activity
20102023
most citedBlazar spectral variability as explained by a twisting inhomogeneous jet

199 citations · 573 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2023★ 7 cited

Exploring TeV candidates of Fermi blazars through machine learning

J. T. Zhu, C. Lin, H. B. Xiao +3

In this work, we make use of a supervised machine learning algorithm based on Logistic Regression (LR) to select TeV blazar candidates from the 4FGL-DR2 / 4LAC-DR2, 3FHL, 3HSP, and…

astro-ph.IM2022★ 27 cited

A Joint Roman Space Telescope and Rubin Observatory Synthetic Wide-Field Imaging Survey

M. A. Troxel, C. Lin, A. Park +22

We present and validate 20 deg of overlapping synthetic imaging surveys representing the full depth of the Nancy Grace Roman Space Telescope High-Latitude Imaging Survey (HLIS)…

astro-ph.HE2020★ 52 cited

The dual nature of blazar fast variability. Space and ground observations of S5 0716+714

C. M. Raiteri, M. Villata, D. Carosati +39

Blazar S5 0716+714 is well-known for its short-term variability, down to intra-day time-scales. We here present the 2-min cadence optical light curve obtained by the TESS space tel…

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.HE2017★ 48 cited

Intrinsic Correlations for Flaring Blazars Detected by Fermi

J. H. Fan, J. H. Yang, H. B. Xiao +6

Blazars are an extreme subclass of active galactic nuclei. Their rapid variability, luminous brightness, superluminal motion, and high and variable polarization are probably due to…