! Proposal 6632, submission 1
! PI: George Miley
! Received Thu Feb 15 06:49:08 EST 1996
! From: miley@strw.LeidenUniv.nl
! Hubble Space Telescope Cycle 6 (1996) Phase II Proposal Template
! $Id: 6632,v 4.1 1997/01/09 21:14:29 pepsa Exp $
! Hubble Space Telescope Cycle 6 (1996) Phase II Proposal Template
! $Id: 6632,v 4.1 1997/01/09 21:14:29 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: Lucas
! Phone: 410-338-4716 , E-mail: lucas@stsci.edu
!
! This partially completed template was generated from a Phase I proposal.
! Name of Phase I Proposal: archive-0619.miley.prop
! Date generated: Fri Dec 22 16:34:51 EST 1995
!
Proposal_Information ! Section 4
Title: MORPHOLOGIES OF HIGH--REDSHIFT RADIO
GALAXIES
Proposal_Category: GO
Scientific_Category: COSMOLOGY
Cycle: 6
Investigators
PI_name: George Miley
PI_Institution: Leiden Observatory
CoI_Name: Patrick McCarthy
CoI_Institution: Observatories of the CIW
Contact: ! Y or N (designate at most one contact)
CoI_Name: Wil van Breugel
CoI_Institution: Lawrence Livermore National Lab
Contact: ! Y or N (designate at most one contact)
CoI_Name: Hyron Spinrad
CoI_Institution: University of California, Berkeley
Contact: ! Y or N (designate at most one contact)
CoI_Name: Huub Rottgering
CoI_Institution: Leiden Observatory
Contact: ! Y or N (designate at most one contact)
CoI_Name: Rob van Ojik
CoI_Institution: Leiden Observatory
Contact: ! Y or N (designate at most one contact)
CoI_Name: Laura Pentericci
CoI_Institution: Leiden Observatory
Contact: ! Y or N (designate at most one contact)
CoI_Name: Duccio Macchetto
CoI_Institution: Space Telescope Science Institute
Contact: ! Y or N (designate at most one contact)
Abstract: ! Free format text (please update)
We propose to continue our study of the continuum and Ly Alpha
morphologies of 20 high--redshift radio galaxies begun in
Cycle 5. Our sample was chosen from 50 candidates to be bright
in both continuum and Ly Alpha. The observations would
elucidate sub-kiloparsec-scale structures in the target
galaxies, allowing study of their alignment and relationships
to the associated radio sources. Of particular interest is a
comparison between the HST clumpiness and the recently
discovered spatially-extended absorption systems in the Ly
Alpha profiles., During Cycle 5 we were allocated time to
begin the project, with 8 broad-band targets and 3 Ly Alpha
LRF test images. The first of these observations show that (i)
features of which are difficult to explain by a single simple
scattering or starburst model, (ii) a variety of different
morphologies, which provide compelling arguments that imaging
a larger sample is essential for understanding the processes
involved, (iii) our exposure times are well chosen to
delineate the morphologies, both in the continuum and Ly
Alpha. The images will also be used to provide the most
interesting targets for a followup spectroscopic and kinematic
study with STIS., The project is providing unique information
relevant to the formation and evolution of radio galaxies, to
relationships between galaxy and quasar activity and to
physical conditions in the early Universe.
Questions ! Free format text (please update)
Observing_Description:
noindent Need for Extension of Sample. At the end of Cycle 5
we will have imaged 8 objects in continuum and 3 in Ly Alpha.
The diversity in morphologies coupled with the need to
disentangle the many effects and various parameters discussed
above provide compelling arguments for imaging a sizeable
sample of distant radio galaxies with the HST, both in the
continuum and in Ly Alpha. Imaging such a sample is also
essential to make most efficient use of future HST time. Here
we propose completing our sample of 20 objects in the
continuum and 10 in Ly Alpha. Our proposed observations can
be used to enable the most interesting targets to be selected
for a followup spectroscopic and kinematic study with STIS
and deep imaging with WFPC2, NIC and the AC. , , noindent
Continuum Imaging. We shall carry out continuum imaging of 5
out of our
sample of 20 radio galaxies known to have z > 2, R -
magnitude < 23.5 and Ly Alpha fluxes > 10^ -15 erg s^ -1cm^
-2 . Two of the 5 targets have already been observed in Cycle 5
but need deeper observations (5 and 6 orbits each respectively)
and 3 of the targets are new and will be observed each for 2
orbits. Our choice of filter is dictated by three criteria.
