! File: 2536C.PROP ! Database: PEPDB ! Date: 17-FEB-1994:07:46:46 coverpage: title_1: DEUTERIUM IN THE LOCAL INTERSTELLAR GAS sci_cat: INTERSTELLAR MEDIUM sci_subcat: LOCAL MEDIUM proposal_for: GO pi_title: DR. pi_fname: ALFRED pi_lname: VIDAL-MADJAR pi_inst: INSTITUTE FOR ASTROPHYSICS, PARIS pi_country: FRANCE pi_phone: 33-1-4320-14-25 keywords_1: INTERSTELLAR DEUTERIUM ABUNDANCE; LOCAL INTERSTELLAR keywords_2: MEDIUM hours_pri: 6.70 num_pri: 7 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: 33-143201425 off_telex: 205671 IAUF ! end of coverpage abstract: line_1: Evaluation of the primordial deuterium abundance is one of the few crucial line_2: observational constraint one may be able to place on cosmological models. line_3: Several approaches were attempted, but none up to now has produced a clear-cut line_4: answer. Even the best available estimations, completed in the interstellar line_5: medium through the Lyman lines of HI and DI, lead to evidences of variations up line_6: to a factor of four. In the local interstellar medium, fluctuations line_7: seem to exist over scales of few parsecs. line_8: It is of prime importance to check the existence of these local variations line_9: and eventually understand their causes. HST with HRS is best adapted to line_10: perform this analysis started with Copernicus and the IUE. In particular, its line_11: high sensitivity allows to use also white dwarfs as target stars at the line_12: Lambda/Delta Lambda = 10^5 resolution. These observations will dramatically line_13: improve the previous error bars because: 1)the stellar continuum is well known, line_14: 2)the detailed line of sight structure is observable; 3)the HI content in each line_15: individual component is accessible. Furthermore, from an extensive high line_16: resolution ground-based survey we have completed toward nearby stars, we line_17: pointed out the presence of several local velocity components. In consequence, line_18: we have eliminated regions in the sky where only averaged cloud properties are line_19: accessible-we are looking for local fluctuations-and selected regions where line_20: confusion is minimized. The expected refined evaluation of the deuterium ! ! end of abstract general_form_proposers: lname: FERLET fname: ROGER inst: INSTITUTE FOR ASTROPHYSICS, CNRS, PARIS country: FRANCE esa: Y ! lname: LALLEMENT fname: ROSINE inst: CNRS, DEPARTMENT OF AERONOMY country: FRANCE esa: Y ! lname: VIDAL-MADJAR fname: ALFRED title: P.I. inst: INSTITUTE FOR ASTROPHYSICS, CNRS, PARIS country: FRANCE esa: Y ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: Among the observational strategies we selected the observation line_2: of white dwarfs to properly evaluate the D/H ratio. We selected line_3: them according to two criteria: first select two opposite line_4: direction in the sky where D/H variations seem to be the line_5: strongest (Sco-Cen and Aur) and second avoid area where confusion line_6: may arise from the complicate structure of the local ISM. line_7: For each of these white dwarfs three exposures in ECH-B mode line_8: are completed centered on FeII (2345A); MgII (2800A); MgI (2854) line_9: to have the velocity structure, the HI content, the ionization line_10: and depletion of each component along with four medium resolution line_11: exposures which will give HI, DI, and different ionization stages line_12: of the important elements N, O, Si, S, C. Only very bright OB stars line_13: could be used in the other observational strategies. Beta and line_14: Epsilon CMa were selected again according to their position in the line_15: sky. Seven ECH-B and nine G160M exposures, with two wavelength line_16: ranges in common for determining the instrumental function, are line_17: completed to analyze in depth the lines of sight, region by region, line_18: and properly evaluate the D/H ratio. line_19: No unusually stringent requirements are foreseen, although we need line_20: accurate (<1km/s) heliocentric velocity scales, and good representa- line_21: tion of the instrumental profile. ! 