! File: 3258C.PROP ! Database: PEPDB ! Date: 19-FEB-1994:00:15:55 coverpage: title_1: SLEUTHING THE DYNAMO: FUTURE-CYCLE CONTINUATION sci_cat: STELLAR ASTROPHYSICS sci_subcat: EARLY EVOLUTION proposal_for: GO longterm: 2 cont_id: 2485 pi_title: DR. pi_fname: THOMAS pi_mi: R. pi_lname: AYRES pi_inst: COLORADO, UNIVERSITY OF pi_country: USA pi_phone: 303-492-4051 keywords_1: OPEN CLUSTER, DWARF, MS STAR, CHROMOSPHERE, CORONA hours_pri: 12.00 num_pri: 10 hrs: Y funds_amount: 170620 funds_length: 24 funds_date: JUL-90 pi_position: RESEARCH PROFESSOR off_fname: THEODORE off_mi: P. off_lname: SNOW off_title: DIRECTOR off_inst: CNTR. ASTROPHYS. & SPACE ASTRON. (CASA) off_addr_1: UNIVERSITY OF COLORADO off_addr_2: CAMPUS BOX 391 (CASA) off_city: BOULDER off_state: CO off_zip: 80309 off_country: USA ! end of coverpage abstract: line_1: Innovative technologies in the 1990s will open new windows line_2: to the interior of the Sun and its hidden dynamics: the GONG line_3: project for helioseismology; rare-earth detectors for solar line_4: neutrinos; and SOLAR PROBE for high-order moments of the mass line_5: distribution. At the same time, newly-commissioned space line_6: observatories will provide unprecedented views of the vacuum- line_7: UV and X-ray emissions of stars in our Galactic neighborhood. line_9: These seemingly unrelated developments are in fact deeply line_10: connected. A central issue of solar-stellar physics is the line_11: nature and origin of magnetic activity: the profound link line_12: between the interior dynamics of a late-type star and the line_13: violent state of its outermost coronal (>10^6 K) layers. As line_14: solar physicists are unlocking the secrets of the hydromag- line_15: netic dynamo deep inside the Sun, we will apply one of the line_16: powerful new astronomical tools of the 1990s -- the HST -- line_17: to document the early evolution of the dynamo and its assoc- line_18: iated external gas-dynamic activity. In particular, we will line_19: obtain high-S/N FUV spectra of young solar-type stars in open line_20: clusters ranging in age from 1/100-th to 1/10-th the Sun. ! ! end of abstract general_form_proposers: lname: AYRES fname: THOMAS title: DR. mi: R. inst: COLORADO, UNIVERSITY OF country: USA ! lname: SIMON fname: THEODORE title: DR. inst: HAWAII, UNIVERSITY OF country: USA ! lname: BASRI fname: GIBOR title: PROF. mi: S. inst: CALIFORNIA, UNIVERSITY OF, BERKELEY country: USA ! lname: STAUFFER fname: JOHN title: DR. mi: R. inst: CFA country: USA ! lname: STERN fname: ROBERT title: DR. mi: A. inst: LOCKHEED PALO ALTO RESEARCH LABS country: USA ! lname: ANTIOCHOS fname: SPIRO title: DR. mi: K. inst: US NAVAL RESEARCH LABORATORY country: USA ! lname: BOOKBINDER fname: JAY title: DR. mi: A. inst: CFA country: USA ! lname: BROWN fname: ALEXANDER title: DR. inst: COLORADO, UNIVERSITY OF country: USA ! lname: DOSCHEK fname: GEORGE title: DR. mi: A. inst: US NAVAL RESEARCH LABORATORY country: USA ! lname: LINSKY fname: JEFFREY title: DR. mi: L. inst: COLORADO, UNIVERSITY OF country: USA ! lname: RAMSEY fname: LAWRENCE title: PROF. mi: W. inst: PENN STATE UNIVERSITY country: USA ! lname: WALTER fname: FREDERICK title: PROF. mi: M. inst: NEW YORK, STATE UNIVERSITY OF (STONY BROOK) country: USA ! ! end of general_form_proposers block general_form_text: question: 2 section: 1 line_1: 2. Scientific Justification line_3: ==> Not required for Phase II <== ! question: 3 section: 1 line_1: 3. Short