Re-submission of FrontierSN3 proposal.
-1181027880
Assigned ID: 23
----- Attempting Submission 1 (Tue Mar 31 16:12:12 GMT 2015) -----
HST Phase I Proposal 23 (frontierSN3.apt) successfully submitted.
Receipt: # 23-1
----- Attempting Submission 2 (Thu Apr 09 22:12:45 GMT 2015) -----
HST Phase I Proposal 23 (frontierSN3.apt) successfully submitted.
Receipt: # 23-2
----- Attempting Submission 3 (Fri Apr 10 20:20:49 GMT 2015) -----
This target is not used in this proposal.
Activating visits A4, A5, A6.
Changed the target and aperture for A5 and A6 to use WFC1-CTE for better CTE.
Changed the BEFORE to be May 31 instead of May 24 (but earlier is still much preferred).
-1806770382
----- Attempting Submission 1 (Thu Jul 23 13:39:39 GMT 2015) -----
----- Attempting Submission 2 (Tue May 03 15:35:51 GMT 2016) -----
----- Attempting Submission 3 (Tue May 10 14:53:34 GMT 2016) -----
----- Attempting Submission 4 (Tue May 10 15:13:31 GMT 2016) -----
HST Phase II Proposal 14208 (14208.apt) successfully submitted.
Receipt: # 14208-4
----- Attempting Submission 5 (Tue May 10 15:16:31 GMT 2016) -----
No errors or warnings for activated visits.
Frontier Fields Supernova Search
The HST Frontier Fields (HFF) program presents an extraordinary opportunity for the detection of lensed, high-redshift transients (primarily supernovae, SNe) out to z~3. Over the last 2 years we have been searching the HFF data and following up lensed transients and their host galaxies with HST imaging and ground-based spectroscopy. We have discovered ~40 SNe, which will contribute to tests of Type Ia SN progenitor models by improving rate measurements reaching to $z\sim2.5$. Our sample also includes a subset of highly magnified objects like the multiply imaged SN Refsdal. Positions and time delays of such multiply imaged transients provide powerful constraints for the dark matter distribution in galaxy clusters. In addition, our collection of lensed Type Ia SNe are providing a rigorous test of cluster mass models by directly measuring the lensing magnification. Finally, the rapid and deep imaging of the HFF program has surprisingly opened up a new discovery space, revealing at least one peculiarly fast and faint astrophysical transient. We propose to extend this program into the third and final year of the Frontier Fields survey, finishing the collection of this unique and diverse sample of distant transients.
This program will execute Target of Opportunity observations to characterize transient sources discovered in the Frontier Fields and other complementary cluster survey programs.
Each observation sequence will be tailored to fit the individual target.
We anticipate spending ~6 orbits on 2-5 candidate SNe that might be at high redshift (z > 1) or significantly magnified (mu > 2). The deep and frequent HFF imaging visits will provide a high S/N and well-sampled light curve in either ACS optical bands or WFC3 IR bands. Our follow-up imaging will provide the complementary bands needed for optical-NIR colors, which are critical for photometric classification and redshift estimation of z > 1 SNe (Riess et al., 2004; Rodney et al., 2012). A typical target in this category might have an AB magnitude of 26.5, requiring a single-orbit visit to get 2-3 filters from the same camera. In some cases we use multiple epochs of imaging are needed to improve the classification and redshift estimate.
We expect the other ~14 orbits will be devoted to one or two objects of particular interest: very high redshift (z > 1.5) and/or strongly lensed (mu > 5) transients like SN HFF14Tom, SN Refsdal, and Spock. These orbits will be used for optical/IR imaging or grism spectroscopy, as appropriate for the source redshift and class. As an example, SN HFF14Tom at z = 1.3 reached a peak brightness at ~24 AB mag in IR bands, and we followed the light curve down to 26.2 AB mag in F140W. The total cost of follow-up was 11 orbits: 5 orbits for ACS G800L grism and 6 single-orbit visits to collect the rest-frame optical light curve using WFC3-IR broad bands. Some objects will require fewer orbits: if they are bright enough for spectroscopy from the ground or if the HFF program provides most of the necessary IR imaging epochs.
