initial submission
-395392600
----- Attempting Submission 1 (Tue Jun 02 03:37:49 GMT 2026) -----
STELa: Survey of Transiting Exoplanets in Lyman-alpha
Atmospheric escape is a key process that sculpts the exoplanetary population, especially for planets smaller than Neptune. Transit observations in the Lyman-alpha line allow for direct studies of atmospheric escape, but progress is reaching the limit of what is possible with small programs targeting one or two new planets at a time. To advance atmospheric escape studies into a new statistical regime, we propose the Survey of Transiting Exoplanets in Lyman-alpha (STELa), a Multi-Cycle Treasury program aimed at efficiently probing atmospheric escape across the entire exoplanetary population using a proven reconnaissance-detection-characterization strategy. STELa's statistical sample will map the role of mass loss throughout the population of known exoplanets, investigate the nature of "transitional" worlds such as those in near radius valley, and probe the physical mechanism driving the atmospheric erosion of sub-Neptunes. A wide array of treasury science will be possible with the STELa dataset, including a new 3D map of the local interstellar medium, the first survey of stellar wind strengths within the astropause, an atlas of host star XUV spectra in the mass-rotation plane, and investigations of exosphere-thermosphere-lower atmosphere connections through synergies with He 10830 and JWST observations. Implementing a broad Lyman-alpha transit survey now is essential to enable the scientific leap from ``stamp collecting'' to population science within the limited remaining life of the only observatory capable of these observations.
Stage 1 (Cycle 32) observations will observe target systems with STIS G140M to measure the stellar Lya flux and STIS G140L to enable XUV reconstructions. One orbit with each instrument will be devoted to each target. The primary outcome of Stage 1 is the identification of targets for which Lya SNR permits the detection of an outflow powered by the reconstructed XUV input.
*Note that activity determinations in target comments are not consistent with activity determinations per STIS ISR 2017-02* Information in the target comments was in most cases automatically generated based on parameters catalogged in the NASA Exoplanets Database and a query of the GALEX source catalog. These parameters and fluxes were used as the basis for an activity determination for FGK stars. Those catagorized as active were subject to the stricter count rate limits applicable for variable targets. These activity classifications were included for M stars as well as part of the automated processing for completeness; however, they were not used for bright object clearance. For all M stars, Ha line equiavelent widths were used as per STIS ISR 2017-02.
As of 2025-04-30, M star activity determinations based on Ha are as follows. Positive values indicate absorption.
TOI-1468 - inactive
TOI-1695 - inactive
TOI-700 - inactive
TOI-1730 - inactive
TOI-620 - inactive
TOI-5388 - inactive
LTT 3780 - inactive
TOI-1801 - inactive
TOI-1266 - inactive
TOI-2136 - inactive
TOI-2095 - inactive
TOI-1231 - inactive
TOI-198 - inactive
LP 791-18 - inactive
TOI-406 - inactive
TOI-1224 - active
K2-72 - active
TOI-1467 - inactive
TOI-2285 - inactive
TOI-2094 - active
LP 714-47 - inactive
TOI-2015 - active
TOI-1728 - inactive
TOI-233 - inactive
TOI-4438 - inactive
TOI-1452 - active
TOI-4336 A - inactive
TOI-904 - inactive
TOI-1696 - inactive
GJ 3090 - inactive
TOI-1235 - inactive
TOI-122 - inactive
K2-9 - inactive
TOI-2079 - inactive
TOI-727 - inactive
K2-3 - inactive
TOI-270 - inactive
TOI-870 - inactive
TOI-133 - inactive
TOI-771 - inactive
K2-18 - inactive
K2-25 - active
L 98-59 - inactive
LTT 1445 A - inactive
TOI-1643 - active
TOI-7481 - inactive
GJ 1214 - inactive
TOI-5799 - inactive
TOI-7309 - inactive
Classifications for M dwarf companions of FGK targets are:
HD5278 Companion (Gaia DR3 4617759518798492800) - active
R. O. Parke Loyd has extensive experience in planning, reducing, and analyzing HST FUV observations, with nine first-author papers published using such data since 2014. He was a key contributor to the discovery of the Lyman-alpha transit of GJ 436 b (Kulow et al. 2014) and later led work placing constraints on its C II and Si III transits. He recently led the discovery of a Lyman-alpha transit from the ~2 Rearth planets in the TOI-776 system. He has PIed 4 HST observing programs, including Lyman-alpha transit programs and was a key contributor in the creation of the treasury-scale MUSCLES and HAZMAT datasets (e.g. Loyd et al. 2016, 2018a, 2018b).
Dr. Shreyas Vissapragada is an expert in observations of atmospheric escape, especially using the metastable helium 10830 triplet in which he has observed over a dozen planets (and used these observations to benchmark planetary outflow models). Recently he is using HST to push towards Lyman-alpha constraints on the Earth-sized exoplanet GJ 12b (GO-17600).
