! Proposal 6244, submission 1 ! PI: Michael Jura ! Received Mon Apr 10 13:45:34 EDT 1995 ! From: pi12@stsci.edu ! 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: Dustin Manning, ! Phone: 410/338-4465, E-mail: manning@stsci.edu ! Proposal_Information ! Section 4 Title: HR 4796A: A Possible Protoplanet? Proposal_Category: GTO/HRS Scientific_Category: ! Uncomment one of the following ! AGN ! Cool Stars ! Galaxies & Clusters Hot Stars ! Interstellar Medium ! Quasars ! Solar System ! Stellar Populations Cycle: 5 Investigators PI_Name: Michael Jura PI_Institution: University of California, Los Angeles CoI_Name: Andrea Ghez ! Repeat as often as necessary CoI_Institution: University of California, Los Angeles Contact: N ! Y or N ! (designate at most one contact) Abstract: ! Free format text (clear and concise) HR 4796A is a main sequence A-type star with more circumstellar dust than is located around Beta Pic. We propose to observe and classify HR 4796D, a close, faint, blue companion to HR 4796A. Is HR 4796D a background or foreground star, or is it physically associated with HR 4796A, perhaps a cloud of dust or a protoplanet? Questions ! Free format text (clear and concise) Observing_Description: We propose to use the FOS aboard HST to obtain a spectrum of the unidentified source HR 4796D using the FOS/RD detector with the G570H grating. The plan for target acquisition is to first acquire HR 4796A, a bright (mv = 5.8) nearby A0V star, using the FOS/BL detector with the G190H grating. After centering HR 4796A via a 4 stage Peak/up, an offset will be performed (sep = 4.9", PA = 315D) centering HR 4796D into the 0.5" aperature of the FOS/RD detector. A final PEAK/UP is performed to accurately center HR 4796D, and then the source is observed. The FOS exposure time is set by requiring a minimum SNR of 20, sufficient to identify normal stellar spectral features. Real_Time_Justification: None Calibration_Justification: None Additional_Comments: None Fixed_Targets ! Section 5.1 Target_Number: 1 Target_Name: HR-4796A-OFFSET Alternate_Names: HD109573 Description: STAR, A0-A3 V-IV Position: RA=12H 36M 1.11S +/- 0.1S, DEC=-39D 52' 11.2" +/- 0.2" Equinox: J2000 RV_or_Z: RA_PM: -0.0034 ! Units are seconds of time per year Dec_PM: -0.044 ! Units are seconds of arc per year Epoch: 2000 Annual_Parallax: Flux: V=5.8 +/- 0.1 ! Include at least V and B-V B-V=0.0 +/- 0.2 TYPE=A0V Comments: Fixed_Targets ! Section 5.1 Target_Number: 2 Target_Name: HR-4796D Alternate_Names: Description: UNIDENTIFIED, Optical Emitter Position: R = 4.9", PA = 315D, FROM 1 Equinox: J2000 RV_or_Z: RA_PM: ! Units are seconds of time per year Dec_PM: ! Units are seconds of arc per year Epoch: 2000 Annual_Parallax: Flux: V=16.3 +/- 1 ! Include at least V and B-V B-V=0.0 +/- 1.0 Comments: Measured R(Johnson) magnitude = 16.3, but V magnitude is uncertain !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! !Scan_Data ! Appendix B ! Scan_Number: ! FGS_Scan: ! Cont_or_Dwell: ! Dwell_Points: ! Dwell_Secs: ! Scan_Width: ! Scan_Length: ! Sides_Angle: ! Number_Lines: ! Scan_Rate: ! First_Line_PA: ! Scan_Frame: ! Length_Offset: ! Width_Offset: !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! ! 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