0
Assigned ID: 3662
----- Attempting Submission 1 (Fri Mar 25 22:49:32 GMT 2022) -----
The number of orbits used exceeds the number allocated
ORBITAL VISIBILITY OVERRUN
ORBITAL VISIBILITY OVERRUN
Re-submission of the phase 2 with repeat of visit 34 as visit 36.
1666763717
----- Attempting Submission 2 (Tue Jul 19 21:11:07 GMT 2022) -----
----- Attempting Submission 3 (Fri Apr 07 13:16:47 GMT 2023) -----
----- Attempting Submission 4 (Wed Apr 12 14:20:26 GMT 2023) -----
----- Attempting Submission 5 (Tue Sep 26 16:12:58 GMT 2023) -----
----- Attempting Submission 6 (Wed Oct 04 08:46:22 GMT 2023) -----
----- Attempting Submission 7 (Fri Oct 06 14:19:59 GMT 2023) -----
----- Attempting Submission 8 (Wed Nov 15 09:29:45 GMT 2023) -----
Exception as can only use FP-POS 3 and 4.
How diverse is the bulk composition of exoplanetary material?
As we move into an epoch of rocky planet detection and characterisation, it is crucial that we can measure the interior composition of exoplanetary material and understand exoplanet diversity. White dwarfs that have accreted chunks of exoplanets are unique laboratories to directly study the bulk composition of exoplanets and investigate geological processes in other planetary systems. We propose to observe 23 white dwarfs which have accreted significant chunks of planets. With Hubble UV spectra we will measure the composition of the parent body that accreted onto each white dwarf, which reveals the unique history of each exoplanet. We will more than double the number of white dwarfs with abundances of all major rock forming elements- moving the field from a story of individual discovery to population statistics. Using this statistical sample we will answer: how diverse is the bulk composition of exoplanetary material?
Technical Set-up: We propose to use the G130M grating in the FUV module with a central wavelength of 1291 A. In accordance with the COS2025 policies, we will only use two FP-POS positions (3 and 4).
COS safety: Our targets are all sufficiently faint that COS safety is not a problem.
CVZ: A few of our targets are located in the continuous viewing zone, but we do not require continuous, uninterrupted observations. Using the visit planner tool, we find that all our targets are schedulable.
Reduced gyro observations: our observations are not time critical, and can be scheduled any time, so reducing the possible observing windows will not affect this proposal. Using the visit planner tool, there are plenty of schedulable opportunities across the cycle for all targets. Target acquisition is required for all of our targets in order to sucessfully complete the proposed observations.
Scheduling: For targets which require >3 orbits, we have split the visits up to ensure maximum schedulability.
SNR: We require a SNR of ~20 around 1320A, close to important lines of carbon.
Ms Laura Rogers, Dr Amy Bonsor, Dr Siyi Xu, Dr Markus Kissler-Patig, Dr Beth Klein, Dr Carl Melis, Prof Ben Zuckerman and Prof Patrick Dufour have been PI or CoI on a number of successful HST/COS proposals related to polluted white dwarfs, and have extensive experience with the preparation of observations, data reduction, and data analysis. Prof Patrick Dufour is an expert on models of white dwarfs, and will fit models to the obtained FUV spectra in order to get updated white dwarf parameters, and the abundances of the exo-planetary material that have polluted the atmospheres of the white dwarfs. Ms Laura Rogers has worked on the optical VLT/X-shooter and KECK/HIRES data of our targets to obtain line strengths and, in collaboration with Prof Patrick Dufour, abundances of the exo-planetary material using the limited available optical lines. Ms Laura Rogers has vast experience analysing spectra, including that of Hubble/COS, and will perform a similar analysis on the HST/COS data as on the optical data. Dr Amy Bonsor is an expert in understanding the composition and geological history of the exo-planetary bodies that have been accreted, crucial to understanding the obtained abundances from Hubble. All team members have experience with and knowledge of observations of polluted white dwarfs and dust discs, and will all be of valuable help with the analysis. Everyone will contribute to the analysis of the data and the preparation of the publications resulting from this proposal.
Exoplanets and Exoplanet Formation
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This object was generated by the targetselector and retrieved from the SIMBAD database.
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EXTRA-SOLAR PLANETARY SYSTEM
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EXTRA-SOLAR PLANETARY SYSTEM
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EXTRA-SOLAR PLANETARY SYSTEM
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EXTRA-SOLAR PLANETARY SYSTEM
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This object was generated by the targetselector and retrieved from the SIMBAD database.
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true
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The scheduling data was generated by CASM 30.3.
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The scheduling data was generated by CASM 30.3.
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COS/FUV spectrum of GaiaJ1617+1620. VISIT 2 - split into two visits for ease of scheduling.
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true
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COS/FUV spectrum of GaiaJ2209+1223. VISIT 1 - split into two visits for ease of scheduling.
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COS/FUV spectrum of GaiaJ2209+1223. VISIT 1 - split into two visits for ease of scheduling.
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(Tic-Orbit
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true
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COS/FUV spectrum of GaiaJ2209+1223. VISIT 2 - split into two visits for ease of scheduling.
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COS/FUV spectrum of GaiaJ2209+1223. VISIT 2 - split into two visits for ease of scheduling.
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true
1
0
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
COS/FUV spectrum of GaiaJ1447-3835.
