! File: 2863C.PROP ! Database: PEPDB ! Date: 17-FEB-1994:19:08:15 coverpage: title_1: HSP DETECTOR DARK COUNT TEST proposal_for: CAL/HSP pi_title: DR. pi_fname: RICHARD pi_mi: L. pi_lname: WHITE pi_inst: SPACE TELESCOPE SCIENCE INSTITUTE pi_country: USA pi_phone: (301) 338-4797 hours_pri: 1.65 hours_par: 68.68 num_pri: 1 hsp: Y pi_position: INSTRUMENT SCIENTIST ! end of coverpage abstract: line_1: This proposal defines the procedure for monitoring the dark count on each of line_2: the HSP detectors to determine the instrumental noise characteristics. It is an line_3: internal test intended to become a routine procedure. Each of the four IDTs line_4: will be sampled at three different cathode locations; the PMT will be line_5: monitored as well. line_6: Note: This is RPSS file # 1379. Revision history: Richards 4/13/88, line_7: Slovak 5/20/88, Richards 6/29/88, line_8: Translate to V2 instructions and line_9: changed sample time to 0.1 sec line_10: Richards 12/28/88 ! ! end of abstract general_form_proposers: lname: WHITE fname: RICHARD title: DR. mi: L. inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! lname: WALTER fname: LISA title: MS. mi: E. inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! ! end of general_form_proposers block general_form_text: question: 2 section: 1 line_1: The justification for the proposed test is to determine the time, temperature line_2: and spatial dependencies of the dark count characteristics of each of the five line_3: HSP detectors. line_5: The four IDTs will be spatially mapped at three different cathode locations line_6: across the face of each detector; the dark from the PMT will also be measured. line_7: Each detector will be tested in both the digital and analog modes of line_8: operation. line_10: This test is to be repeated regularly as it is anticipated that the results line_11: (e.g., mean dark count rates for each detector) will be inputs for the line_12: Calibration Data Base (CDB). line_14: The in-flight results will be compared with the extant data currently available line_15: from ground testing and from previous orbital measurements. ! question: 3 section: 1 line_1: This test is to be performed during dark time, and during the PMT line_2: portion of the test the ST should be pointing at a dark sky target. line_4: 1) IDTs (i=1,4): the HSP is to be configured in the single-color, one aperture line_5: mode (HSP/x, SINGLE) with the detector at nominal high voltage and PAD line_6: settings. Each detector is to be sampled at the central cathode position and at line_7: two other positions along the edge of the cathode, none of which correspond to line_8: any aperture. These three positions have the following detector coordinate line_9: positions: line_10: (a) (H,V) = (2000,1900) line_11: (b) (H,V) = (3600,1900) line_12: (c) (H,V) = (2000,3000) line_14: An integration of 5 minutes in length, sampling at 0.1 second samples, is to be line_15: obtained at each position. The detector high voltage will then be turned off line_16: and a fourth 5 minute integration made at (H,V) = (2000, 1900) line_18: 2) PMT: Operating at the nominal high voltage the dark current is to be sampled line_19: for 5 minutes. The PMT high voltage will then be turned off and a second 5 line_20: minute integration made. Data are to be taken in the ALL format. ! question: 5 section: 1 line_1: This is an internal test for the IDTs, with no external targets required. line_2: For the PMT, the telescope must be pointed at a dark sky position. line_3: To perform the test, it is assumed that each detector has been powered line_4: up for 30 minutes, which is the case if the standard stabilization line_5: times are used. line_6: Dark time and non-SAA passage are required for this test. ! question: 7 section: 1 line_1: The data reduction is planned as follows: for each of the detectors the mean line_2: dark count rate (digital mode) will be determined as a function of cathode line_3: position. After the test is performed enough times, for each cathode position line_4: the mean values will be plotted as a function of (a) detector temperature and line_5: (b) observation time. The data analysis will consist of performing a trend line_6: analysis on the various data series from the data reduction process in order line_7: to determine the potential hysteresis (if any) and to monitor the temporal line_8: development of the noise properties of the various detectors. ! question: 10 section: 1 line_1: Data reduction and analysis will be carried out at STScI with CDBS. ! !end of general form text general_form_address: lname: WHITE fname: R mi: L category: PI inst: ST SCI addr_1: 3700 SAN MARTIN DRIVE city: BALTIMORE state: MD zip: 21218 ! lname: WHITE fname: RICHARD mi: L. category: PI inst: SPACE TELESCOPE SCIENCE INSTITUTE addr_1: 3700 SAN MARTIN DRIVE city: BALTIMORE state: MD zip: 21218 country: USA phone: (301) 338-4797 ! lname: WALTER fname: LISA mi: E. category: CON inst: SPACE TELESCOPE SCIENCE INSTITUTE addr_1: 3700 SAN MARTIN DRIVE city: BALTIMORE state: MD zip: 21218 country: USA phone: (301) 338-5036 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: PMT-DARK-SKY descr_1: DARK SKY POSITION FOR PMT DARKS pos_1: RA = 16H 27M 11S +/- .01", pos_2: DEC = -24D 19' 14" +/- .01" equinox: 2000.0 comment_1: SELECT ONE OF THESE TARGETS AS THE comment_2: PMT DARK SKY POINTING. ! targnum: 2 name_1: PMT-DARK-SKY-2 name_2: BARNARD 5 pos_1: RA = 3H 46.3M +/- 0.1M, pos_2: DEC = +32D 49' +/- 1', equinox: 1975 ! targnum: 3 name_1: PMT-DARK-SKY-3 name_2: BARNARD 227 pos_1: RA = 6H 5.9M +/- 0.1M, pos_2: DEC = +19D 42' +/- 1', equinox: 1975 ! targnum: 4 name_1: PMT-DARK-SKY-4 name_2: BARNARD 46 pos_1: RA = 16H 55.7M +/- 0.1M, pos_2: DEC = -22D 42' +/- 1', equinox: 1975 ! targnum: 5 name_1: PMT-DARK-SKY-5 name_2: BARNARD 100 pos_1: RA = 18H 31.3M +/- 0.1M, pos_2: DEC = -9D 10' +/- 1', equinox: 1975 ! targnum: 6 name_1: PMT-DARK-SKY-6 name_2: BARNARD 362 pos_1: RA = 21H 23.1M +/- 0.1M, pos_2: DEC= +50D 6' +/- 1', equinox: 1975 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 sequence_1: DEFINE sequence_2: DARK-IDT targname: DARK config: # opmode: SINGLE aperture: # sp_element: # num_exp: 1 time_per_exp: 300S priority: 1 param_1: #, ! linenum: 5.000 sequence_1: DEFINE sequence_2: DARK-PMT targname: PMT-DARK-SKY config: HSP/PMT/VIS opmode: SPLIT aperture: 1.0 sp_element: F750W/F320N num_exp: 1 time_per_exp: 300S priority: 1 param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, req_1: DARK TIME / 5-5.5; req_2: SEQ 5-6 NO GAP; req_3: SELECT 1 OF 5.000 OR 5.100 OR 5.200 req_4: OR 5.300 OR 5.400 OR 5.500; req_5: COND IF TARGET FAR FROM SUN; ! linenum: 5.100 sequence_1: DEFINE sequence_2: DARK-PMT targname: PMT-DARK-SKY-2 config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ priority: ^ param_1: ^ ! linenum: 5.200 sequence_1: DEFINE sequence_2: DARK-PMT targname: PMT-DARK-SKY-3 config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ priority: ^ param_1: ^ ! linenum: 5.300 sequence_1: DEFINE sequence_2: DARK-PMT targname: PMT-DARK-SKY-4 config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ priority: ^ param_1: ^ ! linenum: 5.400 sequence_1: DEFINE sequence_2: DARK-PMT targname: PMT-DARK-SKY-5 config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ priority: ^ param_1: ^ ! linenum: 5.500 sequence_1: DEFINE sequence_2: DARK-PMT targname: PMT-DARK-SKY-6 config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ priority: ^ param_1: ^ ! linenum: 6.000 sequence_1: DEFINE sequence_2: DARK-PMT targname: DARK config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ priority: ^ param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: PMT-HV-GAIN=OFF, comment_1: HIGH VOLTAGE OFF. comment_2: CAN SLEW AWAY FROM DARK TARGET comment_3: DURING THIS INTEGRATION. ! linenum: 7.000 sequence_1: USE sequence_2: DARK-IDT config: HSP/VIS aperture: 1.0-A sp_element: F355M