Hsp Time Resolved Photometry Test HSP-04

Details Hsp Time Resolved Photometry Test HSP-04 Hsp Time Resolved Photometry Test HSP-04

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.1383b&link_type=abstract

HST Proposal ID #1383

Physics

Hst Proposal Id #1383

Scientific paper

This proposal defines the procedure for verifying the capability for HSP to continuously integrate at a very high data sampling rate. Using the visual IDT (IDT#3) the Crab Pulsar will be observed in a selected 1.0 arcsec aperture using 10.8 microsecond integration samples. This observation will verify the time resolution of the HSP and determine the HST system time reliability of scientific purposes. Observations of the Crab Pulsar at a 10.8 micosecond sampling rate will also verify the relevant Contract End Item (CEI) specification for the HSP. Revision History: Mark Slovak 11/03/88; Translated to V2 proposal instructions, Sally Laurent 1/30/89; Updated 3/9/89 - Peg Stanley; SV Scrub: 4/17/89 - Sally Laurent; Changed per P. Reppert's comments of 6/6/89 - SALM 8/9/89; Deleted HZ Herculis due to poor reliability in in variability - SALM 9/26/89; Changed pre-req & special req. - SALM 9/27/89; Updated text - SALM 5/25/90; Fixes for aberration problem - SALM 7/30/90; This test has been revised by P. Stanley (7/16/91) to take 1 "orbit's" worth of data over 4 consecutive days rather than 4 consecutive orbits

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