Cannot find file /Users/pbrown/Downloads/HST_UV_sample (7).pdf
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Assigned ID: 1076
----- Attempting Submission 1 (Sat Mar 07 00:59:55 GMT 2020) -----
HST Phase I Proposal 1076 successfully submitted.
Receipt: # 1076-1
----- Attempting Submission 2 (Sat Mar 07 01:05:21 GMT 2020) -----
HST Phase I Proposal 1076 successfully submitted.
Receipt: # 1076-2
Fixed target SN2022vqz is set as the target for visits 25-30
visit planner isn't working on my machine
1056135172
----- Attempting Submission 1 (Tue Jun 30 05:15:01 GMT 2020) -----
----- Attempting Submission 2 (Tue Apr 19 14:48:19 GMT 2022) -----
----- Attempting Submission 3 (Mon May 02 14:10:01 GMT 2022) -----
----- Attempting Submission 4 (Fri Sep 30 16:35:01 GMT 2022) -----
HST Phase II Proposal 16190 successfully submitted.
Receipt: # 16190-4
----- Attempting Submission 5 (Fri Sep 30 19:52:27 GMT 2022) -----
orbit planner looks like it has run, but when I update display it just hangs.
Ultraviolet Spectroscopy of Extreme Standard Candles
Despite their widespread use as standard candles to measure cosmological distances, Type Ia supernovae are not a homogeneous group of explosions. There are variations in optical light curve shape and ejecta velocity, for example. The sensitivity of the UV to differences in progenitor systems, explosion physics, and environmental conditions makes it a vital regime to determine the physical cause and magnitude of the differences and their effect on the optical bands currently used for cosmological measurements. The goal of understanding the range of progenitor and explosion properties of SNe Ia can be advanced by obtaining UV spectra covering the range of Type Ia supernova properties. The proposed observations will sparsely sample the multi-dimensional parameter spaces of the observed and physical differences between various classes. The goal is to bring order to these disparate objects by determining which are actually physically related and by what parameters. Combined with previous HST observations, these observations will form the definitive observational sample for building theoretical models, constraining progenitor environments, and comparing with high-redshift supernovae from past and future observatories including LSST and WFIRST.
This is a ToO proposal to obtain multi-epoch ultraviolet spectroscopy of one each of four extreme subtypes of supernovae Ia.
To follow the UV spectral evolution and facilitate abundance
tomography, we will observe each of the targeted SNe Ia at
six epochs before and near maximum light. Since SNe reach their peak brightness
about 18 days after explosion, this will require a disruptive ToO.
Many very nearby SNe are discovered and characterized at least a week
before peak brightness, sometimes within days of explosion.
Early observations are more sensitive to the
outermost layers of the SN ejecta and exhibit larger variations in the mid-UV
flux, so we will work with our program coordinator to begin HST
observations as soon as is reasonable. We do not require an
ultra-rapid ToO. Ideally we would trigger and begin observing sooner than ten days before maximum light in the optical (several days prior to the minimum in the UV-optical colors for normal SNe Ia), with observations occurring 2, 4, 6, 10, and 14 days later. The exact cadence will be chosen at the time of triggering based on the estimated age of the SN and the time until HST can first observe it.
To measure the flux through the mid-UV we will use STIS with the MAMA detector and the G230L filter plus the 0.2\arcsec x50\arcsec slit. The MAMA detector is necessary because of scattered light on the STIS CCD for red objects.
Swift/UVOT observations obtained prior to triggering will be used to ensure the safety of the field for observations with STIS/MAMA.
We will additionally obtain one near-UV/optical spectrum at each epoch using the G430L grism to measure the NUV spectrum and ensure overlap of our spectra with the optical where the vast majority of SN characterization is performed. The NUV-region just shortward of the atmospheric cutoff is especially crucial to identifying the NUV differences.
The PI Peter Brown leads the Swift SN program and has led three HST programs for ultraviolet spectroscopy of supernovae. He is member of the Las Cumbres Observatory Global Supernova Project, which obtains well sampled optical photometry and spectroscopy for nearby supernovae. The LCO GSP will provide complementary observations in support of this program.