param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=G1.0, req_1: DARK TIME; req_2: REPEAT 7-7.3 EVERY 10D +/- 3D FOR 35 req_3: MORE TIMES; SEQ 7-7.3 NO GAP; req_4: CYCLE 1 / 7-11; comment_1: (H,V) = (2000,1900) ! linenum: 7.100 sequence_1: USE sequence_2: DARK-IDT config: HSP/VIS aperture: 0.4-B sp_element: F355M param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=G1.0, req_1: DARK TIME; comment_1: (H,V) = (3600,1900) ! linenum: 7.200 sequence_1: USE sequence_2: DARK-IDT config: HSP/VIS aperture: 0.4-C sp_element: F160LP param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=G1.0, req_1: DARK TIME; comment_1: (H,V) = (2000,3000) ! linenum: 7.300 sequence_1: USE sequence_2: DARK-IDT config: HSP/VIS aperture: 1.0-A sp_element: F355M param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=OFF, comment_1: (H,V) = (2000,1900) comment_2: HIGH VOLTAGE OFF ! linenum: 8.000 sequence_1: USE sequence_2: DARK-IDT config: HSP/UV1 aperture: 1.0-A sp_element: F240W param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=G1.0, req_1: DARK TIME; req_2: REPEAT 8-8.3 EVERY 10D +/- 3D FOR 35 req_3: MORE TIMES; SEQ 8-8.3 NO GAP; comment_1: (H,V) = (2000,1900) ! linenum: 8.100 sequence_1: USE sequence_2: DARK-IDT config: HSP/UV1 aperture: 0.4-B sp_element: F240W param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=G1.0, req_1: DARK TIME; comment_1: (H,V) = (3600,1900) ! linenum: 8.200 sequence_1: USE sequence_2: DARK-IDT config: HSP/UV1 aperture: 0.4-C sp_element: F140LP param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=G1.0, req_1: DARK TIME; comment_1: (H,V) = (2000,3000) ! linenum: 8.300 sequence_1: USE sequence_2: DARK-IDT config: HSP/UV1 aperture: 1.0-A sp_element: F240W param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=OFF, comment_1: (H,V) = (2000,1900) comment_2: HIGH VOLTAGE OFF ! linenum: 9.000 sequence_1: USE sequence_2: DARK-IDT config: HSP/UV2 aperture: 1.0-A sp_element: F248M param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=G1.0, req_1: DARK TIME; req_2: REPEAT 9-9.3 EVERY 10D +/- 3D FOR 35 req_3: MORE TIMES; SEQ 9-9.3 NO GAP; comment_1: (H,V) = (2000,1900) ! linenum: 9.100 sequence_1: USE sequence_2: DARK-IDT config: HSP/UV2 aperture: 0.4-B sp_element: F248M param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=G1.0, req_1: DARK TIME; comment_1: (H,V) = (3600,1900) ! linenum: 9.200 sequence_1: USE sequence_2: DARK-IDT config: HSP/UV2 aperture: 0.4-C sp_element: F140LP param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=G1.0, req_1: DARK TIME; comment_1: (H,V) = (2000,3000) ! linenum: 9.300 sequence_1: USE sequence_2: DARK-IDT config: HSP/UV2 aperture: 1.0-A sp_element: F248M param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=OFF, comment_1: (H,V) = (2000,1900) comment_2: HIGH VOLTAGE OFF ! linenum: 10.000 sequence_1: USE sequence_2: DARK-IDT config: HSP/POL aperture: POL90 sp_element: F277M param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=G1.0, req_1: DARK TIME; req_2: REPEAT 10-10.3 EVERY 10D +/- 3D FOR 35 req_3: MORE TIMES; SEQ 10-10.3 NO GAP; comment_1: (H,V) = (2000,1900) ! linenum: 10.100 sequence_1: USE sequence_2: DARK-IDT config: HSP/POL aperture: POL45 sp_element: F277M param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=G1.0, req_1: DARK TIME; comment_1: (H,V) = (3600,1900) ! linenum: 10.200 sequence_1: USE sequence_2: DARK-IDT config: HSP/POL aperture: POL90 sp_element: F327M param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=G1.0, req_1: DARK TIME; comment_1: (H,V) = (2000,3000) ! linenum: 10.300 sequence_1: USE sequence_2: DARK-IDT config: HSP/POL aperture: POL90 sp_element: F327M param_1: DATA-FORMAT=ALL, param_2: SAMPLE-TIME=0.1, param_3: ANALOG-SCALE=10, param_4: HV-GAIN=OFF, comment_1: (H,V) = (2000,1900) comment_2: HIGH VOLTAGE OFF ! linenum: 11.000 sequence_1: USE sequence_2: DARK-PMT req_1: REPEAT 11 EVERY 30D +/- 10D FOR 11 req_2: MORE TIMES; ! ! end of exposure logsheet ! No scan data records found