14640( 4) - 01-Aug-2017 16:46:29 - [ 1] HUBBLE SPACE TELESCOPE OBSERVING PROGRAM 14640 Version: 4 Check-in Time: 01-Aug-2017 16:46:29 STScI Edit Number: 0 Title Investigating the FUV Emission of Young M dwarfs with FUMES: the Far Ultraviolet M-dwarf Evolution Survey ------------------------------------------------------------------------------------ Type Cycle GO 24 ------------------------------------------------------------------------------------ Investigators Contact? PI: Dr. John Sebastian Pineda University of Colorado at Boulder Y CoI: Dr. Kevin France University of Colorado at Boulder N ------------------------------------------------------------------------------------ Abstract M 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. ------------------------------------------------------------------------------------ Observations Description ------------------------ 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 14640( 4) - 01-Aug-2017 16:46:29 - [ 2] 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. ------------------------------------------------------------------------------------ 14640( 4) - 01-Aug-2017 16:46:29 - [ 3] TARGET LIST Fixed Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial | Flux data No | Name | Description | Position |Eqnx | Vel. | ------------------------------------------------------------------------------------------------------------------------------------ 2 GJ49 STAR, M V-IV RA=01H02M38.8685S +/- 0.002", J2000 V = 9.56 DEC=+62D20'42.17" +/- 0.002" Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates/PMs and Uncertainty Updated with Initial Gaia Source List Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2000 0.10506756314727868 0.09040000000000001 0.1004 ------------------------------------------------------------------------------------------------------------------------------------ 3 HIP23309 STAR, M V-IV, PRE-MAIN RA=05H00M47.1300S +/- 0.003", J2000 V = 9.977 SEQUENCE STAR DEC=-57D15'25.45" +/- 0.003" Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates/PMs and Uncertainty Updated with Initial Gaia Source List Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2000 0.004375660737389175 0.07440000000000001 0.03734 ------------------------------------------------------------------------------------------------------------------------------------ 4 GJ410 STAR, M V-IV, PRE-MAIN RA=11H02M38.3434S +/- 0.003", J2000 V = 9.572 SEQUENCE STAR DEC=+21D58'1.69" +/- 0.003" Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates/PMs and Uncertainty Updated with Initial Gaia Source List Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2000 0.010423422009723675 -0.052700000000000004 0.08495 ------------------------------------------------------------------------------------------------------------------------------------ 5 HIP112312 STAR, M V-IV, PRE-MAIN RA=22H44M57.9622S +/- 0.003", J2000 V = 12.111 SEQUENCE STAR DEC=-33D15'1.74" +/- 0.006" Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates/PMs and Uncertainty Updated with Initial Gaia Source List Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2000 0.014245601389179087 -0.123 0.04284 ------------------------------------------------------------------------------------------------------------------------------------ 14640( 4) - 01-Aug-2017 16:46:29 - [ 4] TARGET LIST Fixed Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial | Flux data No | Name | Description | Position |Eqnx | Vel. | ------------------------------------------------------------------------------------------------------------------------------------ 6 HIP17695 STAR, M V-IV, PRE-MAIN RA=03H47M23.3402S +/- 0.003", J2000 V = 11.537 SEQUENCE STAR DEC=-01D58'19.98" +/- 0.004" Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates/PMs and Uncertainty Updated with Initial Gaia Source List Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2000 0.011913723967663084 -0.2782 0.062 ------------------------------------------------------------------------------------------------------------------------------------ 7 CD-35-2722 STAR, M V-IV, PRE-MAIN RA=06H09M19.2062S +/- 0.013", J2000 V = 11.083 SEQUENCE STAR DEC=-35D49'31.09" +/- 0.013" Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates/PMs and Uncertainty Updated with Initial Gaia Source List Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2000 -4.111138481295612E-4 -0.0551 0.0436 ------------------------------------------------------------------------------------------------------------------------------------ 8 LP247-13 STAR, M V-IV, PRE-MAIN RA=03H15M37.8910S +/- 0.1", J2000 V = 13.12 SEQUENCE STAR DEC=+37D24'14.02" +/- 0.1" Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates/PMs and Uncertainty Updated with Initial Gaia Source List Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2000 0.01754003152219915 -0.097 0.02907 ------------------------------------------------------------------------------------------------------------------------------------ 10 GJ4334 STAR, M V-IV RA=23H25M41.8683S +/- 0.09", J2000 V = 14.59 DEC=+53D08'10.50" +/- 0.09" Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. Positions and Proper Motion from URAT Parallax Catalogue Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2014 0.11191601159669913 0.3319 0.0402 ------------------------------------------------------------------------------------------------------------------------------------ 14640( 4) - 01-Aug-2017 16:46:29 - [ 5] TARGET LIST Fixed Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial | Flux data No | Name | Description | Position |Eqnx | Vel. | ------------------------------------------------------------------------------------------------------------------------------------ 11 G249-11 STAR, M V-IV RA=05H30M40.7971S +/- 0.1", J2000 V = 14.98 B=16.3 DEC=+68D54'4.37" +/- 0.1" Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. Positions and proper motions from URAT parallax catalogue Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2014 0.0314094104420658 -0.2552 0.0461 ------------------------------------------------------------------------------------------------------------------------------------ 12 LP-55-41 STAR, M V-IV RA=05H02M5.1000S +/- 0.1", J2000 V = 13.858 B=14.92 DEC=+68D27'21.81" +/- 0.1" Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. Positions and PM from URAT Finch+16 Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2014 0.0018880871849640713 -0.2506 0.0326 ------------------------------------------------------------------------------------------------------------------------------------ 14640( 4) - 01-Aug-2017 16:46:29 - [ 6] Visit: 03 (GJ 4334) Visit Requirements: On Hold Comments: Additional Comments: 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. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 GJ4334 STIS/CCD ACQ F28X50LP MIRROR 1 0.1 S (0.1 S) ------------------------------------------------------------------------------------------------------------------------------------ 2 GJ4334 STIS/CCD ACQ/PEA 52X0.1 MIRROR 1 0.1 S (0.1 K S) ------------------------------------------------------------------------------------------------------------------------------------ 3 GJ4334 STIS/FUV TIME-TA 52X0.2 G140L 1425 BUFFER-TIME=2500 1 2000 S -MAMA G see below (2286 S) ------------------------------------------------------------------------------------------------------------------------------------ 4 GJ4334 STIS/FUV TIME-TA 52X0.2 G140L 1425 BUFFER-TIME=3500 1 2000 S -MAMA G see below (3143 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ GJ4334 1 STIS/CCD ACQ F28X50LP MIRROR none none none none 1 N/A GJ4334 2 STIS/CCD ACQ/PEA 52X0.1 MIRROR none none none none 1 N/A K GJ4334 3 STIS/FUV TIME-TA 52X0.2 G140L 1425 none none none none 1 2286.0 S -MAMA G GJ4334 4 STIS/FUV TIME-TA 52X0.2 G140L 1425 none none none none 2 3143.0 S -MAMA G 14640( 4) - 01-Aug-2017 16:46:29 - [ 7] Visit: 04 (GJ49) Visit Requirements: On Hold Comments: Additional Comments: Plan 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. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 GJ49 STIS/CCD ACQ F28X50LP MIRROR 1 0.1 S (0.1 S) ------------------------------------------------------------------------------------------------------------------------------------ 2 GJ49 STIS/CCD ACQ/PEA 52X0.1 MIRROR 1 0.1 S (0.1 K S) ------------------------------------------------------------------------------------------------------------------------------------ 3 GJ49 STIS/FUV TIME-TA 52X0.2 G140L 1425 BUFFER-TIME=2500 1 2000 S -MAMA G see below (2364 S) ------------------------------------------------------------------------------------------------------------------------------------ 4 GJ49 STIS/FUV TIME-TA 52X0.2 G140L 1425 BUFFER-TIME=3500 1 2000 S -MAMA G see below (3221 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ GJ49 1 STIS/CCD ACQ F28X50LP MIRROR none none none none 1 N/A GJ49 2 STIS/CCD ACQ/PEA 52X0.1 MIRROR none none none none 1 N/A K GJ49 3 STIS/FUV TIME-TA 52X0.2 G140L 1425 none none none none 1 2364.0 S -MAMA G GJ49 4 STIS/FUV TIME-TA 52X0.2 G140L 1425 none none none none 2 3221.0 S -MAMA G 14640( 4) - 01-Aug-2017 16:46:29 - [ 8] Visit: 05 (HIP112312) Visit Requirements: On Hold Comments: Additional Comments: Plan to observe HIP112312 over the course of 1 orbits 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. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 HIP112312 STIS/CCD ACQ F28X50LP MIRROR 1 0.1 S (0.1 S) ------------------------------------------------------------------------------------------------------------------------------------ 2 HIP112312 STIS/CCD ACQ/PEA 0.2X0.06 MIRROR 1 0.1 S (0.1 K S) ------------------------------------------------------------------------------------------------------------------------------------ 3 HIP112312 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 BUFFER-TIME=2500 1 2000 S -MAMA G see below (2012 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ HIP112312 1 STIS/CCD ACQ F28X50LP MIRROR none none none none 1 N/A HIP112312 2 STIS/CCD ACQ/PEA 0.2X0.06 MIRROR none none none none 1 N/A K HIP112312 3 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 none none none none 1 2012.0 S -MAMA G 14640( 4) - 01-Aug-2017 16:46:29 - [ 9] Visit: 06 (LP247-13) Visit Requirements: On Hold Comments: Additional Comments: Plan to observe LP247-13 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 AD Leo from StarCat in the FUV. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 LP247-13 STIS/CCD ACQ F28X50LP MIRROR 1 0.1 S (0.1 S) ------------------------------------------------------------------------------------------------------------------------------------ 2 LP247-13 STIS/CCD ACQ/PEA 52X0.1 MIRROR 1 0.1 S (0.1 K S) ------------------------------------------------------------------------------------------------------------------------------------ 3 LP247-13 STIS/FUV TIME-TA 52X0.2 G140L 1425 BUFFER-TIME=2500 1 2000 S -MAMA G see below (2153 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ LP247-13 1 STIS/CCD ACQ F28X50LP MIRROR none none none none 1 N/A LP247-13 2 STIS/CCD ACQ/PEA 52X0.1 MIRROR none none none none 1 N/A K LP247-13 3 STIS/FUV TIME-TA 52X0.2 G140L 1425 none none none none 1 2153.0 S -MAMA G 14640( 4) - 01-Aug-2017 16:46:29 - [ 10] Visit: 07 (HIP17695) Visit Requirements: On Hold Comments: Additional Comments: Plan 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. