activity
20012026
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations · 13.2k across the 70 of their papers we have counts for

collaborators

70 papers

astro-ph.SR2026★ 1 cited

Measuring Rotation Periods in Crowded Star Clusters with TESS: A Proof-of-Concept with NGC 3532

Matthew S. Stafford, Jason L. Curtis, Marcel A. Agüeros

The Transiting Exoplanet Survey Satellite (TESS) has observed nearly the entire sky, producing full-frame images (FFIs) every 30 min (Cycles 12), 10 min (Cycles 34), and now…

astro-ph.SR2025

The Preliminary Mauve Science Programme: Science themes identified for the first year of operations

Mauve Science Collaboration, Marcel Agueros, Don Dixon +22

Mauve is a low-cost small satellite developed and operated by Blue Skies Space Ltd. The payload features a 13 cm telescope connected with a fibre that feeds into a UV-Vis spectrome…

astro-ph.GA2025

Evidence for a Catastrophically Disrupted Open Cluster

Alexis N. Miller, Kyle R. Tregoning, Jeff J. Andrews +5

Of the many discoveries uncovered by the Gaia astrometric mission, some of the most exciting are related to nearby dispersed stellar structures. We analyze one such structure in th…

astro-ph.SR2024

The 100 pc White Dwarf Sample in the SDSS Footprint II. A New Look at the Spectral Evolution of White Dwarfs

Mukremin Kilic, Pierre Bergeron, Simon Blouin +5

We increase the spectroscopic completeness of the 100 pc white dwarf sample in the SDSS footprint with 840 additional spectra. Our spectroscopy is 86% complete for white dwarfs hot…

astro-ph.SR2024

Massive White Dwarfs in the 100 pc Sample: Magnetism, Rotation, Pulsations, and the Merger Fraction

Gracyn Jewett, Mukremin Kilic, Pierre Bergeron +6

We present a detailed model atmosphere analysis of massive white dwarfs with and K in the Montreal White Dwarf Database 100 pc sample and…

astro-ph.SR2024

Lithium, rotation and metallicity in the open cluster M35

D. Cuenda-Muñoz, D. Barrado, M. A. Agüeros +2

Lithium (Li) abundance is an age indicator for G, K, and M stellar types, as its abundance decreases over time for these spectral types. However, despite the observational efforts…