! $Id: 6340,v 5.1 1995/11/17 15:56:19 pepsa Exp $ ! 6340.prop - Ray Lucas - 10/24/95 ! Modified to use flanking fields referencing new HDF center field position ! on 11/14/95 - RAL. ! ! Hubble Space Telescope Cycle 5 (1995) Phase II Proposal Template ! ! 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: Brett Blacker ! Phone: 410 338-1281 , E-mail: blacker@stsci.edu ! ! This partially completed template was generated from a Phase I proposal. ! Date generated: Sun Dec 18 09:50:22 EST 1994 ! Proposal_Information ! Section 4 Title: The HDF Experiments: Flanking Fields Proposal_Category: GO/DD Scientific_Category: Galaxies & Clusters Cycle: 5 Investigators PI_name: Robert E. Williams PI_Institution: Space Telescope Science Institute CoI_Name: Mark Dickinson CoI_Institution: Space Telescope Science Institute Contact: ! Y or N (designate at most one contact) CoI_Name: Harry Ferguson CoI_Institution: Space Telescope Science Institute Contact: Y ! Y or N (designate at most one contact) CoI_Name: Andrew Fruchter CoI_Institution: Space Telescope Science Institute Contact: ! Y or N (designate at most one contact) CoI_Name: Mauro Giavalisco CoI_Institution: Space Telescope Science Institute Contact: ! Y or N (designate at most one contact) CoI_Name: Ron Gilliland CoI_Institution: Space Telescope Science Institute Contact: CoI_Name: Ray Lucas CoI_Institution: Space Telescope Science Institute Contact: ! Y or N (designate at most one contact) CoI_Name: Doug McElroy CoI_Institution: Space Telescope Science Institute Contact: ! Y or N (designate at most one contact) CoI_Name: Larry Petro CoI_Institution: Space Telescope Science Institute Contact: CoI_Name: Marc Postman CoI_Institution: Space Telescope Science Institute Contact: ! Y or N (designate at most one contact) Abstract: ! Free format text (please update) The HDF experiment consists of WFPC2 imaging through the F300W, F450W, F606W, and F814W passbands of one selected field of the sky for 150 orbits of CVZ time. The program will provide multi-wavelength data of unprecedented depth on morphology and spectral energy distribution of faint field galaxies. This proposal consists of ten orbits of observations of flanking fields adjacent to the central HDF field designed primarily for the benefit of ground-based long-slit spectroscopy and for possible follow-up with future HST instruments such as the Advanced Camera, etc. We will use only the F814W passband in this flanking fields program. There are 8 flanking fields, two on either side of the deep field thus forming a strip on the sky, plus two above and two below which allow more flexibility in the angles chosen by ground-based observers for long-slit spectroscopy as well as increasing the area covered for possible follow-up with the Advanced Camera and/or other instruments. The two flanking fields that are in the strip adjacent to the central HDF field will have two orbits of exposures each, with all the rest having a single orbit. Questions ! Free format text (please update) Observing_Description: The HDF observations consist of WFPC2 imaging of the field towards 1236+6213 in the Ursa Major constellation. "Flanking fields" are being observed in order to more greatly benefit observers doing long-slit spectroscopy from the ground, as well as to provide a basis for more possible follow-up work with the Advanced Camera and other possible future instruments. There are 10 non-CVZ orbits dedicated to this flanking fields project. The overall pattern of the mosaic of flanking fields is comprised of a strip with the "deep" HDF field in the center and two fields in a line on either side of it, each aligned such that the outer corner of WF3 fits over the PC1 field of view and is nestled in the inner corner of the WFPC2 chevron