activity
20162026
most citedSpectral energy distribution of M-subdwarfs: A study of their atmospheric properties

19 citations · 32 across the 10 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2026

A near-infrared stellar atlas of the Galactic plane from the VVVX survey

Javier Alonso-García, Maren Hempel, Roberto K. Saito +12

The VISTA Variables in the Via Lactea eXtended (VVVX) ESO public survey observed the Galactic plane and the outer Galactic bulge in the near-infrared to mitigate the effects of ext…

astro-ph.GA2026★ 1 cited

Ancient relic moderately metal-rich bulge cluster Tonantzintla 2

Sergio Ortolani, Stefano O. Souza, Domenico Nardiello +6

The assembly history of the Galactic bulge is intimately tied to the formation of the proto-Milky Way, yet reconstructing this early phase is difficult because mergers and secular…

astro-ph.IM2026

Optimal and Unbiased Fluxes from Up-the-Ramp Detectors under Variable Illumination

Bowen Li, Kevin A. McKinnon, Andrew K. Saydjari +6

Near-infrared (NIR) detectors -- which use non-destructive readouts to measure time-series counts-per-pixel -- play a crucial role in modern astrophysics. Standard NIR flux extract…

astro-ph.SR2025★ 1 cited

Exploring stellar activity in a sample of active M dwarfs

A. S. Rajpurohit, V. Kumar, K. Srivastava Mudit +3

Most M dwarfs show higher chromospheric activity, often exceeding solar levels. Characterizing stellar activity is essential, particularly since these stars are prime targets in th…

astro-ph.GA2025

An SDSS-V 3D Tomographic Na I Map of the ISM: An Initial Study Towards the Smith Cloud

Timothy McQuaid, Joseph N. Burchett, Kate H. R. Rubin +7

High velocity clouds supply the Milky Way with gas that sustains star formation over cosmic timescales. Precise distance measurements are therefore essential to quantify their mass…

astro-ph.SR2025★ 2 cited

A nearly pristine star from the Large Magellanic Cloud

Alexander P. Ji, Vedant Chandra, Selenna Mejias-Torres +28

The first stars formed out of pristine gas, causing them to be so massive that none are expected to have survived until today. If their direct descendants were sufficiently low-mas…