! Hubble Space Telescope Cycle 5 (1995) Phase II Proposal Template ! $Id: 6254,v 3.1 1995/06/15 14:56:13 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: Doug Van Orsow ! Phone: 410 338-4568 , E-mail: vanorsow@stsci.edu ! ! This partially completed template was generated from a Phase I proposal. ! Name of Phase I Proposal: griffiths-915.prop ! Date generated: Sun Dec 18 09:52:02 EST 1994 ! Proposal_Information ! Section 4 Title: GTO PURE PARALLEL PROGRAM - CYCLE 5 Proposal_Category: GTO/OS Scientific_Category: Galaxies & Clusters Cycle: 5 Investigators PI_name: Edward J. Groth PI_Institution: Princeton University CoI_Name: ROBERT BLESS CoI_Institution: UNIVERSITY OF WISCONSIN Contact: ! Y or N (designate at most one contact) CoI_Name: JOHN BRANDT CoI_Institution: UNIVERSITY OF COLORADO Contact: ! Y or N (designate at most one contact) CoI_Name: RICHARD HARMS CoI_Institution: APPLIED RESEARCH CORPORATION Contact: ! Y or N (designate at most one contact) CoI_Name: WILLIAM JEFFERYS CoI_Institution: UNIVERSITY OF TEXAS Contact: ! Y or N (designate at most one contact) CoI_Name: F MACCHETTO CoI_Institution: SPACE TELESCOPE SCIENCE INSTITUTE Contact: ! Y or N (designate at most one contact) CoI_Name: C O'DELL CoI_Institution: RICE UNIVERSITY Contact: ! Y or N (designate at most one contact) CoI_Name: JOHN TRAUGER CoI_Institution: JPL Contact: ! Y or N (designate at most one contact) CoI_Name: JAMES WESTPHAL CoI_Institution: CALIFORNIA INSTITUTE OF TECHNOLOGY Contact: ! Y or N (designate at most one contact) Abstract: ! Free format text (please update) The parallel program described here provides a random sample of galaxies in a large number of high latitude fields. Galactic star counts and the structure of the galactic halo will also be studied. The proposed exposures utilize the WFPC2 in parallel mode when another instrument is prime at high galactic latitude. The expectation is that these fields will represent a fair sample of the universe and the Galactic halo. This is a continuation of proposal 4849 into cycle 4. It is more or less identical except cycle 4 => cycle 5. Questions ! Free format text (please update) Observing_Description: A set of sequences is constructed to fit within exposure opportunities of varying lengths, beginning with single orbit exposures. On long exposure opportunities, the aim is to obtain very deep images of galaxies by concentrating on the F814W and F606W filters. This is a parallel program designed to increase the scientific productivity of the HST by acquiring data relevant for studying distant galaxies and the Galactic halo when the HST is busy but the WFPC is not. The exposure time is determined by the primary exposure time and the ability of the planning and scheduling system to match parallel exposures to primary exposures. Enough exposures are included to provide good chances for matches. Real_Time_Justification: Calibration_Justification: ! Move appropriate text from Real_Time_Justification Additional_Comments: Generic_Targets ! Section 5.3 Target_Number:1 Target_Name:PAR Description:CLUSTER OF GALAXIES Criteria:ABS_BII > 10D Flux: Comments: ! 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: ! 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 ! ORIENTation TO ! ORIENTation TO FROM ! ORIENTation TO FROM NOMINAL ! SAME ORIENTation AS ! CVZ PARallel ! AFTER [BY [TO ]] ! AFTER ! BEFORE ! BETWEEN AND ! GROUP WITHIN