0Assigned ID: 735
----- Attempting Submission 1 (Fri Apr 08 19:42:37 GMT 2016) -----
HST Phase I Proposal 735 (FUVRot_phase1.apt) successfully submitted.
Receipt: # 735-1Applying correction for acquisition exposure time for target CD-35-2722, everything else remains the same.-13192336----- Attempting Submission 1 (Mon Jul 18 22:28:53 GMT 2016) -----
HST Phase II Proposal 14640 (FUVRot_phase2.apt) successfully submitted.
Receipt: # 14640-1
----- Attempting Submission 2 (Mon Jun 26 20:37:06 GMT 2017) -----
HST Phase II Proposal 14640 (FUVRot_phaseII_updated.apt) successfully submitted.
Receipt: # 14640-2
----- Attempting Submission 3 (Tue Aug 01 16:04:36 GMT 2017) -----Investigating the FUV Emission of Young M dwarfs with FUMES: the Far Ultraviolet M-dwarf Evolution SurveyM dwarf stars have become attractive candidates for exoplanet searches and will be a main focus of the upcoming TESS mission, with the continued search for nearby potentially habitable worlds. However, the atmospheric characterization of these exoplanetary systems depends critically on the high energy stellar radiation environment from X-ray to NUV. Strong radiation at these energies can lead to atmospheric mass loss and is a strong driver of photochemistry in planetary atmospheres. Recently, the MUSCLES Treasury Survey (Cycles 19, 22) provided the first comprehensive assessment of the high energy radiation field around old, planet hosting M dwarfs. However, the habitability and potential for such exoplanetary atmospheres to develop life also depends on the evolution of the atmosphere and hence the evolution of the incident radiation field. The strong high energy spectrum of young M dwarfs can have devastating consequences for the potential habitability of a given system. We, thus, propose the Far Ultraviolet M-dwarf Evolution Survey (FUMES) to measure the strong FUV coronal/chromospheric emission features of young M dwarfs (12 - 650 Myr), e.g. He II, C IV, and S IV. FUMES will observe objects with a wide range of rotation rates to directly connect the emission features to the evolution of coronal heating and upper atmospheric structure, and provide observational benchmarks at young ages for models of M dwarf upper atmospheres. Building on results from MUSCLES, we will be able to estimate the whole high energy radiation field and establish the evolutionary picture of the incident radiation throughout the lifetime of exoplanetary systems around early-mid M dwarf hosts.The Far Ultraviolet M-dwarf Evolution Survey will observe 10 early to mid M-dwarf targets spanning rotation periods from ~1 day to ~80 days, focusing on objects with known young ages to understand the evolution of chormospheric/coronal heating and the history of the high-energy radiation field over time, with important implications for the evolutionary history of planetary systems around M dwarfs.
In order to measure the key coronal/chromospheric emission lines, we are observing our targets across the full FUV passband. We will use the STIS G140L mode to provide the greatest combination of spectral coverage and sensitivity, allowing us to measure, in a single exposure, coronal/chromospheric emission features that crucially probe different portions of the corona: He II, 1640 A, C II 1334 A, 1335 A, N V, 1239 A, 1243 A, Si IV 1394 A, 1403 A, and C V, 1548 A, 1550 A. The use of STIS alos protects potential flare events from damaging the more sensitive COS UV detectors.Operating in TIME-TAG mode we will observe the time vriability of the FUV spectrum as well and will be able to measure potential UV flare rates in a number of young M dwarfs. We based our expected emission fluxes on the FUV spectra of the nearby young active M dwarfs, AU Mic for M0-M2 spectral type objects and AD Leo for later type objects, and the SEDs at NUV and redder wavelengths from the MUSCLES survey of GJ876 and GJ832.
This data will be used to compare the emission strengths in objects with different rotational periods and spectral types and compare that data to literature observations to address our science goals.Stellar PhysicsExtrasolar Planets and Planet Formation6falsetruefalsefalsefalsefalseSUPPORTEDSTARM V-IVNOThis object was generated by the targetselector and retrieved from the SIMBAD database.
Coordinates/PMs and Uncertainty Updated with Initial Gaia Source ListJ2000J2000STARM V-IVPRE-MAIN SEQUENCE STARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.
Coordinates/PMs and Uncertainty Updated with Initial Gaia Source ListJ2000J2000STARM V-IVPRE-MAIN SEQUENCE STARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.
