activity
20032024
most citedModelling the spectral energy distribution of galaxies. III. Attenuation of stellar light in spiral galaxies

211 citations · 696 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2024

La Silla-QUEST RR Lyrae Star Survey II: The Crater II Tidal Streams

P. S. Coppi, R. Zinn, C. Baltay +5

We describe photometry improvements in the La Silla--Quest RR Lyrae star (RRLS) survey that enable it to reach distances from the Sun () kpc. We report the re…

astro-ph.GA2022★ 31 cited

PHANGS-JWST First Results: The 21 m Compact Source Population

Hamid Hassani, Erik Rosolowsky, Adam K. Leroy +24

We use PHANGS-JWST data to identify and classify 1271 compact 21 m sources in four nearby galaxies using MIRI F2100W data. We identify sources using a dendrogram-based algorithm…

astro-ph.GA2022★ 21 cited

The Black Hole-Galaxy Connection: Interplay between Feedback, Obscuration, and Host Galaxy Substructure

Stéphanie Juneau, Andy D. Goulding, Julie Banfield +20

There is growing evidence for physical influence between supermassive black holes and their host galaxies. We present a case study of nearby galaxy NGC 7582, for which we find evid…

astro-ph.EP2017★ 21 cited

PSYM-WIDE: a survey for large-separation planetary-mass companions to late spectral type members of young moving groups

Marie-Eve Naud, Étienne Artigau, René Doyon +5

We present the results of a direct-imaging survey for very large separation (100 au), companions around 95 nearby young K5-L5 stars and brown dwarfs. They are high-likelihood ca…

astro-ph.SR2017★ 73 cited

A new interpretation of the period-luminosity sequences of long-period variables

Michele Trabucchi, Peter R. Wood, Josefina Montalbán +3

Period-luminosity (PL) sequences of long period variables (LPVs) are commonly interpreted as different pulsation modes, but there is disagreement on the modal assignment. Here, we…

astro-ph.SR2015

Capella (alpha Aurigae) revisited: New binary orbit, physical properties, and evolutionary state

Guillermo Torres, Antonio Claret, Kresimir Pavlovski +1

Knowledge of the chemical composition and absolute masses of Capella are key to understanding the evolutionary state of this benchmark binary system comprising two giant stars. Pre…