! Proposal 6358, submission 4
! PI: Luis Colina
! Received Fri Mar 22 15:30:12 EST 1996
! From: colina@stsci.edu
! Hubble Space Telescope Cycle 6 (1996) Phase II Proposal Template
! $Id: 6358,v 6.1 1996/03/29 19:59:26 pepsa Exp $
!
! Refer to the HST Phase II Proposal Instructions to fill this out
!
! Anything after a "!" is ignored, and may be deleted
!
! All keywords with multiple entries are comma delimited except the
! Visit_Requirements and Special_Requirements keywords which can be
! delimited with carriage returns or semi-colons, but not commas
!
! For help call your Program Coordinator: Giselle Sleiman
! Phone: 410 338-4753 , E-mail: sleiman@stsci.edu
!
! This partially completed template was generated from a Phase I proposal.
! Name of Phase I Proposal: archive-0773.colina.prop
! Date generated: Fri Nov 10 16:48:06 EST 1995
!
Proposal_Information ! Section 4
Title: UV IMAGING OF CIRCUMNUCLEAR STARBURST
RINGS
Proposal_Category: SNAP
Scientific_Category: G&C
Cycle: 6
Investigators
PI_name: Luis Colina
PI_Institution: Space Telescope Science Institute
CoI_Name: Marisa Garcia-Vargas
CoI_Institution: IUE Observatory, Madrid
Contact: Y ! Y or N (designate at most one contact)
CoI_Name: Miguel Mas-Hesse
CoI_Institution: INTA/LAEFF, Madrid
Contact: N ! Y or N (designate at most one contact)
CoI_Name: Antxon Alberdi
CoI_Institution: INTA/LAEFF, Madrid
Contact: Y ! Y or N (designate at most one contact)
CoI_Name: Alfred Krabbe
CoI_Institution: Max-Planck Institut fur Extraterrestrische
Physik
Contact: N ! Y or N (designate at most one contact)
Abstract: ! Free format text (please update)
We propose to obtain F218W WFPC images of a well
defined sample of nearby galaxies with face-on
circumnuclear starburst rings, and covering different levels
of activity from pure starbursts to Seyfert 1 (AGNs). These
high resolution images will allow to generate
for the first time an homogeneous database with the UV
properties of about 60 individual circumnuclear star-forming
knots. The use of the database will allow for the first time
a direct and quantitative determination of basic ultraviolet
properties of individual nuclear/circumnuclear star-forming
knots, and of the entire starburst ring, such as: (a) their
size and structure, (b) their UV luminosity function and,
(c) their contribution to the UV energy output in composite
AGN+starburst galaxies. The database will help in our understanding
of high redshift blue galaxies, thought to be star-forming galaxies,
where the flux detected in optical filters corresponds to flux emitted
at UV (1500-3000Angstrom) rest frame wavelengths. The
requested UV images will be combined with ROSAT/HRI images to
characterize for the first time the high energy end, i.e. UV
to soft X-rays, of circumnuclear starburst rings.
Questions ! Free format text (please update)
Observing_Description:
We propose to obtain images of a sample of 20 nearby
spiral galaxies with face-on circumnuclear
starburst rings of about 10'' to 15'' in diameter. The sample
covers a range of nuclear activity from pure starbursts
to LINER+HII, Sy2+HII, and Sy1+HII. Each galaxy consists of three to
five high surface brightness independent star-forming knots,
judging from ground-based V and/or HAlpha images. The UV
filter has been selected to be sensitive to the presence of
unobscured UV-luminous clusters of recently formed hot
massive stars. Due to the degradation of the WFPC2 UV
throughput, we require to obtain the images within few days
after the monthly decontamination. Our proposed images would be
obtained as a SNAPSHOT survey with WFPC2, using the F218W band
filter, placing each target in the center of WF3.
Since we are requesting 20 minutes exposures, we request the
observations to be taken with Fine Lock guiding.
Exposure Time - In the following we assume a WFPC2 pixel of
0.1'', and a WFPC2 readout noise (RN) of 5 electrons per pixel.
The 20 minutes of integration time will be equally divided in
two exposures of 10 minutes each, utilizing CR-SPLIT. We
consider that each individual circumnuclear star-forming knot
has on average a size of about 100 parsecs, i.e. a projected
size of 1'' at a distance of 20 Mpc. We also consider that
the brightest circumnuclear star-forming regions in our
sample galaxies are similar to those detected in NGC 1068.
