activity
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

collaborators

156 papers

physics.pop-ph2022★ 1 cited

Exploration of M31 via Black-Hole Slingshots and the "Intergalactic Imperative"

Andrew Gould

I show that a gravitational slingshot using a stellar-mass black hole (BH) orbiting SgrA* could launch robotic spacecraft toward M31 at , a speed that is ultimately limited…

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.IM2020

Rigorous "Rich Argument" in Microlensing Parallax

Andrew Gould

I show that when the observables are well measured up to a discrete degeneracy in the microlensing parallax vector $\vec π_{\rm…

astro-ph.GA2019★ 91 cited

The Separation Distribution of Ultra-Wide Binaries across Galactic Populations

Hai-Jun Tian, Kareem El-Badry, Hans-Walter Rix +1

We present an extensive sample of ultra-wide binary stars in the solar neighborhood, focusing on separations of . Using data from Gaia DR2, we define kinematic sub-p…

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.SR2019★ 15 cited

Spitzer Microlensing parallax reveals two isolated stars in the Galactic bulge

Weicheng Zang, Yossi Shvartzvald, Tianshu Wang +90

We report the mass and distance measurements of two single-lens events from the 2017 Spitzer microlensing campaign. The ground-based observations yield the detection of finite-sour…

astro-ph.SR2019★ 12 cited

Spitzer Microlensing of MOA-2016-BLG-231L : A Counter-Rotating Brown Dwarf Binary in the Galactic Disk

Sun-Ju Chung, Andrew Gould, Jan Skowron +60

We analyze the binary microlensing event MOA-2016-BLG-231, which was observed from the ground and from Spitzer. The lens is composed of very low-mass brown dwarfs (BDs) with $M_1 =…

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.GA2018★ 13 cited

Gaia: Orion's Integral Shaped Filament is a Standing Wave

Amelia M. Stutz, Valentina I. Gonzalez-Lobos, Andrew Gould

The Integral Shaped Filament (ISF) is the nearest molecular cloud with rapid star formation, including massive stars, and it is therefore a star-formation laboratory. We use Gaia p…

astro-ph.SR2018★ 13 cited

A Distant Sample of Halo Wide Binaries from SDSS

Johanna Coronado, María Paz Sepúlveda, Andrew Gould +1

Samples of reliably identified halo wide binaries are scarce. If reasonably free from selection effects and with a small degree of contamination by chance alignments, these wide bi…

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.GA2018★ 75 cited

Two chemically similar stellar overdensities on opposite sides of the plane of the Galaxy

Maria Bergemann, Branimir Sesar, Judith G. Cohen +9

Our Galaxy is thought to have undergone an active evolutionary history dominated by star formation, the accretion of cold gas, and, in particular, mergers up to 10 gigayear ago. Th…

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.SR2016★ 10 cited

TGAS Error Renormalization from the RR Lyrae Period-Luminosity Relation

Andrew Gould, Juna A. Kollmeier, Branimir Sesar

The Gaia team has applied a renormalization to their internally-derived parallax errors $$ σ_{tgas}(π) = \sqrt{[Aσ_{int}(π)]^2 + σ_0^2}; \ \ \ \ (A,σ_0) = (1.4,0.2…

astro-ph.SR2016

Predicted Information Content of Gaia-Hipparcos

Andrew Gould, Juna A. Kollmeier

The Gaia-Tycho release, scheduled for 14 September, is forecast to yield parallax errors of as for about 2 million Tycho stars. We show analytically that the actua…

astro-ph.SR2016★ 7 cited

Gaia Parallax Zero Point From RR Lyrae Stars

Andrew Gould, Juna A. Kollmeier

Like Hipparcos, Gaia is designed to give absolute parallaxes, independent of any astrophysical reference system. And indeed, Gaia's internal zero-point error for parallaxes is like…

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.SR2015★ 129 cited

Slingshot Mechanism in Orion: Kinematic Evidence For Ejection of Protostars by Filaments

Amelia M. Stutz, Andrew Gould

By comparing 3 constituents of Orion A (gas, protostars, and pre-main-sequence stars), both morhologically and kinematically, we derive the following. The gas surface density near…