Description of Proposed Observations line_3: We intend to record diagnostic-quality far-UV spectra of line_4: solar-type stars in young galactic clusters including the line_5: Hyades, the Pleiades, and ALPHA Persei. We selected five line_6: stars from each cluster which meet a number of strict line_7: criteria for membership, very likely are single, and which line_8: have reddening-corrected colors corresponding to G0-G3. line_10: Recording the critical spectral emissions in the far-UV -- line_11: from C III 1175, O V] 1218, and N V 1240 to C IV 1550 and line_12: He II 1640 -- requires two separate grating settings with the line_13: HRS. (Although the FOS is somewhat more sensitive longward line_14: of 1400 A for sharp-line emission sources, the HRS has the line_15: important advantages of: solar-blind D1 detector; and line_16: sufficient spectral resolution to clearly separate key blends line_17: -- like density-sensitive O IV] 1401.2 from Si IV 1402.8). line_19: The two HRS settings are: G140L/1303 and G140L/1533. They line_20: span the range 1160-1676 A, with overlapping coverage of line_21: the critical region 1390-1446 A containing important, faint, line_22: closely-spaced emissions. ! question: 4 section: 1 line_1: 4. Need for HST line_3: We will investigate the high-excitation outer atmospheres line_4: of solar-type stars -- energized by magnetic activity -- as line_5: they age along their MS evolutionary tracks. On the Sun, line_6: co-spatiality between magnetic flux and high-excitation line_7: emissions is emphasized in the 10^5 K vacuum-UV resonance line_8: lines like C IV 1548 and N V 1238; whereas traditional line_9: ``chromospheric'' diagnostics accessible from the ground line_10: -- like Ca II and H-ALPHA -- tend to be contaminated to an line_11: uncertain degree by heating unrelated to magnetic activity, line_12: or suffer from uncertain modes of formation. line_14: Three stars of our sample -- HD28344, HD28992, and HZ1514 -- line_15: have been observed previously with IUE LWP-LO exposures to line_16: record the Mg II 2800 emission. There are no SWP-LO spectra line_17: of our program stars, and previous attempts to expose deep line_18: SWP-LOs of other (X-ray-selected) Hyads have produced only line_19: poor-quality spectral material. ! question: 5 section: 1 line_1: 5. Justification of Exposure Times line_3: We calculated (G140L/1303 + G140L/1533) exposure times to line_4: achieve S/N = 13-22 at Si IV 1403 and 14-25 at C IV 1548. line_5: This ensures S/N >=4 at the critical density-diagnostic line_6: O IV] 1401 (f_1401 >= 0.1 f_1403 in the Sun). line_8: For the Hyades and Pleiades, we estimated f_1548 by scaling line_9: R_1548 (f_1548/f_bol) from measured values of R_2800 (Mg II) line_10: according to the power-law R_1548 = const R_2800^1.5. For line_11: ALPHA Per, we estimated R_2800 from an empirical correlation line_12: with the Rossby number, using the average v_sin_i to define line_13: a mean rotation period. We compensated for reddening line_14: assuming a standard galactic law. line_16: We will observe 2 Hyads with the complete G140L/1303+/1533 line_17: sequence in CYCLE-1, and 2 Pleiades and 2 ALPHA Per stars in line_18: CYCLE-2: the 6 high-priority stars were chosen on the basis line_19: of available X-ray fluxes or v_sin_i's. We will observe the line_20: remaining 9 targets -- 3 Hyads in CYCLE-1; the others in line_21: CYCLE-2 -- with an abbreviated sequence consisting of a