! File: 4611C.PROP ! Database: PEPDB ! Date: 22-FEB-1994:19:38:18 coverpage: title_1: DYNAMICS, MASS LOSS AND RADIATIVE TRANSFER IN SHOCKED ATMOSPHERES: title_2: S CAR AS PROTOTYPE sci_cat: COOL STARS sci_subcat: PULSATING STARS proposal_for: GO pi_title: DR. pi_fname: JAY pi_mi: A. pi_lname: BOOKBINDER pi_inst: SMITHSONIAN ASTROPHYSICAL OBSERVATORY pi_country: USA pi_phone: (617) 495-7058 keywords_1: STARS:PULSATING keywords_2: STARS:SHOCKS hours_pri: 20.06 num_pri: 1 fos: Y hrs: Y time_crit: Y funds_amount: 97727 funds_length: 12 funds_date: NOV-93 pi_position: ASTROPHYSICIST off_fname: IRWIN off_mi: I. off_lname: SHAPIRO off_title: DIRECTOR off_inst: SMITHSONIAN ASTROPHYSICAL OBSERVATORY off_addr_1: 60 GARDEN ST. off_city: CAMBRIDGE off_state: MA off_zip: 02138 off_country: USA off_phone: (617) 495-7100 ! end of coverpage abstract: line_1: Our previous IUE programs to study the evolution of the shock structure line_2: of Miras have produced high-dispersion spectra of the highly variable line_3: Mg II h and k emission lines. These lines possess unusual properties line_4: that appear to be common among Miras, including strong variability on line_5: timescales as short as 2 days, and emission centroids that are shifted line_6: relative to the stellar radial velocity well in excess of the presumed line_7: wind or shock velocity. We propose to obtain a series of closely-spaced line_8: high dispersion Mg II observations to (i) constrain the short timescale line_9: (hours to days) behavior of these lines; with the possibility of line_10: determining whether sound waves -- as opposed to radiation pressure on line_11: dust -- are contributing to the mass loss and (ii) probe the radiative line_12: transfer effects in a multiply shocked atmosphere, which will provide line_13: unique observational inputs to the newly emerging class of theoretical line_14: radiative transfer problems of resonance line transfer (including line_15: partial redistribution) across shock fronts. This investigation into line_16: the dynamic structure of extended stellar atmospheres is part of the line_17: broader question of mass loss in evolved cool stars and their influence line_18: on the ISM. ! ! end of abstract general_form_proposers: lname: BOOKBINDER fname: JAY title: DR. mi: A. inst: SMITHSONIAN ASTROPHYSICAL OBSERVATORY country: USA ! lname: CARPENTER fname: KEN title: DR. mi: G. inst: GSFC country: USA ! lname: BROWN fname: ALEX title: DR. mi: 1. inst: JILA country: USA ! lname: PIJPERS fname: FRANK title: DR. mi: J. inst: UPPSALA ASTONOMICAL OBSERVATORY country: SWEEDEN ! lname: BRUGEL fname: ED title: DR. mi: 2. inst: CASA country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: We have selected the Mira S Carinae as our target for detailed, line_2: high-dispersion observations because it is the only Mira that line_3: possesses a radial velocity high enough (+289 km s$^{-1}$, about 3 line_4: \AA\ at Mg~II) to shift the cores of its emission lines ({\it e.g.}, line_5: Mg~II {\it h} and {\it k}, and Ly-$\alpha$) away from the ISM line_6: absorption, thus making interpretation significantly more line_7: straightforward. It is also one of the UV brightest Miras, and has a line_8: short period (P = 149d) that permits relatively easy scheduling. line_9: However, the physics of its atmosphere and the behavior line_10: of its Mg~II lines is not unique, and is typical of that line_11: of other Miras (Bookbinder, Brugel and Brown 1989, 1992). line_12: To determine the short timescale variability of the atmosphere line_13: will require five observations, separated by 0.01 in phase, line_14: with the initial observation at about optical phase 0.3 to 0.4 The line_15: range of phases ($\approx$ 0.06) and number of observations (five) line_16: were selected to match the periods of sound wave periods if they line_17: