Search Publications

Zodiacal Exoplanets in Time (ZEIT). V. A Uniform Search for Transiting Planets in Young Clusters Observed by K2
DOI: 10.3847/1538-3881/aa9070 Bibcode: 2017AJ....154..224R

Vanderburg, Andrew; Rizzuto, Aaron C.; Kraus, Adam L. +2 more

Detection of transiting exoplanets around young stars is more difficult than for older systems owing to increased stellar variability. Nine young open cluster planets have been found in the K2 data, but no single analysis pipeline identified all planets. We have developed a transit search pipeline for young stars that uses a transit-shaped notch a…

2017 The Astronomical Journal
Gaia 79
A Physical Model-based Correction for Charge Traps in the Hubble Space Telescope’s Wide Field Camera 3 Near-IR Detector and Its Applications to Transiting Exoplanets and Brown Dwarfs
DOI: 10.3847/1538-3881/aa6481 Bibcode: 2017AJ....153..243Z

Schneider, Glenn; Apai, Dániel; Zhou, Yifan +1 more

The Hubble Space Telescope Wide Field Camera 3 (WFC3) near-IR channel is extensively used in time-resolved observations, especially for transiting exoplanet spectroscopy as well as brown dwarf and directly imaged exoplanet rotational phase mapping. The ramp effect is the dominant source of systematics in the WFC3 for time-resolved observations, wh…

2017 The Astronomical Journal
eHST 79
Three’s Company: An Additional Non-transiting Super-Earth in the Bright HD 3167 System, and Masses for All Three Planets
DOI: 10.3847/1538-3881/aa832d Bibcode: 2017AJ....154..122C

Henning, Thomas; Butler, R. Paul; Vogt, Steven S. +55 more

HD 3167 is a bright (V = 8.9), nearby K0 star observed by the NASA K2 mission (EPIC 220383386), hosting two small, short-period transiting planets. Here we present the results of a multi-site, multi-instrument radial-velocity campaign to characterize the HD 3167 system. The masses of the transiting planets are 5.02 ± 0.38 {M}\oplus for…

2017 The Astronomical Journal
Gaia 76
Exploring Dust around HD 142527 down to 0.″025 (4 au) Using SPHERE/ZIMPOL
DOI: 10.3847/1538-3881/aa7560 Bibcode: 2017AJ....154...33A

Ménard, F.; Quanz, S. P.; Avenhaus, H. +25 more

We have observed the protoplanetary disk of the well-known young Herbig star HD 142527 using ZIMPOL polarimetric differential imaging with the very broad band (∼600-900 nm) filter. We obtained two data sets in 2015 May and 2016 March. Our data allow us to explore dust scattering around the star down to a radius of ∼0.″025 (∼4 au). The well-known o…

2017 The Astronomical Journal
Gaia 74
Standard Galactic Field RR Lyrae. I. Optical to Mid-infrared Phased Photometry
DOI: 10.3847/1538-3881/153/3/96 Bibcode: 2017AJ....153...96M

Kollmeier, Juna A.; Madore, Barry F.; Freedman, Wendy L. +6 more

We present a multi-wavelength compilation of new and previously published photometry for 55 Galactic field RR Lyrae variables. Individual studies, spanning a time baseline of up to 30 years, are self-consistently phased to produce light curves in 10 photometric bands covering the wavelength range from 0.4 to 4.5 microns. Data smoothing via the GLO…

2017 The Astronomical Journal
Gaia 71
Orbiting Clouds of Material at the Keplerian Co-rotation Radius of Rapidly Rotating Low-mass WTTs in Upper Sco
DOI: 10.3847/1538-3881/aa5eb9 Bibcode: 2017AJ....153..152S

Pinsonneault, Marc; Cody, Ann Marie; Rebull, Luisa +8 more

Using K2 data, we identified 23 very-low-mass members of the ρ Oph and Upper Scorpius star-forming region as having periodic photometric variability not easily explained by well-established physical mechanisms such as star spots, eclipsing binaries, or pulsation. All of these unusual stars are mid-to-late M dwarfs without evidence of active accret…

2017 The Astronomical Journal
AKARI Gaia 68
An Optical/Near-infrared Investigation of HD 100546 b with the Gemini Planet Imager and MagAO
DOI: 10.3847/1538-3881/aa6cae Bibcode: 2017AJ....153..244R

Esposito, Thomas M.; Oppenheimer, Rebecca; Wolff, Schuyler G. +52 more

We present H band spectroscopic and Hα photometric observations of HD 100546 obtained with the Gemini Planet Imager and the Magellan Visible AO camera. We detect H band emission at the location of the protoplanet HD 100546 b, but show that the choice of data processing parameters strongly affects the morphology of this source. It appears point-lik…

2017 The Astronomical Journal
Gaia 67
A Measurement of Radius Inflation in the Pleiades and Its Relation to Rotation and Lithium Depletion
DOI: 10.3847/1538-3881/153/3/101 Bibcode: 2017AJ....153..101S

Stassun, Keivan G.; Somers, Garrett

Precise measurements of eclipsing binary parameters and statistical studies of young clusters have suggested that some magnetically active low-mass dwarfs possess radii inflated by ∼5%-15% relative to theoretical expectations. If true, this effect should be pronounced in young open clusters, due to the rapid rotation and strong magnetic activity o…

2017 The Astronomical Journal
Gaia 61
Evidence for Atmospheric Cold-trap Processes in the Noninverted Emission Spectrum of Kepler-13Ab Using HST/WFC3
DOI: 10.3847/1538-3881/aa899b Bibcode: 2017AJ....154..158B

Madhusudhan, Nikku; Knutson, Heather A.; Wright, Jason T. +5 more

We observed two eclipses of the Kepler-13A planetary system, on UT 2014 April 28 and UT 2014 October 13, in the near-infrared using Wide Field Camera 3 on the Hubble Space Telescope. By using the nearby binary stars Kepler-13BC as a reference, we were able to create a differential light curve for Kepler-13A that had little of the systematics typic…

2017 The Astronomical Journal
eHST 57
The SEEDS High-Contrast Imaging Survey of Exoplanets Around Young Stellar Objects
DOI: 10.3847/1538-3881/153/3/106 Bibcode: 2017AJ....153..106U

Henning, Thomas; Terada, Hiroshi; Usuda, Tomonori +49 more

We present high-contrast observations of 68 young stellar objects (YSOs) that have been explored as part of the Strategic Exploration of Exoplanets and Disks with Subaru (SEEDS) survey on the Subaru telescope. Our targets are very young (<10 Myr) stars, which often harbor protoplanetary disks where planets may be forming. We achieve a typical c…

2017 The Astronomical Journal
eHST 55