line_22: single grating setting (G140L/1430) with exposure times line_23: designed to achieve S/N >= 15 at C IV 1548. ! question: 6 section: 1 line_1: 6. a. Justification of special scheduling requests line_2: ==> none <== ! question: 6 section: 2 line_1: 6. b. Special calibration requirements line_2: ==> none <== ! question: 7 section: 1 line_1: 7. Data Reduction and Analysis line_3: Calibration of the HRS spectra will be undertaken at the line_4: STSci. Two team members are HRS/GTOs, and we expect to line_5: benefit from their experience. Initially, the spectral line_6: traces will be measured using standard fitting routines line_7: available at Colorado through the IUE RDAF. Subsequently, line_8: emission-measure modelling, density-sensitive line-ratio line_9: tests, and correlations with other diagnostics (like ground- line_10: based Ca K fluxes or ROSAT X-ray detections) will be line_11: conducted by specific team members. ! question: 8 section: 1 line_1: 8. Special Comments line_2: ==> none <== ! question: 9 section: 1 line_1: 9. Previous HST observing Time line_2: ==> none <== ! question: 10 section: 1 line_1: 10. Resources to be Supplied by Institution(s) line_3: Several domestic institutions are involved in our consortium. line_4: The resources and facilities that will be devoted to the line_5: project are extensive and varied. ! !end of general form text general_form_address: lname: AYRES fname: THOMAS mi: R. category: PI inst: COLORADO, UNIVERSITY OF ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: STAR-0338+2428 name_2: HZ314 descr_1: STAR; TYPE=G0 V; OPEN CLUSTER pos_1: RA=3H 38M 22.2S +/- 1", pos_2: DEC=+24D 28' 51" +/- 1" equinox: 1900 pm_or_par: N comment_1: FAR-UV SPECTRA comment_2: OF SOLAR-TYPE STARS comment_3: IN YOUNG GALACTIC CLUSTERS comment_4: PLEIADES G0 V STAR fluxnum_1: 1 fluxval_1: V = +10.6 +/- 0.1, TYPE = G0 V fluxnum_2: 2 fluxval_2: B-V = +0.64 +/- 0.02 fluxnum_3: 2 fluxval_3: E(B-V) = 0.06 +/- 0.02 fluxnum_4: 3 fluxval_4: F-LINE(1548) = 8 +/- 2 E-15 fluxnum_5: 4 fluxval_5: F-LINE(1403) = 20 +/- 5 E-16 ! targnum: 2 name_1: STAR-0341+2403 name_2: HZ1514 descr_1: STAR; TYPE=G0 V; OPEN CLUSTER pos_1: RA=3H 41M 43.0S +/- 1", pos_2: DEC=+24D 3' 21" +/- 1" equinox: 1900 pm_or_par: N comment_1: FAR-UV SPECTRA comment_2: OF SOLAR-TYPE STARS comment_3: IN YOUNG GALACTIC CLUSTERS comment_4: PLEIADES G0 V STAR fluxnum_1: 1 fluxval_1: V = +10.5 +/- 0.1, TYPE = G0 V fluxnum_2: 2 fluxval_2: B-V = +0.64 +/- 0.02 fluxnum_3: 2 fluxval_3: E(B-V) = 0.06 +/- 0.02 fluxnum_4: 3 fluxval_4: F-LINE(1548) = 8 +/- 2 E-15 fluxnum_5: 4 fluxval_5: F-LINE(1403) = 20 +/- 5 E-16 ! targnum: 3 name_1: STAR-0340+2415 name_2: HZ996 descr_1: STAR; TYPE=G0 V; OPEN CLUSTER pos_1: RA=3H 40M 25.0S +/- 1", pos_2: DEC=+24D 15' 32" +/- 1" equinox: 1900 pm_or_par: N comment_1: FAR-UV SPECTRA comment_2: OF SOLAR-TYPE STARS comment_3: IN YOUNG GALACTIC CLUSTERS comment_4: PLEIADES G0 V STAR fluxnum_1: 1 fluxval_1: V = +10.4 +/- 0.1, TYPE = G0 V fluxnum_2: 2 fluxval_2: B-V = +0.64 +/- 0.02 fluxnum_3: 2 fluxval_3: E(B-V) = 0.06 +/- 0.02 fluxnum_4: 3 fluxval_4: F-LINE(1548) = 8 +/- 2 E-15 fluxnum_5: 4 fluxval_5: F-LINE(1403) = 20 +/- 5 E-16 ! targnum: 4 name_1: STAR-0340+2449 name_2: HZ1015 descr_1: STAR; TYPE=G1 V; OPEN CLUSTER pos_1: RA=3H 40M 28.3S +/- 1", pos_2: DEC=+24D 49' 28" +/- 1" equinox: 1900 pm_or_par: N comment_1: FAR-UV SPECTRA comment_2: OF SOLAR-TYPE STARS comment_3: IN YOUNG GALACTIC CLUSTERS comment_4: