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The flat spectrum radio quasar (FSRQ) PKS 0208-512 underwent three outbursts at the optical-near-infrared (OIR) wavelengths during 2008-2011. The second OIR outburst did not have a gamma-ray counterpart despite being comparable in…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Ritaban Chatterjee , Krzysztof Nalewajko , Adam D. Myers

We report on multiwavelength target-of-opportunity observations of the blazar PKS 0735+178, located 2.2$^\circ$ away from the best-fit position of the IceCube neutrino event IceCube-211208A detected on December 8, 2021. The source was in a…

High Energy Astrophysical Phenomena · Physics 2023-07-03 A. Acharyya , C. B. Adams , A. Archer , P. Bangale , J. T. Bartkoske , P. Batista , W. Benbow , A. Brill , J. H. Buckley , J. L. Christiansen , A. J. Chromey , M. Errando , A. Falcone , Q. Feng , G. M. Foote , L. Fortson , A. Furniss , G. Gallagher , W. Hanlon , D. Hanna , O. Hervet , C. E. Hinrichs , J. Hoang , J. Holder , T. B. Humensky , W. Jin , P. Kaaret , M. Kertzman , M. Kherlakian , D. Kieda , T. K. Kleiner , N. Korzoun , S. Kumar , M. J. Lang , M. Lundy , G. Maier , C. E McGrath , M. J. Millard , J. Millis , C. L. Mooney , P. Moriarty , R. Mukherjee , S. O'Brien , R. A. Ong , M. Pohl , E. Pueschel , J. Quinn , K. Ragan , P. T. Reynolds , D. Ribeiro , E. Roache , I. Sadeh , A. C. Sadun , L. Saha , M. Santander , G. H. Sembroski , R. Shang , M. Splettstoesser , A. Kaushik Talluri , J. V. Tucci , V. V. Vassiliev , A. Weinstein , D. A. Williams , S. L. Wong , J. Woo , F. Aharonian , J. Aschersleben , M. Backes , V. Barbosa Martins , R. Batzofin , Y. Becherini , D. Berge , K. Bernlohr , B. Bi , M. Bottcher , C. Boisson , J. Bolmont , M. de Bony de Lavergne , J. Borowska , M. Bouyahiaoui , F. Bradascio , M. Breuhaus , R. Brose , F. Brun , B. Bruno , T. Bulik , C. Burger-Scheidlin , S. Caroff , S. Casanova , R. Cecil , J. Celic , M. Cerruti , T. Chand , S. Chandra , A. Chen , J. Chibueze , O. Chibueze , G. Cotter , S. Dai , J. Damascene Mbarubucyeye , A. Djannati-Atai , A. Dmytriiev , V. Doroshenko , S. Einecke , J. -P. Ernenwein , G. Fichet de Clairfontaine , M. Filipovic , G. Fontaine , M. Fussling , S. Funk , S. Gabici , S. Ghafourizadeh , G. Giavitto , D. Glawion , J. F. Glicenstein , P. Goswami , G. Grolleron , L. Haerer , J. A. Hinton , T. L. Holch , M. Holler , D. Horns , M. Jamrozy , F. Jankowsky , V. Joshi , I. Jung-Richardt , E. Kasai , K. Katarzynski , R. Khatoon , B. Khelifi , S. Klepser , W. Kluzniak , K. Kosack , D. Kostunin , R. G. Lang , S. Le Stum , A. Lemiere , J. P. Lenain , F. Leuschner , T. Lohse , A. Luashvili , I. Lypova , J. Mackey , D. Malyshev , V. Marandon , P. Marchegiani , A. Marcowith , G. Marti-Devesa , R. Marx , A. Mitchell , R. Moderski , L. Mohrmann , A. Montanari , E. Moulin , T. Murach , K. Nakashima , J. Niemiec , A. Priyana Noel , P. O'Brien , L. Olivera-Nieto , E. de Ona Wilhelmi , M. Ostrowski , S. Panny , M. Panter , G. Peron , D. A. Prokhorov , G. Puhlhofer , M. Punch , A. Quirrenbach , P. Reichherzer , A. Reimer , O. Reimer , H. Ren , M. Renaud , F. Rieger , B. Rudak , E. Ruiz-Velasco , V. Sahakian , A. Santangelo , M. Sasaki , J. Schafer , F. Schussler , H. M. Schutte , U. Schwanke , J. N. S. Shapopi , A. Specovius , S. Spencer , L. Stawarz , R. Steenkamp , S. Steinmassl , I. Sushch , H. Suzuki , T. Takahashi , T. Tanaka , R. Terrier , C. van Eldik , M. Vecchi , J. Veh , C. Venter , J. Vink , R. White , A. Wierzcholska , Yu Wun Wong , M. Zacharias , D. Zargaryan , A. A. Zdziarski , A. Zech , S. Zouari , N. Zywucka , K. Mori

Aim of this work is a broad-band study with INTEGRAL, Swift and XMM-Newton satellites of a sample of 9 blazars (7 FSRQ and 2 BL Lac) with redshift up to about 4. The spectral analysis has shown clear evidence of a flattening of the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 S. Gianni' , A. De Rosa , L. Bassani , A. Bazzano , A. J. Dean , P. Ubertini

