activity
19992025
most citedSpitzer SAGE survey of the Large Magellanic Cloud II: Evolved Stars and Infrared Color Magnitude Diagrams

201 citations · 895 across the 30 of their papers we have counts for

collaborators

46 papers

astro-ph.GA2025

Discovery of a nova super-remnant surrounding the recurrent nova LMCN 1971-08a in the Large Magellanic Cloud

Michael W. Healy-Kalesh, Manami Sasaki, Sean D. Points +6

A nova super-remnant (NSR) is a greatly-extended structure grown by repeated nova eruptions sweeping the surrounding material away from a nova into a dense outer shell and are pred…

astro-ph.HE2025★ 1 cited

Studying the multi-phase interstellar medium in the Large Magellanic Cloud with SRG/eROSITA -- I. Analysis of diffuse X-ray emission

Martin G. F. Mayer, Manami Sasaki, Frank Haberl +9

The Large Magellanic Cloud (LMC), being a nearby and actively star-forming satellite galaxy of the Milky Way, is an ideal site to observe the multi-phase interstellar medium (ISM)…

astro-ph.GA2025

IRAS 16475-4609: A Young Compact HII Region Sculpting Its Molecular Environment

Felipe Navarete, Sean D. Points, Augusto Damineli

We present a near-infrared spectroscopic and imaging analysis of the star-forming region IRAS 16475-4609, based on TripleSpec/SOAR spectroscopy and NEWFIRM/CTIO imaging, complement…

astro-ph.GA2024★ 7 cited

The Dark Energy Camera Magellanic Clouds Emission-Line Survey

Sean D. Points, Knox S. Long, William P. Blair +7

We have used the Dark Energy Camera (DECam) on the CTIO Blanco 4-m telescope to perform a new emission-line survey of the Large Magellanic Cloud (LMC) using narrow-band H-alpha and…

astro-ph.HE2024★ 12 cited

First Study of the Supernova Remnant Population in the Large Magellanic Cloud with eROSITA

Federico Zangrandi, Katharina Jurk, Manami Sasaki +11

The study of the entire population of SNRs in a galaxy helps us to understand the underlying stellar populations, the environments, in which the SNRs are evolving, and the stellar…

astro-ph.SR2023★ 8 cited

All-Sky Faint DA White Dwarf Spectrophotometric Standards for Astrophysical Observatories: The Complete Sample

Tim Axelrod, Abhijit Saha, Thomas Matheson +14

Hot DA white dwarfs have fully radiative pure hydrogen atmospheres that are the least complicated to model. Pulsationally stable, they are fully characterized by their effective te…