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Naslov Multiband optical variability of a newly discovered 12 blazars sample from 2013-2019 (Article)
Autori Jovanovic Miljana  Damljanovic Goran M  Taris Francois Gupta Alok C Bhatta Gopal 
Info MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, (2023), vol. 522 br. 1, str. 767-791
Projekat Ministry of Science, Technological Development and Innovation of the Republic of Serbia [451-03-47/2023-01/200002, F-187]; Serbian Academy of Sciences and Arts; Institute of Astronomy and Rozhen NAO BAS through the bilateral joint research project Gaia Celestial Reference Frame (CRF); Chinese Academy of Sciences (CAS) President's International Fellowship Initiative (PIFI) [2016VMB073]; Alfred P. Sloan Foundation; U.S. Department of Energy Office of Science; Centre for High-Performance Computing at the University of Utah; Carnegie Institution for Science; Chilean Participation Group; French Participation Group; Harvard-Smithsonian Centre for Astrophysics; Johns Hopkins University; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo; Korean Participation Group; Lawrence Berkeley National Laboratory; Max-Planck-Institut fuer Astrophysik (MPA Garching); Max-Planck-Institut fur Extraterrestrische Physik (MPE); New Mexico State University, New York University; Shanghai Astronomical Observatory, United Kingdom Participation Group; Yale University
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Naslov Multiband optical variability of a newly discovered 12 blazars sample from 2013-2019 (Article)
Autori Jovanovic Miljana  Damljanovic Goran M  Taris Francois Gupta Alok C Bhatta Gopal 
Info MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, (2023), vol. 522 br. 1, str. 767-791
Projekat Ministry of Science, Technological Development and Innovation of the Republic of Serbia [451-03-47/2023-01/200002]; Serbian Academy of Sciences and Arts; Institute of Astronomy; Chinese Academy of Sciences (CAS) President's International Fellowship Initiative (PIFI) [F-187]; Rozhen NAO BAS; Alfred P. Sloan Foundation; U.S. Department of Energy Office of Science; Centre for High-Performance Computing at the University of Utah; Brazilian Participation Group; Carnegie Institution for Science; Carnegie Mellon University; Chilean Participation Group; French Participation Group; Harvard-Smithsonian Centre for Astrophysics; Instituto de Astrofisica de Canarias; Johns Hopkins University; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo; Korean Participation Group; Lawrence Berkeley National Laboratory; Leibniz Institut fuer Astrophysik Potsdam (AIP); Max-Planck-Institut fuer Astronomie (MPIA Heidelberg); Max-Planck-Institut fuer Astrophysik (MPA Garching); Max-Planck-Institut fuer Extraterrestrische Physik (MPE); National Astronomical Observatories of China; New Mexico State University; New York University; University of Notre Dame; Observatario Nacional/MCTI; Ohio State University; Pennsylvania State University; Shanghai Astronomical Observatory; United Kingdom Participation Group; Universidad Nacional Autonoma de Mexico; University of Arizona; University of Colorado Boulder; University of Oxford; University of Portsmouth; University of Utah; University of Virginia; University of Washington; University of Wisconsin; Vanderbilt University; Yale University; [2016VMB073]
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