pattern of the field just to the east of it. Just above and below the central "deep" field, there are four more fields aligned the same way, two overlapping the two outer edges of the "deep" field chip 2 on the North, and two overlapping the two outer edges of the "deep" field chip 4 on the South. The fields' coordinates are chosen so as to produce an overlap of ~4 arc seconds between adjacent fields. The two inner fields that are adjacent to the central "deep" field will be done in a total of 4 orbits (2 orbits per field, 2 exposures each ) while all the other 6 fields will be done in 6 orbits, 1 orbit per field, and 3 exposures per orbit. These should be sufficient for basic cosmic ray rejection. We are not dithering in the observations of these flanking fields but will instead rely on DARKs for dealing with the hot pixels, etc. All the flanking field exposures are to be done in the F814W filter. All of the flanking field exposures should be done at the SAME ORIENT ( nominally U3=292.0D ) as the central "deep" field so that the extended mosaic of flanking fields is aligned properly and the overlap is preserved among all the adjacent fields. Note that we have NOT attempted to tweak the overlap and roll and target positions of the flanking fields such that the alignment of CCD columns and rows is preserved across the entire mosaic as it was felt not to be a crucial factor by the HDF working group. We have merely requested that all be done at the SAME ORIENT as the central HDF ( U3=292.0D ) so that the overall pattern of desired field coverage for ground-based long slit spectroscopy and possible imaging by the HST Advanced Camera and other instruments is preserved. Each flanking field is in its own separate visit, so therefore all visits should be done at the SAME ORIENT as that used for the central "deep" field. The GROUP 1-8 WITHIN 7D requirement may be relaxed for scheduling purposes so long as the SAME ORIENT is preserved for all, and all are done in a close enough time period to achieve the SAME ORIENT as the central deep field within a reasonably short amount of time, e.g. not a year later, but within days or weeks of the central HDF if possible. Real_Time_Justification: None. Calibration_Justification: ! Move appropriate text from Real_Time_Justification Additional_Comments: Fixed_Targets ! Section 5.1 Target_Number: 1 Target_Name: HDF-123635+621339 Alternate_Names: HDF-FLANK-STRIP-INNER-WEST Description: UNIDENTIFIED, Blank Field, High Latitude Field, GALAXY, High Z Gal, Protogalaxy Position: RA=12H 36M 35.17S +/- 0.01S, ! Most common specification format is DEC=+62D 13' 38.7" +/- 0.1" ! ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: Z = 3.4 RA_PM: ! Units are seconds of time per year Dec_PM: ! Units are seconds of arc per year Epoch: Annual_Parallax: Flux: U-V = 36.0 E-1, V-R = 30.0 E-2, ! Include at least V and B-V U = 28, V = 30, I = 30, U-V = 25.0 E-1, V-R = 5.0 E-1, Comments: High galactic latitude field with b~55D. Extinction is virtually zero, with E(B-V)=0.0000 There are no bright stars in this field. The brightest object in the field has V~19. Target_Number: 2 Target_Name: HDF-123621+621419 Alternate_Names: HDF-FLANK-STRIP-OUTER-WEST Description: UNIDENTIFIED, Blank Field, High Latitude Field, GALAXY, High Z Gal, Protogalaxy Position: RA=12H 36M 20.93S +/- 0.01S, ! Most common specification format is DEC=+62D 14' 19.3" +/- 0.1" ! ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: Z = 3.4 RA_PM: ! Units are seconds of time per year Dec_PM: ! Units are seconds of arc per year Epoch: Annual_Parallax: Flux: U-V = 36.0 E-1, V-R = 30.0 E-2, ! Include at least V and B-V U = 28, V = 30, I = 30, U-V = 25.0 E-1, V-R = 5.0 E-1, Comments: High galactic latitude field with b~55D. Extinction is virtually zero, with E(B-V)=0.0000 There are no bright stars in this field. The brightest object in the field has V~19. Target_Number: 3 Target_Name: HDF-123704+621217 Alternate_Names: HDF-FLANK-STRIP-INNER-EAST Description: UNIDENTIFIED, Blank Field, High Latitude Field, GALAXY, High Z Gal, Protogalaxy Position: RA=12H 37M 03.62S +/- 0.01S, ! Most common specification format is DEC=+62D 12' 17.2" +/- 0.1" ! ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: Z = 3.4 RA_PM: ! Units are seconds of time per year Dec_PM: ! Units are seconds of arc per year Epoch: Annual_Parallax: Flux: U-V = 36.0 E-1, V-R = 30.0 E-2, ! Include at least V and B-V U = 28, V = 30, I = 30, U-V = 25.0 E-1, V-R = 5.0 E-1, Comments: High galactic latitude field with b~55D. Extinction is virtually zero, with E(B-V)=0.0000 There is a somewhat brighter star on WF3. Magnitude and color are unknown at present. It is the same star that is just off the PC1 field of view in the adjacent HDF-FLANK-STRIP-OUTER-EAST field. It is unknown at present whether this star will saturate and/or cause the WF3 CCD to bleed. Target_Number: 4 Target_Name: HDF-123718+621136 Alternate_Names: HDF-FLANK-STRIP-OUTER-EAST Description: UNIDENTIFIED, Blank Field, High Latitude Field, GALAXY, High Z Gal, Protogalaxy Position: RA=12H 37M 17.83S +/- 0.01S, ! Most common specification format is DEC=+62D 11' 36.3" +/- 0.1" ! ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: Z = 3.4 RA_PM: ! Units are seconds of time per year Dec_PM: ! Units are seconds of arc per year Epoch: Annual_Parallax: Flux: U-V = 36.0 E-1, V-R = 30.0 E-2, ! Include at least V and B-V U = 28, V = 30, I = 30, U-V = 25.0 E-1, V-R = 5.0 E-1, Comments: High galactic latitude field with b~55D. Extinction is virtually zero, with E(B-V)=0.0000 There is a somewhat brighter galaxy on WF2, and a somewhat brighter star just off the PC1 field of view. Magnitudes and colors for both are unknown at present. The star is the same star that is on WF3 in the adjacent HDF-FLANK-STRIP-INNER-EAST field. This bright star may cause some reflection or ghosts in the images of this field. Target_Number: 5 Target_Name: HDF-123651+621548 Alternate_Names: HDF-FLANK-NORTHWEST Description: UNIDENTIFIED, Blank Field, High Latitude Field, GALAXY, High Z Gal, Protogalaxy Position: RA=12H 36M 51.03S +/- 0.01S, ! Most common specification format is DEC=+62D 15' 47.6" +/- 0.1" ! ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: Z = 3.4 RA_PM: ! Units are seconds of time per year Dec_PM: ! Units are seconds of arc per year Epoch: Annual_Parallax: Flux: U-V = 36.0 E-1, V-R = 30.0 E-2, ! Include at least V and B-V U = 28, V = 30, I = 30, U-V = 25.0 E-1, V-R = 5.0 E-1, Comments: High galactic latitude field with b~55D. Extinction is virtually zero, with E(B-V)=0.0000 There are no bright stars in this field. The brightest object in the field has V~19. Target_Number: 6 Target_Name: HDF-123705+621507 Alternate_Names: HDF-FLANK-NORTHEAST Description: UNIDENTIFIED, Blank Field, High Latitude Field, GALAXY, High Z Gal, Protogalaxy Position: RA=12H 37M 05.27S +/- 0.01S, ! Most common specification format is DEC=+62D 15' 06.8" +/- 0.1" ! ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: Z = 3.4 RA_PM: ! Units are seconds of time per year Dec_PM: ! Units are seconds of arc per year Epoch: Annual_Parallax: Flux: U-V = 36.0 E-1, V-R = 30.0 E-2, ! Include at least V and B-V U = 28, V = 30, I = 30, U-V = 25.0 E-1, V-R = 5.0 E-1, Comments: High galactic latitude field with b~55D. Extinction is virtually zero, with E(B-V)=0.0000 There are no bright stars in this field. The brightest object in the field has V~19. Target_Number: 7 Target_Name: HDF-123648+621008 Alternate_Names: HDF-FLANK-SOUTHEAST Description: UNIDENTIFIED, Blank Field, High Latitude Field, GALAXY, High Z Gal, Protogalaxy Position: RA=12H 36M 47.77S +/- 0.01S, ! Most common specification format is DEC=+62D 10' 08.4" +/- 0.1" ! ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: Z = 3.4 RA_PM: ! Units are seconds of time per year Dec_PM: ! Units are seconds of arc per year Epoch: Annual_Parallax: Flux: U-V = 36.0 E-1, V-R = 30.0 E-2, ! Include at least V and B-V U = 28, V = 30, I = 30, U-V = 25.0 E-1, V-R = 5.0 E-1, Comments: High galactic latitude field with b~55D. Extinction is virtually zero, with E(B-V)=0.0000 There are no bright stars in this field. The brightest object in the field has V~19. Target_Number: 8 Target_Name: HDF-123634+621049 Alternate_Names: HDF-FLANK-SOUTHWEST Description: UNIDENTIFIED, Blank Field, High Latitude Field, GALAXY, High Z Gal, Protogalaxy Position: RA=12H 36M 33.56S +/- 0.01S, ! Most common specification format is DEC=+62D 10' 49.1" +/- 0.1" ! ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: Z = 3.4 RA_PM: ! Units are seconds of time per year Dec_PM: ! Units are seconds of arc per year Epoch: Annual_Parallax: Flux: U-V = 36.0 E-1, V-R = 30.0 E-2, ! Include at least V and B-V U = 28, V = 30, I = 30, U-V = 25.0 E-1, V-R = 5.0 E-1, Comments: High galactic latitude field with b~55D. Extinction is virtually zero, with E(B-V)=0.0000 There are no bright stars in this field. The brightest object in the field has V~19. ! This is a template for a single visit containing a single exposure ! Repeat exposure and visit blocks as needed Visits ! Section 6 Visit_Number: 01 Visit_Requirements: ORIENT 291.0D TO 293.0D ! Section 7.1 GROUP 1-8 WITHIN 7D On_Hold_Comments: Visit_Comments: Do two orbits of two exposures each in this visit. All should be done at the SAME POSition. Please do at SAME ORIENT as the HDF central (deep) field, which is nominally at U3 ORIENT 292.0D, exactly in the middle of the range specified here. Do all flanking fields at the SAME ORIENT as the central HDF exposures, and consequently do all flanking fields at the SAME ORIENT AS 1 in order to provide a mosaic of contiguous fields for long-slit spectroscopy, etc. GROUP WITHIN requirement may be relaxed as needed for scheduling as long as SAME ORIENT is maintained. Exposure_Number: 01 ! Section 6.5 Target_Name: HDF-123635+621339 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1300S Special_Requirements: EXPAND ! Section 7.2 MIN DUR 1100S MAX DUR 3000S Comments: Exposure_Number: 02 ! Section 6.5 Target_Name: HDF-123635+621339 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1400S Special_Requirements: SAME POS AS 1 ! Section 7.2 EXPAND MIN DUR 1100S MAX DUR 3000S END ORBIT Comments: Exposure_Number: 3 Target_Name: DARK Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: DEF Wavelength: Number_of_Iterations: 1 Time_Per_Exposure: 1800s Optional_Parameters: CR-SPLIT=NO Special_Requirements: Comments: Exposure_Number: 04 ! Section 6.5 Target_Name: HDF-123635+621339 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1300S Special_Requirements: SAME POS AS 1 ! Section 7.2 EXPAND MIN DUR 1100S MAX DUR 3000S Comments: Exposure_Number: 05 ! Section 6.5 Target_Name: HDF-123635+621339 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1400S Special_Requirements: SAME POS AS 1 ! Section 7.2 EXPAND MIN DUR 1100S MAX DUR 3000S END ORBIT Comments: Exposure_Number: 6 Target_Name: DARK Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: DEF Wavelength: Number_of_Iterations: 1 Time_Per_Exposure: 1800s Optional_Parameters: CR-SPLIT=NO Special_Requirements: Comments: Visit_Number: 02 Visit_Requirements: SAME ORIENT AS 1 ! Section 7.1 On_Hold_Comments: Visit_Comments: Do all 3 exposures in a single orbit. Please do at SAME ORIENT as the HDF central (deep) field, which is nominally at U3 