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19932022
most citedReddening and Extinction Toward the Galactic Bulge from OGLE-III: The Inner Milky Way's Rv ~ 2.5 Extinction Curve

590 citations · 8.8k across the 153 of their papers we have counts for

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28 papers · 1 filter

astro-ph.EP2022★ 3 cited

MASADA: From Microlensing Planet Mass-Ratio Function to Planet Mass Function

Andrew Gould

Using current technology, gravitational microlensing is the only method that can measure planet masses over the full parameter space of planet and stellar-host masses and at a broa…

astro-ph.EP2021★ 12 cited

KMT-2021-BLG-0912Lb: A microlensing super Earth around a K-type star

Cheongho Han, Ian A. Bond, Jennifer C. Yee +55

The light curve of the microlensing event KMT-2021-BLG-0912 exhibits a very short anomaly relative to a single-lens single-source form. We investigate the light curve for the purpo…

astro-ph.EP2020★ 29 cited

Masses for Free-Floating Planets and Dwarf Planets

Andrew Gould, Weicheng Zang, Shude Mao +1

The mass and distance functions of free-floating planets (FFPs) would give major insights into the formation and evolution of planetary systems, including any systematic difference…

astro-ph.EP2019

Osculating Versus Intersecting Circles in Space-Based Microlens Parallax Degeneracies

Andrew Gould

I investigate the origin of arc degeneracies in satellite microlens parallax pi_E measurements with only late time data, e.g., t > t0 + t_E as seen from the satellite. I show that…

astro-ph.EP2018★ 38 cited

KMT-2017-BLG-0165Lb: A Super-Neptune mass planet Orbiting a Sun-like Host Star

Youn Kil Jung, Andrew Gould, Weicheng Zang +22

We report the discovery of a low mass-ratio planet , i.e., 2.5 times higher than the Neptune/Sun ratio. The planetary system was discovered from the analysi…

astro-ph.EP2018★ 44 cited

A Universal Break in the Planet-to-Star Mass-Ratio Function of Kepler MKG stars

Ilaria Pascucci, Gijs D. Mulders, Andrew Gould +1

We follow the microlensing approach and quantify the occurrence of Kepler exoplanets as a function of planet-to-star mass ratio, q, rather than planet radius or mass. For planets w…

astro-ph.EP2017★ 100 cited

KELT-20b: A giant planet with a period of P~ 3.5 days transiting the V~ 7.6 early A star HD 185603

Michael B. Lund, Joseph E. Rodriguez, George Zhou +46

We report the discovery of KELT-20b, a hot Jupiter transiting a V~7.6 early A star with an orbital period of P~3.47 days. We identified the initial transit signal in KELT-North sur…

astro-ph.EP2017★ 270 cited

A giant planet undergoing extreme ultraviolet irradiation by its hot massive-star host

B. Scott Gaudi, Keivan G. Stassun, Karen A. Collins +57

The amount of ultraviolet irradiation and ablation experienced by a planet depends strongly on the temperature of its host star. Of the thousands of extra-solar planets now known,…

astro-ph.EP2016★ 17 cited

KELT-12b: A Day, Highly Inflated Hot Jupiter Transiting a Mildly Evolved Hot Star

Daniel J. Stevens, Karen A. Collins, B. Scott Gaudi +46

We report the discovery of KELT-12b, a highly inflated Jupiter-mass planet transiting a mildly evolved host star. We identified the initial transit signal in the KELT-North survey…

astro-ph.EP2016★ 45 cited

KELT-16b: A highly irradiated, ultra-short period hot Jupiter nearing tidal disruption

Thomas E. Oberst, Joseph E. Rodriguez, Knicole D. Colón +47

We announce the discovery of KELT-16b, a highly irradiated, ultra-short period hot Jupiter transiting the relatively bright () star TYC 2688-1839-1. A global analysis of…

astro-ph.EP2016★ 75 cited

KELT-17b: A hot-Jupiter transiting an A-star in a misaligned orbit detected with Doppler tomography

George Zhou, Joseph E. Rodriguez, Karen A. Collins +45

We present the discovery of a hot-Jupiter transiting the V=9.23 mag main-sequence A-star KELT-17 (BD+14 1881). KELT-17b is a 1.31 -0.29/+0.28 Mj, 1.525 -0.060/+0.065 Rj hot-Jupiter…

astro-ph.EP2016★ 20 cited

Microlensing by Kuiper, Oort, and Free-Floating Planets

Andrew Gould

Microlensing is generally thought to probe planetary systems only out to a few Einstein radii. Microlensing events generated by bound planets beyond about 10 Einstein radii general…

astro-ph.EP2015★ 43 cited

KELT-4Ab: An inflated Hot Jupiter transiting the bright (V~10) component of a hierarchical triple