Using the observed ultraviolet fluxes of the NGC 1068
circumnuclear star-forming regions (Bruhweiler et al. 1991,
ApJ 379, 596), each of the individual brightest star-forming
knots in our sample galaxies is assumed to have an observed
UV flux of about 1.0 * 10^-14 ergs cm^-2 s^-1 AA^-1. Assuming
that the spectrum of Vega defines the zero point of the UV
filter (F218W: 4.50 * 10^-9 ergs cm^-2 s^-1 AA^-1) the above
mentioned UV flux corresponds to a surface brightness of ~ 20
mag per pixel. The signal (S) and noise (N) per pixel after N_exp
exposures of T seconds of integration each, (utilizing CR-
SPLIT) is given by: S= 2.5 * 10^11 * N_exp * T *
(QT) * 10^-0.4(Mu/pix) N= (2.5 * 10^11 * N_exp * T * (QT) *
10^-0.4(Mu/pix) + N * RN^2)^1/2, where RN is the readout
noise and (QT)= 0.00057. The requested
integration time will allow to investigate not only the
structure of the brightest star-forming knots but also to
detect fainter knots with a signal-to-noise of ~ 5-10.
Real_Time_Justification:
None
Four of the galaxies in the sample (plus NGC 1068 and NGC
2903) have already been observed with the ROSAT high
resolution imager (HRI) by members of our team or others. We
plan to request ROSAT/HRI observations for the rest of the
sample. The combination of ROSAT/HRI and HST images will
allow to investigate for the first time the UV and soft X-ray
properties of circumnuclear star-forming regions. The
diameter of the circumnuclear rings in the sample galaxies
(10'' to 15'') are such to allow resolving the nuclear and
circumnuclear regions in the HRI images. Broad- and narrow-
band images for most of the galaxies in the sample have
already been obtained by our team, allowing for the
comparison (at low resolution) with the UV mapping provided
by HST.
Calibration_Justification: ! Move appropriate text from Real_Time_Justification
Additional_Comments:
Fixed_Targets ! Section 5.1
Target_Number: 1
Target_Name: NGC1097
Alternate_Names:
Description: GALAXY, Liner, Starburst, Spiral
Position: RA=02H 46M 18.97S +/-0.1S, DEC=-30D 16' 29.2" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=11.1 ! Include at least V and B-V
Comments:
Target_Number: 2
Target_Name: NGC1667
Alternate_Names:
Description: GALAXY, Seyfert, Starburst, Spiral
Position: RA=04H 48M 37.05S +/-0.1S, DEC=-06D 19' 11.5" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=11.8 ! Include at least V and B-V
Comments:
Target_Number: 3
Target_Name: NGC1808
Alternate_Names:
Description: GALAXY, Starburst, Spiral
Position: RA=05H 07M 42.35S +/-0.1S, DEC=-37D 30' 46.1" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=9.8 ! Include at least V and B-V
Comments:
Target_Number: 4
Target_Name: NGC3147
Alternate_Names:
Description: GALAXY, Starburst, Spiral
Position: RA=10H 16M 53.16S +/-0.1S, DEC=+73D 24' 03.5" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=10.5 ! Include at least V and B-V
Comments:
Target_Number: 5
Target_Name: NGC3351
Alternate_Names:
Description: GALAXY, Starburst, Spiral
Position: RA=10H 43M 57.96S +/-0.1S, DEC=+11D 42' 14.3" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=9.6 ! Include at least V and B-V
Comments:
Target_Number: 6
Target_Name: NGC3504
Alternate_Names:
Description: GALAXY, Starburst, Spiral
Position: RA=11H 03M 11.19S +/-0.1S, DEC=+27D 58' 21.5" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=10.9 ! Include at least V and B-V
Comments:
Target_Number: 7
Target_Name: NGC3982
Alternate_Names:
Description: GALAXY, Seyfert, Starburst, Spiral
Position: RA=11H 56M 28.06S +/-0.1S, DEC=+55D 07' 30.0" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=11.0 ! Include at least V and B-V
Comments:
Target_Number: 8
Target_Name: NGC4303
Alternate_Names:
Description: GALAXY, Seyfert, Starburst, Spiral
Position: RA=12H 21M 54.84S +/-0.1S, DEC=+04D 28' 24.8" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=9.6 ! Include at least V and B-V
Comments:
Target_Number: 9
Target_Name: NGC4314
Alternate_Names:
Description: GALAXY, Liner, Starburst, Spiral
Position: RA=12H 22M 31.94S +/-0.1S, DEC=+29D 53' 43.1" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=10.4 ! Include at least V and B-V
