papers

Publications (24)

astro-ph.EP2019

Absence of a thick atmosphere on the terrestrial exoplanet LHS 3844b

Laura Kreidberg, Daniel D. B. Koll, Caroline Morley +16

Most known terrestrial planets orbit small stars with radii less than 60% that of the Sun. Theoretical models predict that these planets are more vulnerable to atmospheric loss tha…

astro-ph.EP2022

Hubble Space Telescope transmission spectroscopy for the temperate sub-Neptune TOI-270d: a possible hydrogen-rich atmosphere containing water vapour

Thomas Mikal-Evans, Nikku Madhusudhan, Jason Dittmann +6

TOI-270d is a temperate sub-Neptune discovered by the Transiting Exoplanet Survey Satellite (TESS) around a bright (J=9.1mag) M3V host star. With an approximate radius of 2RE and e…

astro-ph.SR2025

The Spin-orbit alignment of two short period eclipsing binary systems

Tony Wells, B. C. Addison, R. A. Wittenmyer +8

We present a joint analysis of TESS photometry and radial velocity measurements obtained from the Minerva-Australis facility for two short-period eclipsing binaries, TIC 48227288 a…

astro-ph.EP2019

Identifying Exoplanets with Deep Learning III: Automated Triage and Vetting of TESS Candidates

Liang Yu, Andrew Vanderburg, Chelsea Huang +14

NASA's Transiting Exoplanet Survey Satellite (TESS) presents us with an unprecedented volume of space-based photometric observations that must be analyzed in an efficient and unbia…

astro-ph.EP2014

The MEarth-North and MEarth-South transit surveys: searching for habitable super-Earth exoplanets around nearby M-dwarfs

Jonathan M. Irwin, Zachory K. Berta-Thompson, David Charbonneau +4

Detection and characterization of potentially habitable Earth-size extrasolar planets is one of the major goals of contemporary astronomy. By applying the transit method to very lo…

astro-ph.EP2018

A 2 Earth Radius Planet Orbiting the Bright Nearby K-Dwarf Wolf 503

Merrin S. Peterson, Björn Benneke, Courtney D. Dressing +20

Since its launch in 2009, the Kepler telescope has found thousands of planets with radii between that of Earth and Neptune. Recent studies of the distribution of these planets have…

astro-ph.GA2025

The Discovery of 25 um Interstellar Methanol

Sarah L. Nickerson, Naseem Rangwala, Keeyoon Sung +15

We present the first astrophysical detection of methanol (CH3OH) in the torsional band near 25 um. Using high resolution mid-infrared (MIR) spectroscopy, we identified over seventy…

astro-ph.HE2013

A Wolf in Sheepskin: Extraordinary Supernova 2012au Veiled Behind Ordinary Radio Emission

Atish Kamble, Alicia M. Soderberg, Laura Chomiuk +11

We present extensive radio and X-ray observations of SN\, 2012au, the energetic radio luminous supernova of type Ib that may be a link between subsets of hydrogen-poor superluminou…

astro-ph.EP2018

A TESS Dress Rehearsal: Planetary Candidates and Variables from K2 Campaign 17

Ian J. M. Crossfield, Natalia Guerrero, Trevor David +38

We produce light curves for all ~34,000 targets observed with K2 in Campaign 17 (C17), identifying 34 planet candidates, 184 eclipsing binaries, and 222 other periodic variables. T…

astro-ph.SR2025

Stellar Flares in the TESS Light Curves of Planet-hosting M dwarfs

Benjamin K. Capistrant, Jason Dittmann

M dwarfs are magnetically active stars that frequently produce flares, which have implications for both stellar evolution and exoplanet studies. Flare occurrence rates and activity…

astro-ph.HE2015

A Missing-Link in the Supernova-GRB Connection: The Case of SN 2012ap

Sayan Chakraborti, Alicia Soderberg, Laura Chomiuk +50

Gamma Ray Bursts (GRBs) are characterized by ultra-relativistic outflows, while supernovae are generally characterized by non-relativistic ejecta. GRB afterglows decelerate rapidly…

astro-ph.EP2024

Quantifying the Effect of Short-timescale Stellar Activity Upon Transit Detection in M Dwarfs

Dana Clarice Yaptangco, Sarah Ballard, Jason Dittmann

M dwarf stars comprise 70-80% of the galaxy's stars and host most of its rocky planets. They also importantly differ from Sunlike stars in that they are "active" for billions of ye…

astro-ph.SR2011

LSPM J1112+7626: detection of a 41-day M-dwarf eclipsing binary from the MEarth transit survey