PLEIADES G1 V STAR fluxnum_1: 1 fluxval_1: V = +10.5 +/- 0.1, TYPE = G1 V fluxnum_2: 2 fluxval_2: B-V = +0.65 +/- 0.02 fluxnum_3: 2 fluxval_3: E(B-V) = 0.06 +/- 0.02 fluxnum_4: 3 fluxval_4: F-LINE(1548) = 8 +/- 2 E-15 fluxnum_5: 4 fluxval_5: F-LINE(1403) = 20 +/- 5 E-16 ! targnum: 5 name_1: STAR-0340+2316 name_2: HZ1215 descr_1: STAR; TYPE=G0 V; OPEN CLUSTER pos_1: RA=3H 40M 58.3S +/- 1", pos_2: DEC=+23D 16' 24" +/- 1" equinox: 1900 pm_or_par: N comment_1: FAR-UV SPECTRA comment_2: OF SOLAR-TYPE STARS comment_3: IN YOUNG GALACTIC CLUSTERS comment_4: PLEIADES G0 V STAR fluxnum_1: 1 fluxval_1: V = +10.5 +/- 0.1, TYPE = G0 V fluxnum_2: 2 fluxval_2: B-V = +0.65 +/- 0.02 fluxnum_3: 2 fluxval_3: E(B-V) = 0.06 +/- 0.02 fluxnum_4: 3 fluxval_4: F-LINE(1548) = 8 +/- 2 E-15 fluxnum_5: 4 fluxval_5: F-LINE(1403) = 20 +/- 5 E-16 ! targnum: 6 name_1: STAR-0322+4915 name_2: HE699 descr_1: STAR; TYPE=G1 V; OPEN CLUSTER pos_1: RA=3H 22M 47.8S +/- 1", pos_2: DEC=+49D 15' 10" +/- 1" equinox: 1950 pm_or_par: N comment_1: FAR-UV SPECTRA comment_2: OF SOLAR-TYPE STARS comment_3: IN YOUNG GALACTIC CLUSTERS comment_4: ALPHA PERSEI G1 V STAR fluxnum_1: 1 fluxval_1: V = +11.3 +/- 0.1, TYPE = G1 V fluxnum_2: 2 fluxval_2: B-V = +0.70 +/- 0.02 fluxnum_3: 2 fluxval_3: E(B-V) = 0.09 +/- 0.02 fluxnum_4: 3 fluxval_4: F-LINE(1548) = 15 +/- 5 E-15 fluxnum_5: 4 fluxval_5: F-LINE(1403) = 4 +/- 2 E-16 ! targnum: 7 name_1: STAR-0323+4944 name_2: HE709 descr_1: STAR; TYPE=G0 V; OPEN CLUSTER pos_1: RA=3H 23M 8.3S +/- 1", pos_2: DEC=+49D 44' 08" +/- 1" equinox: 1950 pm_or_par: N comment_1: FAR-UV SPECTRA comment_2: OF SOLAR-TYPE STARS comment_3: IN YOUNG GALACTIC CLUSTERS comment_4: ALPHA PERSEI G0 V STAR fluxnum_1: 1 fluxval_1: V = +10.9 +/- 0.1, TYPE = G0 V fluxnum_2: 2 fluxval_2: B-V = +0.68 +/- 0.02 fluxnum_3: 2 fluxval_3: E(B-V) = 0.09 +/- 0.02 fluxnum_4: 3 fluxval_4: F-LINE(1548) = 15 +/- 5 E-15 fluxnum_5: 4 fluxval_5: F-LINE(1403) = 4 +/- 2 E-16 ! targnum: 8 name_1: STAR-0314+4839 name_2: HE350 descr_1: STAR; TYPE=G0 V; OPEN CLUSTER pos_1: RA=3H 14M 5.6S +/- 1", pos_2: DEC=+48D 39' 12" +/- 1" equinox: 1950 pm_or_par: N comment_1: FAR-UV SPECTRA comment_2: OF SOLAR-TYPE STARS comment_3: IN YOUNG GALACTIC CLUSTERS comment_4: ALPHA PERSEI G0 V STAR fluxnum_1: 1 fluxval_1: V = +11.0 +/- 0.1, TYPE = G0 V fluxnum_2: 2 fluxval_2: B-V = +0.68 +/- 0.02 fluxnum_3: 2 fluxval_3: E(B-V) = 0.09 +/- 0.02 fluxnum_4: 3 fluxval_4: F-LINE(1548) = 15 +/- 5 E-15 fluxnum_5: 4 fluxval_5: F-LINE(1403) = 4 +/- 2 E-16 ! targnum: 9 name_1: STAR-0322+4903 name_2: HE696 descr_1: STAR; TYPE=G3 V; OPEN CLUSTER pos_1: RA=3H 22M 45.4S +/- 1", pos_2: DEC=+49D 3' 05" +/- 1" equinox: 1950 pm_or_par: N comment_1: FAR-UV SPECTRA comment_2: OF SOLAR-TYPE STARS comment_3: IN YOUNG GALACTIC CLUSTERS comment_4: ALPHA PERSEI G3 V STAR fluxnum_1: 1 fluxval_1: V = +11.4 +/- 0.1, TYPE = G3 V fluxnum_2: 2 fluxval_2: B-V = +0.74 +/- 0.02 fluxnum_3: 2 fluxval_3: E(B-V) = 0.09 +/- 0.02 fluxnum_4: 3 fluxval_4: F-LINE(1548) = 15 +/- 5 E-15 fluxnum_5: 4 fluxval_5: F-LINE(1403) = 4 +/- 2 E-16 ! targnum: 10 name_1: STAR-0327+4743 name_2: HE917 descr_1: STAR; TYPE=G1 V; OPEN CLUSTER pos_1: RA=3H 27M 15.5S +/- 1", pos_2: DEC=+47D 43' 10" +/- 1" equinox: 1950 pm_or_par: N comment_1: FAR-UV SPECTRA comment_2: OF SOLAR-TYPE STARS comment_3: IN YOUNG GALACTIC CLUSTERS comment_4: ALPHA PERSEI G1 V STAR fluxnum_1: 1 fluxval_1: V = +11.1 +/- 0.1, TYPE = G1 V fluxnum_2: 2 fluxval_2: B-V = +0.70 +/- 0.02 