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 line of sight, to measure b-values line_6: of 0.4 km/s (1/10 of the spectral resolution corresponding to line_7: 400K 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 complexity 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: In order to minimize the number of exposures, we selected line_2: only 3 ECH-B positions for the white dwarf, and 7 for the B line_3: stars. The observing time released by switching from ECH-A line_4: to B allows to record several G160M positions which will line_5: keep all the science. All fluxes are estimated from published line_6: direct UV observations. Account has been taken for the line_7: scattered light, the decreased stellar flux in the wings of line_8: broad stellar lines and the order blaze when appropriate. line_9: As an example, consider DI and HI toward G191B2B. The flux line_10: at 1215A is 4E-13erg/cm2/s/A, reduced by a factor of line_11: 3 due to the stellar H I broad wing. The HRS G160M + 0.25 line_12: aperture sensitivity is 1E+11 (the scattered light is line_13: negligible). This leads to a 9400S exposure to reach a S/N line_14: ratio of about 120. Additional flux evaluations are given line_15: here for information: 1) HD44743; F(1608) = 16 +/- 5 E-09; line_16: F(1808) = 13 +/- 5 E-09; F(1850) = 10 +/- 5 E-09; F(2343) = 65 line_17: +/- 20 E-10; F(2378) = 64 +/- 20 E-10; F(2585) = 51 +/- 20 E-10 line_18: F(2800) = 39 +/- 20 E-10; F(2852) = 38 +/- 20 E-10. 2) HD52089; line_19: F(1608) = 18 +/- 5 E-09; F(1808) = 14 +/- 5 E-09; F(1850) = 12 line_20: +/- 5 E-09; F(2343) = 72 +/- 20 E-10; F(2378) = 77 +/- 20 E-10; line_21: F(2585) = 64 +/- 20 E-10; F(2800) = 53 +/- 20 E-10; F(2852) = 52 line_22: +/- 20 E-10. ! question: 6 section: 1 line_1: Because we need <1km/s accuracy we will complete a spectral line_2: calibration at each setting of the ECH-B mode. line_3: To reach a better evaluation of the scattered light in the line_4: echelle modes we complete lower resolution spectra with the line_5: holographic gratings. Standard procedures are also used to line_6: resolve the photocathode granularity problem along with line_7: sub-stepping to improve the spectral resolution. line_8: Images of the aperture are also required in order to improve line_9: the wavelength scale. Because this is time consuming, we line_10: assumed that no changes should appear over successive orbits. line_11: We thus required NO GAP between observations completed on a line_12: given star. Also some observations are required to be sche- line_13: duled within 30mn to link them as tightly as possible. ! question: 7 section: 1 line_1: We will make use of the Routine Science Data line_2: Processing and of the Calibration Data Base Software. We will line_3: make additional use of the Science Data Analysis System (SDAS)) line_4: (sdas) or of the MIDAS system, available at STScI, STECF and line_5: our institute. line_6: We have ready access too good computational facilities at our line_7: home institution for any further computations. This includes, line_8: in particular, the profile fitting program initially built line_9: 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 in France. ! !end of general form text general_form_address: lname: VIDAL-MADJAR 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: G191-B2B name_2: WD 0501+527 name_3: EG247 descr_1: STAR; WD; TYPE=DA1B pos_1: RA = 05H 05M 30.62S +/- 0.03", pos_2: DEC = +52D 49' 54.0" +/- 0.03" equinox: 2000 pm_or_par: Y pos_epoch_bj: J pos_epoch_yr: 2000.00 an_prlx_val: 0.0210 an_prlx_unct: 0.0020 comment_1: FLUXES ESTIMATED WITH T = 60000K comment_2: ABSORPTION LINE. comment_3: COORDINATES FROM GSC. comment_4: F(2342) = 20 +/- 2 E-13 comment_5: F(2825) = 10 +/- 1 E-13 fluxnum_1: 1 fluxval_1: V = 11.73 +/- 0.2 fluxnum_2: 2 fluxval_2: U = 10.95 fluxnum_3: 3 fluxval_3: B-V = -0.32 fluxnum_4: 4 fluxval_4: F(1190) = 13 +/- 3 E-12 fluxnum_5: 5 fluxval_5: F(1199) = 13 +/- 3 E-12 fluxnum_6: 6 fluxval_6: F(1206) = 13 +/- 3 E-12 fluxnum_7: 7 fluxval_7: F(1215) = 4 +/- 2 E-13 fluxnum_8: 8 fluxval_8: F(1250) = 13 +/- 