First bright lines (Ly Alpha) should be excluded from the
pass band. Second, the filters should result in as large as
possible detected light signal. Third, the rest-wavelengths
should be as similar as possible over the redshift range. As
a reasonable compromise between these criteria, we shall
observe all z < 2.9 galaxies through F606W, the most
efficient filter. For the z > 2.9 radio galaxies, Ly Alpha
contamination will be avoided by observing through F702W. ,
* The PC is preferable as a detector than the WFC. Although
the signal per pixel will be smaller for the PC, averaging
the signal over 4.7 pixels should result in similar sampling
to the WFC with very slightly degraded signal to noise.
However, we regard the additional spatial resolution provided
by the better sampling as a significant advantage. Our
targets are all small compared with the field of the PC. , *
We request an average of two orbits per target for the
continuum imaging. First results of our Cycle 5 observations
show that this exposure time for the broad-band imaging is
sufficient to delineate the main features of the continuum
morphologies. This choice was based on the following
considerations. Our Cycle 1 (aberrated) exposures were each
of length about 6 x 30m. Both 4C 41.17 and 4C 28.58
contained two or more 0.1" clumps, each of which produced
more than 10\% of the total flux from these galaxies (less
than 2.5 magnitudes fainter than the integrated galaxy
magnitudes). Assume that all the targets have similar ratios
of flux in clumpy structures and that we wish to observe
galaxies down to integrated R-magnitudes < 23.5 (1.5
magnitudes fainter than 4C 41.17). For a 40m minute exposure
through the F606W filter with PC1, a 26th mag clump will
produce 564 electrons per 0.1" by 0.1" PSF (60\% of the
energy is intercepted within this area). The resultant signal
-to-noise per PSF after 2 orbits is about 25. Most of the
targets are 0.5 to 1.5 mag brighter than R = 23.5., ,
Real_Time_Justification:
The project is part of a comprehensive study into the nature
of distant galaxies, involving ground-based optical (incl.
Keck), infrared and radio imaging and optical and IR
spectroscopy. Our proposal builds on several years of
preparatory ground-based programs. We have access to a huge
body of relevant data including:, (i) optical images and
spectra (Kitt Peak, La Silla, Tololo, Las Campanas, Lick, La
Palma), (ii) Ly Alpha spectral profiles with a resolution of
better than 100 km/s. , (iii) 2.2 micron images (UKIRT, Las
Campanas), (iv) radio maps of the total intensity and
polarisations at several frequencies and resolutions (VLA,
MERLIN interferometric array at Jodrell Bank). (e.g. Carilli
et al. 1995). These ground-based data (particularly
comparable resolution radio maps) will be carefully compared
with the HST data. Note that our HST images are comparable in
resolution to the best VLA maps, For the first time they
allow detailed comparisons between radio and optical
morphologies to be made on the kiloparsec scale., (v) We have
a large programme with ISO to search for dust in three of our
proposed targets and we shall complement this with
observations with the SCUBA sub-millimeter bolometer on the
UK/NL JCMT., , Some of us have begun a programme to study the
targets with the Keck Telescope and we intend to follow up
the HST observations spectroscopically with Keck., , One of
us (HR) is involved with WFPC2 observations of a complete
sample of z~ 1 radio galaxies carried out during Cycle 4.
(PI M. Longair). A "low-z" control sample will therefore be
available to allow evolutionary effects to be studied., , Two
of us are (WvB,GM) are involved with WFPC2 imaging of a
similar sample of z > 2 quasars carried out during Cycles 4
and 5. (PI M. Lehnert).
Calibration_Justification: ! Move appropriate text from Real_Time_Justification
Additional_Comments:
Fixed_Targets ! Section 5.1
Target_Number: 1
Target_Name: GAL-1140-26
Alternate_Names:
Description: GALAXY
Position: RA=11H 40M 48.4S +/- 1.0S, ! Most common specification format is
DEC=-26D 29' 08.0" +/- 1.0",
Equinox: J2000
RV_or_Z: Z=2.15
Flux: V=21.4
B-V=0 ! Include at least V and B-V
Comments: FLUXES ARE UNCERTAIN, BUT TARGETS ARE NOT MUCH BRIGHTER.
