! File: 2537C.PROP ! Database: PEPDB ! Date: 17-FEB-1994:07:50:26 coverpage: title_1: PHYSICAL CONDITIONS OF INTERSTELLAR GAS WITHIN 50 PARSECS sci_cat: INTERSTELLAR MEDIUM proposal_for: GO pi_title: DR. pi_fname: ROGER pi_lname: FERLET pi_inst: INSTITUTE FOR ASTROPHYSICS, PARIS pi_country: FRANCE pi_phone: 33-1-4320-1425 keywords_1: PHYSICS OF THE INTERSTELLAR MEDIUM, LOCAL INTERSTELLAR keywords_2: MEDIUM hours_pri: 10.00 num_pri: 3 hrs: X pi_position: DOCTOR off_fname: ALAIN off_lname: OMONT off_title: DIRECTOR off_inst: INSTITUT D'ASTROPHYSIQUE DE PARIS off_addr_1: 98 BIS BD. ARAGO off_city: PARIS off_zip: 75014 off_country: FRANCE off_phone: 33-1-4320-1425 off_telex: 205671 IAUF ! end of coverpage abstract: line_1: Models of the diffuse interstellar medium still lack definite line_2: observational proofs, in particular on small scale lengths (<10pc). They line_3: predict interfaces between cold dense clouds and a hot "coronal" very tenuous line_4: widely spread phase. These interfaces need to be directly obseved and studied line_5: because they offer a unique chance to understand the role of shocks, the nature line_6: of the evaporation zones, the grain destruction, the extent of the warm gas line_7: phase. All these problems can only tackled in details in the very local line_8: interstellar medium where the low column-densities of individual absorption line_9: regions are not hidden and can be well enough located. line_10: From ground-based studies, we have pointed out a new image of the nearby line_11: instellar medium. At least four velocity components are present within 20 pc. line_12: For two of them, we were able to delineate approximate frontiers toward which line_13: it is very promissing to search for interfaces. Furthermore, we found some line_14: evidence for a temperature structure within one of these components, providing line_15: therefore a prime target. line_16: Since visual observations do not offer adequate diagnostic lines and line_17: available UV data do not have the needed spectral resolution, we propose to line_18: perform with HRS a much more complete physical study of the cold and warm local line_19: gas. The selected diagnostic lines are those of AlII, FeII, MnII, MgI, line_20: and CIV, to be observed toward nearby stars in directions where confusion betwee ! ! end of abstract general_form_proposers: lname: BALLET fname: JEAN inst: ATOMIC ENERGY COMMISSION, FRANCE country: FRANCE esa: X ! lname: FERLET fname: ROGER title: P.I. inst: CNRS, INSTITUTE FOR ASTROPHYSICS, PARIS country: FRANCE esa: X ! lname: LALLEMENT fname: ROSINE inst: CNRS, DEPARTMENT OF AERONOMY country: FRANCE esa: X ! lname: VIDAL-MADJAR fname: ALFRED inst: CNRS, INSTITUTE FOR ASTROPHYSICS, PARIS country: FRANCE esa: X ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: The target stars were carefully selected,owing to ground line_2: based studies. Through exposures with ECH-B at 2346A (Fe II), line_3: 2596A (Fe II, Mn II), 2852A (Mg I), 1859A (Al III) and with line_4: G160M at 1671A (Al II), and using the profile fitting method, line_5: we will find the detailed velocity structure of the line of line_6: sight, the neutrals behaviour and will have access to line_7: temperature, electron density, ionization state and depletion line_8: informations. The 1550A line (C IV) will reveal the hotter line_9: phases of the local ISM; being wider, the G160M resolution is line_10: still adequate. G160M spectra will be also completed to line_11: evaluate more precisely the scattered light levels. All the line_12: observations are made in the accumulation mode through the line_13: 0.25 arc sec science aperture, still usable for our very line_14: bright targets, to keep the resolution, with a S/N ratio of line_15: at least 100. No unusually stringent requirements are line_16: foreseen, although we need accurate heliocentric velocity line_17: scales; for this, we add wave lamp calibrations at each line_18: wavelength and at each about 20 min during long exposures. ! question: 4 section: 1 line_1: The proposed programme can only be achieved by line_2: observing