! File: 1372C.PROP ! Database: PEPDB ! Date: 16-FEB-1994:16:30:01 coverpage: title_1: DOPPLER COMPENSATION AND ECHELLE A SCATTERED LIGHT proposal_for: SV/HRS pi_fname: DENNIS pi_mi: C. pi_lname: EBBETS pi_inst: BALL AEROSPACE SYSTEMS GROUP pi_country: USA pi_phone: (303)939-5964 keywords_1: HRS, CALIBRATION, SCIENCE VERIFICATION hours_pri: 3.00 num_pri: 1 hrs: Y ! end of coverpage abstract: line_1: SV Test to validate proper operation of the flight software Doppler line_2: compensation processor, with a few selected measurements of scattered light in line_3: Echelle A. line_5: This is a revised proposal submitted in November 1985 in response to reviews of line_6: the OV-SV programs held since the original June 1985 submission. The only line_7: significant change is the inclusion of observations of the spectral calibration line_8: lamps on the Exposure Logsheets. line_10: Revised April 1989 for SV scrub plan. line_11: retained only orbit with Doppler On line_14: Updated 8/24/89 to change repeat on line 6 to repeat obs of 10 exposures due to line_15: inability to reference repeat lines. (PStanley) ! ! end of abstract general_form_proposers: lname: JURA fname: MIKE inst: UCLA country: USA ! lname: BRANDT fname: J. mi: C. inst: LASP/UNIV OF COLORADO country: USA ! lname: SAVAGE fname: B. mi: D. inst: UNIV. OF WISCONSIN country: USA ! lname: CARPENTER fname: K. mi: G. inst: NASA/GSFC country: USA ! lname: EBBETS fname: D. mi: C. inst: BALL AEROSPACE SYSTEMS GROUP country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: The star will be observed with Echelle A for one full orbit. line_2: Narrow interstellar lines in approximately 10 orders will be line_3: recorded. It will take 8 to 10 minutes to complete an observation of all of line_4: the lines. The complete set will be repeated 9 or 10 line_5: times. The Doppler processor will be active for the entire line_6: observation of the star. line_9: Observations of the on-board spectral calibration lamps will line_10: be made before and after those of the star. line_12: The purpose will be to monitor the stability of the wavelength line_13: calibration so that effects due to detector or spectrograph drifts can be line_14: distinguished from errors in the Doppler compensation process. line_16: If time permits, a scan of the same spectral region will be made line_17: with grating G140M. ! question: 5 section: 1 line_1: SV Prerequisties: line_3: HRS -05.2 Mode II Target Acquisition - Target Locate (Prop 1352) line_9: It is necessary for the the echelle exposures to line_10: span the full time of visibility for a full orbit in order to show line_11: the maximum doppler amplitudes. line_13: Guiding Tolerance: 0.015 arc seconds line_15: SV Minimum Plan: lines 1 - 8 line_16: SV Delta Plan: line 8.2,9 ! question: 6 section: 1 line_1: We wish to verify both the phase and amplitude of the Doppler correction. It line_2: is necessary to observe the target for the equivalent of at line_3: least one full orbit of visibility to encounter the maximum line_4: velocity amplitude variation. ! question: 7 section: 1 line_1: Individual Observations will be overlayed and cross-correlated to measure any line_2: residual shifts. Presence of a sinusoidal shift would be a measure of the line_3: error in the Doppler compensation. If the test is successful - no shifts line_4: detected - no updates or changes will be made by any data base. If an error is line_5: found, it may be traceable to incorrect data base parameters - dispersion line_6: models etc. - which would have to be corrected and updated. line_8: The central depths of saturated absorption lines will be measured to line_9: characterize scattered light. No changes to data bases are