Yi Yang (Weizmann Institute) is an expert on SN Ia polarimetry/geometry, light echoes and dust reddening. Nicholas Suntzeff has extensive experience with supernovae, their standardization, and physical interpretation.
Jujia Zhang (Yunnan Observatories, Chinese Academy of Sciences) studies the various spectral features and the differences between high-velocity and normal type Ia supernovae.
Aleksandar Cikota (Lawrence Berkeley National Laboratory) is an expert on SN polarization/geometry and dust extinction.
Xiaofeng Wang defined the high-velocity subclass and the correlations with color, reddening laws, and velocity. Xiaofeng Wang leads survey projects TNTS, PTSS etc. which can provide suitable SN Ia candidates for UV spectroscopy, and the followup facilities such as Tsinghua-NAOC 0.8-m telescope (dedicated for SN photometry), Tsinghua 0.4-m telescope (dedicated for photometry of bright SNe) , Xinglong 2.16-m telescope, and Lijiang 2.4-m telescope can be used for followup observations.
Lifan Wang is an expert on type Ia supernova colors and spectroscopy. Both Dr. Wangs worked on SN2004dt, a peculiar UV-bright supernova Ia.
Eddie Baron and Peter Hoeflich are experts in the theoretical modeling of supernovae and will help build models to match the observations obtained here, interpret the results, and apply them to the broader sample of supernovae observed in the ultraviolet.
Chris Ashall is an expert on radiation transport modeling (abundance tomography), and observations of peculiar (91bg-like) type Ia supernovae.
Peter Milne has experience working with the UVOT light curves of type Ia supernovae.He has published three studies that utilize the UVOT sample of SN~Ia photometry (Milne et al. 2010, 2013, 2015). He led the team that discovered the existence of the NUVB/NUVR bi-modality in normal SNe~Ia. He is currently preparing a paper on sub-groups within narrow-peaked SNe~Ia. He runs the Super-LOTIS telescope and is a member of the AzTEC project, and will assist with the coordination of ground-based, Swift, and HST observations.
Luis Galbany was/is a member of the SDSS-II SN survey, the DES SN group, the LSST-DESC SN group, and the CSP. He has experience reducing optical and NIR imaging and spectroscopic data.
Andy Howell is PI of the Global Supernova Project, which will be used to get coordinated ground-based optical photometry and spectroscopy. I'm also PI of a Swift Key Project to study photometrically SNe in the UV. The GSP will help to vet targets for submission to HST.
Stellar Physics and Stellar Types
6
false
false
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false
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false
SUPPORTED
EXT-STAR
SUPERNOVA TYPE IA
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NO
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(Tic-Orbit
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:si-vis-utilization 2750
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(Tic-Orbit
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false
3
0
ToO trigger
Timing link suitability includes constraints ([26 After 25 by 2.0 to 3.0 days] [27 After 26 by 2.0 to 3.0 days])
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
/Users/supernova/Documents/OP-cache/vqz_apt-v26.xml
(Tic-Visit
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(Tic-Orbit
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(Tic-Orbit
:proposal-id 16190
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:pcs-time 392
:si-vis-utilization 2773
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(Tic-Orbit
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true
3
0
ToO trigger
Timing link suitability includes constraints ([09 After 08 by 2.0 to 3.0 days] [18 After 09 by 4.0 to 6.0 days])
The scheduling data was generated by CASM 30.1.
CASM was run in Phase II mode.
