0
Assigned ID: 1064
----- Attempting Submission 1 (Fri Apr 11 23:35:30 GMT 2014) -----
HST Phase I Proposal 1064 (isolated_dwarfs.apt) successfully submitted.
----- Attempting Submission 2 (Fri Apr 11 23:45:16 GMT 2014) -----
HST Phase I Proposal 1064 (isolated_dwarfs.apt) successfully submitted.
----- Attempting Submission 3 (Fri Apr 11 23:55:39 GMT 2014) -----
HST Phase I Proposal 1064 (isolated_dwarfs.apt) successfully submitted.
----- Attempting Submission 4 (Fri Apr 11 23:58:33 GMT 2014) -----
HST Phase I Proposal 1064 (isolated_dwarfs.apt) successfully submitted.
----- Attempting Submission 5 (Fri Apr 11 23:59:21 GMT 2014) -----
HST Phase I Proposal 1064 (isolated_dwarfs.apt) successfully submitted.
----- Attempting Submission 6 (Sat Apr 12 00:00:47 GMT 2014) -----
0
----- Attempting Submission 1 (Tue Jul 22 11:01:52 GMT 2014) -----
Completing the Census of Isolated Dwarf Galaxy Star Formation Histories
We propose to complete our census of the ancient star formation histories (SFHs) of isolated dwarf galaxies by obtaining deep ACS/WFC optical imaging of WLM and Pegasus Dwarf Irregular Galaxy (PegDIG). They are the only two systems without previous deep HST imaging that are isolated yet close enough to guarantee that their oldest main sequence turnoffs are accessible with HST. We will measure their lifetime SFHs with an age resolution of < 1 Gyr at all epochs to address questions about growth of stellar mass, the effects of reionization, radial population gradients, and variable star populations in WLM and PegDIG.
This program is a concerted effort between theorists and observers to obtain the best possible observational constraints on the early epochs of star formation in isolated low-mass galaxies, which are essential to the next generation of galaxy simulations. With these new observations we will have completed our efforts to collect precise lifetime SFHs of all nearby isolated dwarfs that are accessible with HST. In combination with archival data, we will create a legacy sample isolated dwarfs with identically derived SFHs, that will be serve as the baseline for the community's understanding of how low-mass galaxies form and evolve over a Hubble time and in the absence of environmental effects of a massive host (e.g., tides, ram pressure).
We propose to image WLM and PegDIG using the F475W and F814W filters of ACS/WFC. These filters yield the optimum combination of throughput and age/metallicity for the subgiant branch and main-sequence turnoffs of old (>10 Gyr) stellar populations in these galaxies at (B, I) ~ (29, 28). Our observations are structured to maximize sensitivity to variable stars with periods of ~0.5 day while minimizing the impact of hot pixels and cosmic rays on photometry of stars near the detection limit. We will also image a flanking field in each galaxy as a coordinated parallel observation with WFC3/UVIS in order to constrain radial population gradients. The parallel observations will achieve nearly the same photometric depth as the ACS observations, using the WFC3/UVIS F475W and F814W filters. Our limiting magnitude requirement is based on the expected magnitude and colors of the subgiant branch and main-sequence turnoff, which contain unique information about the oldest stars in the galaxies. The ACS ETC (v. 22.2) suggests that exposure times of ~26 and ~32 ksec in F475W and F814W respectively are sufficient to achieve S/N ~ 10 at the required depth for optimally extracted PSF photometry in WLM. Because PegDIG is more highly reddened, the corresponding exposure times are longer, ~35 and ~33 ksec in F475W and F814W respectively.
The observing plan closely follows our successful Cycle 20 program targeting the Aquarius dwarf (GO-12925). We have divided the observations as closely as possible into visits of 2 orbits each. Each orbit contains one exposure each in F475W and F814W. The exposures are not CR-SPLIT, but we will eliminate hot pixels and CR hits in the combined images by using a 2-3 pixel dither pattern in between orbits according to the ACS instrument handbook; the dither pattern is to be implemented using POS-TARG commands. This minimizes overheads and maximizes sensitivity to faint stars, while separating exposures in each filter by the duration of an orbit in order to improve sampling of variable light star curves. To ensure that the observations span enough of the light curve phase to identify and characterize any prospective RR Lyrae variables, we wish to group all of our visits in each galaxy together within a roughly 3-day window. This strikes a balance between the desire to densely sample light curves and the necessity to allow for easy schedulability. Both WLM and PegDIG have very low ecliptic latitude and thus must be observed when the Sun-telescope-target angle is greater than 100 degrees. However, earthshine is NOT a strong contributor to the background, so we do not require the LOW-SKY constraint. Instead, we have specified the observing dates to ensure low zodiacal light background by using the visit-level BETWEEN constraint. This gains a few extra minutes per orbit compared to the LOW-SKY constraint and does not strongly impact schedulability.
We are using WFC3 to obtain coordinated parallel observations secondary fields in the target galaxies. The specific placement of this field is not important, except within broad limits designed to keep the secondary field roughly along the major axis of the galaxy. In both cases this can be done without significantly impacting schedulability. For Pegasus, the major axis aligns with spacecraft roll angles near the maximum of schedulability (either 45-65 degrees or 245-265 degrees). For WLM, the placement of the coordinated parallel field has more potential impact on the science goals, because of the larger extent of WLM on the sky and higher crowding in the central regions. In order for the parallel field to sample a WLM field of suitable target density, we have specified a roll angle ORIENT between 255-275 degrees; within this range the exact placement is not critical. Because the science goals are similar for the prime and parallel exposures, visits 2-13 for WLM and 2-15 for PegDIG are constrained to have the SAME ORIENT as visit 1 to allow for deep integrations over the entire primary field as well as the parallel field.