2 E-12 fluxnum_9: 9 fluxval_9: F(1318) = 10 +/- 2 E-12 fluxnum_10: 10 fluxval_10: F(1408) = 10 +/- 2 E-12 ! targnum: 2 name_1: HD44743 name_2: HR2294 name_3: BETA-CMA descr_1: STAR; TYPE=B1 II-III; descr_2: BINARY COMP; V=9.8; SEP=88." pos_1: TBD-RT, pos_2: RA = 06H 22M 41.9S +/- 0.03", pos_3: DEC = -17D 57' 22.0" +/- 0.03" equinox: 2000 pm_or_par: Y pos_epoch_bj: J pos_epoch_yr: 2000.00 ra_pm_val: -0.000913 ra_pm_unct: 0.000067 dec_pm_val: -0.0040 dec_pm_unct: 0.0010 an_prlx_val: 0.0190 an_prlx_unct: 0.0050 rv_or_z: V = +34 comment_1: REFERENCE FOR UV FLUX: comment_2: THE COPERNICUS SURVEY comment_3: SNOW JENKINS, 1977, AP.J.SUPPL. comment_4: F(1550), F(2850) ESTIMATED FROM comment_5: CODE MEADE, 1979, AP.J.SUPPL. comment_6: S/N REQUIRED AT BOTTOM comment_7: OF STELLAR ABSORPTION LINES. fluxnum_1: 1 fluxval_1: V = 1.98 +/- 0.01 fluxnum_2: 2 fluxval_2: B-V = -0.23 fluxnum_3: 3 fluxval_3: F(1199) = 24 +/- 6 E-09 fluxnum_4: 4 fluxval_4: F(1215) = 38 +/- 15 E-10 fluxnum_5: 5 fluxval_5: F(1190) = 11 +/- 5 E-09 fluxnum_6: 6 fluxval_6: F(1259) = 30 +/- 20 E-09 fluxnum_7: 7 fluxval_7: F(1206) = 38 +/- 15 E-10 fluxnum_8: 8 fluxval_8: F(1335) = 30 +/- 20 E-09 fluxnum_9: 9 fluxval_9: F(1408) = 20 +/- 10 E-09 fluxnum_10: 10 fluxval_10: F(1542) = 17 +/- 5 E-09 ! targnum: 3 name_1: HD52089 name_2: HR2618 name_3: EPSILON-CMA descr_1: STAR; TYPE=B2 II; descr_2: BINARY COMP; V=7.5; SEP=7".5 pos_1: TBD-RT, pos_2: RA = 06H 58M 37.5S +/- 0.03", pos_3: DEC = -28D 58' 20.0" +/- 0.03" equinox: 2000 pm_or_par: Y pos_epoch_bj: J pos_epoch_yr: 2000.00 ra_pm_val: 0.000073 ra_pm_unct: 0.000067 dec_pm_val: 0.0020 dec_pm_unct: 0.0010 an_prlx_val: 0.0010 an_prlx_unct: 0.0050 rv_or_z: V = +27 comment_1: REFERENCE FOR UV FLUX: comment_2: THE COPERNICUS SURVEY comment_3: SNOW JENKINS, 1977, AP.J.SUPPL. comment_4: F(1550), F(2850) ESTIMATED FROM comment_5: CODE MEADE, 1979, AP.J.SUPPL. comment_6: S/N REQUIRED AT BOTTOM comment_7: OF STELLAR ABSORPTION LINES. fluxnum_1: 1 fluxval_1: V = 1.50 +/- 0.01 fluxnum_2: 2 fluxval_2: B-V = -0.21 fluxnum_3: 3 fluxval_3: F(1199) = 22 +/- 4 E-09 fluxnum_4: 4 fluxval_4: F(1215) = 3 +/- 1 E-09 fluxnum_5: 5 fluxval_5: F(1190) = 7 +/- 2 E-09 fluxnum_6: 6 fluxval_6: F(1259) = 15 +/- 5 E-09 fluxnum_7: 7 fluxval_7: F(1206) = 4 +/- 1 E-09 fluxnum_8: 8 fluxval_8: F(1335) = 34 +/- 20 E-09 fluxnum_9: 9 fluxval_9: F(1408) = 22 +/- 10 E-09 fluxnum_10: 10 fluxval_10: F(1542) = 17 +/- 5 E-09 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 targname: G191-B2B config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 1.8S fluxnum_1: 1 fluxnum_2: 2 fluxnum_3: 3 priority: 1 param_1: SEARCH-SIZE = 3 param_2: FAINT = 1000.0 param_3: LOCATE = YES req_1: ONBOARD ACQ FOR 1.01-1.11; req_2: CYCLE 1 / 1.00-3.30; req_3: SEQ 1.00-1.11 NO GAP; comment_1: COUNT RATE FOR MIRROR N2 comment_2: 90000 CNTS/S. STEP TIME IS 0.2S comment_3: TO GIVE 18000 CNTS/STEP. ! linenum: 1.010 targname: G191-B2B config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 20.4S fluxnum_1: 1 fluxnum_2: 2 fluxnum_3: 3 priority: 1 req_1: ONBOARD ACQ FOR 1.02-1.11 comment_1: COUNT RATE FOR MIRROR N2 comment_2: 90000 CNTS/S. STEP TIME IS 0.2S comment_3: TO GIVE 18000 CNTS/STEP. ! linenum: 1.020 targname: G191-B2B config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1203.5 num_exp: 10 time_per_exp: 1200.S s_to_n: 120. s_to_n_time: 9600.0S fluxnum_1: 6 priority: 1 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 1.030 targname: G191-B2B config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1247.5 num_exp: 2 time_per_exp: 1500.0S s_to_n: 60. s_to_n_time: 3000.0S fluxnum_1: 8 priority: 1 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 1.040 targname: G191-B2B config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1318.5 num_exp: 2 time_per_exp: 1500.0S s_to_n: 60. s_to_n_time: 3000.0S fluxnum_1: 9 priority: 1 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 1.050 targname: G191-B2B config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1409.0 num_exp: 2 time_per_exp: 1250.0S s_to_n: 60. s_to_n_time: 2500.0S fluxnum_1: 10 priority: 1 