fluxnum_3: 2 fluxval_3: E(B-V) = 0.09 +/- 0.02 fluxnum_4: 3 fluxval_4: F-LINE(1548) = 15 +/- 5 E-15 fluxnum_5: 4 fluxval_5: F-LINE(1403) = 4 +/- 2 E-16 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 2.000 sequence_1: DEFINE sequence_2: DEEP targname: # config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1533 num_exp: # time_per_exp: 190.5S fluxnum_1: 3 priority: 1 param_1: STEP-PATT=5 req_1: CONDITIONAL IF TAC OK; req_2: GROUP 2-3 WITHIN 1D ! linenum: 3.000 sequence_1: DEFINE sequence_2: DEEP targname: # config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1303 num_exp: # time_per_exp: 300.0S fluxnum_1: 4 priority: 2 param_1: STEP-PATT=5 req_1: CONDITIONAL IF TAC OK; req_2: GROUP 2-3 WITHIN 1D ! linenum: 4.000 targname: STAR-0338+2428 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5S s_to_n: 10 fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: SEARCH-SIZE=5, param_2: FAINT=100 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 4.010; req_3: CYCLE 2/4.000-4.100; req_4: SEQ 4.000-4.020 comment_1: FAINT TO BE REVISED comment_2: WHEN N2 CAL AVAILABLE ! linenum: 4.010 targname: STAR-0338+2428 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 73.6S fluxnum_1: 1 priority: 1 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 4.020-4.100 comment_1: STEP-TIME=1.6 SEC comment_2: CENTER IN LSA AFTER NEW DEFCAL ! linenum: 4.020 targname: STAR-0338+2428 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S priority: 1 req_1: CONDITIONAL IF TAC OK comment_1: TAKE MAP AFTER CENTERING comment_2: 200 MSEC INTEGRATIONS ! linenum: 4.100 sequence_1: USE sequence_2: DEEP targname: STAR-0338+2428 num_exp: 10 req_1: CONDITIONAL IF TAC OK; ! linenum: 5.000 targname: STAR-0341+2403 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5S s_to_n: 10 fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: SEARCH-SIZE=5, param_2: FAINT=100 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 5.010; req_3: CYCLE 2/5.000-5.100; req_4: SEQ 5.000-5.020 comment_1: FAINT TO BE REVISED comment_2: WHEN N2 CAL AVAILABLE ! linenum: 5.010 targname: STAR-0341+2403 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 73.6S fluxnum_1: 1 priority: 1 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 5.020-5.100 comment_1: STEP-TIME=1.6 SEC comment_2: CENTER IN LSA AFTER NEW DEFCAL ! linenum: 5.020 targname: STAR-0341+2403 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S priority: 1 req_1: CONDITIONAL IF TAC OK comment_1: TAKE MAP AFTER CENTERING comment_2: 200 MSEC INTEGRATIONS ! linenum: 5.100 sequence_1: USE sequence_2: DEEP targname: STAR-0341+2403 num_exp: 10 ! linenum: 6.000 targname: STAR-0322+4915 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5S s_to_n: 10 fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: SEARCH-SIZE=5, param_2: FAINT=100 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 6.010; req_3: CYCLE 2/6.000-6.100; req_4: SEQ 6.000-6.020 comment_1: FAINT TO BE REVISED comment_2: WHEN N2 CAL AVAILABLE ! linenum: 6.010 targname: STAR-0322+4915 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 73.6S fluxnum_1: 1 priority: 1 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 6.020-6.100 comment_1: STEP-TIME=1.6 SEC comment_2: CENTER IN LSA AFTER NEW DEFCAL ! linenum: 6.020 targname: STAR-0322+4915 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S priority: 1 req_1: CONDITIONAL IF TAC OK comment_1: TAKE MAP AFTER CENTERING comment_2: 200 MSEC INTEGRATIONS ! linenum: 