-
1
A nearby transiting rocky exoplanet that is suitable for atmospheric investigation
Published 2022“…Spectroscopy of transiting exoplanets can be used to investigate their atmospheric properties and habitability. Combining radial velocity (RV) and transit data provides additional information on exoplanet physical properties. …”
Get full text
Article -
2
Exploring the Atmospheric Dynamics of the Extreme Ultrahot Jupiter KELT-9b Using TESS Photometry
Published 2021“…The measured secondary eclipse depth and peak-to-peak atmospheric brightness modulation are and 566 16 ppm, respectively. …”
Get full text
Article -
3
Planetary system around the nearby M dwarf GJ 357 including a transiting, hot, Earth-sized planet optimal for atmospheric characterization
Published 2020“…Therefore, GJ 357 b represents one of the best terrestrial planets suitable for atmospheric characterization with the upcoming JWST and ground-based ELTs.…”
Get full text
Article -
4
TESS Hunt for Young and Maturing Exoplanets (THYME). IV. Three Small Planets Orbiting a 120 Myr Old Star in the Pisces–Eridanus Stream
Published 2022“…Young exoplanets can offer insight into the evolution of planetary atmospheres, compositions, and architectures. We present the discovery of the young planetary system TOI 451 (TIC 257605131, Gaia DR2 4844691297067063424). …”
Get full text
Article -
5
Science Extraction from TESS Observations of Known Exoplanet Hosts
Published 2021“…These include measurements of planetary radii, mass–radius relationships, stellar obliquities, bulk density constraints on interior models, and transmission spectroscopy as a means to study planetary atmospheres. The Transiting Exoplanet Survey Satellite (TESS) has added to the exoplanet inventory by observing a significant fraction of the celestial sphere, including many stars already known to host exoplanets. …”
Get full text
Article -
6
The Transiting Exoplanet Survey Satellite
Published 2018“…For the first time it will be possible to study the masses, sizes, densities, orbits, and atmospheres of a large cohort of small planets, including a sample of rocky worlds in the habitable zones of their host stars.…”
Get full text
Get full text
Get full text
Get full text
Article -
7
Science Extraction from TESS Observations of Known Exoplanet Hosts
Published 2022“…These include measurements of planetary radii, mass–radius relationships, stellar obliquities, bulk density constraints on interior models, and transmission spectroscopy as a means to study planetary atmospheres. The Transiting Exoplanet Survey Satellite (TESS) has added to the exoplanet inventory by observing a significant fraction of the celestial sphere, including many stars already known to host exoplanets. …”
Get full text
Article -
8
TESS Hunt for Young and Maturing Exoplanets (THYME). III. A Two-planet System in the 400 Myr Ursa Major Group
Published 2022“…Exoplanets can evolve significantly between birth and maturity, as their atmospheres, orbits, and structures are shaped by their environment. …”
Get full text
Article -
9
Transits of Known Planets Orbiting a Naked-eye Star
Published 2021“…The combination of the multitransiting planet system, the bright host star, and the diversity of planetary interiors and atmospheres means this will likely become a cornerstone system for atmospheric and orbital characterization of small worlds.…”
Get full text
Article -
10
HD 191939: Three Sub-Neptunes Transiting a Sun-like Star Only 54 pc Away
Published 2022“…Finally, as a promising target for multiwavelength transmission spectroscopy of all three planets' atmospheres, HD 191939 can offer valuable insight into multiple sub-Neptunes born from a protoplanetary disk that may have resembled that of the early Sun.…”
Get full text
Article -
11
A remnant planetary core in the hot-Neptune desert
Published 2022“…Although photoevaporation rates cannot account for the mass loss required to reduce a Jupiter-like gas giant, they can remove a small (a few Earth masses) hydrogen and helium envelope on timescales of several billion years, implying that any remaining atmosphere on TOI-849b is likely to be enriched by water or other volatiles from the planetary interior. …”
Get full text
Article -
12
Stellar Flares from the First TESS Data Release: Exploring a New Sample of M Dwarfs
Published 2021“…Flares may erode exoplanets' atmospheres and impact their habitability, but might also trigger the genesis of life around small stars. …”
Get full text
Article -
13
A super-Earth and two sub-Neptunes transiting the nearby and quiet M dwarf TOI-270
Published 2022“…This enables the characterization of planetary sizes, orbits, bulk compositions, atmospheres and formation histories. These studies are facilitated by small and cool M dwarf host stars. …”
Get full text
Article -
14
Discovery and Characterization of Transiting Super Earths Using an All-Sky Transit Survey and Follow-up by the James Webb Space Telescope
Published 2012“…The principal sources of uncertainty in the prospective JWST characterization of habitable super Earths are super-Earth frequency and the nature of super-Earth atmospheres. Based on our estimates of these uncertainties, we project that JWST will be able to measure the temperature and identify molecular absorptions (water, CO[subscript 2]) in one to four nearby habitable TESS super Earths orbiting lower–main-sequence stars.…”
Get full text
Get full text
Get full text
Get full text
Article -
15
THE TRANSITING EXOPLANET SURVEY SATELLITE: SIMULATIONS OF PLANET DETECTIONS AND ASTROPHYSICAL FALSE POSITIVES
Published 2015“…We also discuss the prospects for follow-up observations to measure the masses and atmospheres of the TESS planets.…”
Get full text
Get full text
Get full text
Article -
16
A giant planet candidate transiting a white dwarf
Published 2021“…Some white dwarfs show evidence for rocky material floating in their atmospheres5, in warm debris disks6–9 or orbiting very closely10–12, which has been interpreted as the debris of rocky planets that were scattered inwards and tidally disrupted13. …”
Get full text
Article -
17
TESS Observations of the WASP-121 b Phase Curve
Published 2021“…We then perform an atmospheric retrieval analysis to infer the dayside atmospheric properties of WASP-121 b, such as its bulk composition, albedo, and heat recirculation. …”
Get full text
Article -
18
TESS Observations of the WASP-121 b Phase Curve
Published 2022“…We then perform an atmospheric retrieval analysis to infer the dayside atmospheric properties of WASP-121 b, such as its bulk composition, albedo, and heat recirculation. …”
Get full text
Article -
19
TESS Phase Curve of the Hot Jupiter WASP-19b
Published 2020“…We measure a secondary eclipse depth of 470[subscript -110][superscript +130] ppm and detect a strong atmospheric brightness modulation signal with a semiamplitude of 319 ± 51 ppm. …”
Get full text
Article -
20
The Multiplanet System TOI-421
Published 2022“…TOI-421 b and TOI-421 c are found to be well-suited for atmospheric characterization. Our atmospheric simulations predict significant Lyα transit absorption, due to strong hydrogen escape in both planets, as well as the presence of detectable CH4 in the atmosphere of TOI-421 c if equilibrium chemistry is assumed.…”
Get full text
Article