROF. mi: A. inst: CALTECH country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: The observations consist of imaging a set of distant clusters in two line_2: colors (except the most distant cluster, for which the rest 4500 line_3: angstrom filter corresponds to a passband beyond the red limit of our line_4: instrument), with total exposures calculated to give comparable line_5: signal-to-noise for all objects. Positions for two of the clusters line_6: are still approximate and need to be verified with GASP, but all line_7: orientations are final. We still need to decide whether to dither line_8: the pointings slightly on the multiple exposures. ! question: 6 section: 1 line_1: All the exposures are specified as non-interruptible. No separate CR line_2: splits are called out because of the multiple exposures. ! question: 13 section: 1 line_1: Three distant cluster will be studied using multicolor imaging to investigate line_2: morphological and photometric evolution of galaxies and clusters. The data will line_3: also be used to perform classical photometric and angular-diameter cosmological line_4: tests. The redshift range covers clusters from 0.72 to 0.92. The clusters line_5: are: 1322+3115, 1322+3027, and 1603+4313. ! !end of general form text general_form_address: lname: FABER fname: SANDRA mi: M. category: CON inst: UC SANTA CRUZ - LICK OBSERVATORY addr_1: NATURAL SCIENCES II city: SANTA CRUZ state: CA zip: 95064 country: USA phone: 408-459-2944 ! lname: WESTPHAL fname: JAMES mi: A. title: PROF. category: PI inst: CALTECH addr_1: M/S 170-25 addr_2: DIVISION OF GEOLOGICAL addr_3: & PLANETARY SCIENCES city: PASADENA state: CA zip: 91125 country: USA phone: 818-395-4900 ! lname: LAUER fname: TOD mi: R. category: CON inst: NOAO addr_1: PO BOX 26732 city: TUCSON state: AZ zip: 85726 country: USA phone: 602-327-5511 ! lname: BAUM fname: WILLIAM category: CON inst: UNIV. WASHINGTON addr_1: 2124 NE PARK ROAD city: SEATTLE state: WA zip: 98105 country: USA phone: 206-527-4306 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: GAL-CLUS1322+3027-POS1 descr_1: F, 406 pos_2: RA = 13H22M29.82S +/-0.01S, pos_3: DEC = +30D26'57" +/-0.1" equinox: 1950.0 pm_or_par: N rv_or_z: Z=0.76 comment_1: COORD UPDATE SMF/AD 2/15/93. comment_2: THESE SHOULD BE FINAL. ! targnum: 2 name_1: GAL-CLUS1322+3027-POS2 descr_1: F, 406 pos_1: RA-OFF = +0.23S +/- 0.01S, pos_2: DEC-OFF = 0" +/- 0.1", pos_3: FROM 1 equinox: 1950.0 pm_or_par: N rv_or_z: Z=0.76 comment_1: COORD UPDATE SMF/AD 2/15/93. comment_2: THESE SHOULD BE FINAL. ! targnum: 3 name_1: GAL-CLUS1603+4313-POS1 descr_1: F, 406 pos_1: RA= 16H02M39.17S +/- 0.01S, pos_2: DEC= +43D12'44" +/- 0.1" equinox: 1950 pm_or_par: N rv_or_z: Z=0.92 comment_1: COORD UPDATE SMF/AD 2/15/93. comment_2: NEED CHECKING. ! targnum: 4 name_1: GAL-CLUS1603+4313-POS2 descr_1: F, 406 pos_1: RA-OFF = 0.0S +/- 0.01S, pos_2: DEC-OFF = +2" +/- 0.1", pos_3: FROM 3 equinox: 1950.0 pm_or_par: N rv_or_z: Z=0.92 comment_1: COORD UPDATE SMF/AD 2/15/93. comment_2: NEED CHECKING. ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 targname: GAL-CLUS1322+3027-POS1 config: WFPC2 opmode: IMAGE aperture: WFALL-FIX sp_element: F606W num_exp: 4 time_per_exp: 2000S priority: 1 param_1: CR-SPLIT=NO req_1: CYCLE 4; req_2: NON-INT; req_3: ORIENT 326.5D +/- 20D; req_4: GROUP 1-4 WITHIN 7D; req_5: POS TARG +10.0,+10.0; comment_1: ALL EXPOSURES TO FIT SNUGLY comment_2: WITHIN ONE ORBIT. ADJUST comment_3: EXP TIME AS NECESSARY. POS comment_4: TARG PUTS TARG COORDS ON PYR comment_5: APEX (ALL OBJECTS). ! linenum: 2.000 targname: GAL-CLUS1322+3027-POS1 config: WFPC2 opmode: IMAGE aperture: WFALL-FIX sp_element: F814W num_exp: 8 time_per_exp: 2000S priority: 1 param_1: CR-SPLIT=NO req_1: CYCLE 4; req_2: NON-INT; req_3: SAME ORIENT FOR 2-4 AS 1; req_4: SAME POS FOR 2 AS 1 comment_1: ALL EXPOSURES TO FIT SNUGLY comment_2: WITHIN ONE ORBIT. ADJUST comment_3: EXP TIME AS NECESSARY. ! linenum: 3.000 targname: GAL-CLUS1322+3027-POS2 config: WFPC2 opmode: IMAGE aperture: WFALL-FIX sp_element: F606W num_exp: 4 time_per_exp: 2000S priority: 1 param_1: CR-SPLIT=NO req_1: CYCLE 4; req_2: NON-INT; req_3: POS TARG +10.0,+10.0; comment_1: ALL EXPOSURES TO FIT SNUGLY comment_2: WITHIN ONE ORBIT. ADJUST comment_3: EXP TIME AS NECESSARY. ! linenum: 4.000 targname: GAL-CLUS1322+3027-POS2 config: WFPC2 opmode: IMAGE aperture: WFALL-FIX sp_element: F814W num_exp: 8 time_per_exp: 2000S priority: 1 param_1: CR-SPLIT=NO req_1: CYCLE 4; req_2: NON-INT; req_3: SAME POS FOR 4 AS 3; comment_1: ALL EXPOSURES TO FIT SNUGLY comment_2: WITHIN ONE ORBIT. ADJUST comment_3: EXP TIME AS NECESSARY. ! linenum: 20.000 targname: GAL-CLUS1603+4313-POS1 config: WFPC2 opmode: IMAGE aperture: WFALL-FIX sp_element: F814W num_exp: 8 time_per_exp: 2000S priority: 2 param_1: CR-SPLIT=NO req_1: CYCLE 4; req_2: NON-INT; req_3: ORIENT 291D +/- 1D; req_4: GROUP 20-21 WITHIN 2D; req_5: POS TARG +10.0,+10.0; comment_1: ALL EXPOSURES TO FIT SNUGLY comment_2: WITHIN ONE ORBIT. ADJUST comment_3: EXP TIME AS NECESSARY. ! linenum: 21.000 targname: GAL-CLUS1603+4313-POS2 config: WFPC2 opmode: IMAGE aperture: WFALL-FIX sp_element: F814W num_exp: 8 time_per_exp: 2000S priority: 2 param_1: CR-SPLIT=NO req_1: CYCLE 4; req_2: NON-INT; req_3: SAME ORIENT FOR 21 AS 20; req_4: POS TARG +10.0,+10.0; comment_1: ALL EXPOSURES TO FIT SNUGLY comment_2: WITHIN ONE ORBIT. ADJUST comment_3: EXP TIME AS NECESSARY. linenum: 30.000 targname: GAL-CLUS1603+4313-POS1 config: WFPC2 opmode: IMAGE aperture: WFALL-FIX sp_element: F814W num_exp: 8 time_per_exp: 2000S priority: 2 param_1: CR-SPLIT=NO req_1: CYCLE 4; req_2: NON-INT; req_3: ORIENT 291D +/- 1D; req_4: GROUP 30-31 WITHIN 2D; req_5: POS TARG +10.0,+10.0; comment_1: ALL EXPOSURES TO FIT SNUGLY comment_2: WITHIN ONE ORBIT. ADJUST comment_3: EXP TIME AS NECESSARY. ! linenum: 31.000 targname: GAL-CLUS1603+4313-POS2 config: WFPC2 opmode: IMAGE aperture: WFALL-FIX sp_element: F814W num_exp: 8 time_per_exp: 2000S priority: 2 param_1: CR-SPLIT=NO req_1: CYCLE 4; req_2: NON-INT; req_3: SAME ORIENT FOR 21 AS 20; req_4: POS TARG +10.0,+10.0; comment_1: ALL EXPOSURES TO FIT SNUGLY comment_2: WITHIN ONE ORBIT. ADJUST comment_3: EXP TIME AS NECESSARY. ! ! end of exposure logsheet ! No scan data records found