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 1.060 targname: G191-B2B 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 fluxnum_3: 3 priority: 1 req_1: SEQ 1.06-1.07 NON-INT 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 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: 2345.9 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 1.09; req_2: SEQ 1.08-1.09 NON-INT ! linenum: 1.090 targname: G191-B2B config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2345.9 num_exp: 1 time_per_exp: 1250.0S s_to_n: 60. s_to_n_time: 2500.0S priority: 1 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 1.091 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2345.9 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 1.092; req_2: SEQ 1.091-1.092 NON-INT ! linenum: 1.092 targname: G191-B2B config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2345.9 num_exp: 1 time_per_exp: 1250.0S s_to_n: 60. s_to_n_time: 2500.0S priority: 1 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 1.100 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2798.5 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 1.11; req_2: SEQ 1.10-1.11 NON-INT ! linenum: 1.110 targname: G191-B2B config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2798.5 num_exp: 1 time_per_exp: 1500.0S s_to_n: 60. s_to_n_time: 3000.0S priority: 1 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 1.115 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2798.5 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 1.12; req_2: SEQ 1.115-1.12 NON-INT ! linenum: 1.120 targname: G191-B2B config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2798.5 num_exp: 1 time_per_exp: 1500.0S s_to_n: 60. s_to_n_time: 3000.0S priority: 1 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.000 targname: HD44743 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 232.2S fluxnum_1: 1 fluxnum_2: 2 fluxnum_3: 3 priority: 2 param_1: MAP = DEF req_1: INT ACQ FOR 2.001-2.10 comment_1: COUNT RATE FOR MIRROR A2 comment_2: 2.0E6 CNTS/S. STEP TIME IS 0.2S comment_3: TO GIVE 90000 CNTS/STEP. ! linenum: 2.001 targname: HD44743 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 20.4S fluxnum_1: 1 fluxnum_2: 2 fluxnum_3: 3 priority: 2 req_1: SEQ 2.001-2.10 NO GAP comment_1: COUNT RATE FOR MIRROR A2 comment_2: 2.0E6 CNTS/S. STEP TIME IS 0.2S comment_3: TO GIVE 90000 CNTS/STEP. ! linenum: 2.020 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1203.5 num_exp: 16 time_per_exp: 94.0S s_to_n: 200. s_to_n_time: 94.0S fluxnum_1: 7 priority: 2 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.030 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1247.5 num_exp: 1 time_per_exp: 57.6S s_to_n: 200. s_to_n_time: 44.4S fluxnum_1: 6 priority: 2 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.040 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1318.5 num_exp: 1 time_per_exp: 57.6S s_to_n: 200. s_to_n_time: 33.2S fluxnum_1: 8 priority: 2 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.050 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1409.0 num_exp: 1 time_per_exp: 57.6S s_to_n: 200. s_to_n_time: 57.6S fluxnum_1: 9 priority: 2 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.060 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1542.5 num_exp: 1 time_per_exp: 84.0S s_to_n: 200. s_to_n_time: 84.0S fluxnum_1: 10 priority: 2 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.070 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1608.0 num_exp: 1 time_per_exp: 84.0S s_to_n: 200. s_to_n_time: 84.0S priority: 2 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.080 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1663.0 num_exp: 1 time_per_exp: 84.0S s_to_n: 200. s_to_n_time: 84.0S priority: 2 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.085 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1203.5 num_exp: 6 time_per_exp: 94.0S s_to_n: 200. s_to_n_time: 94.0S fluxnum_1: 7 priority: 2 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.090 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1810.0 num_exp: 