are due to higher order mode oscillations; we expect to see line_18: variability on a range of timescales from a few minutes, to line_19: hours, and to days. The proposed observations are sensitive to line_20: all of these timescales. line_21: On each of these five dates, observations of the Mg~II {\it h} and line_22: {\it k} line profiles will be made using the GHRS with the ECH-B on line_23: HST. To obtain the Mg~II {\it h} and {\it k} line profiles with ! question: 3 section: 2 line_1: adequate velocity resolution ($\lapprox$ 5 km s$^{-1}$) and good line_2: photometric accuracy, we will employ the R=100,000 mode of line_3: the GHRS, using the ECH-B grating at 2800 \AA\ and the LSA. line_4: This combination (ECH-B,LSA) was selected over (G270M,SSA) because line_5: of difficulty in performing photometric observations with the SSA. line_6: It was also selected because of the uncertainties involved in using line_7: deconvolved line profiles for studying profile variability. The line_8: combination of the ECH-B and the LSA provide high throughput and line_9: adequate spectral resolution, despite problems associated with the line_10: imperfect PSF. line_11: Additional observations will be made to obtain data on the weaker line_12: intersystem lines and other diagnostics, also using the LSA. line_13: The intersystem lines of C~II] are important because they line_14: provide an excellent density diagnostic (formed at the same line_15: temperature as the Mg~II lines) when observed with G270M grating. line_16: This observation will also obtain the Si~II] line at 2335 \AA. The line_17: C~II] and Si~II] lines are optically thin, therefore also provide line_18: information on the velocity field of post-shock regime (from the line_19: centroid of the emission, Judge 1987). The GHRS spectra of these line_20: intersystem lines will be obtained using the LSA with the G270M line_21: grating centered at 2335 \AA. ! question: 3 section: 3 line_1: Finally, a set of exposures on the first and last observing days line_2: using the FOS with the G130H grating (with the 0.25 $\times$ 2'' line_3: slit) will provide the first information (at moderate spectral line_4: resolution) on the existence of other potential UV diagnostics for line_5: Miras. Such diagnostics are expected to include a number of lines line_6: neutral and low ionized lines such as Fe~II, S~I, C~I, C~II, O~I], line_7: and perhaps Ly-$\alpha$. ! question: 4 section: 1 line_1: As we indicate above, our primary goal is to obtain high resolution line_2: Mg~II line {\it h} and {\it k} line profiles over the course of a line_3: single shock cycle, with supporting observations of a number of line_4: density diagnostics and temperature sensitive lines. We have line_5: carefully considered the various alternatives available regarding line_6: trade-offs between spectral resolution and sensitivity. Clearly, for line_7: variability studies it is also important to maintain photometric line_8: accuracy. This combination of requirements led us to select the ECH-B line_9: and LSA to achieve the primary goals of this proposal. {\bf The line_10: multiple observations over the course of five to seven days will allow line_11: us to determine the flux and profile changes that occur in a regime to line_12: which IUE is insensitive and which are in the regime where sound waves line_13: are important.