(Tic-Visit
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(Tic-Orbit
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(Tic-Orbit
:proposal-id 16190
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:pcs-time 392
:si-vis-utilization 2750
:al-overhead-at-end 85
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(Tic-Orbit
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:si-vis-utilization 2750
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:max-dark-utilization 1920
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false
3
0
ToO trigger
Timing link suitability includes constraints ([27 After 26 by 2.0 to 3.0 days] [28 After 27 by 5.0 to 6.0 days])
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
/Users/supernova/Documents/OP-cache/vqz_apt-v27.xml
(Tic-Visit
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(Tic-Orbit
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(Tic-Orbit
:proposal-id 16190
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:orbit-number 2
:pcs-time 392
:si-vis-utilization 2750
:al-overhead-at-end 85
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(Tic-Orbit
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:pcs-time 392
:si-vis-utilization 2750
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:max-dark-utilization 1920
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)
true
3
0
ToO trigger
Timing link suitability includes constraints ([18 After 09 by 4.0 to 6.0 days] [10 After 18 by 4.0 to 6.0 days])
The scheduling data was generated by CASM 30.1.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 16190
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(Tic-Orbit
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(Tic-Orbit
:proposal-id 16190
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:orbit-number 2
:pcs-time 392
:si-vis-utilization 2750
:al-overhead-at-end 85
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(Tic-Orbit
:proposal-id 16190
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)
false
3
0
ToO trigger
Timing link suitability includes constraints ([28 After 27 by 5.0 to 6.0 days] [29 After 28 by 5.0 to 6.0 days])
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
/Users/supernova/Documents/OP-cache/vqz_apt-v28.xml
(Tic-Visit
:proposal-id 16190
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(Tic-Obset
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(Tic-Orbit
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(Tic-Orbit
:proposal-id 16190
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:pcs-time 392
:si-vis-utilization 2750
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(Tic-Orbit
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)
true
3
0
ToO trigger
Timing link suitability includes constraints ([11 After 10 by 4.0 to 6.0 days] [10 After 18 by 4.0 to 6.0 days])
The scheduling data was generated by CASM 30.1.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 16190
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(Tic-Obset
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(Tic-Orbit
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(Tic-Orbit
:proposal-id 16190
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:pcs-time 392
:si-vis-utilization 2750
:al-overhead-at-end 85
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:max-dark-utilization 1920
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:pcs-visibility 3142
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)
(Tic-Orbit
:proposal-id 16190
:visit-id "10"
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:pcs-time 392
:si-vis-utilization 2750
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false
3
0
ToO trigger
Timing link suitability includes constraints ([29 After 28 by 5.0 to 6.0 days] [30 After 29 by 5.0 to 10.0 days])
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
/private/var/folders/lm/1s7yhzbn56l3gt6dp_gzhtgc0000gn/T/OPVisit5415402408967060109.xml
(Tic-Visit
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(Tic-Obset
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(Tic-Orbit
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(Tic-Orbit
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(Tic-Orbit
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)
true
3
0
ToO trigger
Timing link suitability includes constraints ([11 After 10 by 4.0 to 6.0 days])
The scheduling data was generated by CASM 30.1.
CASM was run in Phase II mode.
(Tic-Visit
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(Tic-Orbit
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(Tic-Orbit
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(Tic-Orbit
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false
4
0
ToO trigger
Timing link suitability includes constraints ([30 After 29 by 5.0 to 10.0 days])
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
/private/var/folders/lm/1s7yhzbn56l3gt6dp_gzhtgc0000gn/T/OPVisit12819941039728366070.xml
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(Tic-Orbit
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(Tic-Orbit
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true
4
0
ToO trigger
Timing link suitability includes constraints ([13 After 12 by 2.0 to 3.0 days])
The scheduling data was generated by CASM 30.1.
CASM was run in Phase II mode.
1650611445000
152.3
(Tic-Visit
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(Tic-Orbit
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(Tic-Orbit
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(Tic-Orbit
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(Tic-Orbit
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false
4
0
Timing link suitability includes constraints ([13 After 12 by 2.0 to 3.0 days] [14 After 13 by 2.0 to 3.0 days])
The scheduling data was generated by CASM 30.1.
CASM was run in Phase II mode.
1650931515000
152.0
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(Tic-Orbit
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(Tic-Orbit
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false
3
0
Timing link suitability includes constraints ([14 After 13 by 2.0 to 3.0 days] [15 After 14 by 2.0 to 3.0 days])
The scheduling data was generated by CASM 30.1.
CASM was run in Phase II mode.
1651040112000
152.0
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(Tic-Orbit
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(Tic-Orbit
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false
3
0
Timing link suitability includes constraints ([15 After 14 by 2.0 to 3.0 days] [16 After 15 by 2.0 to 3.0 days])
The scheduling data was generated by CASM 30.1.