resonance lines of different elements in various line_3: stages of ionization, which are only available in the UV. line_4: High spectral resolution is mandatory in order to resolve the line_5: velocity structure of the lines of sight, to measure b-values line_6: of 0.5 km/s (1/10 of the spectral resolution corresponding to line_7: 500K in the case of Mg), i.e. to study individual absorbing line_8: regions. Copernicus studies were limited to O and B stars at line_9: more than 50pc. IUE does not provide the spectral resolution line_10: needed. Ground based telescopes provide the spectral resolu- line_11: tion but not adequate diagnostic lines. Nevertheless our line_12: extensive optical studies have revealed the compexity of the line_13: local ISM and the most suitable regions where to search for line_14: interfaces of diffuse interstellar clouds, and regions where line_15: the overlaps in the velocity space will be minimized. ! question: 5 section: 1 line_1: This study requires a survey type program. In order line_2: to minimize the number of exposures we selected only 6 ECH line_3: grating positions, distributed among the target stars line_4: according to their brightness. All fluxes are estimated line_5: from published direct UV observations or from similar scaled line_6: stars. Account has been taken for the scattered light, for line_7: the ripple function and for the decreased stellar flux in the line_8: wings of broad stellar lines when appropriate. As an example, line_9: consider the Al III line toward Beta Car. The flux at 1859A line_10: is 86E-11 erg/cm2/s/A. The new OTA + 2.0" aperture + GHRS line_11: ECH-B system sensitivity is 1.6E+11, the scattered light is line_12: 0.15 and the ripple is 0.84. This leads to a 408s exposure line_13: to reach a S/N of 100. ! question: 6 section: 1 line_1: Because we need the best possible accuracy in velocities, we line_2: will complete a spectral calibration at each setting of the line_3: HRS instrument and every about 20 min during long exposures. line_4: To reach a better evaluation of the scattered light in the line_5: echelle modes, we plan lower resolution spectra with an line_6: holographic grating. Two exposures for determining the line_7: instrumental profile are also performed. Standard procedures line_8: are used to resolve the photocathode granularity problem line_9: along with sub-stepping to improve the spectral resolution, line_10: and take care of the geomagnetic drift. Images of the line_11: aperture are also required in order to improve the line_12: wavelength scale. Because this is time consuming, we line_13: assumed that no changes should appear over successive orbits. line_14: We thus required NO GAP between observations completed on a line_15: given star. Also some observations are required to be sche- line_16: duled within 30min to link them as tightly as possible. ! question: 7 section: 1 line_1: We will make use of the Routine Science Data Processing line_2: and of the Calibration Data Base Software. We will make line_3: additional use of the Science Data Analysis System (SDAS) line_4: at the Institute, or of the MIDAS system available at our line_5: Institute. We have ready access to good computational line_6: facilities at our home institution for any further analysis. line_7: This includes, in particular, the profile fitting program line_8: initially built for analysing Copernicus data. ! question: 10 section: 1 line_1: As indicated in item 7, extensive data analysis capabilities line_2: exist at our home institutions. All proposers are appointed line_3: by CNRS or CEA in France. ! !end of general form text general_form_address: lname: FERLET fname: ROGER title: DR. category: PI inst: INSTITUT D'ASTROPHYSIQUE DE PARIS addr_1: 98 BIS BD. ARAGO city: PARIS zip: 75014 country: FRANCE ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: HD216956 name_2: HR8728 name_3: ALPHA PISCIS AUSTRINI descr_1: STAR; TYPE=A3 V pos_1: RA = 22H 57M 39.0S +/- 0.03", pos_2: DEC = -29D 37' 20.0" +/- 0.03" equinox: 2000 pm_or_par: Y pos_epoch_bj: J pos_epoch_yr: 2000.00 ra_pm_val: 0.022400 ra_pm_unct: 