activity
20022026
most citedThe Apache Point Observatory Galactic Evolution Experiment (APOGEE)

1.8k citations · 14.6k across the 225 of their papers we have counts for

collaborators
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54 papers · 1 filter

astro-ph.SR2025

NEIDSpecMatch: stellar parameter estimation with NEID spectra using an empirical library

Te Han, Paul Robertson, Caleb I. Cañas +16

We introduce NEIDSpecMatch, a tool developed to extract stellar parameters from spectra obtained with the NEID spectrograph. NEIDSpecMatch is based on SpecMatch-Emp and HPFSpecMatc…

astro-ph.SR2025

A Bayesian Approach to Inferring Accretion Signatures in Young Stellar Objects: A Case Study with VIRUS

Lauren Halstead Willett, Joe P. Ninan, Suvrath Mahadevan +3

The mass accretion rates of young stellar objects (YSOs) are key to understanding how stars form, how their circumstellar disks evolve, and even how planets form. We develop a Baye…

astro-ph.SR2024

Frequency Comb Calibrated Laser Heterodyne Radiometry for Precision Radial Velocity Measurements

Ryan K. Cole, Connor Fredrick, Winter Parts +6

Disk-integrated observations of the Sun provide a unique vantage point to explore stellar activity and its effect on measured radial velocities. Here, we report a new approach for…

astro-ph.SR2024

Magnetic Fields in a sample of planet-hosting M dwarf stars from Kepler, K2, and TESS observed by APOGEE

Fábio Wanderley, Katia Cunha, Verne Smith +8

Stellar magnetic fields have a major impact on space weather around exoplanets orbiting low-mass stars. From an analysis of Zeeman-broadened Fe I lines measured in near-infrared SD…

astro-ph.SR2024

Earths within Reach: Evaluation of Strategies for Mitigating Solar Variability using 3.5 years of NEID Sun-as-a-Star Observations

Eric B. Ford, Chad F. Bender, Cullen H. Blake +15

We present the results of Sun-as-a-star observations by the NEID Solar Telescope at WIYN Observatory, spanning January 1, 2021 through June 30, 2024. We identify 117,060 observatio…

astro-ph.SR2024★ 7 cited

Quiet Please: Detrending Radial Velocity Variations from Stellar Activity with a Physically Motivated Spot Model

Jared C. Siegel, Samuel Halverson, Jacob K. Luhn +15

For solar-type stars, spots and their associated magnetic regions induce radial velocity perturbations through the Doppler rotation signal and the suppression of convective blueshi…

astro-ph.SR2024★ 4 cited

Towards characterising rocky worlds: Trends in chemical make-ups of M dwarfs versus GK dwarfs

Haiyang S. Wang, Sascha P. Quanz, Suvrath Mahadevan +1

Elemental abundances of Sun-like stars are crucial for understanding the detailed properties of their planets. However, measuring elemental abundances in M stars is challenging due…

astro-ph.SR2023

Astrometry and Precise Radial Velocities Yield a Complete Orbital Solution for the Nearby Eccentric Brown Dwarf LHS 1610 b

Evan Fitzmaurice, Gudmundur Stefánsson, Robert D. Kavanagh +18

The LHS 1610 system consists of a nearby ( pc) M5 dwarf hosting a candidate brown dwarf companion in a day, eccentric () orbit. We confirm this brown dwa…

astro-ph.SR2023★ 19 cited

Stellar Characterization and Radius Inflation of Hyades M Dwarf Stars From the APOGEE Survey

Fábio Wanderley, Katia Cunha, Diogo Souto +23

We present a spectroscopic analysis of a sample of 48 M dwarf stars () from the Hyades open cluster using high-resolution H-band spectra from the…

astro-ph.SR2023★ 7 cited

TOI-5375 B: A Very Low Mass Star at the Hydrogen-Burning Limit Orbiting an Early M-type Star

Mika Lambert, Chad F. Bender, Shubham Kanodia +16

The TESS mission detected a companion orbiting TIC 71268730, categorized it as a planet candidate, and designated the system TOI-5375. Our follow-up analysis using radial velocity…

astro-ph.SR2023★ 3 cited

Characterization of low-mass companions to objects of interest observed with APOGEE-N

Caleb I. Cañas, Chad F. Bender, Suvrath Mahadevan +12

We report the characterization of 28 low-mass () companions to objects of interest (KOIs), eight…

astro-ph.SR2022★ 2 cited

The SDSS-HET Survey of Kepler Eclipsing Binaries. A Sample of Four Benchmark Binaries