Jason D. Eastman, Thomas G. Beatty, Robert J. Siverd +42

We report the discovery of KELT-4Ab, an inflated, transiting Hot Jupiter orbiting the brightest component of a hierarchical triple stellar system. The host star is an F star with $…

astro-ph.EP2015★ 2 cited

KELT-7b: A hot Jupiter transiting a bright V=8.54 rapidly rotating F-star

Allyson Bieryla, Karen Collins, Thomas G. Beatty +31

We report the discovery of KELT-7b, a transiting hot Jupiter with a mass of MJ, radius of RJ, and an orbital period of $2.7347749 \pm 0.000…

astro-ph.EP2014★ 72 cited

Optimal Survey Strategies and Predicted Planet Yields for the Korean Microlensing Telescope Network

Calen B. Henderson, B. Scott Gaudi, Cheongho Han +4

The Korean Microlensing Telescope Network (KMTNet) will consist of three 1.6m telescopes each with a 4 deg^{2} field of view (FoV) and will be dedicated to monitoring the Galactic…

astro-ph.EP2014★ 12 cited

WFIRST Ultra-Precise Astrometry I: Kuiper Belt Objects

Andrew Gould

I show that the WFIRST microlensing survey will enable detection and precision orbit determination of Kuiper Belt Objects (KBOs) down to H_=28.2 over an effective area of about 17…

astro-ph.EP2013

Generalized Microlensing Effective Timescale

Andrew Gould

The microlensing effective timescale t_eff=beta*t_E is used frequently in high-magnification (beta << 1) microlensing events, because it is better constrained than either the impac…

astro-ph.EP2013★ 84 cited

Kepler-like Multi-Plexing for Mass Production of Microlens Parallaxes

Andrew Gould, Keith Horne

We show that a wide-field Kepler-like satellite in Solar orbit could obtain microlens parallaxes for several thousand events per year that are identified from the ground, yielding…

astro-ph.EP2013★ 44 cited

KELT-6b: A P~7.9 d Hot Saturn Transiting a Metal-Poor Star with a Long-Period Companion

Karen A. Collins, Jason D. Eastman, Thomas G. Beatty +39

We report the discovery of KELT-6b, a mildly-inflated Saturn-mass planet transiting a metal-poor host. The initial transit signal was identified in KELT-North survey data, and the…

astro-ph.EP2013

Kepler Microlens Planets and Parallaxes

Andrew Gould, Keith Horne

Kepler's quest for other Earths need not end just yet: it remains capable of characterizing cool Earth-mass planets by microlensing, even given its degraded pointing control. If Ke…

astro-ph.EP2013★ 9 cited

OGLE-2011-BLG-0417: A Radial Velocity Testbed for Microlensing

Andrew Gould, In-Gu Shin, Cheongho Han +2

Microlensing experiments are returning increasingly detailed information about the planetary and binary systems that are being detected, far beyond what was originally expected. In…

astro-ph.EP2012★ 42 cited

Geosynchronous Microlens Parallaxes

Andrew Gould

I show that for a substantial fraction of planets detected in a space-based survey, it would be possible to measure the planet and host masses and distances, if the survey satellit…

astro-ph.EP2012★ 74 cited

KELT-3b: A Hot Jupiter Transiting a V=9.8 Late-F Star

Joshua Pepper, Robert J. Siverd, Thomas G. Beatty +31

We report the discovery of KELT-3b, a moderately inflated transiting hot Jupiter with a mass of 1.477 (-0.067, +0.066) M_J, and radius of 1.345 +/- 0.072 R_J, with an orbital perio…

astro-ph.EP2012★ 300 cited

KELT-1b: A Strongly Irradiated, Highly Inflated, Short Period, 27 Jupiter-mass Companion Transiting a mid-F Star

Robert J. Siverd, Thomas G. Beatty, Joshua Pepper +29

We present the discovery of KELT-1b, the first transiting low-mass companion from the wide-field Kilodegree Extremely Little Telescope-North (KELT-North) survey. The V=10.7 primary…