output
20022024
most citedThe Transiting Exoplanet Survey Satellite

4.1k citations

Showing 2022Show all

88 papers · 1 filter

astro-ph.SR202254 cited

white dwarfs within 40 pc III: spectroscopic observations of new candidates in the southern hemisphere

Mairi W. O'Brien, P. -E. Tremblay, N. P. Gentile Fusillo +31

We present a spectroscopic survey of 248 white dwarf candidates within 40 pc of the Sun; of these 244 are in the southern hemisphere. Observations were performed mostly with the Ve…

astro-ph.EP20225 cited

KELT-9 and its ultra-hot Jupiter: stellar parameters, composition, and planetary pollution

Mihkel Kama, Colin P. Folsom, Adam S. Jermyn +1

KELT-9b is an ultra-hot Jupiter observed to be undergoing extreme mass loss. Its A0-type host star has a radiative envelope, which makes its surface layers prone to retaining recen…

astro-ph.GA202242 cited

A Transient "Changing-look'' Active Galactic Nucleus Resolved on Month Timescales from First-year Sloan Digital Sky Survey V Data

Grisha Zeltyn, Benny Trakhtenbrot, Michael Eracleous +32

We report the discovery of a new ``changing-look'' active galactic nucleus (CLAGN) event, in the quasar SDSS J162829.17+432948.5 at z=0.2603, identified through repeat spectroscopy…

astro-ph.SR202228 cited

The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities

Z. Keszthelyi, A. de Koter, Y. Götberg +12

Magnetic fields can drastically change predictions of evolutionary models of massive stars via mass-loss quenching, magnetic braking, and efficient angular momentum transport, whic…

astro-ph.GA202227 cited

An extended [CII] halo around a massive star-forming galaxy at z = 5.3

T. S. Lambert, A. Posses, M. Aravena +8

High-redshift observations are often biased towards massive and bright galaxies that are not necessarily representative of the full population. In order to accurately study galaxy…

astro-ph.EP202213 cited

A dense mini-Neptune orbiting the bright young star HD 18599

Jose I. Vines, James S. Jenkins, Zaira Berdiñas +23

Very little is known about the young planet population because the detection of small planets orbiting young stars is obscured by the effects of stellar activity and fast rotation…