Coordinates/PMs and Uncertainty Updated with Initial Gaia Source ListJ2000J2000STARM V-IVPRE-MAIN SEQUENCE STARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.
Coordinates/PMs and Uncertainty Updated with Initial Gaia Source ListJ2000J2000STARM V-IVPRE-MAIN SEQUENCE STARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.
Coordinates/PMs and Uncertainty Updated with Initial Gaia Source ListJ2000J2000STARM V-IVPRE-MAIN SEQUENCE STARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.
Coordinates/PMs and Uncertainty Updated with Initial Gaia Source ListJ2000J2000STARM V-IVPRE-MAIN SEQUENCE STARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.
Coordinates/PMs and Uncertainty Updated with Initial Gaia Source ListJ2000J2000STARM V-IVNOThis object was generated by the targetselector and retrieved from the SIMBAD database.
Positions and Proper Motion from URAT Parallax CatalogueJ2000J2000STARM V-IVNOThis object was generated by the targetselector and retrieved from the SIMBAD database.
Positions and proper motions from URAT parallax catalogueJ2000B=16.3STARM V-IVNOThis object was generated by the targetselector and retrieved from the SIMBAD database.
Positions and PM from URAT Finch+16J2000B=14.92COS/FUVSpectroscopicNoNoG140L1105COS/FUVSpectroscopicNoNoG140L1280COS/FUVSpectroscopicNoNoG140L1280COS/FUVSpectroscopicNoNoG140L1280COS/FUVSpectroscopicNoNoG140L1280COS/FUVSpectroscopicNoNoG140L1280COS/FUVSpectroscopicNoNoG140L1280COS/FUVSpectroscopicNoNoG140L1105COS/FUVSpectroscopicNoNoG140L1105COS/FUVSpectroscopicNoNoG140L1105/private/var/folders/r6/gkqz5kp523qblvphvg1px5yc0091p7/T/OPVisit4788377875475160610.xmlThe scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.Plan to observe GJ4334 over the course of 2 orbits with STIS FUV-MAMA G140L. The visit will use 2 orbits to build up the signal to noise desired in the key emission line diagnostics of the chromosphere and corona.
Uses the HST full SED of GJ876 from the MUSCLES program as a model for exposure time calculations as well as the FUV spectrum of AD Leo from StarCat in the FUV.(Tic-Visit
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(Tic-Orbit
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)true20The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode./private/var/folders/r6/gkqz5kp523qblvphvg1px5yc0091p7/T/OPVisit372950608267910617.xmlPlan to observe GJ49 over the course of 2 orbits with STIS FUV-MAMA G140L. The visit will use 2 orbits to build up the signal to noise desired in the key emission line diagnostics of the chromosphere and corona.
Uses the HST full SED of GJ832 from the MUSCLES program as a model for exposure time calculations as well as the FUV spectrum of AU Mic from StarCat in the FUV.(Tic-Visit
:proposal-id 14640
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:data-volume 313552
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)
(Tic-Obset
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)
(Tic-Orbit
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(Tic-Orbit
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Uses the HST full SED of GJ876 from the MUSCLES program as a model for exposure time calculations as well as the FUV spectrum of AD Leo from StarCat in the FUV.(Tic-Visit
:proposal-id 14640
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:data-volume 157056
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:coron NIL
)
(Tic-Obset
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(Tic-Orbit
:proposal-id 14640
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Uses the HST full SED of GJ832 from the MUSCLES program as a model for exposure time calculations as well as the FUV spectrum of AD Leo from StarCat in the FUV.(Tic-Visit
:proposal-id 14640
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:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:data-volume 157008
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)
(Tic-Obset
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)
(Tic-Orbit
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:low-sky "N"
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)true10The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode./private/var/folders/r6/gkqz5kp523qblvphvg1px5yc0091p7/T/OPVisit1905693143394040854.xmlPlan to observe HIP17695 over the course of 1 orbits with with STIS FUV-MAMA E140M. This will provide continuous spectral coverage to look at several key chromospheric/coronal emission features, while dispersing the light sufficiently to prevent surpsassing detector count rates.