ORIENT 292.0D, exactly in the middle of the range specified here. Do all flanking fields at the SAME ORIENT as the central HDF exposures, and consequently do all flanking fields at the SAME ORIENT AS 1 in order to provide a mosaic of contiguous fields for long-slit spectroscopy, etc. GROUP WITHIN requirement may be relaxed as needed for scheduling as long as SAME ORIENT is maintained. Exposure_Number: 05 ! Section 6.5 Target_Name: HDF-123621+621419 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 800S Special_Requirements: EXPAND ! Section 7.2 MIN DUR 600S MAX DUR 1000S Comments: Exposure_Number: 06 ! Section 6.5 Target_Name: HDF-123621+621419 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 800S Special_Requirements: SAME POS AS 5 ! Section 7.2 EXPAND MIN DUR 600S MAX DUR 1000S Comments: Exposure_Number: 07 ! Section 6.5 Target_Name: HDF-123621+621419 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 900S Special_Requirements: SAME POS AS 5 ! Section 7.2 EXPAND MIN DUR 600S MAX DUR 1000S END ORBIT Comments: Exposure_Number: 8 Target_Name: DARK Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: DEF Wavelength: Number_of_Iterations: 1 Time_Per_Exposure: 1800s Optional_Parameters: CR-SPLIT=NO Special_Requirements: Comments: Visit_Number: 03 Visit_Requirements: SAME ORIENT AS 1 ! Section 7.1 On_Hold_Comments: Visit_Comments: Do two orbits of two exposures each in this visit. All should be done at the SAME POSition. Please do at SAME ORIENT as the HDF central (deep) field, which is nominally at U3 ORIENT 292.0D, exactly in the middle of the range specified here. Do all flanking fields at the SAME ORIENT as the central HDF exposures, and consequently do all flanking fields at the SAME ORIENT AS 1 in order to provide a mosaic of contiguous fields for long-slit spectroscopy, etc. GROUP WITHIN requirement may be relaxed as needed for scheduling as long as SAME ORIENT is maintained. Exposure_Number: 08 ! Section 6.5 Target_Name: HDF-123704+621217 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1300S Special_Requirements: EXPAND ! Section 7.2 MIN DUR 1100S MAX DUR 3000S Comments: Exposure_Number: 09 ! Section 6.5 Target_Name: HDF-123704+621217 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1400S Special_Requirements: SAME POS AS 8 ! Section 7.2 EXPAND MIN DUR 1100S MAX DUR 3000S END ORBIT Comments: Exposure_Number: 10 Target_Name: DARK Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: DEF Wavelength: Number_of_Iterations: 1 Time_Per_Exposure: 1800s Optional_Parameters: CR-SPLIT=NO Special_Requirements: Comments: Exposure_Number: 11 ! Section 6.5 Target_Name: HDF-123704+621217 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1300S Special_Requirements: SAME POS AS 8 ! Section 7.2 EXPAND MIN DUR 1100S MAX DUR 3000S Comments: Exposure_Number: 12 ! Section 6.5 Target_Name: HDF-123704+621217 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1400S Special_Requirements: SAME POS AS 8 ! Section 7.2 EXPAND MIN DUR 1100S MAX DUR 3000S END ORBIT Comments: Exposure_Number: 13 Target_Name: DARK Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: DEF Wavelength: Number_of_Iterations: 1 Time_Per_Exposure: 1800s Optional_Parameters: CR-SPLIT=NO Special_Requirements: Comments: Visit_Number: 04 Visit_Requirements: SAME ORIENT AS 1 ! Section 7.1 On_Hold_Comments: Visit_Comments: Do all 3 exposures in a single orbit. Please do at SAME ORIENT as the HDF central (deep) field, which is nominally at U3 ORIENT 292.0D, exactly in the middle of the range specified here. Do all flanking fields at the SAME ORIENT as the central HDF exposures, and consequently do all flanking fields at the SAME ORIENT AS 1 in order to provide a mosaic of contiguous fields for long-slit spectroscopy, etc. GROUP WITHIN requirement