Target_Number: 2
Target_Name: GAL-2106-24
Alternate_Names:
Description: GALAXY
Position: RA=21H 06M 58.1S +/- 1.0S, ! Most common specification format is
DEC=-24D 05' 11.0" +/- 1.0",
Equinox: J2000
RV_or_Z: Z=2.49
Flux: V=22.5
B-V=0 ! Include at least V and B-V
Comments: FLUXES ARE UNCERTAIN, BUT TARGETS ARE NOT MUCH BRIGHTER.
Target_Number: 3
Target_Name: GAL-1348+24
Alternate_Names: 4C 24.28
Description: GALAXY
Position: RA=13H 48M 14.9S +/- 1.0S, ! Most common specification format is
DEC=+24D 15' 50.0" +/- 1.0",
Equinox: J2000
RV_or_Z: Z=2.91
Flux: V=22.0
B-V=0 ! Include at least V and B-V
Comments: FLUXES ARE UNCERTAIN, BUT TARGETS ARE NOT MUCH BRIGHTER.
Target_Number: 4
Target_Name: GAL-1908+72
Alternate_Names:
Description: GALAXY
Position: RA=19H 08M 23.7S +/- 1.0S, ! Most common specification format is
DEC=+72D 20' 12.0" +/- 1.0",
Equinox: J2000
RV_or_Z: Z=3.54
Flux: V=21.5
B-V=0 ! Include at least V and B-V
Comments: FLUXES ARE UNCERTAIN, BUT TARGETS ARE NOT MUCH BRIGHTER.
Target_Number: 5
Target_Name: GAL-2144+19
Alternate_Names:
Description: GALAXY
Position: RA=21H 44M 07.4S +/- 1.0S, ! Most common specification format is
DEC=+19D 29' 15.0" +/- 1.0",
Equinox: J2000
RV_or_Z: Z=3.59
Flux: V=21.0
B-V=0 ! Include at least V and B-V
Comments: FLUXES ARE UNCERTAIN, BUT TARGETS ARE NOT MUCH BRIGHTER.
! This is a template for a single visit containing a single exposure
! Repeat exposure and visit blocks as needed
Visits ! Section 6
Visit_Number: 1
Visit_Requirements: PCS MODE Fine ! Section 7.1
On_Hold_Comments:
Visit_Comments: DO 2 EXPOSURES IN THIS VISIT, ONE IN EACH OF TWO
CONSECUTIVE ORBITS. BOTH EXPOSURES SHOULD HAVE
THE SAME EXPOSURE TIME UPON LENGTHENING OR SHORTENING,
AND THE SECOND SHOULD BE DITHERED FROM THE FIRST BY
11 PC PIXELS. BOTH EXPOSURES SHOULD BE AT THE EXACT
SAME ORIENT. BOTH EXPOSURES USE CR-SPLIT=NO IN ORDER
TO MAXIMIZE S/N. PCS MODE FINE SHOULD BE USED FOR
BOTH.
Exposure_Number: 1 ! Section 6.5
Target_Name: GAL-1348+24
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F702W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG 0.0,0.0 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT DEFAULT BEST
CENTER OF PC1.
Exposure_Number: 2 ! Section 6.5
Target_Name: GAL-1348+24
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F702W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG 0.506,0.506 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT POSITION
11 PC PIXELS OFF IN X AND Y FROM BEST CENTER
OF PC1.
Visit_Number: 2
Visit_Requirements: PCS MODE Fine ! Section 7.1
On_Hold_Comments:
Visit_Comments: DO 2 EXPOSURES IN THIS VISIT, ONE IN EACH OF TWO
CONSECUTIVE ORBITS. BOTH EXPOSURES SHOULD HAVE
THE SAME EXPOSURE TIME UPON LENGTHENING OR
SHORTENING,
AND THE SECOND SHOULD BE DITHERED FROM THE FIRST BY
11 PC PIXELS. BOTH EXPOSURES SHOULD BE AT THE EXACT
SAME ORIENT. BOTH EXPOSURES USE CR-SPLIT=NO IN ORDER
TO MAXIMIZE S/N. PCS MODE FINE SHOULD BE USED FOR
BOTH.
