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20002026
most citedObservation of Gravitational Waves from a Binary Black Hole Merger

14.2k citations

Showing astro-ph.SRShow all

18 papers · 1 filter

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.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★ 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★ 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★ 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.SR2020★ 10 cited

Chemical Compositions of Red Giant Stars from Habitable Zone Planet Finder Spectroscopy

Christopher Sneden, Melike Afsar, Zeynep Bozkurt +15

We have used the Habitable Zone Planet Finder (HPF) to gather high resolution, high signal-to-noise near-infrared spectra of 13 field red horizontal-branch (RHB) stars, one open-cl…

astro-ph.SR2020★ 43 cited

Persistent starspot signals on M dwarfs: multi-wavelength Doppler observations with the Habitable-zone Planet Finder and Keck/HIRES

Paul Robertson, Gudmundur Stefansson, Suvrath Mahadevan +23

Young, rapidly-rotating M dwarfs exhibit prominent starspots, which create quasiperiodic signals in their photometric and Doppler spectroscopic measurements. The periodic Doppler s…

astro-ph.SR2020★ 54 cited

Stellar Characterization of M-dwarfs from the APOGEE Survey: A Calibrator Sample for the M-dwarf Metallicities

Diogo Souto, Katia Cunha, Verne V. Smith +18

We present spectroscopic determinations of the effective temperatures, surface gravities and metallicities for 21 M-dwarfs observed at high-resolution (R 22,500) in the \tex…

astro-ph.SR2018★ 11 cited

44 New & Known M Dwarf Multiples In The SDSS-III/APOGEE M Dwarf Ancillary Science Sample

Jacob Skinner, Kevin R. Covey, Chad F. Bender +28

Binary stars make up a significant portion of all stellar systems. Consequently, an understanding of the bulk properties of binary stars is necessary for a full picture of star for…

astro-ph.SR2018★ 25 cited

A VLBI distance and transverse velocity for PSR B1913+16

A. T. Deller, J. M. Weisberg, D. J. Nice +1

Using the Very Long Baseline Array, we have made astrometric observations of the binary pulsar B1913+16 spanning an 18 month period in 2014 - 2015. From these observations we make…

astro-ph.SR2017★ 16 cited

The Rotation of M Dwarfs Observed by the Apache Point Galactic Evolution Experiment

Steven H. Gilhool, Cullen H. Blake, Ryan C. Terrien +3

We present the results of a spectroscopic analysis of rotational velocities in 714 M dwarf stars observed by the SDSS III Apache Point Galactic Evolution Experiment (APOGEE) survey…

astro-ph.SR2015★ 6 cited

Two radio-emission mechanisms in PSR J0901-4624

C. A. Raithel, R. M. Shannon, S. Johnston +1

We have detected sporadic, bright, short-duration radio pulses from PSR J09014624. These pulses are emitted simultaneously with persistent, periodic emission that dominates the…

astro-ph.SR2014★ 122 cited

The Binary Companion of Young, Relativistic Pulsar J1906+0746

Joeri van Leeuwen, Laura Kasian, Ingrid H. Stairs +13

PSR J1906+0746 is a young pulsar in the relativistic binary with the second-shortest known orbital period, of 3.98 hours. We here present a timing study based on five years of obse…

astro-ph.SR2014★ 129 cited

Limitations in timing precision due to single-pulse shape variability in millisecond pulsars

R. M. Shannon, S. Osłowski, S. Dai +17

High-sensitivity radio-frequency observations of millisecond pulsars usually show stochastic, broadband, pulse-shape variations intrinsic to the pulsar emission process. These vari…

astro-ph.SR2014★ 8 cited

Testing the rotating lighthouse model with the double pulsar system PSR J0737-3039A/B

Zhu-Xing Liang, Yi Liang, Joel M. Weisberg

Each of the two pulsars in the double pulsar PSR J0737-3039A/B system exhibits not only the pulses emanating from itself, but also displays modulations near the pulse period of the…

astro-ph.SR2013★ 8 cited

Radio studies of novae: a current status report and highlights of new results

Nirupam Roy, Laura Chomiuk, Jennifer L. Sokoloski +10

Novae, which are the sudden visual brightening triggered by runaway thermonuclear burning on the surface of an accreting white dwarf, are fairly common and bright events. Despite t…