may be relaxed as needed for scheduling as long as SAME ORIENT is maintained. Exposure_Number: 12 ! Section 6.5 Target_Name: HDF-123718+621136 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 800S Special_Requirements: EXPAND ! Section 7.2 MIN DUR 600S MAX DUR 1000S Comments: Exposure_Number: 13 ! Section 6.5 Target_Name: HDF-123718+621136 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 800S Special_Requirements: SAME POS AS 12 ! Section 7.2 EXPAND MIN DUR 600S MAX DUR 1000S Comments: Exposure_Number: 14 Target_Name: DARK Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: DEF Wavelength: Number_of_Iterations: 1 Time_Per_Exposure: 1800s Optional_Parameters: CR-SPLIT=NO Special_Requirements: Comments: Exposure_Number: 15 ! Section 6.5 Target_Name: HDF-123718+621136 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 900S Special_Requirements: SAME POS AS 12 ! Section 7.2 EXPAND MIN DUR 600S MAX DUR 1000S END ORBIT Comments: Exposure_Number: 16 Target_Name: DARK Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: DEF Wavelength: Number_of_Iterations: 1 Time_Per_Exposure: 1800s Optional_Parameters: CR-SPLIT=NO Special_Requirements: Comments: Visit_Number: 05 Visit_Requirements: SAME ORIENT AS 1 ! Section 7.1 On_Hold_Comments: Visit_Comments: Do all 3 exposures in a single orbit. Please do at SAME ORIENT as the HDF central (deep) field, which is nominally at U3 ORIENT 292.0D, exactly in the middle of the range specified here. Do all flanking fields at the SAME ORIENT as the central HDF exposures, and consequently do all flanking fields at the SAME ORIENT AS 1 in order to provide a mosaic of contiguous fields for long-slit spectroscopy, etc. GROUP WITHIN requirement may be relaxed as needed for scheduling as long as SAME ORIENT is maintained. Exposure_Number: 15 ! Section 6.5 Target_Name: HDF-123651+621548 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 800S Special_Requirements: EXPAND ! Section 7.2 MIN DUR 600S MAX DUR 1000S Comments: Exposure_Number: 16 ! Section 6.5 Target_Name: HDF-123651+621548 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 800S Special_Requirements: SAME POS AS 15 ! Section 7.2 EXPAND MIN DUR 600S MAX DUR 1000S Comments: Exposure_Number: 17 ! Section 6.5 Target_Name: HDF-123651+621548 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 900S Special_Requirements: SAME POS AS 15 ! Section 7.2 EXPAND MIN DUR 600S MAX DUR 1000S END ORBIT Comments: Exposure_Number: 18 Target_Name: DARK Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: DEF Wavelength: Number_of_Iterations: 1 Time_Per_Exposure: 1800s Optional_Parameters: CR-SPLIT=NO Special_Requirements: Comments: Visit_Number: 06 Visit_Requirements: SAME ORIENT AS 1 ! Section 7.1 On_Hold_Comments: Visit_Comments: Do all 3 exposures in a single orbit. Please do at SAME ORIENT as the HDF central (deep) field, which is nominally at U3 ORIENT 292.0D, exactly in the middle of the range specified here. Do all flanking fields at the SAME ORIENT as the central HDF exposures, and consequently do all flanking fields at the SAME ORIENT AS 1 in order to provide a mosaic of contiguous fields for long-slit spectroscopy, etc. GROUP WITHIN requirement may be relaxed as needed for scheduling as long as SAME ORIENT is maintained. Exposure_Number: 18 ! Section 6.5 Target_Name: HDF-123705+621507 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 800S Special_Requirements: EXPAND ! Section 7.2 MIN DUR 600S MAX DUR 1000S Comments: Exposure_Number: 19 ! Section 6.5 Target_Name: HDF-123705+621507 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 800S Special_Requirements: SAME POS AS 18 ! Section 7.2 EXPAND MIN DUR 600S MAX DUR 1000S Comments: Exposure_Number: 20 ! Section 6.5 Target_Name: HDF-123705+621507 