} line_14: Our required exposure times for a high dispersion GHRS spectrum of the line_15: Mg~II~{\it h} and {\it k} lines, and a S/N $\approx 20$ at the line_16: half-power points, are $\approx$ 45 minutes near the peak (with a line_17: typical Mg~II~{\it k} line-center flux $\approx$ 3 $\times$ $10^{-13}$ line_18: ergs cm$^{-2}$ s$^{-1}$ \AA$^{-1}$; Bookbinder, Brugel, and Brown line_19: 1989, Davis, Brugel, and Bookbinder 1992). These exposure times are line_20: based on our extensive previous experience with the IUE spectra (see line_21: Figure 1), and the sensitivity of the ECH-B using the Large Science line_22: Aperture (based on the GHRS Handbook dated Jan. 1992). However, since ! question: 4 section: 2 line_1: our primary interest is in characterizing the variability timescales, line_2: we note that flux variations at the 10\% level will be observable (at line_3: $\approx$ 4 $\sigma$) in about 5 minutes. Thus, with a 60 minute line_4: observation, rather than 45, each of our five observations will line_5: contain at least 10 samples with which to search for evidence of very line_6: rapid variability. The 60 minute exposures are also long enough to line_7: yield spectra with a S/N adequate for accurate atmospheric modeling line_8: and studying the changes in the emission and absorption features as a line_9: result of the shock evolution. These exposures are also long enough to line_10: yield a S/N $>$ 5 in the line wings, a fact which is particularly line_11: important for this experiment: a glance at Figure 1 shows that line_12: much of the profile variability is occurring in the line wings. line_14: Similarly, we have estimated the exposure times required for the C~II] line_15: lines based on our deep (600 min) IUE LWP-HI exposure. To obtain the line_16: C~II] lines (2325 \AA, which have a flux of about 2 $\times$ line_17: 10$^{-14}$ ergs cm$^{-2}$ sec$^{-1}$)) at a S/N = 10 -- necessary to line_18: be able to use the multiplet as a density diagnostic -- will require line_19: an exposure time of 75 minutes using the G270M grating and the LSA. line_20: We consider this density diagnostic important enough to pursue, line_21: despite the cost in observing time. The FOS exposure times are based line_22: on being able to obtain a S/N = 4 down to a limiting flux of 5 ! question: 4 section: 3 line_1: $\times$ 10$^{-15}$ ergs cm$^{-2}$ sec$^{-1}$ (near 1240 \AA); about line_2: 60 minutes is required for these exposures. Because of the length of line_3: these observations, they will only be made on the first and last line_4: of the observing days. line_5: This program has a total observing time of 13.25 hours. We have line_6: estimated the spacecraft time and observing efficiency with the line_7: following factors: T$_{exp}$= 795 min, N$_{exp}$= 12, N$_{obj}$= 1, line_8: N{RT} 0, N{OA}=7, N$_{vis}$ = 5 Thus, we arrive at a total spacecraft line_9: time of 19.44 hours, and an observing efficiency of 68.1\%, following line_10: the prescription of the Phase I Proposal Instructions (5/92), p.17. ! question: 5 section: 1 line_1: The proposed observations are time-critical, as the flux of the Mg~II line_2: {\it h} and {\it k} lines depends strongly on the phase of the line_3: pulsation in Mira variables (Brugel, Willson and Cadmus 1986), with line_4: the peak flux usually between phases 0.1 and 0.3 for each shock cycle line_5: (see also Figure 1). To obtain our stated science goals requires a line_6: total of 5 observing runs, spaced approximately one day apart. line_7: With a pulsation period of 149 days for S Car, it is relatively line_8: straightforward to schedule the observations, since we do not care at line_9: which of the maxima we observe. Also, the start dates of observation line_10: are flexible $\pm$ 5 days. ! question: 6 section: 1 line_1: In order to obtain the highly accurate wavelength calibrations that line_2: are necessary to compare the five Mg~II line profiles, and to study line_3: the small-scale changes that are expected, we request a Pt lamp line_4: calibration exposure immediately following each GHRS spectrum taken line_5: with ECH-B. ! !end of general form text general_form_address: lname: BOOKBINDER fname: JAY mi: A. title: DR. category: PI inst: SMITHSONIAN ASTROPHYSICAL OBSERVATORY addr_1: 60 GARDEN STREET city: CAMBRIDGE state: MA zip: 02138 country: USA phone: (617)495-7058 from_date: 01-JUL-93 to_date: 31-DEC-94 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: HD88366 name_2: HR3999 name_3: S-CAR descr_1: A,142,147 pos_1: RA = 10H 09M 22.52S +/- 0.15S, pos_2: DEC = -61D 33' 00.48" +/- 0.6" equinox: 2000 pm_or_par: Y pos_epoch_bj: J pos_epoch_yr: 2000.00 ra_pm_val: -0.012900 dec_pm_val: 0.0660 rv_or_z: V = +289 comment_1: RM_PM_VAL IN *SECONDS PER YEAR*, comment_2: NOT ARC-SEC PER YEAR, comment_3: AS PER THE LATEST INSTRUCTIONS. comment_4: COORDS, PM VALUES FROM SAO CATALOG. comment_5: COORDS, PM MAY BE UPDATED comment_6: V MAX = 4.5, V MIN = 9.0 fluxnum_1: 1 fluxval_1: V = 6.3 +/- 1.3 fluxnum_2: 2 fluxval_2: B-V = 1.6 +/- 0.3 fluxnum_3: 3 fluxval_3: F-LINE(2880) = 1 +/- 0.5 E-12 fluxnum_4: 4 fluxval_4: W-LINE(2880) = 0.7 +/- 0.2 fluxnum_5: 5 fluxval_5: F-LINE(2325) = 2 +/- 0.5 E-14 fluxnum_6: 6 fluxval_6: W-LINE(2325) = 0.3 +/- 0.2 fluxnum_7: 7 fluxval_7: U-B = 1.75 +/- 0.4 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 targname: HD88366 config: FOS/BL opmode: ACQ/PEAK aperture: 4.3 sp_element: G570H wavelength: 1850-5500 num_exp: 1 time_per_exp: 2S fluxnum_1: 1 fluxnum_2: 2 priority: 2 param_1: SEARCH-SIZE-X=1, param_2: SEARCH-SIZE-Y=3, param_3: SCAN-STEP-Y=1.4, param_4: TYPE=UP req_1: CYCLE 3; req_2: SEQ 1-7.5 WITHIN 7D; req_3: ONBOARD ACQ FOR 1.1 comment_1: EXPECTED COUNT RATE = comment_2: THE TIME PER EXPOSURE MUST BE comment_3: CHECKED WITH THE FOS TEAM ! linenum: 1.100 targname: HD88366 config: FOS/BL opmode: ACQ/PEAK aperture: 1.0 sp_element: G570H wavelength: 1850-5500 num_exp: 1 time_per_exp: 3S fluxnum_1: 1 fluxnum_2: 2 priority: 2 param_1: SEARCH-SIZE-X=6, param_2: SEARCH-SIZE-Y=2, param_3: SCAN-STEP-X=0.700, param_4: SCAN-STEP-Y=0.700, param_5: TYPE=UP req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 1.2 comment_1: EXPECTED COUNT RATE = comment_2: THE TIME PER EXPOSURE MUST BE comment_3: CHECKED WITH THE FOS TEAM ! linenum: 1.200 targname: HD88366 config: FOS/BL opmode: ACQ/PEAK aperture: 0.5 sp_element: G570H wavelength: 1850-5500 num_exp: 1 time_per_exp: 4S fluxnum_1: 1 fluxnum_2: 2 priority: 2 param_1: SEARCH-SIZE-X=3, param_2: SEARCH-SIZE-Y=3, param_3: SCAN-STEP-X=0.35, param_4: SCAN-STEP-Y=0.35, param_5: TYPE=UP req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 1.3 comment_1: EXPECTED COUNT RATE = comment_2: THE TIME PER EXPOSURE MUST BE comment_3: CHECKED WITH THE FOS TEAM ! linenum: 1.300 targname: HD88366 config: FOS/BL opmode: ACQ/PEAK aperture: 0.25X2.0 sp_element: G570H wavelength: 1850-5500 num_exp: 1 time_per_exp: 10S fluxnum_1: 1 fluxnum_2: 2 priority: 2 param_1: SEARCH-SIZE-X=7, param_2: SEARCH-SIZE-Y=1, param_3: SCAN-STEP-X=0.067, param_4: TYPE=UP req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 2.0 comment_1: EXPECTED COUNT RATE = comment_2: THE TIME PER EXPOSURE MUST BE comment_3: CHECKED WITH THE FOS TEAM ! linenum: 2.000 targname: HD88366 config: FOS/BL opmode: ACCUM aperture: 0.25X2.0 sp_element: G160L wavelength: 1650-2503 num_exp: 1 time_per_exp: 60M s_to_n: 5 fluxnum_1: 3, fluxnum_2: 4 priority: 2 req_1: CYCLE 3 comment_1: SCIENCE OBSERVATIONS comment_2: TO OBTAIN MISC. DIAGNOSTICS. ! linenum: 4.000 targname: HD88366 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 100S fluxnum_1: 1, fluxnum_2: 2 priority: 1 param_1: BRIGHT=RETURN, param_2: SEARCH-SIZE=5, param_3: LOCATE=YES req_1: CYCLE 3; req_2: AT 03-JAN-94 +/- 5D; req_3: ONBOARD ACQ FOR 4.1 comment_1: STEP-TIME = 4S comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. comment_4: TIMING IS FOR PHASE 0.30 ! linenum: 4.100 targname: HD88366 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 306S fluxnum_1: 1, fluxnum_2: 2 priority: 1 req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 5.0-7.5 comment_1: STEP-TIME =3S;TEXP = 102X THIS. comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. ! linenum: 5.