Exposure_Number: 1 ! Section 6.5
Target_Name: GAL-1908+72
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F702W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG 0.0,0.0 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT DEFAULT BEST
CENTER OF PC1.
Exposure_Number: 2 ! Section 6.5
Target_Name: GAL-1908+72
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F702W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG 0.506,0.506 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT POSITION
11 PC PIXELS OFF IN X AND Y FROM BEST CENTER
OF PC1.
Visit_Number: 3
Visit_Requirements: PCS MODE Fine ! Section 7.1
On_Hold_Comments:
Visit_Comments: DO 2 EXPOSURES IN THIS VISIT, ONE IN EACH OF TWO
CONSECUTIVE ORBITS. BOTH EXPOSURES SHOULD HAVE
THE SAME EXPOSURE TIME UPON LENGTHENING OR
SHORTENING,
AND THE SECOND SHOULD BE DITHERED FROM THE FIRST BY
11 PC PIXELS. BOTH EXPOSURES SHOULD BE AT THE EXACT
SAME ORIENT. BOTH EXPOSURES USE CR-SPLIT=NO IN ORDER
TO MAXIMIZE S/N. PCS MODE FINE SHOULD BE USED FOR
BOTH.
Exposure_Number: 1 ! Section 6.5
Target_Name: GAL-2144+19
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F702W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG 0.0,0.0 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT DEFAULT BEST
CENTER OF PC1.
Exposure_Number: 2 ! Section 6.5
Target_Name: GAL-2144+19
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F702W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG 0.506,0.506 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT POSITION
11 PC PIXELS OFF IN X AND Y FROM BEST CENTER
OF PC1.
Visit_Number: 4
Visit_Requirements: PCS MODE Fine ! Section 7.1
ORIENT 273.801292D TO 273.801292D
On_Hold_Comments:
Visit_Comments: DO 5 EXPOSURES IN THIS VISIT, IN
CONSECUTIVE ORBITS. EXPOSURES SHOULD HAVE
THE SAME EXPOSURE TIME UPON LENGTHENING OR SHORTENING,
AND THEY SHOULD BE DITHERED FROM EACH OTHER BY
11 PC PIXELS. THERE IS ALSO A ZERO-SHIFT IN POSITION
COMPARED WITH CYCLE 5. EXPOSURES SHOULD BE AT THE EXACT
SAME ORIENT AS CYCLE 5. EXPOSURES USE CR-SPLIT=NO IN ORDER
TO MAXIMIZE S/N. PCS MODE FINE SHOULD BE USED.
Exposure_Number: 1 ! Section 6.5
Target_Name: GAL-1140-26
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F606W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG 0.506,0.0 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT DEFAULT BEST
CENTER OF PC1.
Exposure_Number: 2 ! Section 6.5
Target_Name: GAL-1140-26
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F606W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG 0.0,0.506 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT POSITION
11 PC PIXELS OFF IN X AND Y FROM BEST CENTER
OF PC1.
Exposure_Number: 3 ! Section 6.5
Target_Name: GAL-1140-26
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F606W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG -0.506,-0.506 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT DEFAULT BEST
CENTER OF PC1.
Exposure_Number: 4 ! Section 6.5
Target_Name: GAL-1140-26
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F606W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG -0.506,+0.506 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT POSITION
11 PC PIXELS OFF IN X AND Y FROM BEST CENTER
OF PC1.
Exposure_Number: 5 ! Section 6.5
Target_Name: GAL-1140-26
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F606W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG +0.506,-0.506 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT POSITION
11 PC PIXELS OFF IN X AND Y FROM BEST CENTER
OF PC1.
