! File: 1295C.PROP ! Database: PEPDB ! Date: 16-FEB-1994:11:31:06 coverpage: title_1: PHOTOMETRY OF STARS IN OLD MAGELLANIC CLOUD CLUSTERS sci_cat: STELLAR POPULATIONS sci_subcat: MAGELLANIC CLOUDS proposal_for: GTO/FOC pi_fname: IVAN pi_mi: R. pi_lname: KING pi_inst: UC, BERKELEY pi_country: USA pi_phone: 415-642-2206 keywords_1: OPEN CLUSTER--MAGELLANIC CLOUDS hours_pri: 4.00 num_pri: 3 ! end of coverpage abstract: line_1: We will get accurate color-magnitude arrays that reach well below the line_2: main-sequence turnoff in three old clusters in the Magellanic Clouds, allowing line_3: detailed comparison with old clusters of different metal abundances in the line_4: Milky Way. line_6: Simultaneous exposures with the PC on fields in the Clouds will also determine line_7: the main-sequence turnoff for them. ! ! end of abstract general_form_proposers: lname: KING fname: IVAN mi: R. inst: UC, BERKELEY country: USA ! lname: CANNON fname: R. mi: D. inst: ROYAL OBSERVATORY, EDINBURGH country: UNITED KINGDOM esa: X ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: on each cluster: line_2: f/96, F480LP, 1500 s (par. PC, F555W) line_3: f/96, F430W, 1500s (par. PC, F785W) line_4: f/96, F342W, 600s (par. PC, F785W) line_5: on L11, add another set of exp. with the 2 cameras swapped in position line_7: Cycle 1: None. line_8: Cycle 2: Exp. 8, 9, and (10-15 or 16-17 or 16-19). line_9: Cycles 3-5: Exp. 7. ! question: 4 section: 1 line_1: resolving power ! question: 7 section: 1 line_1: to be done at ROE Starlink node ! question: 8 section: 1 line_1: roll angles are all specified ! question: 10 section: 1 line_1: Berkeley: VAX, S/W, offices, postdoc, RA's line_2: ROE: VAX, S/W, offices, personnel ! question: 12 section: 1 line_1: Note that 2 of the exposures are required to have roll angle opposite by 180 line_2: deg. ! question: 13 section: 1 line_1: Color-magnitude arrays of 3 old clusters, two in SMC and one in LMC. Parallel line_2: obs. with PC for color-magnitude arrays of Cloud field stars. ! !end of general form text general_form_address: lname: KING fname: IVAN mi: R. title: DR. category: PI inst: UC BERKELEY addr_1: ASTRONOMY DEPT. city: BERKELEY state: CA zip: 94720 country: USA phone: 415-642-2206 telex: 820181 UBC AST RAL ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: LINDSAY-1 descr_1: SMC CLUSTER pos_1: RA=00H01M23.0S+/-.1S, pos_2: DEC=-73D44'56"+/-1" equinox: 1950 pm_or_par: NO rv_or_z: V=0 acqpr_1: EXT plate_req: NO fluxnum_1: 1 fluxval_1: V=22.5 fluxnum_2: 2 fluxval_2: B=23.0 fluxnum_3: 3 fluxval_3: U=23.0 fluxnum_4: 4 fluxval_4: I=22.0 ! targnum: 2 name_1: LINDSAY-11 descr_1: ^ pos_1: RA=00H25M35.5S+/-.1S, pos_2: DEC=-73D03'31"+/-1" equinox: ^ pm_or_par: ^ rv_or_z: ^ acqpr_1: ^ plate_req: ^ fluxnum_1: 1 fluxval_1: V=22.5 fluxnum_2: 2 fluxval_2: B=23.0 fluxnum_3: 3 fluxval_3: U=23.0 fluxnum_4: 4 fluxval_4: I=22.0 ! targnum: 3 name_1: HODGE-11 descr_1: LMC CLUSTER pos_1: RA=06H14M50.5S+/-.1S, pos_2: DEC=-69D49'48"+/-1" equinox: ^ pm_or_par: ^ rv_or_z: ^ acqpr_1: ^ plate_req: ^ fluxnum_1: 1 fluxval_1: V=22.5 fluxnum_2: 2 fluxval_2: B=23.0 fluxnum_3: 3 fluxval_3: U=23.0 fluxnum_4: 4 fluxval_4: I=22.0 ! targnum: 4 name_1: L11-OFF1 descr_1: FIELD IN SMC CLUSTER pos_1: R=10", pos_2: PA=270D,FROM 2 equinox: ^ pm_or_par: ^ rv_or_z: ^ acqpr_1: ^ plate_req: ^ fluxnum_1: 1 fluxval_1: V=22.5 fluxnum_2: 2 fluxval_2: B=23.0 fluxnum_3: 3 fluxval_3: U=23.0 fluxnum_4: 4 fluxval_4: I=22.0 ! targnum: 5 name_1: L11-OFF2 descr_1: ^ pos_1: R=35", pos_2: PA=270D,FROM 2 equinox: ^ pm_or_par: ^ rv_or_z: ^ acqpr_1: ^ plate_req: ^ fluxnum_1: 1 fluxval_1: V=22.5 fluxnum_2: 2 fluxval_2: B=23.0 fluxnum_3: 3 fluxval_3: U=23.0 fluxnum_4: 4 fluxval_4: I=22.0 ! targnum: 6 name_1: H11-OFF descr_1: FIELD IN LMC CLUSTER pos_1: R=10", pos_2: PA=90D,FROM 3 equinox: ^ pm_or_par: ^ rv_or_z: ^ acqpr_1: ^ plate_req: ^ fluxnum_1: 1 fluxval_1: V=22.5 fluxnum_2: 2 fluxval_2: B=23.0 fluxnum_3: 3 fluxval_3: U=23.0 fluxnum_4: 4 fluxval_4: I=22.0 ! targnum: 7 name_1: FLD-L1 descr_1: FIELD NEAR SMC CLUSTER L1 pos_1: RA=00H01M23S, pos_2: DEC=-73D44'56", pos_3: REGION, R=7' equinox: 1950 pm_or_par: ^ rv_or_z: ^ ! targnum: 8 name_1: FLD-L11 descr_1: FIELD NEAR SMC CLUSTER L11 pos_1: RA=00H25M35S, pos_2: DEC=-73D03'31", pos_3: REGION, R=7' equinox: 1950 pm_or_par: ^ rv_or_z: ^ ! targnum: 9 name_1: FLD-H11 descr_1: FIELD NEAR LMC CLUSTER H11 pos_1: RA=06H14M50S, pos_2: DEC=-69D49'48", pos_3: REGION, R=7' equinox: 1950 pm_or_par: ^ rv_or_z: ^ comment_1: TARGETS 2 AND 3 WILL NOT BE comment_2: POINTED AT; THEY ARE QUOTED ONLY comment_3: IN ORDER TO DEFINE TARGETS 4-6. comment_4: TARGETS 7-9 ARE PARALLEL FIELDS comment_5: FOR PC WHILE FOC96 IS OBSERVING comment_6: PRIMARY TARGETS. ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 sequence_1: DEF sequence_2: STD targname: # config: FOC/96 opmode: IMAGE aperture: 512X1024 sp_element: F430W num_exp: 1 time_per_exp: 1500S s_to_n: 30 fluxnum_1: 2 priority: # ! linenum: 2.000 sequence_1: ^ targname: # config: FOC/96 opmode: ^ aperture: 512X1024 sp_element: F480LP num_exp: ^ time_per_exp: ^ s_to_n: 50 fluxnum_1: 1 priority: # req_1: SAME ORIENT FOR 2 AS 1; req_2: SAME POS FOR 2 AS 1 ! linenum: 3.000 sequence_1: ^ targname: # config: FOC/96 opmode: ^ aperture: 512X1024 sp_element: F342W num_exp: ^ time_per_exp: 600S s_to_n: 20 fluxnum_1: 3 priority: # req_1: SAME ORIENT FOR 3 AS 1; req_2: SAME POS FOR 3 AS 1 ! linenum: 4.000 sequence_1: DEFINE sequence_2: STDPAR targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F555W num_exp: 1 time_per_exp: 1500S priority: # ! linenum: 5.000 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F785LP num_exp: 1 time_per_exp: 1500S priority: # param_1: CR-SPLIT=NO ! linenum: 6.000 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F785LP num_exp: 1 time_per_exp: 600S priority: # param_1: CR-SPLIT=NO ! linenum: 7.000 sequence_1: USE sequence_2: STD targname: LINDSAY-1 priority: 1 req_1: ORIENT 00D+/-30D; req_2: CYCLE 2 /7-9; req_3: DARK TIME ! linenum: 8.000 sequence_1: ^ targname: L11-OFF1 priority: 2 req_1: ORIENT 00D+/-10D; req_2: DARK TIME ! linenum: 9.000 sequence_1: ^ targname: H11-OFF priority: ^ req_1: ORIENT 00D +/- 30D; req_2: DARK TIME comment_1: ORIENT 180D +/- 30D IS EQUALLY comment_2: ACCEPTABLE. ! linenum: 10.000 targname: L11-OFF2 config: PC opmode: IMAGE aperture: ALL sp_element: F555W num_exp: 1 time_per_exp: 1500S s_to_n: 60 fluxnum_1: 1 priority: 3 req_1: ORIENT 180D +/- 0.1D FROM 8; req_2: SELECT 1 