most citedA millisecond pulsar candidate in a 21-hr orbit: 3FGL J0212.1+5320

26 citations · 45 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2025

Detection of -band photometric periodicity in the T8 dwarfs 2MASS J09393548-2448279 and EQ J1959-3338

P. A. Miles-Páez, S. Metchev, M. R. Zapatero Osorio +1

Aims: We aim to study the near-infrared variability of the T8 dwarfs 2MASS J09393548-2448279 and EQ J1959-3338 by analyzing their -band photometric signal, which can provide new…

astro-ph.SR20232 cited

Time-resolved Optical Polarization Monitoring of the Most Variable Brown Dwarf

Elena Manjavacas, Paulo A. Miles-Paez, Theodora Karalidi +3

Recent atmospheric models for brown dwarfs suggest that the existence of clouds in substellar objects is not needed to reproduce their spectra, nor their rotationally-induced photo…

astro-ph.SR202310 cited

The photometric periods of rapidly rotating field ultra-cool dwarfs

Paulo A. Miles-Páez, Stanimir A. Metchev, Benjamin George

We use 1-m class telescopes and the Transiting Exoplanet Survey Satellite (TESS) to explore the photometric variability of all known rapidly rotating ( km\,s$^{-…

astro-ph.EP20239 cited

Polarized Signatures of a Habitable World: Comparing Models of an Exoplanet Earth with Visible and Near-infrared Earthshine Spectra

Kenneth E. Gordon, Theodora Karalidi, Kimberly M. Bott +3

In the JWST, Extremely Large Telescopes, and LUVOIR era, we expect to characterize a number of potentially habitable Earth-like exoplanets. However, the characterization of these w…

astro-ph.SR201619 cited

Optical and near-infrared linear polarization of low and intermediate-gravity ultra-cool dwarfs

P. A. Miles-Páez, M. R. Zapatero Osorio, E. Pallé +1

We aim to study the optical and near-infrared linear polarimetric properties of a sample of young M7-L7 dwarfs (1-500 Myr) with spectroscopic signatures of low- and interm…

astro-ph.HE201626 cited

A millisecond pulsar candidate in a 21-hr orbit: 3FGL J0212.1+5320

Manuel Linares, Paulo Miles-Páez, Pablo Rodríguez-Gil +4

We present the discovery of a variable optical counterpart to the unidentified gamma-ray source 3FGL J0212.1+5320, and argue this is a new compact binary millisecond pulsar (MSP) c…