! $Id: 5136,v 13.1 1994/07/27 15:24:52 pepsa Exp $ COVERPAGE: TITLE_1: A COLOR-MAGNITUDE ARRAY IN THE BULGE OF M31 SCI_CAT:GALAXIES & CLUSTERS SCI_SUBCAT:STELLAR POPULATIONS PROPOSAL_FOR:GTO/OS PI_TITLE: PROF. PI_FNAME:IVAN PI_MI:R. PI_LNAME:KING PI_INST:U. CALIF. PI_COUNTRY: U.S.A. PI_PHONE: 510-642-2206 HOURS_PRI:2.0 HOURS_PAR:2.0 NUM_PRI:2 NUM_PAR:2 WF_PC: Y FOC: Y FOS: HRS: HSP: FGS: REALTIME: TIME_CRIT: FUNDS_AMOUNT:0 FUNDS_LENGTH: 12 FUNDS_DATE: JAN-94 PI_POSITION:PROF. OFF_FNAME: OFF_MI: OFF_LNAME: OFF_TITLE: OFF_INST: OFF_ADDR_1: OFF_ADDR_2: OFF_ADDR_3: OFF_CITY: OFF_STATE: OFF_ZIP: OFF_COUNTRY: OFF_PHONE: OFF_TELEX: ABSTRACT: LINE_1:The FOC will be used to get a color-magnitude array at the edge of LINE_2:the bulge of M31. Parallel exposures with WFPC2 will search for LINE_3:UV-bright objects about 2' from the center. LINE_4: LINE_5: LINE_6: LINE_7: LINE_8: LINE_9: LINE_10: LINE_11: LINE_12: LINE_13: LINE_14: LINE_15: LINE_16: LINE_17: LINE_18: LINE_19: LINE_20: GENERAL_FORM_PROPOSERS: LNAME:KING FNAME:IVAN MI:R. TITLE:PROF. INST:U. CALIF. COUNTRY:U.S.A. ESA: GENERAL_FORM_TEXT: QUESTION:3 SECTION:1 LINE_1:The primary program is to do a B-V CMD at the edge of the M31 LINE_2:bulge. Simulations indicate that the FOC/96 will resolve stars LINE_3:in this field down to the limit of 1-hour exposures. LINE_4: LINE_5:The parallel program is to look for UV-bright objects at about LINE_6:2 arcmin from the center of M31 (mainly PSGB stars). There are LINE_7:other UV-search proposals, but none at this distance from the LINE_8:center. LINE_9: LINE_10: LINE_11: LINE_12: LINE_13: LINE_14: LINE_15: LINE_16: LINE_17: LINE_18: LINE_19: LINE_20: LINE_21: LINE_22: LINE_23: GENERAL_FORM_ADDRESS: LNAME:KING FNAME:IVAN TITLE:PROF. MI:R. CATEGORY:PI INST:U. CALIF., BERKELEY ADDR_1:ASTRON. DEPT. ADDR_2:UNIV. OF CALIFORNIA CITY:BERKELEY STATE:CA ZIP:94720 COUNTRY:U.S.A. PHONE:510-642-2206 TELEX: FROM_DATE:1-JAN-93 TO_DATE:31-DEC-94 FIXED_TARGETS: TARGNUM:1 NAME_1:NGC224-OFF4 NAME_2:(M31 BULGE) NAME_3: DESCR_1:E, DESCR_2:301, DESCR_3:913 POS_1:RA=00H40M30.5S +/- 0.1S, POS_2:DEC=+40D56'25" +/- 1" EQUINOX:1950 COMMENT_1:THIS FIELD IS 6.5' FROM THE COMMENT_2:CENTER OF M31, ON THE COMMENT_3:LESS-OBSCURED SIDE OF THE COMMENT_4:MINOR AXIS. GENERIC_TARGETS: TARGNUM_1:2 NAME_1:NGC224-FLD DESCR_1:E, DESCR_2:301, DESCR_3:913 CRITERIA_1:RA=00H40M30.5S, CRITERIA_2:DEC=+40D56'25", CRITERIA_3:R=5' COMMENT_1:THIS IS A PARALLEL FIELD, FOR COMMENT_2:STUDY OF UV-BRIGHT STARS 3.5' OFF COMMENT_3:THE CENTER OF M31. THE FIELD NO COMMENT_4:LONGER CONFLICTS WITH THOSE OF COMMENT_5:ANY OTHER UV STUDIES. EXPOSURE_LOGSHEET: LINENUM:1.0 SEQUENCE_1:DEF SEQUENCE_2:FOC1 TARGNAME:NGC224-OFF4 CONFIG:FOC/96 OPMODE:IMAGE APERTURE:512X512 SP_ELEMENT:# NUM_EXP:1 TIME_PER_EXP:2322S PRIORITY: 1 LINENUM:1.1 SEQUENCE_1:DEF SEQUENCE_2:FOC2 TARGNAME:NGC224-OFF4 CONFIG:FOC/96 OPMODE:IMAGE APERTURE:512X512 SP_ELEMENT:# NUM_EXP:1 TIME_PER_EXP:2656S PRIORITY: 1 LINENUM:1.5 SEQUENCE_1:DEF SEQUENCE_2:PAR24 TARGNAME:NGC224-FLD CONFIG:WFPC2 OPMODE:IMAGE APERTURE:WFALL SP_ELEMENT:F170W PARAM_1:CR-SPLIT=NO NUM_EXP:1 TIME_PER_EXP:2400S PRIORITY: 1 LINENUM:1.6 SEQUENCE_1:DEF SEQUENCE_2:PAR28 TARGNAME:NGC224-FLD CONFIG:WFPC2 OPMODE:IMAGE APERTURE:WFALL SP_ELEMENT:F170W PARAM_1:CR-SPLIT=NO NUM_EXP:1 TIME_PER_EXP:2800S PRIORITY: 1 LINENUM:2.0 SEQUENCE_1:USE SEQUENCE_2:FOC1 SP_ELEMENT:F480LP REQ_1:CYCLE 4 /2-3.5; REQ_2:ORIENT 210D +/- 10D COMMENT_1:ALL EXPOSURE LINES CAN COMMENT_2:BE TAKEN ON A SINGLE GSACQ LINENUM:2.5 SEQUENCE_1:USE SEQUENCE_2:PAR24 REQ_1:PAR COMMENT_1:PAR WITH 2 LINENUM:3.0 SEQUENCE_1:USE SEQUENCE_2:FOC2 SP_ELEMENT:F430W REQ_1:SAME POS FOR 3 AS 2; REQ_2:SAME ORIENT FOR 3 AS 2; LINENUM:3.5 SEQUENCE_1:USE SEQUENCE_2:PAR28 REQ_1:PAR COMMENT_1:PAR WITH 3 !~~~RPSS~~~,KING,5136s.prop, 8-MAR-1994 17:08