0.000067 dec_pm_val: -0.1610 dec_pm_unct: 0.0010 an_prlx_val: 0.1490 an_prlx_unct: 0.0050 rv_or_z: V = +7 comment_1: REFERENCE FOR UV FLUX - comment_2: CODE MEADE, 1979, AP.J.SUPPL. comment_3: S/N REQUIRED AT BOTTOM OF comment_4: STELLAR ABSORPTION LINES. fluxnum_1: 1 fluxval_1: V = 1.16 +/- 0.2 fluxnum_2: 2 fluxval_2: B-V = +.09 fluxnum_3: 3 fluxval_3: F(1550) = 20 +/- 15 E-11 fluxnum_4: 4 fluxval_4: F(1670) = 55 +/- 20 E-11 fluxnum_5: 5 fluxval_5: F(1859) = 105 +/- 40 E-11 fluxnum_6: 6 fluxval_6: F(2345) = 62 +/- 20 E-11 fluxnum_7: 7 fluxval_7: F(2596) = 70 +/- 30 E-11 fluxnum_8: 8 fluxval_8: F(2852) = 82 +/- 30 E-11 ! targnum: 2 name_1: HD102647 name_2: HR4534 name_3: BETA LEONIS descr_1: STAR; TYPE=A3 V pos_1: RA = 11H 49M 03.5S +/- 0.03", pos_2: DEC = +14D 34' 19.0" +/- 0.03" equinox: 2000 pm_or_par: Y pos_epoch_bj: J pos_epoch_yr: 2000.00 ra_pm_val: -0.033133 ra_pm_unct: 0.000067 dec_pm_val: -0.1190 dec_pm_unct: 0.0010 an_prlx_val: 0.0820 an_prlx_unct: 0.0050 comment_1: REFERENCE FOR UV FLUX - comment_2: CODE MEADE, 1979, AP.J.SUPPL. comment_3: S/N REQUIRED AT BOTTOM OF comment_4: STELLAR ABSORPTION LINES. fluxnum_1: 1 fluxval_1: V = 2.14 +/- 0.01 fluxnum_2: 2 fluxval_2: B-V = +0.09 fluxnum_3: 3 fluxval_3: F(1550) = 8 +/- 4 E-11 fluxnum_4: 4 fluxval_4: F(1670) = 28 +/- 10 E-11 fluxnum_5: 5 fluxval_5: F(1859) = 52 +/- 15 E-11 fluxnum_6: 6 fluxval_6: F(2345) = 30 +/- 10 E-11 fluxnum_7: 7 fluxval_7: F(2596) = 35 +/- 10 E-11 fluxnum_8: 8 fluxval_8: F(2852) = 37 +/- 10 E-11 ! targnum: 3 name_1: HD80007 name_2: HR3685 name_3: BETA CARINAE descr_1: STAR; TYPE=A2 IV pos_1: RA = 09H 13M 12.1S +/- 0.03", pos_2: DEC = -69D 43' 02.0" +/- 0.03" equinox: 2000 pm_or_par: Y pos_epoch_bj: J pos_epoch_yr: 2000.00 ra_pm_val: -0.029400 ra_pm_unct: 0.000067 dec_pm_val: 0.1020 dec_pm_unct: 0.0010 an_prlx_val: 0.0210 an_prlx_unct: 0.0020 rv_or_z: V = -5 comment_1: REFERENCE FOR UV FLUX - comment_2: CODE MEADE, 1979, AP.J.SUPPL. comment_3: S/N REQUIRED AT BOTTOM OF comment_4: STELLAR ABSORPTION LINES. fluxnum_1: 1 fluxval_1: V = 1.68 +/- 0.2 fluxnum_2: 2 fluxval_2: B-V = -0.00 fluxnum_3: 3 fluxval_3: F(1550) = 95 +/- 40 E-11 fluxnum_4: 4 fluxval_4: F(1670) = 87 +/- 30 E-11 fluxnum_5: 5 fluxval_5: F(1859) = 86 +/- 30 E-11 fluxnum_6: 6 fluxval_6: F(2345) = 52 +/- 20 E-11 fluxnum_7: 7 fluxval_7: F(2596) = 55 +/- 15 E-11 fluxnum_8: 8 fluxval_8: F(2852) = 56 +/- 15 E-11 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.010 targname: HD216956 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 1.8S fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: SEARCH-SIZE = 3 param_2: BRIGHT = 65535.0 param_3: FAINT = 8000.0 param_4: LOCATE = YES req_1: ONBOARD ACQ FOR 1.02; req_2: CYCLE 1; comment_1: COUNT RATE FOR MIRROR A2 comment_2: STEP TIME IS 0.2S comment_3: TO GIVE 25000 CNTS/STEP. ! linenum: 1.020 targname: HD216956 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 1 fluxnum_2: 2 priority: 1 req_1: ONBOARD ACQ FOR 1.03-1.05; req_2: CYCLE 1; comment_1: STEP TIME IS 0.2S ! linenum: 1.030 targname: HD216956 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1859.55 num_exp: 1 time_per_exp: 276.0S s_to_n: 100. s_to_n_time: 276.0S fluxnum_1: 5 priority: 1 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 1.040 targname: HD216956 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1542.5 num_exp: 3 time_per_exp: 1214.0S s_to_n: 140. s_to_n_time: 3642.0S fluxnum_1: 3 priority: 1 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 1.050 targname: HD216956 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1663.0 num_exp: 1 time_per_exp: 616.0S s_to_n: 100. s_to_n_time: 616.0S fluxnum_1: 4 priority: 1 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 1.055 targname: HD216956 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 1.8S fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: SEARCH-SIZE = 3 param_2: BRIGHT = 65535.0 param_3: FAINT = 8000.0 param_4: LOCATE = YES req_1: ONBOARD ACQ FOR 1.056; req_2: CYCLE 1; comment_1: COUNT RATE FOR MIRROR A2 comment_2: STEP TIME IS 0.2S comment_3: TO GIVE 25000 CNTS/STEP. ! linenum: 1.056 targname: HD216956 