6.100 sequence_1: USE sequence_2: DEEP targname: STAR-0322+4915 num_exp: 7 ! linenum: 7.000 targname: STAR-0323+4944 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5S s_to_n: 10 fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: SEARCH-SIZE=5, param_2: FAINT=100 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 7.010; req_3: CYCLE 2/7.000-7.100; req_4: SEQ 7.000-7.020 comment_1: FAINT TO BE REVISED comment_2: WHEN N2 CAL AVAILABLE ! linenum: 7.010 targname: STAR-0323+4944 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 73.6S fluxnum_1: 1 priority: 1 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 7.020-7.100 comment_1: STEP-TIME=1.6 SEC comment_2: CENTER IN LSA AFTER NEW DEFCAL ! linenum: 7.020 targname: STAR-0323+4944 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S priority: 1 req_1: CONDITIONAL IF TAC OK comment_1: TAKE MAP AFTER CENTERING comment_2: 200 MSEC INTEGRATIONS ! linenum: 7.100 sequence_1: USE sequence_2: DEEP targname: STAR-0323+4944 num_exp: 7 ! linenum: 7.500 sequence_1: DEFINE sequence_2: QUIK targname: # config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1430 num_exp: # time_per_exp: 300.0S fluxnum_1: 3 priority: 1 param_1: STEP-PATT=5 req_1: CONDITIONAL IF TAC OK ! linenum: 8.000 targname: STAR-0340+2415 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5S s_to_n: 10 fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: SEARCH-SIZE=5, param_2: FAINT=100 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 8.010; req_3: CYCLE 2/8.000-8.100; req_4: SEQ 8.000-8.020 comment_1: FAINT TO BE REVISED comment_2: WHEN N2 CAL AVAILABLE ! linenum: 8.010 targname: STAR-0340+2415 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 73.6S fluxnum_1: 1 priority: 1 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 8.020-8.100 comment_1: STEP-TIME=1.6 SEC comment_2: CENTER IN LSA AFTER NEW DEFCAL ! linenum: 8.020 targname: STAR-0340+2415 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S priority: 1 req_1: CONDITIONAL IF TAC OK comment_1: TAKE MAP AFTER CENTERING comment_2: 200 MSEC INTEGRATIONS ! linenum: 8.100 sequence_1: USE sequence_2: QUIK targname: STAR-0340+2415 num_exp: 7 ! linenum: 9.000 targname: STAR-0340+2449 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5S s_to_n: 10 fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: SEARCH-SIZE=5, param_2: FAINT=100 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 9.010; req_3: CYCLE 2/9.000-9.100; req_4: SEQ 9.000-9.020 comment_1: FAINT TO BE REVISED comment_2: WHEN N2 CAL AVAILABLE ! linenum: 9.010 targname: STAR-0340+2449 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 73.6S fluxnum_1: 1 priority: 1 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 9.020-9.100 comment_1: STEP-TIME=1.6 SEC comment_2: CENTER IN LSA AFTER NEW DEFCAL ! linenum: 9.020 targname: STAR-0340+2449 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S priority: 1 req_1: CONDITIONAL IF TAC OK comment_1: TAKE MAP AFTER CENTERING comment_2: 200 MSEC INTEGRATIONS ! linenum: 9.100 sequence_1: USE sequence_2: QUIK targname: STAR-0340+2449 num_exp: 7 ! linenum: 10.000 targname: STAR-0340+2316 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5S s_to_n: 10 fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: SEARCH-SIZE=5, param_2: FAINT=100 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 10.010; req_3: CYCLE 2/10.000-10.100; req_4: SEQ 10.000-10.020 comment_1: FAINT TO BE REVISED comment_2: WHEN N2 CAL AVAILABLE ! linenum: 10.010 targname: STAR-0340+2316 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 73.6S fluxnum_1: 1 priority: 1 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 10.020-10.100 comment_1: STEP-TIME=1.6 SEC comment_2: CENTER IN LSA AFTER NEW DEFCAL ! linenum: 10.020 targname: STAR-0340+2316 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S priority: 1 req_1: CONDITIONAL IF TAC OK comment_1: TAKE MAP AFTER CENTERING comment_2: 200 MSEC INTEGRATIONS ! linenum: 10.100 sequence_1: USE sequence_2: QUIK targname: STAR-0340+2316 num_exp: 7 ! linenum: 11.000 targname: STAR-0314+4839 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5S s_to_n: 10 fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: SEARCH-SIZE=5, param_2: FAINT=100 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 11.010; req_3: CYCLE 2/11.000-11.100; req_4: SEQ 11.000-11.020 comment_1: FAINT TO BE REVISED comment_2: WHEN N2 CAL AVAILABLE ! linenum: 11.010 targname: STAR-0314+4839 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 73.6S fluxnum_1: 1 priority: 1 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 11.020-11.100 comment_1: STEP-TIME=1.6 SEC comment_2: CENTER IN LSA AFTER NEW DEFCAL ! linenum: 11.020 targname: STAR-0314+4839 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S priority: 1 req_1: CONDITIONAL IF TAC OK comment_1: TAKE MAP AFTER CENTERING comment_2: 200 MSEC INTEGRATIONS ! linenum: 11.100 sequence_1: USE sequence_2: QUIK targname: STAR-0314+4839 num_exp: 4 ! linenum: 12.000 targname: STAR-0322+4903 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5S s_to_n: 10 fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: SEARCH-SIZE=5, param_2: FAINT=100 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 12.010; req_3: CYCLE 2/12.000-12.100; req_4: SEQ 12.000-12.020 comment_1: FAINT TO BE REVISED comment_2: WHEN N2 CAL AVAILABLE ! linenum: 12.010 targname: STAR-0322+4903 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 73.6S fluxnum_1: 1 priority: 1 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 12.020-12.100 comment_1: STEP-TIME=1.6 SEC comment_2: CENTER IN LSA AFTER NEW DEFCAL ! linenum: 12.020 targname: STAR-0322+4903 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S priority: 1 req_1: CONDITIONAL IF TAC OK comment_1: TAKE MAP AFTER CENTERING comment_2: 200 MSEC INTEGRATIONS ! linenum: 12.100 sequence_1: USE sequence_2: QUIK targname: STAR-0322+4903 num_exp: 4 ! linenum: 13.000 targname: STAR-0327+4743 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5S s_to_n: 10 fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: SEARCH-SIZE=5, param_2: FAINT=100 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 13.010; req_3: CYCLE 2/13.000-13.100; req_4: SEQ 13.000-13.020 comment_1: FAINT TO BE REVISED comment_2: WHEN N2 CAL AVAILABLE ! linenum: 13.010 targname: STAR-0327+4743 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 73.6S fluxnum_1: 1 priority: 1 req_1: CONDITIONAL IF TAC OK; req_2: ONBOARD ACQ FOR 13.020-13.100 comment_1: STEP-TIME=1.6 SEC comment_2: CENTER IN LSA AFTER NEW DEFCAL ! linenum: 13.020 targname: STAR-0327+4743 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S priority: 1 req_1: CONDITIONAL IF TAC OK comment_1: TAKE MAP AFTER CENTERING comment_2: 200 MSEC INTEGRATIONS ! linenum: 13.100 sequence_1: USE sequence_2: QUIK targname: STAR-0327+4743 num_exp: 4 ! ! end of exposure logsheet ! No scan data records found