Uses the HST full SED of GJ876 from the MUSCLES program as a model for exposure time calculations as well as the FUV spectrum of AD Leo from StarCat in the FUV.(Tic-Visit
:proposal-id 14640
:visit-id "07"
:proposal-version -1
:trans-version "20170613"
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:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:si-bright-earth-limb-angle 20.0
:data-volume 157056
:tdrss-contact-duration 0
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)
(Tic-Obset
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)
(Tic-Orbit
:proposal-id 14640
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:orbit-number 1
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:si-vis-utilization 2869
:al-overhead-at-end 0
:internal-dur-at-end 440
:dark-offset NIL
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:low-sky "N"
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)true10The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode./private/var/folders/r6/gkqz5kp523qblvphvg1px5yc0091p7/T/OPVisit1021438619609932711.xmlPlan to observe HIP23309 over the course of 1 orbits with STIS FUV-MAMA G140L. This will provide continuous spectral coverage to sensitively measure several key chromospheric/coronal emission features.
Uses the HST full SED of GJ832 from the MUSCLES program as a model for exposure time calculations as well as the FUV spectrum of AU Mic from StarCat in the FUV.(Tic-Visit
:proposal-id 14640
:visit-id "08"
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:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:si-bright-earth-limb-angle 20.0
:data-volume 157008
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:coron NIL
)
(Tic-Obset
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(Tic-Orbit
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:low-sky "N"
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)true10The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode./private/var/folders/r6/gkqz5kp523qblvphvg1px5yc0091p7/T/OPVisit5222768087131943292.xmlPlan to observe CD-35-2722 over the course of 1 orbit with STIS FUV-MAMA G140L. This will provide continuous spectral coverage to sensitively measure several key chromospheric/coronal emission features.
Uses the HST full SED of GJ832 from the MUSCLES program as a model for exposure time calculations as well as the FUV spectrum of AU Mic from StarCat in the FUV.(Tic-Visit
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:si-bright-earth-limb-angle 20.0
:data-volume 157008
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:coron NIL
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(Tic-Obset
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(Tic-Orbit
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)true10The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode./private/var/folders/r6/gkqz5kp523qblvphvg1px5yc0091p7/T/OPVisit3913266003956588487.xmlPlan to observe GJ410 over the course of 1 orbits with STIS FUV-MAMA G140L. This will provide continuous spectral coverage to sensitively measure several key chromospheric/coronal emission features.
Uses the HST full SED of GJ832 from the MUSCLES program as a model for exposure time calculations as well as the FUV spectrum of AU Mic from StarCat in the FUV.(Tic-Visit
:proposal-id 14640
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:date "01-Aug-2017 10:03:37.0"
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:data-volume 157008
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:coron NIL
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(Tic-Obset
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(Tic-Orbit
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)true10/private/var/folders/r6/gkqz5kp523qblvphvg1px5yc0091p7/T/OPVisit9001380138752824237.xmlThe scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.Plan to observe G249-11 over the course of 3 orbits with STIS FUV-MAMA G140L. The visit will use 3 orbits to build up the signal to noise desired in the key emission line diagnostics of the chromosphere and corona.
Uses the HST full SED of GJ876 from the MUSCLES program as a model for exposure time calculations.(Tic-Visit
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:si-bright-earth-limb-angle 20.0
:data-volume 487520
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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(Tic-Orbit
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(Tic-Orbit
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(Tic-Orbit
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)true30/private/var/folders/r6/gkqz5kp523qblvphvg1px5yc0091p7/T/OPVisit1631935630539649468.xmlThe scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.Plan to observe LP55-41 over the course of 3 orbits with STIS FUV-MAMA G140L. The visit will use 3 orbits to build up the signal to noise desired in the key emission line diagnostics of the chromosphere and corona.
Uses the HST full SED of GJ876 from the MUSCLES program as a model for exposure time calculations.(Tic-Visit
:proposal-id 14640
:visit-id "12"
:proposal-version -1
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:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 3
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 487520
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14640
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:obset-id "12"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14640
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:orbit-number 1
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:al-overhead-at-end 0
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:dark-offset NIL
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:low-sky "N"
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)
(Tic-Orbit
:proposal-id 14640
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:orbit-number 2
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:al-overhead-at-end 0
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:dark-offset NIL
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:low-sky "N"
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)
(Tic-Orbit
:proposal-id 14640
:visit-id "12"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 3324
:al-overhead-at-end 0
:internal-dur-at-end 582
:dark-offset NIL
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:low-sky "N"
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)true30