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20102026
most citedThe TESS Objects of Interest Catalog from the TESS Prime Mission

392 citations · 3.2k across the 146 of their papers we have counts for

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astro-ph.SR2026

Paving the Road to the Habitable Worlds Observatory with High-Resolution Imaging I: New and Archival Speckle Observations of Potential HWO Target Stars

Zachary D. Hartman, Catherine A. Clark, Michael B. Lund +15

One of the key goals of the Habitable Worlds Observatory (HWO) is to directly image about 25 potentially habitable exoplanets and determine their properties. This challenge will re…

astro-ph.SR2024

The POKEMON Speckle Survey of Nearby M Dwarfs. III. The Stellar Multiplicity Rate of M Dwarfs within 15 pc

Catherine A. Clark, Gerard T. van Belle, Elliott P. Horch +8

M dwarfs are ubiquitous in our galaxy, and the rate at which they host stellar companions, and the properties of these companions, provides a window into the formation and evolutio…

astro-ph.SR2023

The POKEMON Speckle Survey of Nearby M Dwarfs. II. Observations of 1125 Targets

Catherine A. Clark, Gerard T. van Belle, Elliott P. Horch +7

Stellar multiplicity is correlated with many stellar properties, yet multiplicity measurements have proven difficult for the M dwarfs -- the most common type of star in our galaxy…

astro-ph.SR2022★ 15 cited

Three low-mass companions around aged stars discovered by TESS

Zitao Lin, Tianjun Gan, Sharon X. Wang +42

We report the discovery of three transiting low-mass companions to aged stars: a brown dwarf (TOI-2336b) and two objects near the hydrogen burning mass limit (TOI-1608b and TOI-252…

astro-ph.SR2022★ 21 cited

Probable Dormant Neutron Star in a Short-Period Binary System

Tsevi Mazeh, Simchon Faigler, Dolev Bashi +24

We have identified 2XMM J125556.57+565846.4, at a distance of 600 pc, as a binary system consisting of a normal star and a probable dormant neutron star. Optical spectra exhibit a…

astro-ph.SR2022★ 19 cited

A Dearth of Close-In Stellar Companions to M-dwarf TESS Objects of Interest

Catherine A. Clark, Gerard T. van Belle, David R. Ciardi +5

TESS has proven to be a powerful resource for finding planets, including those that orbit the most prevalent stars in our galaxy: the M dwarfs. Identification of stellar companions…

astro-ph.SR2022★ 22 cited

TOI-2119: A transiting brown dwarf orbiting an active M-dwarf from NASA's TESS mission

Theron W. Carmichael, Jonathan M. Irwin, Felipe Murgas +27

We report the discovery of TOI-2119b, a transiting brown dwarf (BD) that orbits and is completely eclipsed by an active M-dwarf star. Using light curve data from the Transiting Exo…

astro-ph.SR2021★ 42 cited

First results on RR Lyrae stars with the TESS space telescope: untangling the connections between mode content, colors and distances

László Molnár, Attila Bódi, András Pál +25

The TESS space telescope is collecting continuous, high-precision optical photometry of stars throughout the sky, including thousands of RR Lyrae stars. In this paper, we present r…

astro-ph.SR2021★ 39 cited

TOI-1278 B: SPIRou unveils a rare Brown Dwarf Companion in Close-In Orbit around an M dwarf

Étienne Artigau, Guillaume Hébrard, Charles Cadieux +39

We present the discovery of an M brown dwarf (BD) companion to the M0V star TOI-1278. The system was first identified through a percent-deep transit in TESS…

astro-ph.SR2020★ 44 cited

TOI-811b and TOI-852b: New transiting brown dwarfs with similar masses and very different radii and ages from the TESS mission

Theron W. Carmichael, Samuel N. Quinn, George Zhou +17

We report the discovery of two transiting brown dwarfs (BDs), TOI-811b and TOI-852b, from NASA's Transiting Exoplanet Survey Satellite mission. These two transiting BDs have simila…

astro-ph.SR2020★ 8 cited

Long-Period High-Amplitude Red Variables in the KELT Survey

R. Alex Arnold, M. Virginia McSwain, Joshua Pepper +8

We present a sample of 4,132 Mira-like variables (red variables with long periods and high amplitudes) in the Kilodegree Extremely Little Telescope (KELT) survey. Of these, 814 are…

astro-ph.SR2019★ 10 cited

Eclipsing binaries in the open cluster Ruprecht 147. II: EPIC 219568666

Guillermo Torres, Andrew Vanderburg, Jason L. Curtis +7

We report our spectroscopic monitoring of the detached, grazing, and slightly eccentric 12-day double-lined eclipsing binary EPIC 219568666 in the old nearby open cluster Ruprecht…

astro-ph.SR2019★ 19 cited

MOBSTER -- III. HD 62658: a magnetic Bp star in an eclipsing binary with a non-magnetic 'identical twin'