Comments:
Target_Number: 10
Target_Name: NGC4321
Alternate_Names:
Description: GALAXY, Starburst, Spiral
Position: RA=12H 22M 54.88S +/-0.1S, DEC=+15D 49' 18.7" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=9.3 ! Include at least V and B-V
Comments:
Target_Number: 11
Target_Name: NGC4995
Alternate_Names:
Description: GALAXY, Starburst, Spiral
Position: RA=13H 09M 40.42S +/-0.1S, DEC=-07D 50' 01.3" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=10.8 ! Include at least V and B-V
Comments:
Target_Number: 12
Target_Name: NGC3504R
Alternate_Names:
Description: GALAXY, Seyfert 2, Starburst, Spiral
Position: RA= 11H 03M 11.2S +/-0.1S, DEC=+27D 58' 22.0" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=12.0 ! Include at least V and B-V
Comments:
Target_Number: 13
Target_Name: NGC5248
Alternate_Names:
Description: GALAXY, Starburst, Spiral
Position: RA=13H 37M 31.80S +/-0.1S, DEC=+08D 53' 07.9" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=10.0 ! Include at least V and B-V
Comments:
Target_Number: 14
Target_Name: NGC5427
Alternate_Names:
Description: GALAXY, Seyfert, Starburst, Spiral
Position: RA=14H 03M 26.01S +/-0.1S, DEC=-06D 01' 51.1" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=11.3 ! Include at least V and B-V
Comments:
Target_Number: 15
Target_Name: NGC5728
Alternate_Names:
Description: GALAXY, Seyfert, Starburst, Spiral
Position: RA=14H 42M 23.85S +/-0.1S, DEC=-17D 15' 11.0" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=11.5 ! Include at least V and B-V
Comments:
Target_Number: 16
Target_Name: NGC5953
Alternate_Names:
Description: GALAXY, Seyfert, Starburst, Spiral
Position: RA=15H 34M 32.5S +/-0.1S, DEC=+15D 11' 37.8" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=12.4 ! Include at least V and B-V
Comments:
Target_Number: 17
Target_Name: NGC6574
Alternate_Names:
Description: GALAXY, Starburst, Spiral
Position: RA=18H 11M 51.18S +/-0.1S, DEC=+14D 58' 54.7" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=11.2 ! Include at least V and B-V
Comments:
Target_Number: 18
Target_Name: NGC5930
Alternate_Names:
Description: GALAXY, Starburst, Spiral
Position: RA=15H 26M 07.9S +/-0.1S, DEC=+41D 40' 33.3" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: ! Include at least V and B-V
Comments:
Target_Number: 19
Target_Name: NGC7469
Alternate_Names:
Description: GALAXY, Seyfert, Starburst, Spiral
Position: RA=23H 03M 15.55S +/-0.1S, DEC=+08D 52' 26.2" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=12.2 ! Include at least V and B-V
Comments:
Target_Number: 20
Target_Name: NGC7552
Alternate_Names:
Description: GALAXY, Starburst, Spiral
Position: RA=23H 16M 10.66S +/-0.1S, DEC=-42D 35' 04.7" +/-1"
! RA=0H 0M 0.00S +/- 0S,
! DEC=0D 0' 0.0" +/- 0",
! PLATE-ID=0000
Equinox: 2000
RV_or_Z:
RA_PM: ! Units are seconds of time per year
Dec_PM: ! Units are seconds of arc per year
Epoch:
Annual_Parallax:
Flux: V=11.1 ! Include at least V and B-V
Comments:
! This is a template for a single visit containing a single exposure
! Repeat exposure and visit blocks as needed
Visits ! Section 6
Visit_Requirements: ! Section 7.1
! Uncomment or copy visit level special requirements needed
! Most of these requirements (including ORIENT) will limit scheduling
! PCS MODE [Fine | Gyro]
! GUIDing TOLerance <angle>
! ORIENTation <angle1> TO <angle2>
! ORIENTation <angle1> TO <angle2> FROM <visit>
! ORIENTation <angle1> TO <angle2> FROM NOMINAL
! SAME ORIENTation AS <visit>
! CVZ
! PARallel
! AFTER <visit> [BY <time1> [TO <time2>]]
! AFTER <date>
! BEFORE <date>
! BETWEEN <date1> AND <date2>
! GROUP <visit-list> WITHIN <time>
! PERIOD <time> AND ZERO-PHASE <date>
! SEQ <visit-list> WITHIN <time>
! ON HOLD [FOR <visit>]
Visit_Number: 1
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 1 ! Section 6.5
Target_Name: NGC1097
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 2
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 2 ! Section 6.5
Target_Name: NGC1667
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 3
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 3 ! Section 6.5