We report on Gemini, NuSTAR and 8-year Fermi observations of the most distant blazar QSO~J0906$+$6930 ($z=5.48$). We construct a broadband spectral energy distribution (SED) and model the SED using a synchro-Compton model. The measurements…

High Energy Astrophysical Phenomena · Physics 2018-04-11 Hongjun An , Roger W. Romani

In this presentation, we report the results of intraday variability in the optical (BVRI bands) and hard X-ray band (3-79 keV) in a number of blazars. In the optical microvariability studies of the blazars S5 0716+714 and BL Lac, we…

High Energy Astrophysical Phenomena · Physics 2022-10-18 Gopal Bhatta

The detection of high-redshift ($z>$3) blazars enables the study of the evolution of the most luminous relativistic jets over cosmic time. More importantly, high-redshift blazars tend to host massive black holes and can be used to constrain…

High Energy Astrophysical Phenomena · Physics 2017-04-25 Large Area Telescope Collaboration

To provide the census of the sources contributing to the X-ray background peak above 10 keV, NuSTAR is performing extragalactic surveys using a three-tier "wedding cake" approach. We present the NuSTAR survey of the COSMOS field, the medium…

We present NuSTAR observations of the bright Seyfert 2 galaxy NGC 2110 obtained in 2012, when the source was at the highest flux level ever observed, and in 2013, when the source was at a more typical flux level. We include archival…

High-redshift blazars are the most powerful extragalactic astrophysical sources ever detected in the high-energy gamma-ray band. In this study, we present a temporal and spectral analysis of the high-redshift blazar B3 1343+451 based on 14…

High Energy Astrophysical Phenomena · Physics 2024-07-08 Fan Wu , Wen Hu , Benzhong Dai

We present the results from the Suzaku observation of the powerful radio-loud quasar RBS315 (z=2.69), for which a previous XMM-Newton observation showed an extremely flat X-ray continuum up to 10 keV (photon index Gamma=1.26) and…

We report the first results of timing and spectral studies of \textit{Nuclear Spectroscopic Telescope Array (NuSTAR)} observations of six TeV emitting high-frequency peaked blazars: 1ES 0347$-$121, 1ES 0414$+$009, RGB J0710$+$591, 1ES…

High Energy Astrophysical Phenomena · Physics 2018-06-06 Ashwani Pandey , Alok C. Gupta , Paul J. Wiita

We present the results of the optical monitoring of 18 southern blazars in the V and R Johnson-Cousins bands. Our main objective is to study the variations in the optical flux and theis relationship with the colour and spectral…

High Energy Astrophysical Phenomena · Physics 2024-11-26 L. Zibecchi , I. Andruchow , E. Ej. Marchesini , S. A. Cellone , J. A. Combi

We present the results of the power spectral density (PSD) analysis for the blazars Mrk\,421 and PKS\,2155$-$304, using good-quality, densely sampled light curves at multiple frequencies, covering 17 decades of the electromagnetic spectrum,…

High Energy Astrophysical Phenomena · Physics 2020-04-22 Arti Goyal

We present the results obtained from a comprehensive timing and spectral study of two high-mass X-ray binary sources using NuSTAR observations. These two sources, IGR J16320-4751 and IGR J16479-4514, were discovered by INTEGRAL and have…

High Energy Astrophysical Phenomena · Physics 2023-06-05 Varun , Gayathri Raman

We present the results from a multiwavelength campaign of the powerful Gamma-ray quasar PKS 1510-089. This campaign commenced with a deep Suzaku observation lasting three days for a total exposure time of 120 ks, and continued with Swift…

The Burst Alert Telescope (BAT) onboard Swift detected bright emission from 15--195 keV from the source SWIFT~J0746.3+2548 (J0746 in the following), identified with the optically-faint (R ~ 19), z=2.979 quasar SDSS J074625.87+244901.2. Here…

Astrophysics · Physics 2009-11-11 Rita M. Sambruna

The regular monitoring of flat-spectrum radio quasars (FSRQs) in $\gamma$-rays by Fermi-LAT since past 12 years indicated six sources who exhibited extreme $\gamma$-ray outbursts crossing daily flux of $10^{-5}$ photons/cm$^{2}$/s. We…

High Energy Astrophysical Phenomena · Physics 2021-04-20 Abhradeep Roy , Sonal R. Patel , Arkadipta Sarkar , Anshu Chatterjee , Varsha R. Chitnis

We present multiwavelength data for twelve blazars observed from 2008-2010 as part of an ongoing optical-infrared photometric monitoring project. Sources were selected to be bright, southern (dec < 20 deg) blazars observed by the Fermi…

High Energy Astrophysical Phenomena · Physics 2015-06-03 E. W. Bonning , C. M. Urry , C. Bailyn , M. Buxton , R. Chatterjee , P. Coppi , G. Fossati , J. Isler , L. Maraschi

The X-ray emission from active galactic nuclei (AGN) is believed to come from a combination of inverse Compton scattering of photons from the accretion disk and reprocessing of the direct X-ray emission by reflection. We present hard (10-80…

High Energy Astrophysical Phenomena · Physics 2023-12-01 Cora A. DeFrancesco , Xinyu Dai , Mark Mitchell , Abderahmen Zoghbi , Christopher W. Morgan
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