activity
20052019
most citedBlazar spectral variability as explained by a twisting inhomogeneous jet

199 citations · 387 across the 8 of their papers we have counts for

collaborators

8 papers

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.SR2019★ 2 cited

Absolute dimensions of the low-mass eclipsing binary system NSVS 10653195

Ramon Iglesias-Marzoa, Maria J. Arevalo, Mercedes Lopez-Morales +3

Low-mass stars in eclipsing binary systems show radii larger and effective temperatures lower than theoretical stellar models predict for isolated stars with the same masses. Eclip…

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.HE2017★ 47 cited

Dissecting the long-term emission behaviour of the BL Lac object Mrk 421

M. I. Carnerero, C. M. Raiteri, M. Villata +4

We report on long-term multi-wavelength monitoring of blazar Mrk 421 by the GASP-WEBT collaboration and Steward Observatory, and by the Swift and Fermi satellites. We study the sou…

astro-ph.EP2009★ 25 cited

Transit timing analysis of CoRoT-1b

Sz. Csizmadia, S. Renner, P. Barge +33

CoRoT, the pioneer space-based transit search, steadily provides thousands of high-precision light curves with continuous time sampling over periods of up to 5 months. The transits…

astro-ph2006★ 8 cited

NSVS01031772: A New 0.50+0.54 Msun Detached Eclipsing Binary

Mercedes Lopez-Morales, Jerome A. Orosz, J. Scott Shaw +4

We report the discovery of a new detached eclipsing binary known as NSVS01031772 with component masses M_1= 0.5428 +/- 0.0027Msun, M_2= 0.4982 +/- 0.0025Msun, and radii R_1= 0.5260…