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Assigned ID: 93
----- Attempting Submission 1 (Tue Apr 07 20:57:05 GMT 2015) -----
HST Phase I Proposal 93 (cy23fei.apt) successfully submitted.
Receipt: # 93-1
The number of orbits used exceeds the number allocated
Phase 2 revised to convert all 4-orbit visits into 3-orbit, or less, visits.
-2108779329
----- Attempting Submission 1 (Thu Jul 02 16:45:02 GMT 2015) -----
----- Attempting Submission 2 (Fri Sep 25 03:47:11 GMT 2015) -----
BOT: all targets previously observed safely by STIS
Orbit Planner was run ("Run All Tools)
Visit Planner was run (ditto)
The Intersection of Atomic Physics and Astrophysics: Identifying UV Fe I Lines from Metal-Poor Turnoff Stars
Observational surveys are expanding, recording ever-fainter sources from the ultraviolet to the infrared. Needed to characterize them are observational ultraviolet templates at high spectral resolution and low metallicity for the oldest populations, and the laboratory astrophysics data essential to model objects such as stars and nebulae at all ages, metallicities, and redshifts.
We address this by proposing to complete the high-resolution UV spectral coverage of four key metal-poor turnoff stars. These are ideal as metal-poor templates of old stars and as the "laboratory source" for the identification of the thousands of lines of neutral iron that appear in stellar spectra, but are absent from or not identified in laboratory spectra. By matching existing stellar spectra to calculations of energy levels, line wavelengths, and gf-values, Peterson & Kurucz (2015) identified 66 Fe I levels with energies up to 8.4eV, yielding 2000 new lines from 1600 Angstroms to 5.4 microns, and empirical gf-values for 640 of these. The proposed work should yield ~500 new levels and ~10,000 new Fe I lines.
The new energy levels and line parameters also will be posted on the Kurucz website. The new spectra, and supporting theoretical calculations, will be integrated into the publicly available HST Advanced Spectral Library (ASTRAL) Treasury Project. This will leverage the utility of these archival spectral templates and atlases in such diverse areas as nucleosynthesis at early epochs, infrared analysis of dust-obscured giants, reconstructing the populations of nearby globular clusters and dwarf galaxies from their integrated light, and deriving age and metallicity for old, distant galaxies.
The observing program is very straightforward and follows essentially exactly that proposed at Phase I (with the exception that one target was eliminated by the TAC). The (four remaining) targets all are relatively bright stars, with accurate Hipparcos coordinates and proper motions. All of the program exposures will use standard E230H settings (2013, 2263, 2513, 2763, 3012), through the default spectroscopic slit (0.2x0.09: SPCH). All of the targets have been observed previously, safely, by STIS; and all have sufficient STIS and IUE spectra to define accurate SEDs (for use with the STIS spectroscopic ETC). The narrow SPCH slit precludes possible interference from nearly stars, which already are eliminated as a concern by virtue of the previous STIS (and IUE) NUV spectra. Even the brightest exposure is an order of magnitude below any of the NUV MAMA detector local or global bright limits. These metal-poor F/G stars are not known to flare, and even if they did, the influence on the broad-band NUV intensities would be minimal, since the major enhanced effects are confined to the FUV and X-ray regions.
Tagret acquisitions initially are by the CDD, with the MIRROR and ND3 filter; exposure times are set to yield more than adequate counts. The SPCH peak-ups are performed in dispersed light with the low-res optical grating, G430L, and the CCD; the minimal (0.2 s) exposure times yield roughly a million, or more, total counts; but avoid saturation of the spectral segment.
The (extensive) observations of targets HD-84937 and HD-94028 were divided into a series of 10 and 5 visits, respectively, of 4 orbits each. The smaller programs for HD-140283 and HD-211998 were done with pairs of 3-orbit visits. In order to minimize "breathing" effects (de-focusing of the telescope image due to environmental changes), the shortest-wavelength exposures (most susceptible to these effects) were placed at the ends of each visit. The visits were designed to ensure maximum fixed-pattern mitigation.