CASM was run in Phase II mode.
1651948960000
143.2
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(Tic-Orbit
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(Tic-Orbit
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(Tic-Orbit
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false
3
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1652634818000
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(Tic-Orbit
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(Tic-Orbit
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false
3
0
Timing link suitability includes constraints ([17 After 16 by 4.0 to 6.0 days])
The scheduling data was generated by CASM 30.1.
CASM was run in Phase II mode.
1653297742000
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(Tic-Obset
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)
(Tic-Orbit
:proposal-id 16190
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)
(Tic-Orbit
:proposal-id 16190
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:orbit-number 2
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:si-vis-utilization 2535
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(Tic-Orbit
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false
3
0
Timing link suitability includes constraints ([20 After 19 by 2.0 to 3.0 days])
The scheduling data was generated by CASM 28.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 16190
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:trans-version "20200619"
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)
(Tic-Obset
:proposal-id 16190
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:obset-id "19"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16190
:visit-id "19"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2747
:al-overhead-at-end 0
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
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)
(Tic-Orbit
:proposal-id 16190
:visit-id "19"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2750
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)
false
2
0
ToO trigger
Timing link suitability includes constraints ([20 After 19 by 2.0 to 3.0 days] [21 After 20 by 2.0 to 3.0 days])
The scheduling data was generated by CASM 28.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 16190
:visit-id "20"
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:trans-version "20200619"
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:number-of-orbits 2
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:si-bright-earth-limb-angle 20.0
:data-volume 229696
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16190
:visit-id "20"
:obset-id "20"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16190
:visit-id "20"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2747
: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 3142
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16190
:visit-id "20"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2750
:al-overhead-at-end 85
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)
false
2
0
ToO trigger
Timing link suitability includes constraints ([21 After 20 by 2.0 to 3.0 days] [22 After 21 by 2.0 to 3.0 days])
The scheduling data was generated by CASM 28.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 16190
:visit-id "21"
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:trans-version "20200619"
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:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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)
(Tic-Obset
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)
(Tic-Orbit
:proposal-id 16190
:visit-id "21"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2747
:al-overhead-at-end 0
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:dark-utilization 0
:max-dark-utilization 1920
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)
(Tic-Orbit
:proposal-id 16190
:visit-id "21"
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:si-vis-utilization 2750
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
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:pcs-gap 0
)
false
2
0
ToO trigger
Timing link suitability includes constraints ([22 After 21 by 2.0 to 3.0 days] [23 After 22 by 4.0 to 6.0 days])
The scheduling data was generated by CASM 28.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 16190
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:trans-version "20200619"
:date "30-Jun-2020 00:12:21.0"
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)
(Tic-Obset
:proposal-id 16190
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:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16190
:visit-id "22"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2747
:al-overhead-at-end 0
:internal-dur-at-end 113
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
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)
(Tic-Orbit
:proposal-id 16190
:visit-id "22"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2750
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
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)
false
2
0
ToO trigger
Timing link suitability includes constraints ([23 After 22 by 4.0 to 6.0 days] [24 After 23 by 4.0 to 6.0 days])
The scheduling data was generated by CASM 28.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 16190
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:trans-version "20200619"
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(Tic-Obset
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)
(Tic-Orbit
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)
(Tic-Orbit
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:si-vis-utilization 2750
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:dark-offset NIL
:dark-utilization 0
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:pcs-gap 0
)
false
2
0
ToO trigger
Timing link suitability includes constraints ([24 After 23 by 4.0 to 6.0 days])
The scheduling data was generated by CASM 28.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 16190
:visit-id "24"
:proposal-version -1
:trans-version "20200619"
:date "30-Jun-2020 00:02:27.0"
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(Tic-Obset
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)
(Tic-Orbit
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:orbit-number 1
:pcs-time 393
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:al-overhead-at-end 0
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:dark-offset NIL
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)
(Tic-Orbit
:proposal-id 16190
:visit-id "24"
:orbit-number 2
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:si-vis-utilization 2750
:al-overhead-at-end 85
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)
false
2
0
ToO trigger