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20012023
most citedThe Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey

1.5k citations · 11.8k across the 198 of their papers we have counts for

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Showing 2021Show all

11 papers · 1 filter

astro-ph.IM2021★ 5 cited

UV Spectropolarimetry with Polstar: Protoplanetary Disks

John P. Wisniewski, Andrei V. Berdyugin, Svetlana V. Berdyugina +13

Polstar is a proposed NASA MIDEX mission that would feature a high resolution UV spectropolarimeter capable of measure all four Stokes parameters onboard a 60cm telescope. The miss…

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.EP2021★ 10 cited

Multiband imaging of the HD 36546 debris disk: a refined view from SCExAO/CHARIS

Kellen Lawson, Thayne Currie, John P. Wisniewski +21

We present the first multi-wavelength (near-infrared; ) imaging of HD 36546's debris disk, using the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) system co…

astro-ph.IM2021★ 21 cited

Ultraviolet Spectropolarimetry: on the origin of rapidly rotating B stars

C. E. Jones, J. Labadie-Bartz, D. V. Cotton +12

UV spectroscopy and spectropolarimetry hold the key to understanding certain aspects of massive stars that are largely inaccessible with optical or longer wavelength observations.…

astro-ph.EP2021★ 86 cited

The Warm Neptune GJ 3470b has a Polar Orbit

Gudmundur Stefansson, Suvrath Mahadevan, Cristobal Petrovich +34

The warm Neptune GJ 3470b transits a nearby (pc) bright slowly rotating M1.5-dwarf star. Using spectroscopic observations during two transits with the newly commissioned NEID…

astro-ph.SR2021★ 20 cited

Outbursts and stellar properties of the classical Be star HD 6226

Noel D. Richardson, Olivier Thizy, Jon E. Bjorkman +58

The bright and understudied classical Be star HD 6226 has exhibited multiple outbursts in the last several years during which the star grew a viscous decretion disk. We analyze 659…

astro-ph.EP2021★ 4 cited

High-contrast integral field spectropolarimetry of planet-forming disks with SCExAO/CHARIS

Kellen Lawson, Thayne Currie, John P. Wisniewski +10

We describe a new high-contrast imaging capability well suited for studying planet-forming disks: near-infrared (NIR) high-contrast spectropolarimetric imaging with the Subaru Coro…

astro-ph.EP2021★ 1 cited

A Search for Planetary Metastable Helium Absorption in the V1298 Tau System

Shreyas Vissapragada, Guðmundur Stefánsson, Michael Greklek-McKeon +28

Early in their lives, planets endure extreme amounts of ionizing radiation from their host stars. For planets with primordial hydrogen and helium-rich envelopes, this can lead to s…

astro-ph.EP2021★ 25 cited

TOI-532b: The Habitable-zone Planet Finder confirms a Large Super Neptune in the Neptune Desert orbiting a metal-rich M dwarf host

Shubham Kanodia, Gudmundur Stefansson, Caleb I. Canas +30

We confirm the planetary nature of TOI-532b, using a combination of precise near-infrared radial velocities with the Habitable-zone Planet Finder, TESS light curves, ground based p…

astro-ph.SR2021★ 55 cited

New Candidate Extreme T Subdwarfs from the Backyard Worlds: Planet 9 Citizen Science Project

Aaron M. Meisner, Adam C. Schneider, Adam J. Burgasser +29

Schneider et al. (2020) presented the discovery of WISEA J041451.67-585456.7 and WISEA J181006.18-101000.5, which appear to be the first examples of extreme T-type subdwarfs (esdTs…

astro-ph.SR2021★ 7 cited

Variability of Disk Emission in Pre-Main Sequence and related Stars. V. Occultation Events from the innermost disk region of the Herbig Ae Star HD 163296

Monika Pikhartova, Zachary C. Long, Korash D. Assani +8

HD 163296 is a Herbig Ae star that underwent a dramatic 0.8 magnitude drop in brightness in the V photometric band in 2001 and a brightening in the near-IR in 2002. Because t…