IVOA Registry (Virtual Observatory)2022 · Astronomical catalogue
Transiting planet HATS-18b…We present extensive photometry of HATS-18 from which we measure 27 times of mid-transit.… …Two further transit times were measured from data from the Transiting Exoplanet Survey Satellite (TESS) and three more taken from the literature.…
IVOA Registry (Virtual Observatory)2019 · Astronomical catalogue
WASP-121 b Swift UVOT near-UV transit observations…Today, ongoing mass loss has been confirmed in a few individual systems via transit observations in the ultraviolet spectral range.… …We measure a broad-band NUV transit depth of 2.10+/-0.29%.…
IVOA Registry (Virtual Observatory)2020 · Astronomical catalogue
HAT-P-41b transmission spectra with HST WFC3/UVIS…We test the G280 grism mode on the hot Jupiter HAT-P-41b over two consecutive transits to determine its viability for the characterization of exoplanet atmospheres.… …We obtain a broadband transit depth precision of 29-33ppm and a precision of on average 200ppm in 10nm spectroscopic bins.…
IVOA Registry (Virtual Observatory)2021 · Astronomical catalogue
HST spectral light curve of HAT-P-41…The planet was observed in transit with Hubble STIS and WFC3 as part of the Hubble Panchromatic Comparative Exoplanet Treasury (PanCET) program, and we combine those data with warm… …Spitzer transit observations.…
IVOA Registry (Virtual Observatory)2014 · Astronomical catalogue
GALEX observations of exoplanet host stars…The case is strengthened to a level of significance to 2.3{sigma} when transit-detected close-in planets are included.… …This is most likely because the RV-selected sample of stars is significantly less active than the field population of comparable stars, while the transit-selected sample is similarly…
IVOA Registry (Virtual Observatory)2020 · Astronomical catalogue
HST/STIS FUV spectra of K2-18…We found that the average blueshifted emission of K2-18 decreases by 67%+/-18% during the transit of the planet compared to the pre-transit emission, tentatively indicating the presence… …This interpretation is not definitive because it relies on one partial transit.…
IVOA Registry (Virtual Observatory)2018 · Astronomical catalogue
A catalog of cool dwarf targets for the TESS…We present a catalog of cool dwarf targets (V-J>2.7, T_eff_~<4000 K) and their stellar properties for the upcoming Transiting Exoplanet Survey Satellite (TESS), for the purpose of determining… …TESS has the opportunity to search tens of thousands of nearby, cool, late K- and M-type dwarfs for transiting exoplanets, an order of magnitude more than current or previous transiting…
IVOA Registry (Virtual Observatory)2016 · Astronomical catalogue
HST/COS observations of 7 white dwarfs…The search for transiting habitable exoplanets has broadened to include several types of stars that are smaller than the Sun in an attempt to increase the observed transit depth and… …We use archival Hubble Space Telescope data from the Cosmic Origins Spectrograph to search for transiting rocky planets around UV-bright WDs.…
IVOA Registry (Virtual Observatory)2025 · Astronomical catalogue
M dwarfs flares timing & energy from TESS & Swift…Ultraviolet flare emission can drive photochemistry in exoplanet atmospheres and even serve as the primary source of uncertainty in atmospheric retrievals.… …We present new near-UV (NUV) and optical observations of flares from three M dwarfs obtained at 20s cadence with Swift and the Transiting Exoplanet Survey Satellite (TESS), along with…
IVOA Registry (Virtual Observatory)2022 · Astronomical catalogue
5-55000{AA} spectrum of TOI 560…The absorption signal repeats during a partial transit obtained a month later, but is marginally stronger and bluer, perhaps reflecting changes in the stellar wind environment.… …We find that our models generally overpredict the measured magnitude of the absorption during transit, the size of the blueshift, or both.…
IVOA Registry (Virtual Observatory)2022 · Astronomical catalogue
Fiducial stellar spectrum of HD 63433…Using Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograph, we measure a transit depth of 11.1{+/-}1.5% in the blue wing and 8{+/-}3% in the red.… …This signal is unlikely to be due to stellar variability, but should be confirmed by an upcoming second transit observation with HST.…
IVOA Registry (Virtual Observatory)2021 · Astronomical catalogue
Synthetic XUV spectra of GJ 3470…Neptune-size exoplanets seem particularly sensitive to atmospheric evaporation, making it essential to characterize the stellar high-energy radiation that drives this mechanism.… …Here we report on three additional transit observations from the Panchromatic Comparative Exoplanet Treasury program, obtained with the HST Cosmic Origin Spectrograph.…
IVOA Registry (Virtual Observatory)2022 · Astronomical catalogue
Data and parameters for subgiant sample…Accordingly, they are prime asteroseismic targets for the Transiting Exoplanet Survey Satellite (TESS) mission.…
IVOA Registry (Virtual Observatory)2024 · Astronomical catalogue
Photometry & spectroscopy follow-up of ASASSN-20hx…From Transiting Exoplanet Survey Satellite data, we determine that the ANT began to brighten on 2020 June 22.8 with a linear rise in flux for at least the first week.…
IVOA Registry (Virtual Observatory)2022 · Astronomical catalogue
Follow-up photometry of ASASSN-14ko…The Transiting Exoplanet Survey Satellite observed an outburst during Sectors 4-6, revealing a rise time of 5.60+/-0.05days in the optical and a decline that is best fit with an exponential…