! File: 5260C.PROP ! Database: PEPDB ! Date: 24-FEB-1994:03:28:02 coverpage: title_1: SEARCH FOR OPTICAL VARIABILITY ASSOCIATED WITH BLACK HOLESI title_2: RPT FOR HOPR 94 sci_cat: STELLAR ASTROPHYSICS proposal_for: RPT/HSP cont_id: 3255 pi_fname: ROBERT pi_mi: C. pi_lname: BLESS pi_inst: WISCONSIN, UNIVERSITY OF pi_country: USA pi_phone: (608) 262-1715 keywords_1: VARIABLE, INTERACTING BINARIES, BLACK HOLES hours_pri: 6.22 num_pri: 4 ! end of coverpage abstract: line_1: It has been suggested that luminous matter passing line_2: through an accretion disk towards the event horizon line_3: of a black hole is likely to emit a short series of line_4: pulses at an increasing frequency. These so-called line_5: dying pulses trains would have a period of the order line_6: of milliseconds for stellar mass black holes. A line_7: search for such pulse trains will be made among 3 line_8: candidate objects. Revision History: based on 1094 line_9: targets from 3255 with LMCX-3 replaced with V404 line_10: Cyg--MJN 3/19/92; Resubmit GX339-4 target (HOPR94) line_11: MJT 8/18/93. ! ! end of abstract general_form_proposers: lname: VAN CITTERS fname: G. mi: W. inst: NATIONAL SCIENCE FOUNDATION country: USA ! lname: BLESS fname: ROBERT mi: C. inst: WISCONSIN, UNIVERSITY OF country: USA ! lname: DOLAN fname: JOSEPH mi: F. inst: NASA, GODDARD SPACE FLIGHT CENTER country: USA ! lname: ELLIOT fname: JAMES mi: L. inst: MASSACHUSETTS INSTITUTE OF TECHNOLOGY country: USA ! lname: ROBINSON fname: EDWARD mi: L. inst: TEXAS, UNIVERSITY OF country: USA ! lname: WHITE fname: RICHARD mi: L. inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: Each object would be monitored for 30 minutes to an line_2: hour using about 100 microsec integration times with line_3: a broad filter. Each target should be observed more line_4: than once (during different x-ray intensity states, line_5: for example). ! question: 4 section: 1 line_1: ST is required in order to eliminate atmospheric line_2: noise, to observe in the UV where burst amplitudes line_3: are expected to be larger than in the visual, and to line_4: be able to use small apertures. ! question: 13 section: 1 line_1: A search is to be made in black hole candidate line_2: objects for "dying pulse trains" indicative of line_3: matter spiraling towards the event horizon of a line_4: black hole. ! !end of general form text general_form_address: lname: BLESS fname: ROBERT mi: C. category: PI inst: UNIVERSITY OF WISCONSIN addr_1: SPACE ASTRONOMY LAB. addr_2: 1150 UNIVERSITY AVE. city: MADISON state: WI zip: 53706 country: USA phone: (608) 262-1715 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: GX339-4 descr_1: X-RAY BINARY pos_1: RA = 17H 02M 49.363S +/- 1.0", pos_2: DEC = -48D 47' 22.477" +/- 1.0" equinox: 2000 comment_1: POSREF = ROBINSON fluxnum_1: 1 fluxval_1: V = 18 +/- 3 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 10.000 targname: GX339-4 config: HSP/UV2 opmode: ACQ num_exp: 1 time_per_exp: 9M fluxnum_1: 1 priority: 1 param_1: DATA-FORMAT=WORD, req_1: CYCLE 2 / 10.0-11.0; req_2: ONBOARD ACQ FOR 11.0; req_3: PCS MODE FINE / 10-11; ! linenum: 11.000 targname: GX339-4 config: HSP/UV2 opmode: SINGLE aperture: 10.0 sp_element: F140LP num_exp: 3 time_per_exp: 20M fluxnum_1: 1 priority: 1 param_1: SAMPLE-TIME=0.0001, param_2: DATA-FORMAT=BYTE, req_1: REPEAT 10.0-11.0 EVERY 30D +/- 7D req_2: FOR 2 MORE TIMES; req_3: NON-INT; req_4: RT-ANALYSIS; comment_1: PREFER TDRSS DOWNLINK RATHER comment_2: THAN TAPE RECORDER. ! ! end of exposure logsheet ! No scan data records found