M. E. Shultz, C. Johnston, J. Labadie-Bartz +9

HD 62658 (B9p V) is a little-studied chemically peculiar star. Light curves obtained by the Kilodegree Extremely Little Telescope (KELT) and Transiting Exoplanet Survey Satellite (…

astro-ph.SR2019★ 13 cited

An Extreme-mass Ratio, Short-period Eclipsing Binary Consisting of a B Dwarf Primary and a Pre-main Sequence M Star Companion Discovered by KELT

Daniel J. Stevens, George Zhou, Marshall C. Johnson +16

We present the discovery of \thisstar\ (HD 58730), a very low mass ratio () eclipsing binary (EB) identified by the Kilodegree Extremely Little Teles…

astro-ph.SR2019

New Beta Cephei stars with KELT

Jonathan Labadie-Bartz, Gerald Handler, Joshua Pepper +9

We present the results of a search for Galactic Beta Cephei stars, which are massive pulsating stars with both pressure modes and mixed modes. Thus, these stars can serve as benchm…

astro-ph.SR2017★ 100 cited

Variability Properties of 4 Million Sources in the Input Catalog Observed with the Kilodegree Extremely Little Telescope Survey

Ryan J. Oelkers, Joseph E. Rodriguez, Keivan G. Stassun +10

The Kilodegree Extremely Little Telescope (KELT) has been surveying more than of the celestial sphere for nearly a decade. While the primary science goal of the survey is th…

astro-ph.SR2017★ 20 cited

Identification of Young Stellar Variables with KELT for K2 II: The Upper Scorpius Association

Megan Ansdell, Ryan J. Oelkers, Joseph E. Rodriguez +13

High-precision photometry from space-based missions such as K2 and TESS enables detailed studies of young star variability. However, because space-based observing campaigns are oft…

astro-ph.SR2017★ 38 cited

Outbursts and Disk Variability in Be Stars

Jonathan Labadie-Bartz, S. Drew Chojnowski, David G. Whelan +16

In order to study the growth and evolution of circumstellar disks around classical Be stars, we analyze optical time-series photometry from the KELT survey with simultaneous infrar…

astro-ph.SR2017★ 23 cited

A Bright Short Period M-M Eclipsing Binary from the KELT Survey: Magnetic Activity and the Mass-Radius Relationship for M-dwarfs

Jack B. Lubin, Joseph E. Rodriguez, George Zhou +26

We report the discovery of KELT J041621-620046, a moderately bright (J10.2) M dwarf eclipsing binary system at a distance of 393 pc. KELT J041621-620046 was first identi…

astro-ph.SR2017★ 45 cited

Identification of Young Stellar Variables with KELT for K2 I: Campaign 13 Taurus Dippers and Rotators

Joseph E. Rodriguez, Megan Ansdell, Ryan J. Oelkers +13

One of the most well-studied young stellar associations, Taurus-Auriga, will be observed by the extended Kepler mission, K2, in the spring of 2017. K2 Campaign 13 (C13) will be a u…

astro-ph.SR2017★ 25 cited

The Mysterious Dimmings of the T Tauri Star V1334 Tau

Joseph E. Rodriguez, George Zhou, Phillip A. Cargile +35

We present the discovery of two extended 0.12 mag dimming events of the weak-lined T-Tauri star V1334. The start of the first event was missed but came to an end in late 2003…

astro-ph.SR2016★ 18 cited

Absolute dimensions of the eccentric eclipsing binary V541 Cygni

G. Torres, C. D. McGruder, R. J. Siverd +6

We report new spectroscopic and photometric observations of the main-sequence, detached, eccentric, double-lined eclipsing binary V541 Cyg (P = 15.34 days, e = 0.468). Using these…

astro-ph.SR2016★ 16 cited

Sonneberg plate photometry for Boyajian's Star in two passbands

Michael Hippke, Peter Kroll, Frank Matthei +10

The F3 main sequence star KIC 8462852 (Boyajian's Star) showed deep (up to 20%) day-long brightness dips of unknown cause during the 4 years of the Kepler mission. A 0.164 mag (16%…

astro-ph.SR2016★ 75 cited

Photometric Variability of the Be Star Population

Jonathan Labadie-Bartz, Joshua Pepper, M. Virginia McSwain +11

Be stars have generally been characterized by the emission lines in their spectra, and especially the time variability of those spectroscopic features. They are known to also exhib…