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 900S Special_Requirements: SAME POS AS 18 ! Section 7.2 EXPAND MIN DUR 600S MAX DUR 1000S END ORBIT Comments: Exposure_Number: 21 Target_Name: DARK Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: DEF Wavelength: Number_of_Iterations: 1 Time_Per_Exposure: 1800s Optional_Parameters: CR-SPLIT=NO Special_Requirements: Comments: Visit_Number: 07 Visit_Requirements: SAME ORIENT AS 1 ! Section 7.1 On_Hold_Comments: Visit_Comments: Do all 3 exposures in a single orbit. Please do at SAME ORIENT as the HDF central (deep) field, which is nominally at U3 ORIENT 292.0D, exactly in the middle of the range specified here. Do all flanking fields at the SAME ORIENT as the central HDF exposures, and consequently do all flanking fields at the SAME ORIENT AS 1 in order to provide a mosaic of contiguous fields for long-slit spectroscopy, etc. GROUP WITHIN requirement may be relaxed as needed for scheduling as long as SAME ORIENT is maintained. Exposure_Number: 21 ! Section 6.5 Target_Name: HDF-123648+621008 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 800S Special_Requirements: EXPAND ! Section 7.2 MIN DUR 600S MAX DUR 1000S Comments: Exposure_Number: 22 ! Section 6.5 Target_Name: HDF-123648+621008 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 800S Special_Requirements: SAME POS AS 21 ! Section 7.2 EXPAND MIN DUR 600S MAX DUR 1000S Comments: Exposure_Number: 23 ! Section 6.5 Target_Name: HDF-123648+621008 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 900S Special_Requirements: SAME POS AS 21 ! Section 7.2 EXPAND MIN DUR 600S MAX DUR 1000S END ORBIT Comments: Exposure_Number: 24 Target_Name: DARK Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: DEF Wavelength: Number_of_Iterations: 1 Time_Per_Exposure: 1800s Optional_Parameters: CR-SPLIT=NO Special_Requirements: Comments: Visit_Number: 08 Visit_Requirements: SAME ORIENT AS 1 ! Section 7.1 On_Hold_Comments: Visit_Comments: Do all 3 exposures in a single orbit. Please do at SAME ORIENT as the HDF central (deep) field, which is nominally at U3 ORIENT 292.0D, exactly in the middle of the range specified here. Do all flanking fields at the SAME ORIENT as the central HDF exposures, and consequently do all flanking fields at the SAME ORIENT AS 1 in order to provide a mosaic of contiguous fields for long-slit spectroscopy, etc. GROUP WITHIN requirement may be relaxed as needed for scheduling as long as SAME ORIENT is maintained. Exposure_Number: 24 ! Section 6.5 Target_Name: HDF-123634+621049 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 800S Special_Requirements: EXPAND ! Section 7.2 MIN DUR 600S MAX DUR 1000S Comments: Exposure_Number: 25 ! Section 6.5 Target_Name: HDF-123634+621049 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 800S Special_Requirements: SAME POS AS 24 ! Section 7.2 EXPAND MIN DUR 600S MAX DUR 1000S Comments: Exposure_Number: 26 ! Section 6.5 Target_Name: HDF-123634+621049 Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: F814W Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 900S Special_Requirements: SAME POS AS 24 ! Section 7.2 EXPAND MIN DUR 600S MAX DUR 1000S END ORBIT Comments: Exposure_Number: 27 Target_Name: DARK Config: WFPC2 Opmode: IMAGE Aperture: WFALL-FIX Sp_Element: DEF Wavelength: Number_of_Iterations: 1 Time_Per_Exposure: 1800s Optional_Parameters: CR-SPLIT=NO Special_Requirements: 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: Henry Ferguson ! STScI, 3700 San Martin Drive Baltimore, MD 21218 Ship_Via: Hand deliver ! UPS (2-day) or OVERNIGHT ! Overnight shipping done at PI expense Recipient_Email: ferguson@stsci.edu ! ! ! Let us know what you think of this template and software! ! Please send a list of your likes and dislikes to your Program Coordinator.