1688598954000
92.5831504379604
(Tic-Visit
:proposal-id 17185
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(Tic-Orbit
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)
true
1
0
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
COS/FUV spectrum of GaiaJ0720-4250.
1682355892000
107.13480156493301
(Tic-Visit
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(Tic-Orbit
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)
true
1
0
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
COS/FUV spectrum of GaiaJ1153-1536. VISIT 1 - split into two visits for ease of scheduling.
(Tic-Visit
:proposal-id 17185
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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
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
COS/FUV spectrum of GaiaJ1153-1536. VISIT 2 - split into two visits for ease of scheduling.
(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
The scheduling data was generated by CASM 31.0.
CASM was run in Phase II mode.
COS/FUV spectrum of GaiaJ0737+1541. VISIT 1 - split into two visits for ease of scheduling.
(Tic-Visit
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)
(Tic-Obset
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)
(Tic-Orbit
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:si-vis-utilization 2763
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:pcs-gap 0
)
(Tic-Orbit
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(Tic-Orbit
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true
3
0
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
COS/FUV spectrum of GaiaJ0737+1541. VISIT 2 - split into two visits for ease of scheduling.
1679992913000
97.91000000000003
(Tic-Visit
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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
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
COS/FUV spectrum of SDSSJ2248+2632
1685115261000
254.56127121337443
(Tic-Visit
:proposal-id 17185
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:number-of-orbits 2
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)
(Tic-Obset
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(Tic-Orbit
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:orbit-number 1
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)
(Tic-Orbit
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:max-dark-utilization 1920
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)
true
2
0
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
COS/FUV spectrum of JL-59
1688060037000
323.46371492067783
(Tic-Visit
:proposal-id 17185
:visit-id "25"
:proposal-version -1
:trans-version "20220516"
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:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 313184
:tdrss-contact-duration 0
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)
(Tic-Obset
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)
(Tic-Orbit
:proposal-id 17185
:visit-id "25"
:orbit-number 1
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:si-vis-utilization 3126
:al-overhead-at-end 0
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3519
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
COS/FUV spectrum of GD424.
1680753956000
22.84585894768199
(Tic-Visit
:proposal-id 17185
:visit-id "26"
:proposal-version -1
:trans-version "20220516"
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:number-of-orbits 3
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:si-bright-earth-limb-angle 20.0
:data-volume 226272
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:coron NIL
)
(Tic-Obset
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:visit-id "26"
:obset-id "26"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 17185
:visit-id "26"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 3126
:al-overhead-at-end 0
:internal-dur-at-end 95
:dark-offset NIL
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:max-dark-utilization 1920
:low-sky "N"
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:pcs-gap 0
)
(Tic-Orbit
:proposal-id 17185
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:orbit-number 2
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:si-vis-utilization 3127
:al-overhead-at-end 0
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: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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:si-vis-utilization 3127
:al-overhead-at-end 0
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
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:pcs-gap 0
)
true
3
0
COS/FUV spectrum of GD424.
1698116708000
188.73228570539857
(Tic-Visit
:proposal-id 17185
:visit-id "31"
:proposal-version -1
:trans-version "20220630"
:date "12-Apr-2023 15:18:29.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 147952
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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)
(Tic-Orbit
:proposal-id 17185
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:orbit-number 1
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)
(Tic-Orbit
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:max-dark-utilization 1920
:low-sky "N"
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)
true
2
0
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
COS/FUV spectrum of GaiaJ0218+3625.
1689269474000
258.5949639370061
(Tic-Visit
:proposal-id 17185
:visit-id "27"
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:trans-version "20220516"
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:number-of-orbits 3
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:si-bright-earth-limb-angle 20.0
:data-volume 191488
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)
(Tic-Obset
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)
(Tic-Orbit
:proposal-id 17185
:visit-id "27"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2807
:al-overhead-at-end 0
:internal-dur-at-end 86
:dark-offset NIL
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:pcs-gap 0
)
(Tic-Orbit
:proposal-id 17185
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:al-overhead-at-end 0
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)
(Tic-Orbit
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:al-overhead-at-end 0
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3200
:pcs-gap 0
)
true
3
0
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
COS/FUV spectrum of GaiaJ1030-1435
1699050715000
279.0502337710757
(Tic-Visit
:proposal-id 17185
:visit-id "28"
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:trans-version "20220516"
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:number-of-orbits 2
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:si-bright-earth-limb-angle 20.0
:data-volume 165328
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 17185
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)
(Tic-Orbit
:proposal-id 17185
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:orbit-number 1
:pcs-time 393
:si-vis-utilization 2756
:al-overhead-at-end 0
:internal-dur-at-end 105
:dark-offset NIL
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:low-sky "N"
:pcs-visibility 3149
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)
(Tic-Orbit
:proposal-id 17185
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:orbit-number 2
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:si-vis-utilization 2757
:al-overhead-at-end 0
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3149
:pcs-gap 0
)
true
2
0
The scheduling data was generated by CASM 30.3.
CASM was run in Phase II mode.
COS/FUV spectrum of SDSS-J115506.22+264924.2.
1684662060000
123.20145232533929
(Tic-Visit
:proposal-id 17185
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:number-of-orbits 3
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)
(Tic-Obset
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)
(Tic-Orbit
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)
(Tic-Orbit
:proposal-id 17185
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:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
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:max-dark-utilization 1920
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)
(Tic-Orbit
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:al-overhead-at-end 0
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:dark-offset NIL
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:max-dark-utilization 1920
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)
true
3
0