1 time_per_exp: 88.8S s_to_n: 200. s_to_n_time: 88.8S priority: 2 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.100 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1859.5 num_exp: 1 time_per_exp: 106.8S s_to_n: 200. s_to_n_time: 106.8S priority: 2 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.101 targname: HD44743 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 232.2S fluxnum_1: 1 fluxnum_2: 2 fluxnum_3: 3 priority: 2 param_1: MAP = DEF req_1: INT ACQ FOR 2.102-2.26 comment_1: COUNT RATE FOR MIRROR A2 comment_2: 2.0E6 CNTS/S. STEP TIME IS 0.2S comment_3: TO GIVE 90000 CNTS/STEP. ! linenum: 2.102 targname: HD44743 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 20.4S fluxnum_1: 1 fluxnum_2: 2 fluxnum_3: 3 priority: 2 req_1: SEQ 2.102-2.26 NO GAP comment_1: COUNT RATE FOR MIRROR A2 comment_2: 2.0E6 CNTS/S. STEP TIME IS 0.2S comment_3: TO GIVE 90000 CNTS/STEP. ! linenum: 2.110 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 14.4S fluxnum_1: 1 fluxnum_2: 2 priority: 2 req_1: SEQ 2.11-2.12 NON-INT comment_1: MEASUREMENT OF RELATIVE OFFSET comment_2: BETWEEN TARGET AND LAMP ! linenum: 2.120 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 14.4S priority: 2 comment_1: MEASUREMENT OF RELATIVE OFFSET comment_2: BETWEEN TARGET AND LAMP ! linenum: 2.130 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 1810.0 num_exp: 1 time_per_exp: 180.0S priority: 2 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CALIB FOR 2.14; req_2: SEQ 2.13-2.14 NON-INT ! linenum: 2.140 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 1810.0 num_exp: 1 time_per_exp: 445.6S s_to_n: 200. s_to_n_time: 445.6S priority: 2 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.150 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 1859.5 num_exp: 1 time_per_exp: 150.0S priority: 2 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 2.16; req_2: SEQ 2.15-2.16 NON-INT ! linenum: 2.160 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 1859.5 num_exp: 1 time_per_exp: 587.2S s_to_n: 200. s_to_n_time: 587.2S priority: 2 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.170 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2345.0 num_exp: 1 time_per_exp: 120.0S priority: 2 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 2.18; req_2: SEQ 2.17-2.18 NON-INT ! linenum: 2.180 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2345.0 num_exp: 1 time_per_exp: 83.2S s_to_n: 200. s_to_n_time: 83.2S priority: 2 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.190 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2377.8 num_exp: 1 time_per_exp: 100.0S priority: 2 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 2.20; req_2: SEQ 2.19-2.20 NON-INT ! linenum: 2.200 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2377.8 num_exp: 1 time_per_exp: 138.8S s_to_n: 200. s_to_n_time: 138.8S priority: 2 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.210 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2581.0 num_exp: 1 time_per_exp: 100.0S priority: 2 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 2.22; req_2: SEQ 2.21-2.22 NON-INT ! linenum: 2.220 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2581.0 num_exp: 1 time_per_exp: 98.4S s_to_n: 200. s_to_n_time: 98.4S priority: 2 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.230 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2798.5 num_exp: 1 time_per_exp: 90.0S priority: 2 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 2.24; req_2: SEQ 2.23-2.24 NON-INT ! linenum: 2.240 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2798.5 num_exp: 1 time_per_exp: 100.4S s_to_n: 200. s_to_n_time: 100.4S priority: 2 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 2.250 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2854.0 num_exp: 1 time_per_exp: 90.S priority: 2 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 2.26; req_2: SEQ 2.25-2.26 NON-INT ! linenum: 2.260 targname: HD44743 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2854.0 num_exp: 1 time_per_exp: 165.2S s_to_n: 200. s_to_n_time: 