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 1 fluxnum_2: 2 priority: 1 req_1: ONBOARD ACQ FOR 1.06-1.15; req_2: CYCLE 1; comment_1: STEP TIME IS 0.2S ! linenum: 1.060 targname: HD216956 config: HRS opmode: ACCUM aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 14.4S fluxnum_1: 1 fluxnum_2: 2 priority: 1 req_1: SEQ 1.06-1.07 NON-INT; req_2: SEQ 1.06-1.15 NO GAP; req_3: CYCLE 1; comment_1: MEASUREMENT OF RELATIVE OFFSET comment_2: BETWEEN TARGET AND LAMP ! linenum: 1.070 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 14.4S priority: 1 req_1: CYCLE 1; comment_1: MEASUREMENT OF RELATIVE OFFSET comment_2: BETWEEN TARGET AND LAMP ! linenum: 1.080 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 1859.55 num_exp: 1 time_per_exp: 140.0S priority: 1 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD, param_3: COMB = FOUR req_1: CALIB FOR 1.09; req_2: SEQ 1.08-1.09 NON-INT; req_3: CYCLE 1; ! linenum: 1.090 targname: HD216956 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 1859.55 num_exp: 1 time_per_exp: 1198.0S s_to_n: 100. s_to_n_time: 1198.0S fluxnum_1: 5 priority: 1 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD, param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 1.100 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2345.91 num_exp: 1 time_per_exp: 80.0S priority: 1 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD, param_3: COMB = FOUR req_1: CALIB FOR 1.11; req_2: SEQ 1.10-1.11 NON-INT; req_3: CYCLE 1; ! linenum: 1.110 targname: HD216956 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2345.91 num_exp: 1 time_per_exp: 217.0S s_to_n: 100. s_to_n_time: 217.0S fluxnum_1: 6 priority: 1 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD, param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 1.120 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2596.84 num_exp: 1 time_per_exp: 90.0S priority: 1 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD, param_3: COMB = FOUR req_1: CALIB FOR 1.13; req_2: SEQ 1.12-1.13 NON-INT; req_3: CYCLE 1; ! linenum: 1.130 targname: HD216956 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2596.84 num_exp: 1 time_per_exp: 318.0S s_to_n: 100. s_to_n_time: 318.0S fluxnum_1: 7 priority: 1 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD, param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 1.140 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2854.85 num_exp: 1 time_per_exp: 130.0S priority: 1 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD, param_3: COMB = FOUR req_1: CALIB FOR 1.15; req_2: SEQ 1.14-1.15 NON-INT; req_3: CYCLE 1; ! linenum: 1.150 targname: HD216956 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2854.85 num_exp: 1 time_per_exp: 828.0S s_to_n: 200. s_to_n_time: 828.0S fluxnum_1: 8 priority: 1 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD, param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.010 targname: HD102647 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 1.8S fluxnum_1: 1 fluxnum_2: 2 priority: 2 param_1: SEARCH-SIZE = 3, param_2: BRIGHT = 65535.0, param_3: FAINT = 3000.0, param_4: LOCATE = YES req_1: ONBOARD ACQ FOR 2.02; req_2: CYCLE 1; comment_1: COUNT RATE FOR MIRROR A2 comment_2: STEP TIME IS 0.2S comment_3: TO GIVE 9200 CNTS/STEP. ! linenum: 2.020 targname: HD102647 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 1 fluxnum_2: 2 priority: 2 req_1: ONBOARD ACQ FOR 2.03-2.05; req_2: CYCLE 1; comment_1: STEP TIME IS 0.2S ! linenum: 2.030 targname: HD102647 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1859.55 num_exp: 1 time_per_exp: 540.0S s_to_n: 100. s_to_n_time: 540.0S fluxnum_1: 5 priority: 2 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.040 targname: HD102647 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1542.5 num_exp: 6 time_per_exp: 1161.0S s_to_n: 120. s_to_n_time: 6966.0S fluxnum_1: 3 priority: 2 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.050 targname: HD102647 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1663.0 num_exp: 1 time_per_exp: 1212.0S s_to_n: 100. s_to_n_time: 1212.0S fluxnum_1: 4 priority: 2 