activity
20012021
most citedBlazar spectral variability as explained by a twisting inhomogeneous jet

199 citations · 405 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2021★ 4 cited

New Photometry and Spectroscopy of DW Cnc

S. H. Ramirez, O. Segura Montero, R. Michel +1

We present new observations of the cataclysmic variable DW Cancri, after the system recovered from a low state. We performed a power spectrum analysis that reveals a clear signal o…

astro-ph.HE2019★ 30 cited

Investigating the multiwavelength behaviour of the flat spectrum radio quasar CTA 102 during 2013-2017

F. D'Ammando, C. M. Raiteri, M. Villata +94

We present a multiwavelength study of the flat-spectrum radio quasar CTA 102 during 2013-2017. We use radio-to-optical data obtained by the Whole Earth Blazar Telescope, 15 GHz dat…

astro-ph.HE2017★ 199 cited

Blazar spectral variability as explained by a twisting inhomogeneous jet

C. M. Raiteri, M. Villata

Blazar emission is dominated by non-thermal radiation from a relativistic jet pointing toward us, therefore undergoing Doppler beaming. This is responsible for flux enhancement and…

astro-ph.SR2017★ 42 cited

The white dwarf binary pathways survey - II. Radial velocities of 1453 FGK stars with white dwarf companions from LAMOST DR4

A. Rebassa-Mansergas, J. J. Ren, P. Irawati +18

We present the second paper of a series of publications aiming at obtaining a better understanding regarding the nature of type Ia supernovae (SNIa) progenitors by studying a large…

astro-ph.SR2016★ 1 cited

CCD photometry of the Globular Cluster NGC 6093

A. Ruelas-Mayorga, L. J. Sanchez, C. A. Bernal-Herrera +3

In this paper we present photometric CCD observations of the globular cluster NGC 6093 (M80) in filters B, V , R and I. We produce the colour-magnitude diagrams for this object and…

astro-ph.SR2016

ROTSE1 J164341.65+251748.1: a new W UMa-type eclipsing binary

R. Michel, J. Echevarria, T. Cang +2

ROTSE1 J164341.65+251748.1 was photometrically observed in the V band during three epochs with the 0.84-m telescope of the San Pedro Mártir Observatory in Mexico. Based on addition…