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 HIP17695 STIS/CCD ACQ F28X50LP MIRROR 1 0.1 S (0.1 S) ------------------------------------------------------------------------------------------------------------------------------------ 2 HIP17695 STIS/CCD ACQ/PEA 0.2X0.06 MIRROR 1 0.1 S (0.1 K S) ------------------------------------------------------------------------------------------------------------------------------------ 3 HIP17695 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 BUFFER-TIME=2500 1 2000 S -MAMA G see below (1974 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ HIP17695 1 STIS/CCD ACQ F28X50LP MIRROR none none none none 1 N/A HIP17695 2 STIS/CCD ACQ/PEA 0.2X0.06 MIRROR none none none none 1 N/A K HIP17695 3 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 none none none none 1 1974.0 S -MAMA G 14640( 4) - 01-Aug-2017 16:46:29 - [ 11] Visit: 08 (HIP23309) Visit Requirements: On Hold Comments: Additional Comments: Plan 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. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 HIP23309 STIS/CCD ACQ F28X50LP MIRROR 1 0.1 S (0.1 S) ------------------------------------------------------------------------------------------------------------------------------------ 2 HIP23309 STIS/CCD ACQ/PEA 52X0.1 MIRROR 1 0.1 S (0.1 K S) ------------------------------------------------------------------------------------------------------------------------------------ 3 HIP23309 STIS/FUV TIME-TA 52X0.1 G140L 1425 BUFFER-TIME=2500 1 2000 S -MAMA G see below (2350 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ HIP23309 1 STIS/CCD ACQ F28X50LP MIRROR none none none none 1 N/A HIP23309 2 STIS/CCD ACQ/PEA 52X0.1 MIRROR none none none none 1 N/A K HIP23309 3 STIS/FUV TIME-TA 52X0.1 G140L 1425 none none none none 1 2350.0 S -MAMA G 14640( 4) - 01-Aug-2017 16:46:29 - [ 12] Visit: 09 (CD-35-2722) Visit Requirements: On Hold Comments: Additional Comments: Plan 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. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 CD-35-2722 STIS/CCD ACQ F28X50LP MIRROR 1 0.1 S (0.1 S) ------------------------------------------------------------------------------------------------------------------------------------ 2 CD-35-2722 STIS/CCD ACQ/PEA 52X0.1 MIRROR 1 0.1 S (0.1 K S) ------------------------------------------------------------------------------------------------------------------------------------ 3 CD-35-2722 STIS/FUV TIME-TA 52X0.2 G140L 1425 BUFFER-TIME=2500 1 2000 S -MAMA G see below (2153 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ CD-35-2722 1 STIS/CCD ACQ F28X50LP MIRROR none none none none 1 N/A CD-35-2722 2 STIS/CCD ACQ/PEA 52X0.1 MIRROR none none none none 1 N/A K CD-35-2722 3 STIS/FUV TIME-TA 52X0.2 G140L 1425 none none none none 1 2153.0 S -MAMA G 14640( 4) - 01-Aug-2017 16:46:29 - [ 13] Visit: 10 (GJ410) Visit Requirements: On Hold Comments: Additional Comments: Plan 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. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 GJ410 STIS/CCD ACQ F28X50LP MIRROR 1 0.1 S (0.1 S) ------------------------------------------------------------------------------------------------------------------------------------ 2 GJ410 STIS/CCD ACQ/PEA 52X0.1 MIRROR 1 0.1 S (0.1 K S) ------------------------------------------------------------------------------------------------------------------------------------ 3 GJ410 STIS/FUV TIME-TA 52X0.1 G140L 1425 BUFFER-TIME=2500 1 2000 S -MAMA G see below (2126 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ GJ410 1 STIS/CCD ACQ F28X50LP MIRROR none none none none 1 N/A GJ410 2 STIS/CCD ACQ/PEA 52X0.1 MIRROR none none none none 1 N/A K GJ410 3 STIS/FUV TIME-TA 52X0.1 G140L 1425 none none none none 1 2126.0 S -MAMA G 14640( 4) - 01-Aug-2017 16:46:29 - [ 14] Visit: 11 (G249-11) Visit Requirements: On Hold Comments: Additional Comments: 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. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 G249-11 STIS/CCD ACQ F28X50LP MIRROR 1 0.1 S (0.1 S) ------------------------------------------------------------------------------------------------------------------------------------ 2 G249-11 STIS/CCD ACQ/PEA 52X0.1 MIRROR 1 0.1 S (0.1 K S) ------------------------------------------------------------------------------------------------------------------------------------ 3 G249-11 STIS/FUV TIME-TA 52X0.2 G140L 1425 BUFFER-TIME=2500 1 2000 S -MAMA G see below (2439 S) ------------------------------------------------------------------------------------------------------------------------------------ 4 G249-11 STIS/FUV TIME-TA 52X0.2 G140L 1425 BUFFER-TIME=3500 1 3000 S -MAMA G see below (3296 S) ------------------------------------------------------------------------------------------------------------------------------------ 5 G249-11 STIS/FUV TIME-TA 52X0.2 G140L 1425 BUFFER-TIME=3500 1 3000 S -MAMA G see below (3296 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ G249-11 1 STIS/CCD ACQ F28X50LP MIRROR none none none none 1 N/A G249-11 2 STIS/CCD ACQ/PEA 52X0.1 MIRROR none none none none 1 N/A K G249-11 3 STIS/FUV TIME-TA 52X0.2 G140L 1425 none none none none 1 2439.0 S -MAMA G G249-11 4 STIS/FUV TIME-TA 52X0.2 G140L 1425 none none none none 2 3296.0 S -MAMA G G249-11 5 STIS/FUV TIME-TA 52X0.2 G140L 1425 none none none none 3 3296.0 S -MAMA G 14640( 4) - 01-Aug-2017 16:46:29 - [ 15] Visit: 12 (LP55-41) Visit Requirements: On Hold Comments: Additional Comments: 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. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 LP-55-41 STIS/CCD ACQ F28X50LP MIRROR 1 0.1 S (0.1 S) ------------------------------------------------------------------------------------------------------------------------------------ 2 LP-55-41 STIS/CCD ACQ/PEA 52X0.1 MIRROR 1 0.3 S (0.3 K S) ------------------------------------------------------------------------------------------------------------------------------------ 3 LP-55-41 STIS/FUV TIME-TA 52X0.2 G140L 1425 BUFFER-TIME=2600 1 2000 S -MAMA G see below (2436 S) ------------------------------------------------------------------------------------------------------------------------------------ 4 LP-55-41 STIS/FUV TIME-TA 52X0.2 G140L 1425 BUFFER-TIME=3500 1 3000 S -MAMA G see below (3296 S) ------------------------------------------------------------------------------------------------------------------------------------ 5 LP-55-41 STIS/FUV TIME-TA 52X0.2 G140L 1425 BUFFER-TIME=3500 1 3000 S -MAMA G see below (3296 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ LP-55-41 1 STIS/CCD ACQ F28X50LP MIRROR none none none none 1 N/A LP-55-41 2 STIS/CCD ACQ/PEA 52X0.1 MIRROR none none none none 1 N/A K LP-55-41 3 STIS/FUV TIME-TA 52X0.2 G140L 1425 none none none none 1 2436.0 S -MAMA G LP-55-41 4 STIS/FUV TIME-TA 52X0.2 G140L 1425 none none none none 2 3296.0 S -MAMA G LP-55-41 5 STIS/FUV TIME-TA 52X0.2 G140L 1425 none none none none 3 3296.0 S -MAMA G 14640( 4) - 01-Aug-2017 16:46:29 - [ 16] Summary Form for Proposal 14640 Item Used in this proposal ------------------------------------------------------------------------------------------------------------------------------------ Apertures 0.2X0.06, 0.2X0.2, 52X0.1, 52X0.2, F28X50LP ------------------------------------------------------------------------------------------------------------------------------------ Configurations STIS/CCD, STIS/FUV-MAMA ------------------------------------------------------------------------------------------------------------------------------------ Opmodes ACQ, ACQ/PEAK, TIME-TAG ------------------------------------------------------------------------------------------------------------------------------------ Optional Parameters BUFFER-TIME=2500, BUFFER-TIME=2600, BUFFER-TIME=3500 ------------------------------------------------------------------------------------------------------------------------------------ Spectral Elements E140M, G140L, MIRROR ------------------------------------------------------------------------------------------------------------------------------------ Target Names CD-35-2722, G249-11, GJ410, GJ4334, GJ49, HIP112312, HIP17695, HIP23309, LP-55-41, LP247-13 ------------------------------------------------------------------------------------------------------------------------------------