165.2S priority: 2 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.000 targname: HD52089 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 232.2S fluxnum_1: 1 fluxnum_2: 2 fluxnum_3: 3 priority: 2 param_1: MAP = DEF req_1: INT ACQ FOR 3.001-3.10 comment_1: COUNT RATE FOR MIRROR A2 comment_2: 2.0E6 CNTS/S. STEP TIME IS 0.2S comment_3: TO GIVE 90000 CNTS/STEP. ! linenum: 3.001 targname: HD52089 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 20.4S fluxnum_1: 1 fluxnum_2: 2 fluxnum_3: 3 priority: 2 req_1: SEQ 3.001-3.10 NO GAP comment_1: COUNT RATE FOR MIRROR A2 comment_2: 2.0E6 CNTS/S. STEP TIME IS 0.2S comment_3: TO GIVE 90000 CNTS/STEP. ! linenum: 3.020 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1203.5 num_exp: 16 time_per_exp: 100.0S s_to_n: 200. s_to_n_time: 100.0S fluxnum_1: 7 priority: 3 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.030 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1247.5 num_exp: 1 time_per_exp: 57.6S s_to_n: 200. s_to_n_time: 42.0S fluxnum_1: 6 priority: 3 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.040 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1318.5 num_exp: 1 time_per_exp: 57.6S s_to_n: 200. s_to_n_time: 30.4S fluxnum_1: 8 priority: 3 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.050 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1409.0 num_exp: 1 time_per_exp: 57.6S s_to_n: 200. s_to_n_time: 53.2S fluxnum_1: 9 priority: 3 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.060 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1542.5 num_exp: 1 time_per_exp: 84.0S s_to_n: 200. s_to_n_time: 84.0S fluxnum_1: 10 priority: 3 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.070 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1608.0 num_exp: 1 time_per_exp: 76.0S s_to_n: 200. s_to_n_time: 76.0S priority: 3 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.080 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1663.0 num_exp: 1 time_per_exp: 72.8S s_to_n: 200. s_to_n_time: 72.8S priority: 3 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.090 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1810.0 num_exp: 1 time_per_exp: 80.0S s_to_n: 200. s_to_n_time: 80.0S priority: 3 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.100 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1859.5 num_exp: 1 time_per_exp: 88.8S s_to_n: 200. s_to_n_time: 88.8S priority: 3 param_1: STEP-PATT = 5 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.101 targname: HD52089 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 232.2S fluxnum_1: 1 fluxnum_2: 2 fluxnum_3: 3 priority: 2 param_1: MAP = DEF req_1: INT ACQ FOR 3.102-3.30 comment_1: COUNT RATE FOR MIRROR A2 comment_2: 2.0E6 CNTS/S. STEP TIME IS 0.2S comment_3: TO GIVE 90000 CNTS/STEP. ! linenum: 3.102 targname: HD52089 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 20.4S fluxnum_1: 1 fluxnum_2: 2 fluxnum_3: 3 priority: 2 req_1: SEQ 3.102-3.30 NO GAP comment_1: COUNT RATE FOR MIRROR A2 comment_2: 2.0E6 CNTS/S. STEP TIME IS 0.2S comment_3: TO GIVE 90000 CNTS/STEP. ! linenum: 3.110 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 14.4S fluxnum_1: 1 fluxnum_2: 2 priority: 3 req_1: SEQ 3.11-3.12 NON-INT comment_1: MEASUREMENT OF RELATIVE OFFSET comment_2: BETWEEN TARGET AND LAMP ! linenum: 3.120 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 14.4S priority: 3 comment_1: MEASUREMENT OF RELATIVE OFFSET comment_2: BETWEEN TARGET AND LAMP ! linenum: 3.130 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 1810.0 num_exp: 1 time_per_exp: 180.0S priority: 3 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR req_1: CALIB FOR 3.14; req_2: SEQ 3.13-3.14 NON-INT ! linenum: 3.140 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 1810.0 num_exp: 1 time_per_exp: 417.6S s_to_n: 200. s_to_n_time: 417.6S priority: 3 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.150 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 1859.5 num_exp: 1 time_per_exp: 150.0S priority: 3 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 3.16; req_2: SEQ 