Kelly Hambleton, Andrej Prsa, Scott W. Fleming +2

The purpose of this work is to extend a sample of accurately modeled, benchmark-grade eclipsing binaries with accurately determined masses and radii. We select four "well-behaved"…

astro-ph.SR2022★ 11 cited

Detection of p-mode Oscillations in HD 35833 with NEID and TESS

Arvind F. Gupta, Jacob K. Luhn, Jason T. Wright +15

We report the results of observations of p-mode oscillations in the G0 subgiant star HD 35833 in both radial velocities and photometry with NEID and TESS, respectively. We achieve…

astro-ph.SR2022★ 20 cited

The Active Chromospheres of Lithium-Rich Red Giant Stars

Christopher Sneden, Melike Afsar, Zeynep Bozkurt +17

We have gathered near-infrared -band high resolution spectra of nearly 300 field red giant stars with known lithium abundances in order to survey their \species{He}{i} 1083…

astro-ph.SR2022★ 4 cited

Modeling Stellar Surface Features on Subgiant Star with an M-dwarf Companion

Maria C. Schutte, Leslie Hebb, Simon Lowry +7

Understanding magnetic activity on the surface of stars other than the Sun is important for exoplanet analyses to properly characterize an exoplanet's atmosphere and to further cha…

astro-ph.SR2022

Leveraging space-based data from the nearest Solar-type star to better understand stellar activity signatures in radial velocity data

Tamar Ervin, Samuel Halverson, Abigail Burrows +8

Stellar variability is a key obstacle in reaching the sensitivity required to recover Earth-like exoplanetary signals using the radial velocity (RV) detection method. To explore ac…

astro-ph.SR2022★ 2 cited

Modeling Stellar Oscillations and Granulation in Radial Velocity Time Series: A Fourier-based Method

Zhao Guo, Eric B. Ford, Dennis Stello +4

Tens of thousands of solar-like oscillating stars have been observed by space missions. Their photometric variability in the Fourier domain can be parameterized by a sum of two sup…

astro-ph.SR2022★ 20 cited

Rotational modulation of spectroscopic Zeeman signatures in low-mass stars

Ryan C. Terrien, Allison Keen, Katy Oda +24

Accurate tracers of the stellar magnetic field and rotation are cornerstones for the study of M dwarfs and for reliable detection and characterization of their exoplanetary compani…

astro-ph.SR2022★ 23 cited

An eccentric Brown Dwarf eclipsing an M dwarf

Caleb I. Cañas, Suvrath Mahadevan, Chad F. Bender +16

We report the discovery of a brown dwarf transiting the early M dwarf TOI-2119 on an eccentric orbit () at an orbital period of $7.2008…

astro-ph.SR2022★ 46 cited

Detailed Chemical Abundances for a Benchmark Sample of M Dwarfs from the APOGEE Survey

Diogo Souto, Katia Cunha, Verne V. Smith +16

Individual chemical abundances for fourteen elements (C, O, Na, Mg, Al, Si, K, Ca, Ti, V, Cr, Mn, Fe, and Ni) are derived for a sample of M-dwarfs using high-resolution near-infrar…

astro-ph.SR2021★ 18 cited

Gaia 20eae: A newly discovered episodically accreting young star

Arpan Ghosh, Saurabh Sharma, Joe. P. Ninan +18

The Gaia Alert System issued an alert on 2020 August 28, on Gaia 20eae when its light curve showed a 4.25 magnitude outburst. We present multi-wavelength photometric and spec…

astro-ph.SR2021★ 15 cited

High resolution near-infrared spectroscopy of a flare around the ultracool dwarf vB 10

Shubham Kanodia, Lawrence W. Ramsey, Marissa Maney +20

We present high-resolution observations of a flaring event in the M8 dwarf vB 10 using the near-infrared Habitable zone Planet Finder (HPF) spectrograph on the Hobby Eberly Telesco…

astro-ph.SR2021★ 16 cited

: Distinguishing Planet-induced Doppler Signatures from Granulation with a Synthetic Spectra Generator

Michael L. Palumbo, Eric B. Ford, Jason T. Wright +3

Owing to recent advances in radial-velocity instrumentation and observation techniques, the detection of Earth-mass planets around Sun-like stars may soon be primarily limited by i…

astro-ph.SR2021★ 1 cited

Double-lined spectroscopic binaries in the APOGEE DR16 and DR17 data

Marina Kounkel, Kevin R. Covey, Keivan G. Stassun +25

APOGEE spectra offer 1 km s precision in the measurement of stellar radial velocities (RVs). This holds even when multiple stars are captured in the same spectrum,…