! File: 1194C.PROP
! Database: PEPDB
! Date: 16-FEB-1994:05:28:33
coverpage:
title_1: IMAGING AND SPECTROSCOPY OF THE NEARBY QSO 2130+099:
title_2: FUTURE-CYCLE CONTINUATION
sci_cat: QUASARS & AGN
sci_subcat: QUASAR ABSORPTION
proposal_for: GTO/HRS
pi_fname: SARA
pi_lname: HEAP
pi_inst: NASA/GSFC
pi_country: USA
pi_phone: 301-286-5359
keywords_1: QUASARS, SPIRAL GALAXY, STELLAR POPULATION, MORPHOLOGY
hours_pri: 5.00
num_pri: 1
! end of coverpage
abstract:
line_1: We will make four types of observations of the nearby QSO
line_2: 2130+099: (1) images with the PC: (2) UV maps of the nucleus
line_3: with the GHRS N2 mirror; (3) UV spectrum of the nucleus
line_4: with either FOS or GHRS/D1 and (4) UV spectrum of a knot
line_5: in the spiral arm of the host galaxy.
!
! end of abstract
general_form_proposers:
lname: HEAP
fname: SARA
inst: NASA/GSFC
country: USA
!
! end of general_form_proposers block
general_form_text:
question: 2
section: 1
line_1: QSO 2130+099 is a nearby QSO with z=0.061 and v=14.4. Our
line_2: recent studies of this object including image-deconvolution
line_3: indicate that the host galaxy is a barred spiral with a central
line_4: surface brightness, mu(B)=21.3 mag per sq. arcsec and a scale
line_5: length of 4 kpc. We will continue our studies of this object
line_6: with the HST/WFPC and GHRS by making four types of
line_7: observations: (1) images of the quasar-host galaxy with the
line_8: PC; (2) UV maps of the nucleus with the GHRS; (3) UV spectrum
line_9: of the nucleus with the GHRS; and (4) off-nuclear ultraviolet
line_10: spectrum of the host galaxy with the GHRS. We shall use the
line_11: UV spectrum of the nucleus to search for "nearby" Lyman
line_12: alpha clouds.
!
question: 3
section: 1
line_1: Schedule in Cycle 3 AFTER the repair mission.
line_2: Schedule the GHRS observations in dark time, so that
line_3: geocoronal Ly alpha emission doesn't swamp the target.
!
question: 4
section: 1
line_1: Only the HST can give the required angular resolution and
line_2: UV throughput and spectral resolution.
!
question: 5
section: 1
line_1: Lines 20-22 call for GHRS field maps that are not standard.
!
question: 7
section: 1
line_1: Astrometric reduction of the PC images will be done at the
line_2: STScI in order to obtain precise coordinates of the region
line_3: for GHRS observations. Reduction and analysis of the data
line_4: will be done at GSFC.
!
question: 13
section: 1
line_1: We will obtain images and UV spectra of QSO 2130+099.
!
!end of general form text
general_form_address:
lname: HEAP
fname: SARA
category: PI
inst: NASA/GSFC
addr_1: CODE 681
city: GREENBELT,
state: MD
zip: 20771
country: USA
phone: (301)-286-5359
!
! end of general_form_address records
fixed_targets:
targnum: 1
name_1: QSO2130+099-NUCLEUS
name_2: II-ZW-136
descr_1: E, 313,321,910,928
pos_1: RA=21H32M27.91S+/-0.75",
pos_2: DEC=10D08'20.2"+/-0.75",
pos_3: PLATE-ID=02KW
equinox: 2000
pm_or_par: NO
rv_or_z: Z=0.061
comment_1: POSITION DETERMINED FROM GSSS.
fluxnum_1: 1
fluxval_1: V=14.4+/-0.2
fluxnum_2: 2
fluxval_2: F-LINE(1216)=2.6E-12
!
targnum: 2
name_1: QSO2130+099-OFFSET
descr_1: SPIRAL ARM OF HOST GALAXY
pos_1: R=10" +/- 2",
pos_2: PA=240D +/- 40D,
pos_3: FROM 1
equinox: ^
pm_or_par: ^
rv_or_z: ^
fluxnum_1: 1
fluxval_1: SURF(V)=22.0+/-1.0
!