Drs. James Owen, Ruth Murray-Clay, and Hilke Schlichting are leaders in the field of exoplanetary atmospheric scape and sub-Neptune evolution (e.g., Owen and Alvarez, 2016; Murray-Clay et al., 2009; Gupta and Schlichting 2019). Dr. Owen was one of the founders of the XUV evaporation theory and Dr. Schilchting of core-powered mass loss. Dr. Owen's student Ethan Schreyer developed the outflow model that will be used in this work. Dr. Akash Gupta and Dr. James Rogers are expert in population modeling under the influence of atmospheric escape due to core-powered mass loss and photoevaporation (Gupta and Schlichting 2019, Rogers et al. 2023). Dr. Murray-Clay and her students are experts in outflow modeling, having developed both 3D and 1D outflow models (e.g., McCann et al. 2019).
Dr. Allison Youngblood is the PI of multiple HST programs to study exoplanets and their host stars in the UV, including a large ~200 orbit survey of the UV emission from JWST Cycle 1 transiting exoplanet host stars (GO-16701) and a Lyman alpha transit of the sub-Neptune TOI-1231b.
Dr. Evgenya Shkolnik has been studying exoplanets and the stellar activity of their host stars, including star- planet interactions, for over 20 years, ranging from systems around Sun-like stars down to the lowest mass M dwarfs, including extensive studies of the Sun-as-a-star. She is also the PI or Co-I of several HST programs, including those studying the UV evolution of K and M stars.
David Ardila is an expert in UV instrumentation and observations. He serves as lead instrument scientist on the Star-Planet Activity Research CubeSat and has served leadership roles in UV mission concepts like UV-SCOPE.
Drs. Sarah Peacock and Travis Barman are experts in modeling stellar and giant planet atmospheres. A modified PHOENIX model they have developed can be used to predict the EUV emission of a low-mass star by matching the model-simulated FUV emission to observations (Peacock et al. 2019). Dr. Peacock is also the PI of an HST program that obtained Lyman alpha observations of 6 M and K type stars with exceptionally large radial velocities that Doppler shift their Lyman alpha emission away from contaminating sources to reveal the intrinsic profiles.
Dr. Girish Duvvuri is an expert in the XUV reconstructions using a DEM method scalable to large numbers of datasets (Duvvuri et al. 2021). He is PI of an archival HST program to reconstruct XUV spectra for a broad sample of targets with existing FUV spectra (AR-17054).
Mercedes Lopez-Morales is an expert in the study of exoplanet atmospheres via transmission spectroscopy. She has led HST and ground-based transmission spectroscopy surveys, namely The HST PanCET program, GO: 14767, PIs: Sing & Lopez-Morales and The Arizona-CfA-Catolica-Carnegie Exoplanet Spectroscopy Survey, ACCESS, PIs: Lopez-Morales, Apai, Jordan.
Exoplanets and Exoplanet Formation
0
false
true
true
false
false
false
false
AVAILABLE
STAR
EXTRA-SOLAR PLANETARY SYSTEM
G V-IV
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
STAR
EXTRA-SOLAR PLANETARY SYSTEM
M V-IV
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
STAR
EXTRA-SOLAR PLANETARY SYSTEM
M V-IV
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
STAR
EXTRA-SOLAR PLANETARY SYSTEM
K V-IV
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
STAR
EXTRA-SOLAR PLANETARY SYSTEM
M V-IV
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
STAR
EXTRA-SOLAR PLANETARY SYSTEM
K V-IV
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
STAR
EXTRA-SOLAR PLANETARY SYSTEM
K V-IV
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
STAR
EXTRA-SOLAR PLANETARY SYSTEM
G V-IV
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
STAR
EXTRA-SOLAR PLANETARY SYSTEM
K V-IV
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
STAR
EXTRA-SOLAR PLANETARY SYSTEM
M V-IV
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
STAR
EXTRA-SOLAR PLANETARY SYSTEM
M V-IV
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
STAR
EXTRA-SOLAR PLANETARY SYSTEM
F3-F9
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
STAR
EXTRA-SOLAR PLANETARY SYSTEM
M V-IV
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
STIS/FUV-MAMA
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Spectroscopic
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G140L
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STIS/FUV-MAMA
Spectroscopic
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G140M
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STIS/FUV-MAMA
Spectroscopic
No
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G140L
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STIS/FUV-MAMA
Spectroscopic
No
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G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
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G140L
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STIS/FUV-MAMA
Spectroscopic
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G140M
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STIS/FUV-MAMA
Spectroscopic
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G140L
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STIS/FUV-MAMA
Spectroscopic
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G140M
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STIS/FUV-MAMA
Spectroscopic
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G140L
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Spectroscopic
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G140M
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Spectroscopic
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Spectroscopic
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G140M
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Spectroscopic
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G140L
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Spectroscopic
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G140M
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STIS/FUV-MAMA
Spectroscopic
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G140L
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STIS/FUV-MAMA
Spectroscopic
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G140M
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STIS/FUV-MAMA
Spectroscopic
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G140L
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STIS/FUV-MAMA
Spectroscopic
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G140M
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STIS/FUV-MAMA
Spectroscopic
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G140L
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STIS/FUV-MAMA
Spectroscopic
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G140M
1222
STIS/FUV-MAMA
Spectroscopic
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G140L
1425
STIS/FUV-MAMA
Spectroscopic
No
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G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
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G140L
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STIS/FUV-MAMA
Spectroscopic
No
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G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
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G140L
1425
STIS/FUV-MAMA
Spectroscopic
No
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G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
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G140L
1425
STIS/FUV-MAMA
Spectroscopic
No
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G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
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G140L
1425
STIS/FUV-MAMA
Spectroscopic
No
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G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
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G140L
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STIS/FUV-MAMA
Spectroscopic
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G140M
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Spectroscopic
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G140L
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G140M
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G140L
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Spectroscopic
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G140M
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Spectroscopic
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G140L
