! +====================+ ! | PED OUTPUT PRODUCT | ! +====================+ ! ! /data/charon4/smov/1066.prop ! Generated by PREPROCESSOR, version 7.0.1b ! Date: Thu Feb 27 11:29:34 EST 1997 Proposal_Information Title: NICMOS Examples of Attached Parallels Proposal_Category: GO Scientific_Category: COSMOLOGY Cycle: 7 Investigators PI_Name: Joan Smith PI_Institution: University 1 CoI_Name: John Brown CoI_Institution: University 2 Contact: Abstract: Examples of NICMOS ATTACHED PARALLELS, including suggested MULTIACCUM sequences. Questions Observing_Description: As described in the NICMOS Handbook (pp. 27-28) and in the Phase 2 Update, proposers are asked to add attached parallels to their NICMOS primary observations, whenever this does not affect the primary science. Attached parallels are defined as observations in the two NICMOS cameras which are not used for the primary science. Some proposers may have already requested the use of all three Cameras for their science, but some other may have not (e.g., it is not needed for their science). Those who didn't, should follow the guidelines given in the Handbook and the Phase 2 Update. It should be kept in mind that there is the potential for the three NICMOS Cameras to come back to parfocality once in orbit. Since attached parallels will be most useful when long integration times are available, the recommendation is to add attached parallels whenever the exposure times in the prime Camera are LONGER than 10 minutes at EACH fixed telescope pointing. Below two examples are given (one for each visit) of attached parallels: one for broad band filters, to be applied to extragalactic observations, to Galactic Plane observations, and to Molecular Cloud observations when more than 4 orbits are available (see the Handbook); the other for narrow band filters, which should be implemented when observations of Molecular clouds require less than 4 orbits. For illustrative purposes, in the first example, NIC2 is the primary Camera; in the second example NIC1 is primary. The suggested readout mode is MULTIACCUM, with the sequence SPARSE256, in all cases. N.B.: In general, users should define a Generic Target (see below) for the NICMOS attached parallels. In this way, they will not need to specify a value of the ORIENT for the pointings of the parallel detectors. The same Generic Target can be used for all exposures and all visits in the proposal. The specification of the Generic Target is not needed when the primary observation already requires an ORIENT. Proposers are encouraged to process through RPS2 their primary proposal, BEFORE adding the attached parallels, to ensure that the efficiency of the observations is not affected by the subsequent addition of attached parallels. Real_Time_Justification: Calibration_Justification: Additional_Comments: Fixed_Targets Target_Number: 1 Target_Name: HDF Alternate_Names: Hubble,Deep Description: GALAXY,PROTOGALAXY Position: RA=12H 36M 49.40S +/- 0.02S,DEC=62D 10' 58.0" +/- 0.7" Equinox: J2000 RV_or_Z: RA_PM: 0.0 Dec_PM: 0.0 Epoch: Annual_Parallax: 0.0 Flux: F(1.60)=0.00 Comments: The value of the flux is in units of Jy, at 1.6 microns Target_Number: 2 Target_Name: MC Alternate_Names: Molecular,Cloud Description: ISM Position: RA=14H 36M 49.40S +/- 0.02S,DEC=02D 10' 58.0" +/- 0.7" Equinox: J2000 RV_or_Z: RA_PM: 0.0 Dec_PM: 0.0 Epoch: Annual_Parallax: 0.0 Flux: F(1.60)=0.00 Comments: The value of the flux is in units of Jy, at 1.6 microns Solar_System_Targets Generic_Targets Target_Number: 3 Target_Name: PARALLEL-TARGET-1 Description: UNIDENTIFIED,INFRARED EMITTER,BLANK FIELD Criteria: Flux: V = 22 B-V = 0.86 +/- 0.2 Comments: GENERIC TARGET FOR ATTACHED PARALLEL OBSERVATIONS. ACTUAL POINTING IS NOT CRITICAL. Scan_Data Visits Visit_Number: 01 Visit_Requirements: On_Hold_Comments: Visit_Comments: In this visit, the primary observation is towards (e.g.) extralactic targets; NIC2 is the primary Camera; in the primary exposure, the Special requirement PAR 2-3 WITH 1 must be specified. Exposure_Number: 1 Target_Name: HDF Config: NIC2 Opmode: MULTIACCUM Aperture: NIC2 Sp_Element: F160W Wavelength: Optional_Parameters: SAMP-SEQ=STEP256,NSAMP=12 Number_of_Iterations: 1 Time_Per_Exposure: DEF Special_Requirements: PAR 2-3 WITH 1 Comments: Exposure_Number: 2 Target_Name: PARALLEL-TARGET-1 Config: NIC1 Opmode: MULTIACCUM Aperture: NIC1 Sp_Element: F160W Wavelength: Optional_Parameters: SAMP-SEQ=SPARS256,NSAMP=4 Number_of_Iterations: 1 Time_Per_Exposure: DEF Special_Requirements: Comments: the filter should be changed to F110W during the subsequent exposure, if multifilter observations of the same target are obtained. Exposure_Number: 3 Target_Name: PARALLEL-TARGET-1 Config: NIC3 Opmode: MULTIACCUM Aperture: NIC3 Sp_Element: F110W Wavelength: Optional_Parameters: SAMP-SEQ=SPARS256,NSAMP=4 Number_of_Iterations: 1 Time_Per_Exposure: DEF Special_Requirements: Comments: the filter should be changed to F160W during the subsequent exposure, if multifilter observations of the same target are obtained. Visit_Number: 02 Visit_Requirements: On_Hold_Comments: Visit_Comments: In this visit, the primary observation is towards a Molecular Cloud and the total time allocation is less than 4 orbits; NIC1 is the primary Camera; in the primary exposure, the Special requirement PAR 2-3 WITH 1 must be specified. Exposure_Number: 1 Target_Name: MC Config: NIC1 Opmode: MULTIACCUM Aperture: NIC1 Sp_Element: F166N Wavelength: Optional_Parameters: SAMP-SEQ=STEP256,NSAMP=12 Number_of_Iterations: 1 Time_Per_Exposure: DEF Special_Requirements: PAR 2-3 WITH 1 Comments: Exposure_Number: 2 Target_Name: PARALLEL-TARGET-1 Config: NIC2 Opmode: MULTIACCUM Aperture: NIC2 Sp_Element: F212N Wavelength: Optional_Parameters: SAMP-SEQ=SPARS256,NSAMP=4 Number_of_Iterations: 1 Time_Per_Exposure: DEF Special_Requirements: Comments: the filter should be changed to F215N during the subsequent exposure, if multifilter observations of the same target are obtained. Exposure_Number: 3 Target_Name: PARALLEL-TARGET-1 Config: NIC3 Opmode: MULTIACCUM Aperture: NIC3 Sp_Element: F164N Wavelength: Optional_Parameters: SAMP-SEQ=SPARS256,NSAMP=4 Number_of_Iterations: 1 Time_Per_Exposure: DEF Special_Requirements: Comments: the filter should be changed to F166N during the subsequent exposure, if multifilter observations of the same target are obtained. Data_Distribution ! Defaults indicated; change if desired Medium: 8MM Ship_To: PI_Address Recipient_Email: ! Let us know what you think of this template and software! ! Please send a list of your likes and dislikes to your Program Coordinator