! end of fixed targets
! No solar system records found
! No generic target records found
exposure_logsheet:
linenum: 3.000
targname: QSO2130+099-NUCLEUS
config: PC
opmode: IMAGE
aperture: PC6
sp_element: F547M
num_exp: 1
time_per_exp: 20M
priority: 1
param_1: PRE-FLASH=YES
req_1: EARLY ACQ FOR 4-22;
req_2: CYCLE 3
comment_1: F547M INCLUDES REDSHIFTED H-BETA
comment_2: AND [OIII] SPIRAL INDICATORS .
!
linenum: 4.000
targname: QSO2130+099-NUCLEUS
config: PC
opmode: IMAGE
aperture: PC6
sp_element: F547M
num_exp: 1
time_per_exp: 20M
priority: 1
param_1: PRE-FLASH=YES
req_1: EARLY ACQ FOR 10-12;
req_2: CYCLE 9
comment_1: REPEAT OF LINE 3,
comment_2: DO AFTER THE REPAIR WITH WFPC2
!
linenum: 10.000
targname: QSO2130+099-NUCLEUS
config: FOS/BL
opmode: ACQ/BINARY
aperture: 4.3
sp_element: MIRROR
num_exp: 1
time_per_exp: 10S
priority: 1
req_1: ONBOARD ACQ FOR 11;
req_2: CYCLE 3
comment_1: DO 10-12 BEFORE THE REPAIR OF HST
!
linenum: 11.000
targname: QSO2130+099-NUCLEUS
config: FOS/BL
opmode: ACCUM
aperture: 1.0
sp_element: G130H
wavelength: 1150-1608
num_exp: 1
time_per_exp: 60M
priority: 1
req_1: CYCLE 3
!
linenum: 12.000
targname: QSO2130+099-OFFSET
config: FOS/BL
opmode: ACCUM
aperture: 1.0
sp_element: G130H
wavelength: 1150-1608
num_exp: 1
time_per_exp: 60M
priority: 1
req_1: CYCLE 3
!
linenum: 20.000
targname: QSO2130+099-NUCLEUS
config: HRS
opmode: ACQ
aperture: 2.0
sp_element: MIRROR-N2
num_exp: 1
time_per_exp: 18.0S
priority: 1
param_1: LOCATE=YES,
param_2: FAINT=100
req_1: ONBOARD ACQ FOR 21-22;
req_2: DARK TIME; SEQ 21-22 NON-INT;
req_3: CYCLE 9
comment_1: EXPECTED COUNT/RATE > 2200,
comment_2: BASED ON IUE SPECTRA. GEOCORONA
comment_3: NOT A PROBLEM FOR FAINT HOST
comment_4: GALAXY IF SCHEDULED DURING DARK
comment_5: TIME. FORMERLY CYCLE 0
!
linenum: 21.000
targname: QSO2130+099-NUCLEUS
config: HRS
opmode: IMAGE
aperture: 2.0
sp_element: MIRROR-N2
num_exp: 2
time_per_exp: 256S
priority: 1
param_1: NX=16,
param_2: DELTA-X=4,NY=16, DELTA-Y=4
req_1: CYCLE 9
comment_1: SHOULD PRODUCE A FULL MAP OF
comment_2: THE LARGE APERTURE. STEP-TIME=1.
comment_3: FORMERLY CYCLE 0.
!
linenum: 22.000
targname: QSO2130+099-NUCLEUS
config: HRS
opmode: IMAGE
aperture: 2.0
sp_element: MIRROR-N2
num_exp: 1
time_per_exp: 3.2M
priority: 1
param_1: NX=64,DELTA-X=1,
param_2: NY=3,DELTA-Y=4
req_1: CYCLE 9
comment_1: THIS SCAN SHOULD BE CENTERED
comment_2: ON THE CENTER OF THE LSAP.
comment_3: STEP-TIME=1. FORMERLY CYCLE 0.
!
! end of exposure logsheet
! No scan data records found