Additional comments: Both WLM (GO-6813) and PegDIG (GO-5915) have previous WFPC2 imaging. However, these data are not deep enough to meet the science goals of this program.
RESOLVED STELLAR POPULATIONS
Default
false
false
false
false
false
SUPPORTED
GALAXY
MAGELLANIC IRREGULAR
Most stars fainter than B = 25, I = 24. Limit is B ~ 29, I ~28.
DDO221
J2000
J2000
GALAXY
MAGELLANIC IRREGULAR
Most stars fainter than B = 25, I = 24. Limit is B ~ 29, I ~28.
DDO216
J2000
J2000
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F475W
WFC3/UVIS
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F475W
WFC3/UVIS
Imaging
No
No
F814W
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The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
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:proposal-version -1
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(Tic-Orbit
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(Tic-Orbit
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false
2
0
Timing link suitability includes constraints ([Group (01 02 03 04 05 06 07 08 09 10 11 12 13) Within 3.0 days])
Hst Same orient constraint links visits (01 02 03 04 05 06 07 08 09 10 11 12 13)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 13768
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:proposal-version -1
:trans-version "20140605"
:date "22-Jul-2014 09:18:24.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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false
1
0
Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
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:trans-version "20140605"
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(Tic-Obset
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(Tic-Orbit
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(Tic-Orbit
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true
2
0
Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
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(Tic-Orbit
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true
2
0
Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
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:trans-version "20140605"
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(Tic-Obset
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(Tic-Orbit
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(Tic-Orbit
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true
2
0
Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 13768
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:trans-version "20140605"
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(Tic-Orbit
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(Tic-Orbit
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true
2
0
Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
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:trans-version "20140605"
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(Tic-Obset
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(Tic-Orbit
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(Tic-Orbit
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true
2
0
Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 13768
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:trans-version "20140605"
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(Tic-Obset
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:pcs-mode "FGS"
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(Tic-Orbit
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(Tic-Orbit
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)
true
2
0
Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 13768
:visit-id "20"
:proposal-version -1
:trans-version "20140605"
:date "22-Jul-2014 09:22:03.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 2
:saa-model "29"
:si-bright-earth-limb-angle 20.0
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(Tic-Obset
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:obset-id "20"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13768
:visit-id "20"
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:si-vis-utilization 2767
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)
(Tic-Orbit
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:si-vis-utilization 2935
:al-overhead-at-end 0
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:max-dark-utilization 1920
:low-sky "N"
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:pcs-gap 0
)
true
2
0
Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 13768
:visit-id "21"
:proposal-version -1
:trans-version "20140605"
:date "22-Jul-2014 09:22:45.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 2
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:si-bright-earth-limb-angle 20.0
:data-volume 2291872
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:coron NIL
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(Tic-Obset
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:obset-id "21"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13768
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:si-vis-utilization 2767
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)
(Tic-Orbit
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:max-dark-utilization 1920
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)
true
2
0
Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 13768
:visit-id "22"
:proposal-version -1
:trans-version "20140605"
:date "22-Jul-2014 09:23:36.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 2
:saa-model "29"
:si-bright-earth-limb-angle 20.0
:data-volume 2291872
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:coron NIL
)
(Tic-Obset
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:visit-id "22"
:obset-id "22"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13768
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:orbit-number 1
:pcs-time 333
:si-vis-utilization 2767
:al-overhead-at-end 0
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)
(Tic-Orbit
:proposal-id 13768
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:orbit-number 2
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:si-vis-utilization 2935
:al-overhead-at-end 0
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3226
:pcs-gap 0
)
true
2
0
Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 13768
:visit-id "23"
:proposal-version -1
:trans-version "20140605"
:date "22-Jul-2014 09:24:09.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 2
:saa-model "29"
:si-bright-earth-limb-angle 20.0
:data-volume 2291872
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 13768
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:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13768
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:orbit-number 1
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:al-overhead-at-end 0
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)
(Tic-Orbit
:proposal-id 13768
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:si-vis-utilization 2935
:al-overhead-at-end 0
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:max-dark-utilization 1920
:low-sky "N"
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:pcs-gap 0
)
true
2
0
Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 13768
:visit-id "24"
:proposal-version -1
:trans-version "20140605"
:date "22-Jul-2014 09:24:10.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 2
:saa-model "29"
:si-bright-earth-limb-angle 20.0
:data-volume 2291872
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:coron NIL
)
(Tic-Obset
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:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13768
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:si-vis-utilization 2767
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)
(Tic-Orbit
:proposal-id 13768
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:orbit-number 2
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:low-sky "N"
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:pcs-gap 0
)
true
2
0
Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 13768
:visit-id "25"
:proposal-version -1
:trans-version "20140605"
:date "22-Jul-2014 09:24:11.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 2
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:si-bright-earth-limb-angle 20.0
:data-volume 2291872
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)
(Tic-Obset
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)
(Tic-Orbit
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)
(Tic-Orbit
:proposal-id 13768
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:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3226
:pcs-gap 0
)
true
2
0
Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 13768
:visit-id "26"
:proposal-version -1
:trans-version "20140605"
:date "22-Jul-2014 09:24:12.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 2
:saa-model "29"
:si-bright-earth-limb-angle 20.0
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:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 13768
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)
(Tic-Orbit
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(Tic-Orbit
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true
2
0
Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
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(Tic-Orbit
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true
2
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Timing link suitability includes constraints ([Group (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28) Within 3.0 days])
Hst Same orient constraint links visits (14 15 16 17 18 19 20 21 22 23 24 25 26 27 28)
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
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true
1
0