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_3: SEQ 5.0-5.2 NON-INT; req_4: CALIB FOR 5.1 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES comment_3: EXP TIME FOR ALL WAVECALS MUST comment_4: BE CHECKED WITH GHRS TEAM ! linenum: 5.100 targname: HD88366 config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2802 num_exp: 6 time_per_exp: 5M s_to_n: 20 fluxnum_1: 3, fluxnum_2: 4 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=ON req_1: CYCLE 3 comment_1: SCIENCE OBSERVATION comment_2: THE MG II LINES (AT +289 KM/S) comment_3: THE TIME PER EXPOSURE MUST BE 300S, comment_4: RATHER THAN SOME RANDOM NUMBER. ! linenum: 5.200 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_2: CALIB FOR 5.1 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 6.000 targname: HD88366 config: HRS opmode: ACCUM aperture: 2.0 sp_element: G270M wavelength: 2335 num_exp: 3 time_per_exp: 18.75M s_to_n: 20 fluxnum_1: 5, fluxnum_2: 6 priority: 1 param_1: STEP-PATT=5, param_2: FP-SPLIT=FOUR, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=ON req_1: CYCLE 3 comment_1: SCIENCE OBSERVATION comment_2: THE C II] LINES (AT +289 KM/S) ! linenum: 7.300 targname: HD88366 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 306S fluxnum_1: 1, fluxnum_2: 2 priority: 1 req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 7.31-7.5 comment_1: STEP-TIME =3S;TEXP = 102X THIS. comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. ! linenum: 7.310 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_2: SEQ 7.31-7.5 NON-INT; req_3: CALIB FOR 7.4 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 7.400 targname: HD88366 config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2802 num_exp: 6 time_per_exp: 5M s_to_n: 20 fluxnum_1: 3, fluxnum_2: 4 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=ON req_1: CYCLE 3 comment_1: SCIENCE OBSERVATION comment_2: THE MG II LINES (AT +289 KM/S) comment_3: THE TIME PER EXPOSURE MUST BE 300S, comment_4: RATHER THAN SOME RANDOM NUMBER. ! linenum: 7.500 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_3: CALIB FOR 7.4 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 8.000 targname: HD88366 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 100S fluxnum_1: 1, fluxnum_2: 2 priority: 1 param_1: BRIGHT=RETURN, param_2: SEARCH-SIZE=5, param_3: LOCATE=YES req_1: CYCLE 3; req_2: AFTER 5.0 BY 1D +/- 5H; req_3: ONBOARD ACQ FOR 8.1 comment_1: STEP-TIME = 4S comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. comment_4: SECOND SERIES OF OBSERVATIONS ! linenum: 8.100 targname: HD88366 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 306S fluxnum_1: 1, fluxnum_2: 2 priority: 1 req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 9.0-9.5 comment_1: STEP-TIME =3S;TEXP = 102X THIS. comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. ! linenum: 9.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_2: SEQ 9.0-9.2 NON-INT; req_3: CALIB FOR 9.1 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 9.100 targname: HD88366 config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2802 num_exp: 6 time_per_exp: 5M s_to_n: 20 fluxnum_1: 3, fluxnum_2: 4 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=ON req_1: CYCLE 3 comment_1: SCIENCE OBSERVATION comment_2: THE MG II LINES (AT +289 KM/S) comment_3: THE TIME PER EXPOSURE MUST BE 300S, comment_4: RATHER THAN SOME RANDOM NUMBER. ! linenum: 9.200 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_2: CALIB FOR 9.1 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 9.250 targname: HD88366 config: HRS opmode: ACCUM aperture: 2.0 sp_element: G270M wavelength: 2335 num_exp: 3 time_per_exp: 18.75M s_to_n: 20 fluxnum_1: 5, fluxnum_2: 6 priority: 1 param_1: STEP-PATT=5, param_2: FP-SPLIT=FOUR, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=ON req_1: CYCLE 3 comment_1: SCIENCE OBSERVATION comment_2: THE C II] LINES (AT +289 KM/S) comment_3: THE TIME PER EXPOSURE MUST BE 300S, comment_4: RATHER THAN SOME RANDOM NUMBER. ! linenum: 9.300 targname: HD88366 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 306S fluxnum_1: 1, fluxnum_2: 2 priority: 1 req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 9.31-9.5 comment_1: STEP-TIME =3S;TEXP = 102X THIS. comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. ! linenum: 9.310 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_2: SEQ 9.31-9.5 NON-INT; req_3: CALIB FOR 9.4 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 9.400 targname: HD88366 config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2802 num_exp: 6 time_per_exp: 5M s_to_n: 20 fluxnum_1: 3, fluxnum_2: 4 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=ON req_1: CYCLE 3 comment_1: SCIENCE OBSERVATION comment_2: THE MG II LINES (AT +289 KM/S) comment_3: THE TIME PER EXPOSURE MUST BE 300S, comment_4: RATHER THAN SOME RANDOM NUMBER. ! linenum: 9.500 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_3: CALIB FOR 9.4 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 10.000 targname: HD88366 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 100S fluxnum_1: 1, fluxnum_2: 2 priority: 1 param_1: BRIGHT=RETURN, param_2: SEARCH-SIZE=5, param_3: LOCATE=YES req_1: CYCLE 3; req_2: AFTER 5.0 BY 2D +/- 5H; req_3: ONBOARD ACQ FOR 10.1 comment_1: STEP-TIME = 4S comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. comment_4: THIRD SERIES OF OBSERVATIONS ! linenum: 10.100 targname: HD88366 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 306S fluxnum_1: 1, fluxnum_2: 2 priority: 1 req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 11.0-13.5 comment_1: STEP-TIME =3S;TEXP = 102X THIS. comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. ! linenum: 11.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_2: SEQ 11.0-11.2 NON-INT; req_3: CALIB FOR 11.1 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 11.100 targname: HD88366 config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2802 num_exp: 6 time_per_exp: 5M s_to_n: 20 fluxnum_1: 3, fluxnum_2: 4 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=ON req_1: CYCLE 3 comment_1: SCIENCE OBSERVATION comment_2: THE MG II LINES (AT +289 KM/S) comment_3: THE TIME PER EXPOSURE MUST BE 300S, comment_4: RATHER THAN SOME RANDOM NUMBER. ! linenum: 11.200 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_2: CALIB FOR 11.1 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 12.000 targname: HD88366 config: HRS opmode: ACCUM aperture: 2.0 sp_element: G270M wavelength: 2335 num_exp: 3 time_per_exp: 18.75M s_to_n: 20 fluxnum_1: 5, fluxnum_2: 6 priority: 1 param_1: STEP-PATT=5, param_2: FP-SPLIT=FOUR, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=ON req_1: CYCLE 3 comment_1: SCIENCE OBSERVATION comment_2: THE C II] LINES (AT +289 KM/S) ! linenum: 13.300 targname: HD88366 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 306S fluxnum_1: 1, fluxnum_2: 2 priority: 1 req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 13.31-13.5 comment_1: STEP-TIME =3S;TEXP = 102X THIS. comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. ! linenum: 13.310 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_2: SEQ 13.31-13.5 NON-INT; req_3: CALIB FOR 13.4 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 13.400 targname: HD88366 config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2802 num_exp: 6 time_per_exp: 5M s_to_n: 20 fluxnum_1: 3, fluxnum_2: 4 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=ON req_1: CYCLE 3 comment_1: SCIENCE OBSERVATION comment_2: THE MG II LINES (AT +289 KM/S) comment_3: THE TIME PER EXPOSURE MUST BE 300S, comment_4: RATHER THAN SOME RANDOM NUMBER. ! linenum: 13.500 