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An Ultra-short Period Rocky Super-Earth with a Secondary Eclipse and a Neptune-like Companion around K2-141
DOI: 10.3847/1538-3881/aaa5b5 Bibcode: 2018AJ....155..107M

Kristiansen, Martti H.; Vanderburg, Andrew; Latham, David W. +44 more

Ultra-short period (USP) planets are a class of low-mass planets with periods shorter than one day. Their origin is still unknown, with photo-evaporation of mini-Neptunes and in situ formation being the most credited hypotheses. Formation scenarios differ radically in the predicted composition of USP planets, and it is therefore extremely importan…

2018 The Astronomical Journal
Gaia 121
Dynamical Constraints on the HR 8799 Planets with GPI
DOI: 10.3847/1538-3881/aae150 Bibcode: 2018AJ....156..192W

Duchêne, Gaspard; Esposito, Thomas M.; Oppenheimer, Rebecca +52 more

The HR 8799 system uniquely harbors four young super-Jupiters whose orbits can provide insights into the system’s dynamical history and constrain the masses of the planets themselves. Using the Gemini Planet Imager, we obtained down to one milliarcsecond precision on the astrometry of these planets. We assessed four-planet orbit models with differ…

2018 The Astronomical Journal
Gaia 109
A Catalog of Cool Dwarf Targets for the Transiting Exoplanet Survey Satellite
DOI: 10.3847/1538-3881/aab710 Bibcode: 2018AJ....155..180M

Muirhead, Philip S.; Lépine, Sébastien; Mann, Andrew W. +5 more

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 which cool dwarfs should be observed using two minute observations. TESS has the opportunity to search tens of thousands of nearby, cool, late…

2018 The Astronomical Journal
Gaia 107
The Solar Neighborhood XLIV: RECONS Discoveries within 10 parsecs
DOI: 10.3847/1538-3881/aac262 Bibcode: 2018AJ....155..265H

Henry, Todd J.; Winters, Jennifer G.; Jao, Wei-Chun +7 more

We describe the 44 systems discovered to be within 10 pc of the Sun by the RECONS team, primarily via the long-term astrometry program at the CTIO/SMARTS 0.9 m that began in 1999. The systems—including 41 with red dwarf primaries, 2 white dwarfs, and 1 brown dwarf—have trigonometric parallaxes greater than 100 mas, with errors of 0.4-2.4 mas in al…

2018 The Astronomical Journal
eHST 100
The Faint End of the z = 5 Quasar Luminosity Function from the CFHTLS
DOI: 10.3847/1538-3881/aaaab4 Bibcode: 2018AJ....155..131M

Fan, Xiaohui; Jiang, Linhua; McGreer, Ian D. +1 more

We present results from a spectroscopic survey of z ∼ 5 quasars in the CFHT Legacy Survey. Using both optical color selection and a likelihood method, we select 97 candidates over an area of 105 deg2 to a limit of i AB < 23.2, and 7 candidates in the range 23.2 < i AB < 23.7 over an area of 18.5 deg2<…

2018 The Astronomical Journal
eHST 96
Zodiacal Exoplanets in Time (ZEIT). VI. A Three-planet System in the Hyades Cluster Including an Earth-sized Planet
DOI: 10.3847/1538-3881/aa9791 Bibcode: 2018AJ....155....4M

Vanderburg, Andrew; Bieryla, Allyson; Latham, David W. +11 more

Planets in young clusters are powerful probes of the evolution of planetary systems. Here we report the discovery of three planets transiting EPIC 247589423, a late-K dwarf in the Hyades (≃800 Myr) cluster, and robust detection limits for additional planets in the system. The planets were identified from their K2 light curves as part of our survey…

2018 The Astronomical Journal
Gaia 91
Measuring the Recoverability of Close Binaries in Gaia DR2 with the Robo-AO Kepler Survey
DOI: 10.3847/1538-3881/aad80a Bibcode: 2018AJ....156..259Z

Baranec, Christoph; Law, Nicholas M.; Riddle, Reed +6 more

We use the Robo-AO survey of Kepler planetary candidate host stars, the largest adaptive optics survey yet performed, to measure the recovery rate of close stellar binaries in Gaia DR2. We find that Gaia recovers binaries down to 1″ at magnitude contrasts as large as six; closer systems are not resolved, regardless of secondary brightness. Gaia DR…

2018 The Astronomical Journal
Gaia 90
The Near-infrared Transmission Spectra of TRAPPIST-1 Planets b, c, d, e, f, and g and Stellar Contamination in Multi-epoch Transit Spectra
DOI: 10.3847/1538-3881/aade4f Bibcode: 2018AJ....156..178Z

Apai, Dániel; Zhou, Yifan; Rackham, Benjamin V. +1 more

The seven approximately Earth-sized transiting planets in the TRAPPIST-1 system provide a unique opportunity to explore habitable- and nonhabitable-zone small planets within the same system. Its habitable-zone exoplanets—due to their favorable transit depths—are also worlds for which atmospheric transmission spectroscopy is within reach with the H…

2018 The Astronomical Journal
eHST 89
Revisiting the Phase Curves of WASP-43b: Confronting Re-analyzed Spitzer Data with Cloudy Atmospheres
DOI: 10.3847/1538-3881/aaaebc Bibcode: 2018AJ....155..150M

Mendonça, João M.; Demory, Brice-Olivier; Heng, Kevin +1 more

Recently acquired Hubble and Spitzer phase curves of the short-period hot Jupiter WASP-43b make it an ideal target for confronting theory with data. On the observational front, we re-analyze the 3.6 and 4.5 µm Spitzer phase curves and demonstrate that our improved analysis better removes residual red noise due to intra-pixel sensitivity, whi…

2018 The Astronomical Journal
eHST 88
Zodiacal Exoplanets in Time (ZEIT). VIII. A Two-planet System in Praesepe from K2 Campaign 16
DOI: 10.3847/1538-3881/aadf37 Bibcode: 2018AJ....156..195R

Vanderburg, Andrew; Rizzuto, Aaron C.; Kraus, Adam L. +5 more

Young planets offer a direct view of the formation and evolution processes that produced the diverse population of mature exoplanet systems known today. The repurposed Kepler mission K2 is providing the first sample of young transiting planets by observing populations of stars in nearby, young clusters and stellar associations. We report the detec…

2018 The Astronomical Journal
Gaia 87