contemplated. ! question: 10 section: 1 line_1: Data analysis facilities line_2: Personnel line_3: Travel and publications support ! !end of general form text general_form_address: lname: JURA fname: MIKE category: CON inst: UCLA addr_1: DEPARTMENT OF ASTRONOMY city: LOS ANGELES state: CA zip: 90024 country: USA phone: 213-825-4302 ! lname: CARPENTER fname: KENNETH mi: G. inst: NASA/GSFC addr_1: CODE 680 city: GREENBELT state: MD zip: 20771 country: USA phone: 301-286 3453 ! lname: SAVAGE fname: BLAIR mi: D. category: CON inst: UNIV. OF WISCONSIN addr_1: DEPT. OF ASTRONOMY city: MADISON state: WI zip: 53706 country: USA phone: 608-262-4909 ! lname: EBBETS fname: DENNIS mi: C. category: PI inst: BALL AEROSPACE SYSTEMS GROUP addr_1: P.O. BOX 1062 FT-3 addr_2: COMMERCE AND ARAPHOE STS. city: BOULDER state: CO zip: 80306 country: USA phone: 303-939-5964 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: DELTA-SCO descr_1: BRIGHT, EARLY TYPE STAR pos_1: RA=16H 00M 20.04S +/- 0.5S, pos_2: DEC=-22D 37' 17.5" +/- 3.0", pos_3: PLATE-ID=001B equinox: 2000 pm_or_par: Y pos_epoch_yr: 1950.00 ra_pm_val: -0.000667 ra_pm_unct: 0.000067 dec_pm_val: -0.0250 dec_pm_unct: 0.0010 comment_1: SAO COORDINATES fluxnum_1: 1 fluxval_1: V=2.32 fluxnum_2: 2 fluxval_2: F-CONT(1355)=1.5 E-8 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 targname: DELTA-SCO config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A1 num_exp: 1 time_per_exp: 57.8S fluxnum_1: 1 priority: 1 param_1: MAP=END-POINT,FAINT=400, param_2: SEARCH-SIZE=5, req_1: ONBOARD ACQ FOR 3,6; req_2: CYCLE 0 / 1-9; ! linenum: 3.000 targname: ^ config: ^ opmode: IMAGE aperture: ^ sp_element: ^ num_exp: 1 time_per_exp: 96.8S fluxnum_1: 1 priority: 1 param_1: DELTA-X=1, param_2: DELTA-Y=1, param_3: PRECISION=HIGH, ! linenum: 4.000 targname: WAVE config: HRS opmode: OSCAN aperture: SC2 sp_element: ECH-A wavelength: 1514.703 num_exp: 1 time_per_exp: 340S s_to_n: 100 priority: 1 param_1: STEP-PATT=7, param_2: DOPPLER=DEF, param_3: OSCAN-MIN=37, param_4: OSCAN-MAX=46, param_5: COMB=NO, req_1: CALIB FOR 6; req_2: SEQ 4-8; comment_1: POSITION CARROUSEL FOR MLAMBDA=56044. ! linenum: 5.000 targname: ^ config: ^ opmode: ^ aperture: SC1 sp_element: ^ wavelength: ^ num_exp: 1 time_per_exp: ^ priority: 1 param_1: ^ req_1: CALIB FOR 6 ! linenum: 6.000 targname: DELTA-SCO config: ^ opmode: ^ aperture: 0.25 sp_element: ^ wavelength: ^ num_exp: 10 time_per_exp: ^ s_to_n: 80 fluxnum_1: 2 priority: 1 param_1: ^ comment_1: CONTINUALLY REPEAT LINE 6 FOR THE comment_2: EQUIVALENT OF ONE FULL ORBIT OF comment_3: TARGET VISIBILTIY. ! linenum: 7.000 targname: WAVE config: ^ opmode: ^ aperture: SC2 sp_element: ^ wavelength: ^ num_exp: 1 time_per_exp: ^ priority: 1 param_1: ^ req_1: CALIB FOR 6 ! linenum: 8.000 targname: ^ config: ^ opmode: ^ aperture: SC1 sp_element: ^ wavelength: ^ num_exp: 1 time_per_exp: ^ priority: 1 param_1: ^ req_1: CALIB FOR 6 ! linenum: 8.200 targname: DELTA-SCO config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A1 num_exp: 1 time_per_exp: 57.8S fluxnum_1: 1 priority: 1 param_1: MAP=END-POINT, param_2: FAINT=400, param_3: SEARCH-SIZE=5, req_1: ONBOARD ACQ FOR 9; req_2: COND IF SV DELTA PLAN; ! linenum: 9.000 targname: DELTA-SCO config: HRS opmode: WSCAN aperture: 0.25 sp_element: G140M wavelength: 1190-1610 num_exp: 1 time_per_exp: 840S s_to_n: 80 fluxnum_1: 2 priority: 1 param_1: WAVE-STEP=20, param_2: STEP-PATT=3, req_1: COND IF SV DELTA PLAN comment_1: 21 EXPS ON 20 A CENTERS: comment_2: 1200, 1220, 1240, ... 1600. comment_3: COMPUTE SPYBAL AT 1200, 1320, comment_4: 1440, 1560. NOTE: WAVELENGTH comment_5: RANGE SHOULD BE 1186.5-1613.5 comment_6: RPSS LIMIT=10 CHARACTERS. ! ! end of exposure logsheet ! No scan data records found