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.055 targname: HD102647 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 1.8S fluxnum_1: 1 fluxnum_2: 2 priority: 2 param_1: SEARCH-SIZE = 3, param_2: BRIGHT = 65535.0, param_3: FAINT = 3000.0, param_4: LOCATE = YES req_1: ONBOARD ACQ FOR 2.056; req_2: CYCLE 1; comment_1: COUNT RATE FOR MIRROR A2 comment_2: STEP TIME IS 0.2S comment_3: TO GIVE 9200 CNTS/STEP. ! linenum: 2.056 targname: HD102647 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 1 fluxnum_2: 2 priority: 2 req_1: ONBOARD ACQ FOR 2.06-2.15; req_2: CYCLE 1; comment_1: STEP TIME IS 0.2S ! linenum: 2.060 targname: HD102647 config: HRS opmode: ACCUM aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 14.4S fluxnum_1: 1 fluxnum_2: 2 priority: 2 req_1: SEQ 2.06-2.07 NON-INT; req_2: SEQ 2.06-2.15 NO GAP; req_3: CYCLE 1; comment_1: MEASUREMENT OF RELATIVE OFFSET comment_2: BETWEEN TARGET AND LAMP ! linenum: 2.070 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 14.4S priority: 2 req_1: CYCLE 1; comment_1: MEASUREMENT OF RELATIVE OFFSET comment_2: BETWEEN TARGET AND LAMP ! linenum: 2.080 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 1859.55 num_exp: 1 time_per_exp: 140.0S priority: 2 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CALIB FOR 2.09; req_2: SEQ 2.08-2.09 NON-INT; req_3: CYCLE 1; ! linenum: 2.090 targname: HD102647 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 1859.55 num_exp: 1 time_per_exp: 1215.0S s_to_n: 100. s_to_n_time: 2430.0S fluxnum_1: 5 priority: 2 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.091 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 1859.55 num_exp: 1 time_per_exp: 140.0S priority: 2 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CALIB FOR 2.092; req_2: SEQ 2.091-2.092 NON-INT; req_3: CYCLE 1; ! linenum: 2.092 targname: HD102647 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 1859.55 num_exp: 1 time_per_exp: 1215.0S s_to_n: 100. s_to_n_time: 2430.0S fluxnum_1: 5 priority: 2 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.100 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2345.91 num_exp: 1 time_per_exp: 80.0S priority: 2 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CALIB FOR 2.11; req_2: SEQ 2.10-2.11 NON-INT; req_3: CYCLE 1; ! linenum: 2.110 targname: HD102647 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2345.91 num_exp: 1 time_per_exp: 450.0S s_to_n: 100. s_to_n_time: 450.0S fluxnum_1: 6 priority: 2 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.120 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2596.84 num_exp: 1 time_per_exp: 90.0S priority: 2 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CALIB FOR 2.13; req_2: SEQ 2.12-2.13 NON-INT; req_3: CYCLE 1; ! linenum: 2.130 targname: HD102647 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2596.84 num_exp: 1 time_per_exp: 649.0S s_to_n: 100. s_to_n_time: 649.0S fluxnum_1: 7 priority: 2 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.140 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2854.85 num_exp: 1 time_per_exp: 130.0S priority: 2 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CALIB FOR 2.15; req_2: SEQ 2.14-2.15 NON-INT; req_3: CYCLE 1; ! linenum: 2.150 targname: HD102647 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2854.85 num_exp: 1 time_per_exp: 1100.0S s_to_n: 200. s_to_n_time: 2200.0S fluxnum_1: 8 priority: 2 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.151 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2854.85 num_exp: 1 time_per_exp: 130.0S priority: 2 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CALIB FOR 2.152; req_2: SEQ 2.151-2.152 NON-INT; req_3: CYCLE 1; ! linenum: 2.152 targname: HD102647 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2854.85 num_exp: 1 time_per_exp: 1100.0S s_to_n: 200. s_to_n_time: 2200.0S fluxnum_1: 8 priority: 2 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.010 targname: HD80007 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 1.8S fluxnum_1: 1 fluxnum_2: 2 priority: 3 param_1: SEARCH-SIZE = 3 param_2: BRIGHT = 65535.0 param_3: FAINT = 9000.0 param_4: LOCATE = YES req_1: ONBOARD ACQ FOR 3.02; req_2: CYCLE 1; comment_1: COUNT RATE FOR MIRROR A2 comment_2: STEP TIME IS 0.2S comment_3: TO GIVE 28000 CNTS/STEP. ! linenum: 3.020 targname: HD80007 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 1 fluxnum_2: 2 priority: 3 req_1: ONBOARD ACQ FOR 3.03-3.05; req_2: CYCLE 1; comment_1: STEP TIME IS 0.2S ! linenum: 3.030 targname: HD80007 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1859.55 num_exp: 1 time_per_exp: 325.0S s_to_n: 100. s_to_n_time: 325.0S fluxnum_1: 5 priority: 3 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.040 targname: HD80007 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1542.5 num_exp: 1 time_per_exp: 760.0S s_to_n: 140. s_to_n_time: 760.0S fluxnum_1: 3 priority: 3 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.050 targname: HD80007 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1663.0 num_exp: 1 time_per_exp: 388.0S s_to_n: 100. s_to_n_time: 388.0S fluxnum_1: 4 priority: 3 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.055 targname: HD80007 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 1.8S fluxnum_1: 1 fluxnum_2: 2 priority: 3 param_1: SEARCH-SIZE = 3 param_2: BRIGHT = 65535.0 param_3: FAINT = 9000.0 param_4: LOCATE = YES req_1: ONBOARD ACQ FOR 3.056; req_2: CYCLE 1; comment_1: COUNT RATE FOR MIRROR A2 comment_2: STEP TIME IS 0.2S comment_3: TO GIVE 28000 CNTS/STEP. ! linenum: 3.056 targname: HD80007 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 1 fluxnum_2: 2 priority: 3 req_1: ONBOARD ACQ FOR 3.06-3.15; req_2: CYCLE 1; comment_1: STEP TIME IS 0.2S ! linenum: 3.060 targname: HD80007 config: HRS opmode: ACCUM aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 14.4S fluxnum_1: 1 fluxnum_2: 2 priority: 3 req_1: SEQ 3.06-3.07 NON-INT; req_2: SEQ 3.06-3.15 NO GAP; req_3: CYCLE 1; comment_1: MEASUREMENT OF RELATIVE OFFSET comment_2: BETWEEN TARGET AND LAMP ! linenum: 3.070 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 14.4S priority: 3 req_1: CYCLE 1; comment_1: MEASUREMENT OF RELATIVE OFFSET comment_2: BETWEEN TARGET AND LAMP ! linenum: 3.080 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 1859.55 num_exp: 1 time_per_exp: 140.0S priority: 3 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CALIB FOR 3.09; req_2: SEQ 3.08-3.09 NON-INT; req_3: CYCLE 1; ! linenum: 3.090 targname: HD80007 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 1859.55 num_exp: 1 time_per_exp: 1468.0S s_to_n: 100. s_to_n_time: 1468.0S fluxnum_1: 5 priority: 3 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.100 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2345.91 num_exp: 1 time_per_exp: 80.0S priority: 3 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CALIB FOR 3.11; req_2: SEQ 3.10-3.11 NON-INT; req_3: CYCLE 1; ! linenum: 3.110 targname: HD80007 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2345.91 num_exp: 1 time_per_exp: 261.0S s_to_n: 100. s_to_n_time: 261.0S fluxnum_1: 6 priority: 3 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.120 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2596.84 num_exp: 1 time_per_exp: 150.0S priority: 3 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CALIB FOR 3.13; req_2: SEQ 3.12-3.13 NON-INT; req_3: CYCLE 1; ! linenum: 3.130 targname: HD80007 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2596.84 num_exp: 1 time_per_exp: 405.0S s_to_n: 100. s_to_n_time: 405.0S fluxnum_1: 7 priority: 3 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.140 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2854.85 num_exp: 1 time_per_exp: 145.0S priority: 3 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CALIB FOR 3.15; req_2: SEQ 3.14-3.15 NON-INT; req_3: CYCLE 1; ! linenum: 3.150 targname: HD80007 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2854.85 num_exp: 1 time_per_exp: 1600.0S s_to_n: 200. s_to_n_time: 1600.0S fluxnum_1: 8 priority: 3 param_1: STEP-PATT = 7, param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CYCLE 1; comment_1: S/N PER SUBSTEP PIXEL. ! ! end of exposure logsheet ! 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