activity
20062024
most citedA Spitzer mid-infrared spectral survey of mass-losing carbon stars in the Large Magellanic Cloud

126 citations · 402 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2024★ 42 cited

The Mira Distance to M101 and a 4% Measurement of H0

Caroline D. Huang, Wenlong Yuan, Adam G. Riess +8

The giant spiral galaxy M101 is host to the nearest recent Type Ia Supernova (SN 2011fe) and thus has been extensively monitored in the near-infrared to study the late-time lightcu…

astro-ph.SR2019★ 40 cited

An Infrared Census Of Dust In Nearby Galaxies With Spitzer (DUSTiNGS): V. The Period-luminosity Relation For Dusty Metal-Poor AGB Stars

Steven R. Goldman, Martha L. Boyer, Kristen B. McQuinn +10

The survey for DUST In Nearby Galaxies with Spitzer (DUSTiNGS) has identified hundreds of candidate dust-producing Asymptotic Giant Branch (AGB) stars in several nearby metal-poor…

astro-ph.SR2012★ 36 cited

Characterizing Low-Mass Binaries From Observation of Long Time-scale Caustic-crossing Gravitational Microlensing Events

I. -G. Shin, C. Han, J. -Y. Choi +119

Despite astrophysical importance of binary star systems, detections are limited to those located in small ranges of separations, distances, and masses and thus it is necessary to u…

astro-ph.SR2012★ 39 cited

The Spitzer Spectroscopic Survey of S-type Stars

K. Smolders, P. Neyskens, J. A. D. L. Blommaert +28

S-type AGB stars are thought to be in the transitional phase between M-type and C-type AGB stars. Because of their peculiar chemical composition, one may expect a strong influence…

astro-ph.GA2012★ 38 cited

The Cepheid distance to the Local Group Galaxy NGC 6822

M. W. Feast, P. A. Whitelock, J. W. Menzies +1

Recent estimates of the Cepheid distance modulus of NGC 6822 differ by 0.18 mag. To investigate this we present new multi-epoch JHKs photometry of classical Cepheids in the central…

astro-ph.SR2009★ 3 cited

Period-Luminosity Relation for Type II Cepheids

Noriyuki Matsunaga, Michael W. Feast, John W. Menzies

We have estimated JHKs magnitudes corrected to mean intensity for LMC type II Cepheids found in the OGLE-III survey. Period-luminosity relations (PLRs) are derived in JHKs as well…