0
Assigned ID: 229
----- Attempting Submission 1 (Thu Apr 06 14:33:02 GMT 2017) -----
HST Phase I Proposal 229 (uvdwarfs_constrainedorients.apt) successfully submitted.
Receipt: # 229-1
----- Attempting Submission 2 (Fri Apr 07 19:10:30 GMT 2017) -----
HST Phase I Proposal 229 (uvdwarfs_constrainedorients.apt) successfully submitted.
Receipt: # 229-2
ORBITAL VISIBILITY OVERRUN
ORBITAL VISIBILITY OVERRUN
ORBITAL VISIBILITY OVERRUN
02/11/19 ROYLE - Added visit 73 as exact repeat of visit failed visit 23
12/21/18: orient and exposure durations changed for visit 14 due to changes in guide star availability.
12/18/18: orient and exposure durations changed for visit 19 due to changes in guide star availability.
08/24: orients changed for visits 8 and 20 for guide star availability.
Please inspect the schedulability windows for the suite of targets. The worst case targets have individual windows of 13-15 days, with all of these having a
second (usually only slightly smaller) window in 2019—but these targets' windows tend to be bunched in time (e.g., they have approximately the same
short schedulability windows). If the schedulability windows look risky, I could explore the SCHED restrictions more fully.
340024033
----- Attempting Submission 1 (Thu Jul 20 21:04:40 GMT 2017) -----
HST Phase II Proposal 15275 (uvdwarfs_phase2.apt) successfully submitted.
Receipt: # 15275-1
----- Attempting Submission 2 (Thu Aug 24 17:30:16 GMT 2017) -----
----- Attempting Submission 3 (Tue Dec 18 21:47:20 GMT 2018) -----
----- Attempting Submission 4 (Fri Dec 21 19:55:47 GMT 2018) -----
----- Attempting Submission 5 (Mon Feb 11 16:00:28 GMT 2019) -----
orbit planner and visit planner were both run for visit 14, the visit that was updated in this resubmission.
Securing HST's UV Legacy in the Local Volume: Probing Star Formation and the Interstellar Medium in Low Mass Galaxies
We propose WFC3 ultraviolet imaging of the stellar populations of a volume limited sample of 22 low-mass, nearby (<3.5 Mpc), star-forming galaxies, extending HST's resolved stellar populations legacy to include UV observations of the lowest mass and lowest metallicity star-forming environments. We will derive bolometric luminosities, effective temperatures, and constrain the line-of-sight dust extinction for millions of stars in the Local Volume. This will enable us to (1) measure the spatially- and temporally-resolved recent star formation history; (2) infer the unobscured UV flux of the stellar populations; (3) produce high resolution maps of the dust column density and grain size; and (4) reveal the drivers of dust emission. We will directly measure the quantities required to understand the link between star formation and the interstellar medium on sub-kiloparsec scales, test and calibrate widely-used star formation rate indicators, and provide critical constraints on stellar feedback processes. Our team has obtained, reduced, analyzed, and publicly released data from over 1500 orbits of HST imaging of resolved stellar populations in crowded fields, and we are already producing the above measurements for higher mass and metallicity galaxies.
The UV data will yield new insight into the baryonic physics of galaxy formation, producing quantitative constraints on the energies and timescales of interactions between gas, dust, and stars in the low-mass, low-metallicity regime. When combined with existing data from HST, Spitzer, VLA, GALEX, and CARMA, the proposed UV data will make these galaxies a benchmark for ISM studies in low metallicity environments.
The strategy is to obtain UV imaging in two filters, covering the majority of the star forming region in a sample of 22 dwarf galaxies at the edge of the Local Group and in the Local Volume, out to a maximum distance of 3.5 Mpc. The UV imaging locations are chosen to overlap with existing, deep optical archival HST imaging (ACS or WFPC2), and also to overlap WFC3 IR imaging when available, which will provide 4 or 6 filter photometry when the UV imaging is combined with the archival imaging. Parallel imaging in two optical bands is obtained with ACS.
Galaxies within 2.5 Mpc are observed in 2 orbits, while galaxies more distant than 2.5 Mpc are observed in 3 orbits. In the first orbit, WFC3/UVIS and ACS run in parallel to obtain 4 primary exposures in F336W and 4 parallel exposures in F814W. In the second orbit, WFC3/UVIS and ACS run in parallel to obtain 4 primary exposures in F275W and 4 parallel exposures in F606W. When a third orbit is obtained, 2 primary exposures in each of F336W, F275W, and 2 parallel exposures in each of F814W and F606W are taken. All exposures are dithered. Dithers are set up to obtain Nyquist sampling in F336W and to cover the UVIS chip gap. Obtaining at least 4 exposures per filter, and at least 2 exposures on each side of the chip gap, should allow all data to be cleaned of cosmic rays.
All exposure times are optimized to have the shutters of both cameras open during all buffer dumps. Thus, the exposure times are somewhat asymmetric.
Stellar Populations
Stellar Populations
6
false
false
true
false
false
false
false
SUPPORTED
GALAXY
AMORPHOUS IRREGULAR
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the NED database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F275W
WFC3/UVIS
Imaging
No
No
F336W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
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The scheduling data was generated by CASM 25.2.
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The scheduling data was generated by CASM 25.2.
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false
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The scheduling data was generated by CASM 25.2.
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false
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The scheduling data was generated by CASM 25.2.
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The scheduling data was generated by CASM 25.2.
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The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
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The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
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The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
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The scheduling data was generated by CASM 26.2.2.
CASM was run in Phase II mode.
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false
3
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The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
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false
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The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
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false
3
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The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
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(Tic-Orbit
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:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3260
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15275
:visit-id "22"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 3038
:al-overhead-at-end 122
:internal-dur-at-end 668
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3260
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15275
:visit-id "22"
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:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3260
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)
false
3
0
The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
1545457534000
72.0
(Tic-Visit
:proposal-id 15275
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:si-bright-earth-limb-angle 20.0
:data-volume 6875664
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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)
(Tic-Orbit
:proposal-id 15275
:visit-id "23"
:orbit-number 1
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:al-overhead-at-end 122
:internal-dur-at-end 668
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3217
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)
(Tic-Orbit
:proposal-id 15275
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:si-vis-utilization 2995
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:dark-offset NIL
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(Tic-Orbit
:proposal-id 15275
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:orbit-number 3
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
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)
false
3
0
The scheduling data was generated by CASM 26.2.2.
CASM was run in Phase II mode.
/private/var/folders/h2/_3b1kkv56nn2rfp1zrxtm0sc0006z1/T/OPVisit12074221661199627616.xml
Repeat of failed visit 23
(Tic-Visit
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:number-of-orbits 3
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:si-bright-earth-limb-angle 20.0
:data-volume 6875664
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15275
:visit-id "53"
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)
(Tic-Orbit
:proposal-id 15275
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:max-dark-utilization 1920
:low-sky "N"
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:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15275
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:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15275
:visit-id "53"
:orbit-number 3
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:si-vis-utilization 2995
:al-overhead-at-end 122
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3157
:pcs-gap 0
)
false
3
3
The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
1517368229000
160.0
(Tic-Visit
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(Tic-Obset
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)
(Tic-Orbit
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)
(Tic-Orbit
:proposal-id 15275
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)
(Tic-Orbit
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:dark-offset NIL
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)
false
3
0