COSMOLOGY
0
false
false
false
false
false
false
SUPPORTED
EXT-STAR
GRAVITATIONAL LENS
SUPERNOVA
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
EXT-STAR
GRAVITATIONAL LENS
SUPERNOVA
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
EXT-STAR
GRAVITATIONAL LENS
SUPERNOVA
J2000
J2000
STAR
SUPERNOVA TYPE II
NO
J2000
J2000
EXT-STAR
GRAVITATIONAL LENS
SUPERNOVA
J2000
J2000
STAR
SUPERNOVA TYPE II
NO
J2000
J2000
STAR
SUPERNOVA
SN discovered in HFF or GLASS fields
WFC3/IR
Imaging
No
No
F105W
WFC3/IR
Imaging
No
No
F110W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
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No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/IR
Imaging
No
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F140W
WFC3/IR
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No
No
F153M
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F850LP
ACS/WFC
Spectroscopic
No
No
G800L
WFC3/IR
Imaging
No
No
F105W
WFC3/IR
Imaging
No
No
F110W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/IR
Imaging
No
No
F140W
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F850LP
ACS/WFC
Spectroscopic
No
No
G800L
WFC3/IR
Imaging
No
No
F105W
WFC3/IR
Imaging
No
No
F110W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/IR
Imaging
No
No
F140W
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F850LP
ACS/WFC
Spectroscopic
No
No
G800L
POS-TARG
DITHER
0.173
LINE
0.112
false
false
81.785
4
23.884
WFC3-UVIS-DITHER-BOX
2
false
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:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2992
:pcs-gap 0
)
false
2
0
Template Observation.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
NOTE: this template observation is "on hold" below.
Currently set to SCHED100.
(Tic-Visit
:proposal-id 14208
:visit-id "06"
:proposal-version -1
:trans-version "20150609"
:date "23-Jul-2015 08:38:26.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 1693968
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14208
:visit-id "06"
:obset-id "06"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14208
:visit-id "06"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2640
:al-overhead-at-end 0
:internal-dur-at-end 1037
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2992
:pcs-gap 0
)
false
1
0
Template Observation.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
NOTE: this template visit is On Hold below.
(Tic-Visit
:proposal-id 14208
:visit-id "07"
:proposal-version -1
:trans-version "20150609"
:date "23-Jul-2015 09:32:55.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "29"
:si-bright-earth-limb-angle 20.0
:data-volume 1965344
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14208
:visit-id "07"
:obset-id "07"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14208
:visit-id "07"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2659
:al-overhead-at-end 100
:internal-dur-at-end 794
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2992
:pcs-gap 0
)
false
1
0
This is a template for future ToO observations.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
NOTE: this template observation is "on hold" below.
Currently set to SCHED100.
(Tic-Visit
:proposal-id 14208
:visit-id "08"
:proposal-version -1
:trans-version "20150609"
:date "23-Jul-2015 09:37:01.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 1763616
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14208
:visit-id "08"
:obset-id "08"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14208
:visit-id "08"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2659
:al-overhead-at-end 0
:internal-dur-at-end 999
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2992
:pcs-gap 0
)
false
1
0
Template observation.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
NOTE: this template observation is "on hold" below.
Currently set to SCHED100.
(Tic-Visit
:proposal-id 14208
:visit-id "09"
:proposal-version -1
:trans-version "20150609"
:date "23-Jul-2015 09:38:28.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 2134880
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14208
:visit-id "09"
:obset-id "09"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14208
:visit-id "09"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2659
:al-overhead-at-end 0
:internal-dur-at-end 1075
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2992
:pcs-gap 0
)
false
1
0
Template observation.