Visit_Number: 5
Visit_Requirements: PCS MODE Fine ! Section 7.1
ORIENT 55.51840D TO 55.51840D
On_Hold_Comments:
Visit_Comments: ORIENT IS CHOSEN TO AVOID DIFFRACTION SPIKES OF
FOREGROUND STAR. HENCE ALLOWABLE ORIENTS ARE ALSO
EVERY 90 DEG FROM THAT SPECIFIED. HENCE,
ORIENT 55D TO 90D
OR ORIENT 145D TO 180D
OR ORIENT 235D TO 270D
OR ORIENT 325D TO 360D
DO 4 EXPOSURES IN THIS VISIT, IN
CONSECUTIVE ORBITS. EXPOSURES SHOULD HAVE
THE SAME EXPOSURE TIME UPON LENGTHENING OR SHORTENING,
AND THEY SHOULD BE DITHERED FROM EACH OTHER BY
11 PC PIXELS. THERE IS ALSO A ZERO-SHIFT IN POSITION
COMPARED TO CYCLE 5. EXPOSURES SHOULD BE AT THE EXACT
SAME ORIENT. EXPOSURES USE CR-SPLIT=NO IN ORDER
TO MAXIMIZE S/N. PCS MOD E FINE SHOULD BE USED.
ORIENT IS CHOSEN TO AVOID DIFFRACTION SPIKES FROM
FOREGROUND STAR. SPECIFIED ABSOLUTE ORIENT IS TO MATCH
THAT OF OUR DATA FROM THE PREVIOUS CYCLE.
Exposure_Number: 1 ! Section 6.5
Target_Name: GAL-2106-24
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F606W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG +0.506,-0.506 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT DEFAULT BEST
CENTER OF PC1.
Exposure_Number: 2 ! Section 6.5
Target_Name: GAL-2106-24
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F606W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG 0.506,0.0 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT POSITION
11 PC PIXELS OFF IN X AND Y FROM BEST CENTER
OF PC1.
Exposure_Number: 3 ! Section 6.5
Target_Name: GAL-2106-24
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F606W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG -0.506,+0.506 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT DEFAULT BEST
CENTER OF PC1.
Exposure_Number: 4 ! Section 6.5
Target_Name: GAL-2106-24
Config: WFPC2
Opmode: IMAGE
Aperture: PC1
Sp_Element: F606W
Wavelength:
Optional_Parameters: CR-SPLIT=NO
Number_of_Iterations: 1
Time_Per_Exposure: 2400S
Special_Requirements: POS TARG -0.506,-0.506 ! Section 7.2
MAX DUR 3000S
MIN DUR 1800S
END ORBIT
Comments: DO SINGLE NON-CR-SPLIT EXPOSURE AT POSITION
11 PC PIXELS OFF IN X AND Y FROM BEST CENTER
OF PC1.
! Visits ! Section 6
! Visit_Number:
!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>
! DROP TO GYRO IF NECESSARY [NO REACQuisition]
! ORIENTation <angle1> TO <angle2>
! ORIENTation <angle1> TO <angle2> FROM <visit>
! ORIENTation <angle1> TO <angle2> FROM NOMINAL
! SAME ORIENTation AS <visit>
! CVZ
! PARallel
! SCHEDulability <percentage>
! 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-list>]
! On_Hold_Comments:
! Visit_Comments:
! Exposure_Number: ! Section 6.5
! Target_Name:
! Config:
! Opmode:
! Aperture:
! Sp_Element:
! Wavelength:
! Optional_Parameters:
!Number_of_Iterations:
! Time_Per_Exposure:
! Special_Requirements: ! Section 7.2
! Uncomment or copy exposure level special requirements needed
! INTeractive ACQuisition FOR <exp-list>
! ONBOARD ACQuisition FOR <exp-list>
! SAVE OFFSET <id>
! USE OFFSET <id>
! 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
! REQuires EPHEMeris CORRection <id>
! END ORBIT
! EXPAND
! LOW-SKY
! MAXimum DURation [<time> | <%>]
! MINimum DURation [<time> | <%>]
! NO SPLIT
! PHASE <number1[0,1]> TO <number2[0,1]>
! SEQuence <exp-list> NON-INTerruptible
! SHADOW
! 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: PI_Address ! STSCI or PI_Address or <free-text>
! PI Address from Phase I is:
!
! Postbus 9513
! NielsBohrweg 2
! Leiden
! NL 2300 RA
!
!
Ship_Via: UPS ! 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