! File: 1379C.PROP ! Database: PEPDB ! Date: 16-FEB-1994:16:38:02 coverpage: title_1: HSP DETECTOR DARK COUNT TEST HSP-I1 proposal_for: OV/HSP pi_title: DR. pi_fname: ROBERT pi_mi: C. pi_lname: BLESS pi_inst: UNIVERSITY OF WISCONSIN pi_country: USA pi_phone: (608) 262-1715 keywords_1: ORBITAL VERIFICATION hours_pri: 2.00 hsp: Y pi_position: PROF. OF ASTRONOMY ! 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: SLOVAK fname: MARK title: DR. mi: H. inst: UNIVERSITY OF WISCONSIN country: USA ! lname: DOLAN fname: JOSEPH title: DR. mi: F. inst: GODDARD SPACE FLIGHT CENTER country: USA ! lname: BLESS fname: ROBERT title: DR. mi: C. inst: UNIVERSITY OF WISCONSIN 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. ! 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 the dark earth. 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. line_21: Each detector is turned off after the line_22: required data is obtained. ! question: 5 section: 1 line_1: HSP tests HSP-iA through -iF must be completed before this test is line_2: initiated. AT LEAST 24 HOURS MUST BE ALLOWED AFTER THE INITIAL TURN-ON line_3: OF THE LAST DETECTOR IN HSP-iF BEFORE THIS TEST IS PERFORMED. This is line_4: an internal test and no external targets are observed. Dark time is line_5: required for the entire test, and for the PMT portion of the test it line_6: test it is required that the ST be pointing at the dark earth. To line_7: perform the test, it is assumed that each detector has been successfully line_8: powered up for 30 minutes, which is the line_9: case if the standard stabilization times line_10: are used. line_12: 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 supported at the Space Astronomy Lab at the line_2: University of Wisconsin in Madison. ! !end of general form text general_form_address: lname: DOLAN fname: JOSEPH mi: F. title: DR. category: CON inst: GSFC addr_1: CODE 681 city: GREENBELT state: MD zip: 20771 country: USA phone: (301) 286-6846 ! lname: SLOVAK fname: MARK mi: H. category: CON inst: UNIVERSITY OF WISCONSIN addr_1: 475 N. CHARTER STREET city: MADISON state: WI zip: 53706 country: USA phone: (608) 262-7542 ! lname: BLESS fname: ROBERT mi: C. category: PI inst: UNIVERSITY OF WISCONSIN addr_1: 475 N. CHARTER STREET city: MADISON state: WI zip: 53706 country: USA phone: (608) 262-1715 ! ! 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; req_2: SEQ 5-6; comment_1: SAMPLE PMT DARK CURRENT comment_2: AT NOMINAL HV ! linenum: 6.000 sequence_1: ^ targname: ^ 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: SAMPLE PMT DARK CURRENT WITH HIGH comment_2: VOLTAGE OFF. ! linenum: 6.500 targname: DARK config: S/C opmode: DATA aperture: NONE num_exp: 1 time_per_exp: 5M priority: 1 param_1: REALTIME=CMD, req_1: BEFORE 7 BY 12M +/- 5M; comment_1: UPLINK REQUIRED FOR CONTINGENCY IN comment_2: THE EVENT OF FAILURE IN HIGH VOLTAGE comment_3: TEST (HSP1502) ! 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_3: SEQ 7-7.3 NO GAP; req_4: DARK TIME; comment_1: SAMPLE VIS IDT. comment_2: (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: SAMPLE VIS IDT. comment_2: (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: SAMPLE VIS IDT. comment_2: (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: SAMPLE VIS IDT. comment_2: (H,V) = (2000,1900) comment_3: HIGH VOLTAGE OFF comment_4: POWER DOWN DETECTOR WHEN DONE ! 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: SEQ 8-8.3 NO GAP; req_2: DARK TIME; comment_1: SAMPLE UV1 IDT. comment_2: (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: SAMPLE UV1 IDT. comment_2: (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: SAMPLE UV1 IDT. comment_2: (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: SAMPLE UV1 IDT. comment_2: (H,V) = (2000,1900) comment_3: HIGH VOLTAGE OFF comment_4: POWER DOWN DETECTOR WHEN DONE ! 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: SEQ 9-9.3 NO GAP; req_2: DARK TIME; comment_1: SAMPLE UV2 IDT. comment_2: (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: SAMPLE UV2 IDT. comment_2: (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: SAMPLE UV2 IDT. comment_2: (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: SAMPLE UV2 IDT. comment_2: (H,V) = (2000,1900) comment_3: HIGH VOLTAGE OFF comment_4: POWER DOWN DETECTOR WHEN DONE ! 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: SEQ 10-10.3 NO GAP; req_2: DARK TIME; comment_1: SAMPLE POL IDT. comment_2: (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: SAMPLE POL IDT. comment_2: (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: SAMPLE POL IDT. comment_2: (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: SAMPLE POL IDT. comment_2: (H,V) = (2000,1900) comment_3: HIGH VOLTAGE OFF comment_4: POWER DOWN DETECTOR WHEN DONE ! linenum: 11.000 sequence_1: USE sequence_2: DARK-PMT comment_1: SAMPLE PMT. comment_2: POWER DOWN DETECTOR WHEN DONE ! ! end of exposure logsheet ! No scan data records found