OF 10-15 OR 16-19 OR 20-21; req_3: CYCLE 2 / 10-21; req_4: DARK TIME comment_1: LINES 10-21. CAN BE TAKEN WITH comment_2: SUN NEAR V1,+V3 PLANE. comment_3: BUT SOLAR ANGLE WILL BE BETTER IF comment_4: THESE ARE TAKEN WITH SUN NEAR 30D comment_5: OFF V1,+V3, AROUND MAY 1 ! linenum: 11.000 targname: FLD-L11 config: FOC/96 opmode: IMAGE aperture: 512X1024 sp_element: F430W num_exp: ^ time_per_exp: ^ s_to_n: 30 priority: 3 req_1: PAR WITH 10; req_2: DARK TIME ! linenum: 12.000 targname: L11-OFF2 config: PC opmode: ^ aperture: ALL sp_element: F785LP num_exp: ^ time_per_exp: ^ s_to_n: 50 fluxnum_1: 4 priority: 3 param_1: CR-SPLIT=NO req_1: SAME ORIENT FOR 12 AS 10; req_2: SAME POS FOR 12 AS 10; req_3: DARK TIME ! linenum: 13.000 targname: FLD-L11 config: FOC/96 opmode: IMAGE aperture: 512X1024 sp_element: F480LP num_exp: ^ time_per_exp: ^ s_to_n: ^ priority: 3 req_1: PAR WITH 12; req_2: DARK TIME ! linenum: 14.000 targname: L11-OFF2 config: PC opmode: ^ aperture: ALL sp_element: F785LP num_exp: ^ time_per_exp: 600S s_to_n: 30 fluxnum_1: 4 priority: 3 param_1: CR-SPLIT=NO req_1: SAME ORIENT FOR 14 AS 10; req_2: SAME POS FOR 14 AS 10; req_3: DARK TIME ! linenum: 15.000 targname: FLD-L11 config: FOC/96 opmode: IMAGE aperture: 512X1024 sp_element: F342W num_exp: ^ time_per_exp: ^ s_to_n: 20 priority: 3 req_1: PAR WITH 14; req_2: DARK TIME ! linenum: 16.000 targname: L11-OFF2 config: PC opmode: ^ aperture: ALL sp_element: F785LP num_exp: ^ time_per_exp: 1500S s_to_n: 50 fluxnum_1: 4 priority: 3 param_1: CR-SPLIT=NO req_1: ORIENT 180D+/- 10D; req_2: SELECT 1 OF 10-15 OR 16-19 OR 20-21; req_3: DARK TIME ! linenum: 17.000 targname: FLD-L11 config: FOC/96 opmode: IMAGE aperture: 512X1024 sp_element: F430W num_exp: ^ time_per_exp: ^ s_to_n: 30 priority: 3 req_1: PAR WITH 16; req_2: DARK TIME ! linenum: 18.000 targname: L11-OFF2 config: PC opmode: ^ aperture: ALL sp_element: F785LP num_exp: ^ time_per_exp: 600S s_to_n: 30 fluxnum_1: 4 priority: 3 param_1: CR-SPLIT=NO req_1: SAME ORIENT FOR 18 AS 16; req_2: SAME POS FOR 18 AS 16; req_3: DARK TIME ! linenum: 19.000 targname: FLD-L11 config: FOC/96 opmode: IMAGE aperture: 512X1024 sp_element: F342W num_exp: ^ time_per_exp: ^ s_to_n: 20 priority: 3 req_1: PAR WITH 18; req_2: DARK TIME comment_1: IF TIME RESTRICTIONS APPLY, TAKE comment_2: 20-21 OR 16-19 INSTEAD OF 10-15. IF comment_3: POSSIBLE, NO PC READOUT BETWEEN 12 comment_4: AND 14 OR BETWEEN 16 AND 18. ! linenum: 20.000 targname: L11-OFF2 config: PC opmode: IMAGE aperture: ALL sp_element: F785LP num_exp: 1 time_per_exp: 1500S s_to_n: 50 fluxnum_1: 4 priority: 3 req_1: ORIENT 180D+/- 10D; req_2: DARK TIME ! linenum: 21.000 targname: FLD-L11 config: FOC/96 opmode: IMAGE aperture: 512X1024 sp_element: F430W num_exp: ^ time_per_exp: ^ s_to_n: 30 priority: 3 req_1: PAR WITH 20; req_2: SELECT 1 OF 10-15 OR 16-19 OR 20-21; req_3: DARK TIME ! linenum: 22.000 sequence_1: USE sequence_2: STDPAR targname: FLD-L1 priority: 1 req_1: PAR WITH 7; req_2: DARK TIME ! linenum: 23.000 sequence_1: ^ targname: FLD-L11 priority: 2 req_1: PAR WITH 8; req_2: DARK TIME ! linenum: 24.000 sequence_1: ^ targname: FLD-H11 priority: 2 req_1: PAR WITH 9; req_2: DARK TIME ! ! end of exposure logsheet ! No scan data records found