Jonathan M. Irwin, Samuel N. Quinn, Zachory K. Berta +13

We report the detection of eclipses in LSPM J1112+7626, which we find to be a moderately bright (I_C = 12.14 +/- 0.05) very low-mass binary system with an orbital period of 41.0323…

astro-ph.EP2019

Lyman-alpha in the GJ 1132 System: Stellar Emission and Planetary Atmospheric Evolution

William C. Waalkes, Zachory Berta-Thompson, Vincent Bourrier +6

GJ 1132b, which orbits an M dwarf, is one of the few known Earth-sized planets, and at 12 pc away it is one of the closest known transiting planets. Receiving roughly 19x Earth's i…

astro-ph.SR2019

How to Constrain Your M dwarf II: the mass-luminosity-metallicity relation from 0.075 to 0.70

Andrew W. Mann, Trent Dupuy, Adam L. Kraus +11

The mass-luminosity relation for late-type stars has long been a critical tool for estimating stellar masses. However, there is growing need for both a higher-precision relation an…

astro-ph.SR2015

An Activity-Rotation Relationship and Kinematic Analysis of Nearby Mid-to-Late-type M Dwarfs

Andrew A. West, Kolby L. Weisenburger, Jonathan Irwin +4

Using spectroscopic observations and photometric light curves of 238 nearby M dwarfs from the MEarth exoplanet transit survey, we examine the relationships between magnetic activit…

astro-ph.EP2026

Searching for Extragalactic Exoplanets: A Survey of the Sagittarius Dwarf Galaxy Stream with TESS

William Schap, Jason Dittmann, Elizabeth Lada

To date no exoplanets have been detected outside the Milky Way, and their extragalactic occurrence rates are poorly constrained. Using available data from TESS we perform the first…

astro-ph.EP2019

An Eccentric Massive Jupiter Orbiting a Sub-Giant on a 9.5 Day Period Discovered in the Transiting Exoplanet Survey Satellite Full Frame Images

Joseph E. Rodriguez, Samuel N. Quinn, Chelsea X. Huang +71

We report the discovery of TOI-172 b from the Transiting Exoplanet Survey Satellite (TESS) mission, a massive hot Jupiter transiting a slightly evolved G-star with a 9.48-day orbit…

astro-ph.EP2025

HD 35843: A Sun-like star hosting a long period sub-Neptune and inner super-Earth

Katharine Hesse, Ismael Mireles, François Bouchy +52

We report the discovery and confirmation of two planets orbiting the metal-poor Sun-like star, HD 35843 (TOI 4189). HD 35843 c is a temperate sub-Neptune transiting planet with an…

astro-ph.EP2019

Near-resonance in a system of sub-Neptunes from TESS

Samuel N. Quinn, Juliette C. Becker, Joseph E. Rodriguez +78

We report the Transiting Exoplanet Survey Satellite () detection of a multi-planet system orbiting the K0 dwarf TOI 125. We find evidence for up to five planets, wit…

astro-ph.EP2017

The Science Case for an Extended Spitzer Mission

Jennifer C. Yee, Giovanni G. Fazio, Robert Benjamin +45

Although the final observations of the Spitzer Warm Mission are currently scheduled for March 2019, it can continue operations through the end of the decade with no loss of photome…

astro-ph.EP2020

Simultaneous Optical Transmission Spectroscopy of a Terrestrial, Habitable-Zone Exoplanet with Two Ground-Based Multi-Object Spectrographs

Hannah Diamond-Lowe, Zachory Berta-Thompson, David Charbonneau +2

Investigating the atmospheres of rocky exoplanets is key to performing comparative planetology between these worlds and the terrestrial planets that reside in the inner solar syste…

astro-ph.EP2018

TESS Discovery of an ultra-short-period planet around the nearby M dwarf LHS 3844

Roland Vanderspek, Chelsea X. Huang, Andrew Vanderburg +45

Data from the newly-commissioned \textit{Transiting Exoplanet Survey Satellite} (TESS) has revealed a "hot Earth" around LHS 3844, an M dwarf located 15 pc away. The planet has a r…

astro-ph.EP2025

Limits on the atmospheric metallicity and aerosols of the sub-Neptune GJ 3090 b from high-resolution CRIRES+ spectroscopy

Luke T. Parker, João M. Mendonça, Hannah Diamond-Lowe +9

The sub-Neptune planets have no solar system analogues, and their low bulk densities suggest thick atmospheres containing degenerate quantities of volatiles and H/He, surrounding c…