Target_Name: NGC1808
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 4
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 4 ! Section 6.5
Target_Name: NGC3147
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 5
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 5 ! Section 6.5
Target_Name: NGC3351
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 6
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 6 ! Section 6.5
Target_Name: NGC3504
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 7
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 7 ! Section 6.5
Target_Name: NGC3982
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 8
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 8 ! Section 6.5
Target_Name: NGC4303
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 9
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 9 ! Section 6.5
Target_Name: NGC4314
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 10
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 10 ! Section 6.5
Target_Name: NGC4321
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 11
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 11 ! Section 6.5
Target_Name: NGC4995
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 12
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 12 ! Section 6.5
Target_Name: NGC3504R
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 13
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 13 ! Section 6.5
Target_Name: NGC5248
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 14
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 14 ! Section 6.5
Target_Name: NGC5427
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 15
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 15 ! Section 6.5
Target_Name: NGC5728
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 16
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 16 ! Section 6.5
Target_Name: NGC5953
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 17
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 17 ! Section 6.5
Target_Name: NGC6574
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 18
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 18 ! Section 6.5
Target_Name: NGC5930
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 19
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 19 ! Section 6.5
Target_Name: NGC7469
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
Visit_Number: 20
On_Hold_Comments:
Visit_Comments: Imges should preferably be obtained within the first 7/10 days after the WFPC2 monthly decontamination.
Exposure_Number: 20 ! Section 6.5
Target_Name: NGC7552
Config: WFPC2
Opmode: IMAGE
Aperture: WF3-FIX
Sp_Element: F218W
Wavelength:
Optional_Parameters: CR-SPLIT=DEF, CR-TOLERANCE=0.0
Number_of_Iterations: 1
Time_Per_Exposure: 20M
Special_Requirements: ! Section 7.2
! Uncomment or copy exposure level special requirements needed
! INTeractive ACQuisition FOR <exp-list>
! ONBOARD ACQuisition FOR <exp-list>
! POSition TARGet <x-value>,<y-value>
! SAME POSition AS <exp>
! DO FOR TARGets <targ-list> ! FGS only
! PARallel WITH <exp>
! GROUP-FGS <exp-list> WITHIN <time>
! SPATIAL SCAN <#> [<exp-list> | SINGLE-EXP ]
! RT ANALYSIS [FOR <exp-list>]
! REQuires UPLINK
! DARK TIME
! END ORBIT
! EXPAND
! MAXimum DURation [<time> | <%>]
! MINimum DURation [<time> | <%>]
! NO SPLIT
! PHASE <number1[0,1]> TO <number2[0,1]>
! SEQuence <exp-list> NON-INTerruptible
Comments:
Data_Distribution ! Defaults indicated; change if desired
Medium: 8MM ! 8MM or 6250BPI or 1600BPI
Blocking_Factor: 10 ! 10 or 1
! Only astronomers with very old 9-
! track tape drives should consider
! a blocking factor of 1
Ship_To: Luis Colina ! STSCI or PI_Address or <free-text>
! PI Address from Phase I is:
!
3700 San Martin Drive
Baltimore
MD 21218
!
!
Ship_Via: ! UPS (2-day) or OVERNIGHT
! Overnight shipping done at PI expense
Recipient_Email: ! Needed if Ship_To: is not PI_Address
! <free-text>
! Let us know what you think of this template and software!
! Please send a list of your likes and dislikes to your Program Coordinator