output
19922026
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations

Showing 2025 · astro-ph.SRShow all

6 papers · 2 filters

astro-ph.SR2025

Discovery of the pre-main-sequence eclipsing binary MML 48

Y. Gómez Maqueo Chew, L. Hebb, H. C. Stempels +12

We present the discovery of the eclipsing binary MML 48, which is a member of Upper Centaurus Lupus, has an associated age of 16 Myr, and is composed of two young, low-mass stars.…

astro-ph.SR2025★ 3 cited

A Large Catalog of DA White Dwarf Characteristics Using SDSS and Gaia Observations

Nicole R. Crumpler, Vedant Chandra, Nadia L. Zakamska +12

We present a catalog of 8545 and 19,257 unique DA white dwarfs observed in SDSS Data Release 19 and previous SDSS data releases, respectively. This is the largest catalog of both s…

astro-ph.SR2025

Rotational Variables: Kepler Versus ASAS-SN

Jack Stethem, Christopher S. Kochanek, Anya Phillips +2

Rotational variables are stars that vary in brightness due to star spots modulated by rotation. They are probes of stellar magnetism, binarity, and evolution. Phillips et al. (2023…

astro-ph.SR2025★ 2 cited

Calibration of Binary Population Synthesis Models Using White Dwarf Binaries from APOGEE, GALEX and Gaia

A. C. Rubio, K. Breivik, C. Badenes +5

The effectiveness and stability of mass transfer in binaries system are crucial in determining its final product. Rapid binary population synthesis (BPS) codes simplify the complex…

astro-ph.SR2025★ 1 cited

ALEXIS: Recreating the X-Ray Emission from the Full Solar Disk as a Linear Combination of Discrete Regions in the Extreme Ultraviolet and Soft X-Rays

Jorge R Padial Doble, Kelly Holley-Bockelmann

Despite a wealth of multi-wavelength, spatially resolved, time-domain solar activity data, an accurate and complete temporo-spatial solar flare census is unavailable, which impedes…

astro-ph.SR2025★ 6 cited

Testing the Rossby Paradigm: Weakened Magnetic Braking in early K-type Stars

Travis S. Metcalfe, Pascal Petit, Jennifer L. van Saders +12

There is an intricate relationship between the organization of large-scale magnetic fields by a stellar dynamo and the rate of angular momentum loss due to magnetized stellar winds…