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STIS/FUV-MAMA
Spectroscopic
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G140M
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Spectroscopic
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G140L
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Spectroscopic
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G140M
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STIS/FUV-MAMA
Spectroscopic
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G140L
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Spectroscopic
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G140M
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G140M
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STIS/FUV-MAMA
Spectroscopic
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G140L
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STIS/FUV-MAMA
Spectroscopic
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G140M
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STIS/FUV-MAMA
Spectroscopic
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G140L
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STIS/FUV-MAMA
Spectroscopic
No
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G140M
1222
STIS/FUV-MAMA
Spectroscopic
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G140L
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STIS/FUV-MAMA
Spectroscopic
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G140M
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STIS/FUV-MAMA
Spectroscopic
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G140L
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STIS/FUV-MAMA
Spectroscopic
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G140M
1222
STIS/FUV-MAMA
Spectroscopic
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G140L
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STIS/FUV-MAMA
Spectroscopic
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Spectroscopic
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G140L
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Spectroscopic
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G140M
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Spectroscopic
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G140L
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Spectroscopic
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Spectroscopic
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Spectroscopic
No
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Spectroscopic
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G140L
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Spectroscopic
No
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G140M
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STIS/FUV-MAMA
Spectroscopic
No
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G140L
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Spectroscopic
No
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Spectroscopic
No
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Spectroscopic
No
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Spectroscopic
No
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G140L
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Spectroscopic
No
No
G140M
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Spectroscopic
No
No
G140L
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Spectroscopic
No
No
G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
No
G140L
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STIS/FUV-MAMA
Spectroscopic
No
No
G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
No
G140L
1425
STIS/FUV-MAMA
Spectroscopic
No
No
G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
No
G140L
1425
STIS/FUV-MAMA
Spectroscopic
No
No
G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
No
G140L
1425
STIS/FUV-MAMA
Spectroscopic
No
No
G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
No
G140L
1425
STIS/FUV-MAMA
Spectroscopic
No
No
G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
No
G140L
1425
STIS/FUV-MAMA
Spectroscopic
No
No
G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
No
G140L
1425
STIS/FUV-MAMA
Spectroscopic
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G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
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G140L
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STIS/FUV-MAMA
Spectroscopic
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G140M
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G140L
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Spectroscopic
No
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G140M
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G140L
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No
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G140M
1222
STIS/FUV-MAMA
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No
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G140L
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STIS/FUV-MAMA
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G140M
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No
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G140L
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Spectroscopic
No
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G140M
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STIS/FUV-MAMA
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G140L
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Spectroscopic
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G140M
1222
STIS/FUV-MAMA
Spectroscopic
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G140L
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STIS/FUV-MAMA
Spectroscopic
No
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G140M
1222
STIS/FUV-MAMA
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G140L
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Spectroscopic
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G140M
1222
STIS/FUV-MAMA
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G140L
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Spectroscopic
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G140M
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STIS/FUV-MAMA
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G140L
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STIS/FUV-MAMA
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G140M
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STIS/FUV-MAMA
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No
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G140M
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G140L
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Spectroscopic
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G140M
1222
STIS/FUV-MAMA
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No
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G140L
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Spectroscopic
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G140M
1222
STIS/FUV-MAMA
Spectroscopic
No
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G140L
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Spectroscopic
No
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1222
STIS/FUV-MAMA
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G140M
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STIS/FUV-MAMA
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G140L
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1222
STIS/FUV-MAMA
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No
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G140L
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Spectroscopic
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1222
STIS/FUV-MAMA
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G140L
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G140M
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STIS/FUV-MAMA
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G140L
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STIS/FUV-MAMA
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POS-TARG
BACKGROUND
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LINE
false
true
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STIS-ALONG-SLIT
1
false
POS-TARG
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false
true
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