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19942025
most citedRelativistic ejecta from XRF 060218 and the rate of cosmic explosions

513 citations · 13k across the 114 of their papers we have counts for

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astro-ph.SR2021★ 44 cited

Carnegie Supernova Project: The First Homogeneous Sample of "Super-Chandrasekhar Mass"/2003fg-like Type Ia Supernova

C. Ashall, J. Lu, E. Y. Hsiao +38

We present a multi-wavelength photometric and spectroscopic analysis of thirteen "Super-Chandrasekhar Mass"/2003fg-like type Ia Supernova (SNe~Ia). Nine of these objects were obser…

astro-ph.SR2020★ 34 cited

The Cluster Ages Experiment (CASE). VIII. Age and Distance of the Globular Cluster 47 Tuc from the Analysis of Two Detached Eclipsing Binaries

I. B. Thompson, A. Udalski, A. Dotter +20

We use photometric and spectroscopic observations of the eclipsing binary E32 in the globular cluster 47 Tuc to derive the masses, radii, and luminosities of the component stars. T…

astro-ph.SR2019★ 27 cited

Chemical Compositions of Field and Globular Cluster RR~Lyrae Stars: II. omega Centauri

D. Magurno, C. Sneden, G. Bono +21

We present a detailed spectroscopic analysis of RR Lyrae (RRL) variables in the globular cluster NGC 5139 (omega Cen). We collected optical (4580-5330 A), high resolution (R = 34,0…

astro-ph.SR2018★ 31 cited

New Near-Infrared light-curve templates for RR Lyrae variables

V. F. Braga, P. B. Stetson, G. Bono +34

We provide homogeneous optical (UBVRI) and near-infrared (JHK) time series photometry for 254 cluster (omega Cen, M4) and field RR Lyrae (RRL) variables. We ended up with more than…

astro-ph.SR2018★ 87 cited

Carnegie Supernova Project-II: The Near-infrared Spectroscopy Program

E. Y. Hsiao, M. M. Phillips, G. H. Marion +42

Shifting the focus of Type Ia supernova (SN Ia) cosmology to the near-infrared (NIR) is a promising way to significantly reduce the systematic errors, as the strategy minimizes our…

astro-ph.SR2018★ 30 cited

Chemical Compositions of Field and Globular Cluster RR Lyrae Stars: I. NGC 3201

D. Magurno, C. Sneden, V. F. Braga +7

We present a detailed spectroscopic analysis of horizontal branch stars in the globular cluster NGC 3201. We collected optical (4580-5330 A), high resolution (~34,000), high signal…