OPTICAL SPECTROSCOPIC OBSERVATIONS OF γ-RAY BLAZAR CANDIDATES. I. PRELIMINARY RESULTS
A. Paggi(Istituto Nazionale di Fisica Nucleare, Sezione di Torino), S. Funk(Friedrich-Alexander-Universität Erlangen-Nürnberg), Marco Landoni(Arcetri Astrophysical Observatory), H. Otí-Floranes, M. Giroletti(Istituto di Radioastronomia di Bologna), V. Chavushyan(National Institute of Astrophysics, Optics and Electronics), E. Jiménez‐Bailón(Universidad Nacional Autónoma de México), J. E. Grindlay(Community Farm Alliance), G. Tosti(University of Perugia), N. Masetti(Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna), D. Milisavljević(Harvard University Press), H. A. Smith(Center for Astrophysics Harvard & Smithsonian), Juan Rafael Martínez-Galarza(Center for Astrophysics Harvard & Smithsonian), R. D’Abrusco(Astronomical Observatory of Rome), R. Margutti(Harvard University Press), F. Massaro(Istituto Nazionale di Fisica Nucleare, Sezione di Torino)
Cited by 70
Related Papers
Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi Large Area Telescope Data
|Physical Review Letters|2015|1.1k
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models
|The Astrophysical Journal Letters|2017|1k
The operational environment and rotational acceleration of asteroid (101955) Bennu from OSIRIS-REx observations
|Nature Communications|2019|903
Observations of the Crab nebula with HESS
|Astronomy and Astrophysics|2006|861
An Exceptional Very High Energy Gamma-Ray Flare of PKS 2155-304
|The Astrophysical Journal|2007|824