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_3: CALIB FOR 13.4 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 14.000 targname: HD88366 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 100S fluxnum_1: 1, fluxnum_2: 2 priority: 1 param_1: BRIGHT=RETURN, param_2: SEARCH-SIZE=5, param_3: LOCATE=YES req_1: CYCLE 3; req_2: AFTER 5.0 BY 3D +/- 5H; req_3: ONBOARD ACQ FOR 14.1 comment_1: STEP-TIME = 4S comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. comment_4: FOURTH SERIES OF OBSERVATIONS ! linenum: 14.100 targname: HD88366 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 306S fluxnum_1: 1, fluxnum_2: 2 priority: 1 req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 15.0-15.5 comment_1: STEP-TIME =3S;TEXP = 102X THIS. comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. ! linenum: 15.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_2: SEQ 15.0-15.2 NON-INT; req_3: CALIB FOR 15.1 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 15.100 targname: HD88366 config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2802 num_exp: 6 time_per_exp: 5M s_to_n: 20 fluxnum_1: 3, fluxnum_2: 4 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=ON req_1: CYCLE 3 comment_1: SCIENCE OBSERVATION comment_2: THE MG II LINES (AT +289 KM/S) comment_3: THE TIME PER EXPOSURE MUST BE 300S, comment_4: RATHER THAN SOME RANDOM NUMBER. ! linenum: 15.200 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_2: CALIB FOR 15.1 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 15.300 targname: HD88366 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 306S fluxnum_1: 1, fluxnum_2: 2 priority: 1 req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 15.31-15.5 comment_1: STEP-TIME =3S;TEXP = 102X THIS. comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. ! linenum: 15.310 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_2: SEQ 15.31-15.5 NON-INT; req_3: CALIB FOR 15.4 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 15.400 targname: HD88366 config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2802 num_exp: 6 time_per_exp: 5M s_to_n: 20 fluxnum_1: 3, fluxnum_2: 4 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=ON req_1: CYCLE 3 comment_1: SCIENCE OBSERVATION comment_2: THE MG II LINES (AT +289 KM/S) comment_3: THE TIME PER EXPOSURE MUST BE 300S, comment_4: RATHER THAN SOME RANDOM NUMBER. ! linenum: 15.500 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_3: CALIB FOR 15.4 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 16.000 targname: HD88366 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 100S fluxnum_1: 1, fluxnum_2: 2 priority: 1 param_1: BRIGHT=RETURN, param_2: SEARCH-SIZE=5, param_3: LOCATE=YES req_1: CYCLE 3; req_2: AFTER 5.0 BY 4D +/- 5H; req_3: SEQ 16.0 - 21.0 WITHIN 7D; req_4: ONBOARD ACQ FOR 16.1 comment_1: STEP-TIME = 4S comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. comment_4: FIFTH SERIES OF OBSERVATIONS ! linenum: 16.100 targname: HD88366 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 306S fluxnum_1: 1, fluxnum_2: 2 priority: 1 req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 17.0-19.2 comment_1: STEP-TIME =3S;TEXP = 102X THIS. comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. ! linenum: 17.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_2: SEQ 17.0-17.2 NON-INT; req_3: CALIB FOR 17.1 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 17.100 targname: HD88366 config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2802 num_exp: 6 time_per_exp: 5M s_to_n: 20 fluxnum_1: 3, fluxnum_2: 4 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=ON req_1: CYCLE 3 comment_1: SCIENCE OBSERVATION comment_2: THE MG II LINES (AT +289 KM/S) comment_3: THE TIME PER EXPOSURE MUST BE 300S, comment_4: RATHER THAN SOME RANDOM NUMBER. ! linenum: 17.200 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_2: CALIB FOR 17.1 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 18.000 targname: HD88366 config: HRS opmode: ACCUM aperture: 2.0 sp_element: G270M wavelength: 2335 num_exp: 3 time_per_exp: 18.75M s_to_n: 20 fluxnum_1: 5, fluxnum_2: 6 priority: 1 param_1: STEP-PATT=5, param_2: FP-SPLIT=FOUR, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=ON req_1: CYCLE 3 comment_1: SCIENCE OBSERVATION comment_2: THE C II] LINES (AT +289 KM/S) ! linenum: 18.500 targname: HD88366 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 306S fluxnum_1: 1, fluxnum_2: 2 priority: 1 req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 19.0-19.2 comment_1: STEP-TIME =3S;TEXP = 102X THIS. comment_2: EXPECTED COUNT RATE = 540 CPS comment_3: EXTRAPOLATED FROM GAMMA DRA. ! linenum: 19.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_2: SEQ 19.0-19.2 NON-INT; req_3: CALIB FOR 19.1 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 19.100 targname: HD88366 config: HRS opmode: ACCUM aperture: 2.0 sp_element: ECH-B wavelength: 2802 num_exp: 6 time_per_exp: 5M s_to_n: 20 fluxnum_1: 3, fluxnum_2: 4 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=ON req_1: CYCLE 3 comment_1: SCIENCE OBSERVATION comment_2: THE MG II LINES (AT +289 KM/S) comment_3: THE TIME PER EXPOSURE MUST BE 300S, comment_4: RATHER THAN SOME RANDOM NUMBER. ! linenum: 19.200 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2802 num_exp: 1 time_per_exp: 2.5M s_to_n: 20 priority: 1 param_1: STEP-PATT=7, param_2: FP-SPLIT=NO, param_3: COMB=FOUR, param_4: CENSOR=NO, param_5: DOPPLER=OFF req_1: CYCLE 3; req_3: CALIB FOR 19.1 NO SLEW comment_1: SCIENCE OBSERVATION comment_2: WAVECAL FOR THE MG II LINES ! linenum: 20.000 targname: HD88366 config: FOS/BL opmode: ACQ/PEAK aperture: 4.3 sp_element: G570H wavelength: 1850-5500 num_exp: 1 time_per_exp: 2S fluxnum_1: 1 fluxnum_2: 2 priority: 2 param_1: SEARCH-SIZE-X=1, param_2: SEARCH-SIZE-Y=3, param_3: SCAN-STEP-Y=1.4, param_4: TYPE=UP req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 20.1 comment_1: EXPECTED COUNT RATE = comment_2: EXP. TIME MUST BE CHECKED comment_3: WITH THE FOS TEAM ! linenum: 20.100 targname: HD88366 config: FOS/BL opmode: ACQ/PEAK aperture: 1.0 sp_element: G570H wavelength: 1850-5500 num_exp: 1 time_per_exp: 3S fluxnum_1: 1 fluxnum_2: 2 priority: 2 param_1: SEARCH-SIZE-X=6, param_2: SEARCH-SIZE-Y=2, param_3: SCAN-STEP-X=0.700, param_4: SCAN-STEP-Y=0.700, param_5: TYPE=UP req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 20.2 comment_1: EXPECTED COUNT RATE = comment_2: EXP. TIME MUST BE CHECKED comment_3: WITH THE FOS TEAM ! linenum: 20.200 targname: HD88366 config: FOS/BL opmode: ACQ/PEAK aperture: 0.5 sp_element: G570H wavelength: 1850-5500 num_exp: 1 time_per_exp: 4S fluxnum_1: 1 fluxnum_2: 2 priority: 2 param_1: SEARCH-SIZE-X=3, param_2: SEARCH-SIZE-Y=3, param_3: SCAN-STEP-X=0.35, param_4: SCAN-STEP-Y=0.35, param_5: TYPE=UP req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 20.3 comment_1: EXPECTED COUNT RATE = comment_2: EXP. TIME MUST BE CHECKED comment_3: WITH THE FOS TEAM ! linenum: 20.300 targname: HD88366 config: FOS/BL opmode: ACQ/PEAK aperture: 0.25X2.0 sp_element: G570H wavelength: 1850-5500 num_exp: 1 time_per_exp: 10S fluxnum_1: 1 fluxnum_2: 2 priority: 2 param_1: SEARCH-SIZE-X=7, param_2: SEARCH-SIZE-Y=1, param_3: SCAN-STEP-X=0.067, param_4: TYPE=UP req_1: CYCLE 3; req_2: ONBOARD ACQ FOR 21.0 comment_1: EXPECTED COUNT RATE = comment_2: EXP. TIME MUST BE CHECKED comment_3: WITH THE FOS TEAM ! linenum: 21.000 targname: HD88366 config: FOS/BL opmode: ACCUM aperture: 0.25X2.0 sp_element: G160L wavelength: 1650-2503 num_exp: 1 time_per_exp: 60M s_to_n: 5 fluxnum_1: 3, fluxnum_2: 4 priority: 2 req_1: CYCLE 3 comment_1: SCIENCE OBSERVATIONS comment_2: TO OBTAIN MISC. DIAGNOSTICS. ! ! end of exposure logsheet ! No scan data records found