Postscript (24 September 2015)
After the Phase2 submission, we were asked by the Long Range Planning Group to convert our fifteen 4-orbit visits (for HD-84937 and HD-94028) into shorter versions to help the scheduling process. The Telescope Time Review Board then approved two additional orbits for the program, to make up for the loss of exposure time that accompanies the somewhat less efficient 3-orbit visits. The modified program (which affects only the HD-84937 and HD-94028 visits) consists of fourteen 3-orbit visits and one 2-orbit visit for HD-84937, and seven 3-orbit visits for HD-94028. The visits were restructured so that, aside from one exception, each consists of exposures in a single setting. The effective time sequence in each visit allows breathing effects to be recognized more easily. The shorter sequences also make throughput losses due to slight pointing drifts less likely.
COOL STARS
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F3-F9
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This object was generated by the targetselector and retrieved from the SIMBAD database.
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)
(Tic-Orbit
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
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)
true
3
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
/private/var/folders/wk/kryl66hd5l148rf9p2bj1m2c0000gn/T/OPVisit2776760180386143729.xml
(Tic-Visit
:proposal-id 14161
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:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 279984
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14161
:visit-id "C0"
:obset-id "C0"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14161
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:orbit-number 1
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:si-vis-utilization 2885
:al-overhead-at-end 0
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:dark-offset NIL
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:max-dark-utilization 1920
:low-sky "N"
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)
(Tic-Orbit
:proposal-id 14161
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:si-vis-utilization 2996
:al-overhead-at-end 194
:internal-dur-at-end 0
:dark-offset NIL
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)
(Tic-Orbit
:proposal-id 14161
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:si-vis-utilization 2996
:al-overhead-at-end 194
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
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)
true
3
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
/private/var/folders/wk/kryl66hd5l148rf9p2bj1m2c0000gn/T/OPVisit8337876754365432309.xml
(Tic-Visit
:proposal-id 14161
:visit-id "C1"
:proposal-version -1
:trans-version "20150609"
:date "24-Sep-2015 18:07:30.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 297392
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14161
:visit-id "C1"
:obset-id "C1"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14161
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:orbit-number 1
:pcs-time 333
:si-vis-utilization 2885
:al-overhead-at-end 0
:internal-dur-at-end 113
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3218
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)
(Tic-Orbit
:proposal-id 14161
:visit-id "C1"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2996
:al-overhead-at-end 194
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3218
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)
(Tic-Orbit
:proposal-id 14161
:visit-id "C1"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2996
:al-overhead-at-end 194
:internal-dur-at-end 319
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3218
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)
true
3
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
/private/var/folders/wk/kryl66hd5l148rf9p2bj1m2c0000gn/T/OPVisit7780324458644970818.xml
(Tic-Visit
:proposal-id 14161
:visit-id "D0"
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:trans-version "20150609"
:date "24-Sep-2015 18:07:33.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 279984
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14161
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:obset-id "D0"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14161
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:orbit-number 1
:pcs-time 333
:si-vis-utilization 3263
:al-overhead-at-end 0
:internal-dur-at-end 113
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3596
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14161
:visit-id "D0"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 3374
:al-overhead-at-end 194
:internal-dur-at-end 0
:dark-offset NIL
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)
(Tic-Orbit
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:dark-offset NIL
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)
true
3
0
/private/var/folders/wk/kryl66hd5l148rf9p2bj1m2c0000gn/T/OPVisit6027879495123878320.xml
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 14161
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:number-of-orbits 3
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:data-volume 297392
:tdrss-contact-duration 0
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)
(Tic-Obset
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)
(Tic-Orbit
:proposal-id 14161
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:orbit-number 1
:pcs-time 333
:si-vis-utilization 3263
:al-overhead-at-end 0
:internal-dur-at-end 113
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3596
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14161
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:orbit-number 2
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:si-vis-utilization 3374
:al-overhead-at-end 194
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
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:low-sky "N"
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)
(Tic-Orbit
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:orbit-number 3
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:al-overhead-at-end 194
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:dark-offset NIL
:dark-utilization 0
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)
true
3
0