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20022023
most citedThe Transiting Exoplanet Survey Satellite

4.1k citations

Showing 2017Show all

82 papers · 1 filter

astro-ph.GA2017124 cited

Copious Amounts of Dust and Gas in a z=7.5 Quasar Host Galaxy

Bram Venemans, Fabian Walter, Roberto Decarli +10

We present IRAM/NOEMA and JVLA observations of the quasar J1342+0928 at z=7.54 and report detections of copious amounts of dust and [CII] emission in the interstellar medium (ISM)…

astro-ph.EP201748 cited

Elemental Abundances of Kepler Objects of Interest in APOGEE. I. Two Distinct Orbital Period Regimes Inferred from Host Star Iron Abundances

Robert F. Wilson, Johanna Teske, Steven R. Majewski +13

The Apache Point Observatory Galactic Evolution Experiment (APOGEE) has observed 600 transiting exoplanets and exoplanet candidates from \textit{Kepler} (Kepler Objects of In…

physics.hist-ph2017

Cosmological Black Hole Observations and Kant's Transcendental Aesthetic

Juna A. Kollmeier

Kant put forward the notion of the Transcendental Aesthetic (TA) in his manuscript . In this note I review the TA in light of the detection…

astro-ph.SR201710 cited

BANYAN. X. Discovery of a wide, low-gravity L-type companion to a fast-rotating M3 dwarf

Marie-Eve Desrochers, Etienne Artigau, Jonathan Gagné +4

We report the discovery of a substellar-mass co-moving companion to 2MASS J22501512+2325342, an M3 candidate member of the young (130--200 Myr) AB Doradus Moving Group (ABDMG). Thi…

astro-ph.HE2017

The Rise and Peak of the Luminous Type IIn SN 2017hcc/ATLAS17lsn from ASAS-SN and Swift UVOT Data

J. L. Prieto, Ping Chen, Subo Dong +7

We present observations of the rise and peak of the Type IIn supernova SN 2017hcc/ATLAS17lsn obtained by the All-Sky Automated Survey for Supernovae (ASAS-SN) and Swift UVOT. The l…

astro-ph.EP201716 cited

ALMA and VLA Observations of the HD 141569 System

Jacob Aaron White, A. C. Boley, M. A. MacGregor +2

We present VLA 9 mm (33 GHz) observations of the HD 141569 system from semester 16A. The observations achieve a resolution of 0.25 arcsec ( au) and a sensitivity of $4.7~μ\…