! $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