3.15-3.16 NON-INT ! linenum: 3.160 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 1859.5 num_exp: 1 time_per_exp: 479.2S s_to_n: 200. s_to_n_time: 479.2S priority: 3 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.170 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2345.0 num_exp: 1 time_per_exp: 120.0S priority: 3 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 3.18; req_2: SEQ 3.17-3.18 NON-INT ! linenum: 3.180 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2345.0 num_exp: 2 time_per_exp: 75.6S s_to_n: 200. s_to_n_time: 75.6S priority: 3 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.185 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2345.0 num_exp: 1 time_per_exp: 120.0S priority: 3 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 3.19; req_2: SEQ 3.185-3.19 NON-INT; ! linenum: 3.190 targname: HD52089 config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2345.0 num_exp: 2 time_per_exp: 57.6S s_to_n: 200. s_to_n_time: 24.0S priority: 3 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.200 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2377.8 num_exp: 1 time_per_exp: 100.0S priority: 3 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 3.21; req_2: SEQ 3.20-3.21 NON-INT ! linenum: 3.210 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2377.8 num_exp: 1 time_per_exp: 116.4S s_to_n: 200. s_to_n_time: 116.4S priority: 3 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.220 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2581.0 num_exp: 1 time_per_exp: 100.0S priority: 3 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 3.23; req_2: SEQ 3.22-3.23 NON-INT ! linenum: 3.230 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2581.0 num_exp: 2 time_per_exp: 79.2S s_to_n: 200. s_to_n_time: 79.2S priority: 3 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.235 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2581.0 num_exp: 1 time_per_exp: 100.0S priority: 3 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 3.24; req_2: SEQ 3.235-3.24 NON-INT ! linenum: 3.240 targname: HD52089 config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2581.0 num_exp: 2 time_per_exp: 57.6S s_to_n: 200. s_to_n_time: 26.4S priority: 3 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.250 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2798.5 num_exp: 1 time_per_exp: 90.0S priority: 3 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 3.26; req_2: SEQ 3.25-3.26 NON-INT ! linenum: 3.260 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2798.5 num_exp: 2 time_per_exp: 75.6S s_to_n: 200. s_to_n_time: 75.6S priority: 3 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.265 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2798.5 num_exp: 1 time_per_exp: 90.0S priority: 3 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 3.27; req_2: SEQ 3.265-3.27 NON-INT ! linenum: 3.270 targname: HD52089 config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2800.0 num_exp: 2 time_per_exp: 57.6S s_to_n: 200. s_to_n_time: 26.8S priority: 3 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.280 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2854.0 num_exp: 1 time_per_exp: 90.S priority: 3 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 3.29; req_2: SEQ 3.28-3.29 NON-INT ! linenum: 3.290 targname: HD52089 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2854.0 num_exp: 2 time_per_exp: 120.8S s_to_n: 200. s_to_n_time: 120.8S priority: 3 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! linenum: 3.295 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2854.0 num_exp: 1 time_per_exp: 90.S priority: 3 param_1: STEP-PATT = 7 param_2: COMB = FOUR req_1: CALIB FOR 3.30; req_2: SEQ 3.295-3.30 NON-INT ! linenum: 3.300 targname: HD52089 config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2854.0 num_exp: 2 time_per_exp: 57.6S s_to_n: 200. s_to_n_time: 43.2S priority: 3 param_1: STEP-PATT = 7 param_2: FP-SPLIT = STD param_3: COMB = FOUR comment_1: S/N PER SUBSTEP PIXEL. ! ! end of exposure logsheet ! No scan data records found