activity
19992026
most citedEvidence for Accretion: High-Resolution X-ray Spectroscopy of the Classical T Tauri Star TW Hydrae

399 citations · 2.9k across the 79 of their papers we have counts for

collaborators

81 papers

astro-ph.SR2026

A Multiwavelength View of Oph II: Disentangling the Variability of the Multi-Star Component C

Sean J. Gunderson, Walter W. Golay, Jackson Codd +8

We present a multiwavelength analysis of the star Oph C, covering X-ray, optical, near-infrared, and radio observations to test for the presence of interferometrically-detected…

astro-ph.IM2026

X-ray grating spectroscopy as a mission enhancement

Hans Moritz Guenther, Ehud Behar, Joel N. Bregman +27

We propose to add instruments to any potential future X-ray mission with focussing optics that is considered in NASA's ASTRA framework. Such an instrument is a necessity to study A…

astro-ph.IM2026

CIAO: Chandra's Data Analysis System for X-Ray Astronomy and Beyond

Antonella Fruscione, Jonathan McDowell, Douglas Burke +13

The Chandra Interactive Analysis of Observations (CIAO) software, developed by the Chandra X-ray Center, has been the data analysis package for the Chandra X-ray Observatory since…

astro-ph.SR2025

Chandra/HETG and NuSTAR Observations of V750 Ara, a Cas-type Star

David P. Huenemoerder, Sean J. Gunderson, Richard Ignace +6

We present 197 ks HETG and 95 ks NuSTAR spectra of the Cas-type object V750 Ara. The high-resolution X-ray spectra show that the target is similar to other objects of this cla…

astro-ph.SR2025

X-ray Polarimetry of Accreting White Dwarfs: A Case Study of EX Hydrae

Sean J. Gunderson, Swati Ravi, Herman L. Marshall +5

We present the first first X-ray polarization measurements of a white dwarf, the intermediate polar EX Hya. We measured significant polarization only in the 2 -- 3 keV energy band…

astro-ph.SR2025

A Multiwavelength View of Oph I: Resolving the X-ray Source Between A and B

Sean J. Gunderson, Jackson Codd, Walter W. Golay +12

We present a multiwavelength analysis of the central stellar pair of Oph, components A and B. Using recent high-resolution \textit{Chandra X-ray Observatory} observations, we d…