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Title: MAGIC gamma-ray and multi-frequency observations of flat spectrum radio quasar PKS 1510-089 in early 2012

Journal Article · · Astronomy and Astrophysics
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Aims. We report amongst more than fifty blazars detected in very high energy (VHE, E> 100 GeV) γ rays, only three belong to the subclass of flat spectrum radio quasars (FSRQs). The detection of FSRQs in the VHE range is challenging, mainly because of their soft spectra in the GeV-TeV regime. MAGIC observed PKS 1510-089 (z = 0.36) starting 2012 February 3 until April 3 during a high activity state in the high energy (HE, E> 100 MeV) γ-ray band observed by AGILE and Fermi. MAGIC observations result in the detection of a source with significance of 6.0 standard deviations (σ). We study the multi-frequency behaviour of the source at the epoch of MAGIC observation, collecting quasi-simultaneous data at radio and optical (GASP-WEBT and F-Gamma collaborations, REM, Steward, Perkins, Liverpool, OVRO, and VLBA telescopes), X-ray (Swift satellite), and HE γ-ray frequencies. Methods. We study the VHE γ-ray emission, together with the multi-frequency light curves, 43 GHz radio maps, and spectral energy distribution (SED) of the source. The quasi-simultaneous multi-frequency SED from the millimetre radio band to VHE γ rays is modelled with a one-zone inverse Compton model. We study two different origins of the seed photons for the inverse Compton scattering, namely the infrared torus and a slow sheath surrounding the jet around the Very Long Baseline Array (VLBA) core. Results. We find that the VHE γ-ray emission detected from PKS 1510-089 in 2012 February-April agrees with the previous VHE observations of the source from 2009 March-April. We find no statistically significant variability during the MAGIC observations on daily, weekly, or monthly time scales, while the other two known VHE FSRQs (3C 279 and PKS 1222+216) have shown daily scale to sub-hour variability. The γ-ray SED combining AGILE, Fermi and MAGIC data joins smoothly and shows no hint of a break. The multi-frequency light curves suggest a common origin for the millimetre radio and HE γ-ray emission, and the HE γ-ray flaring starts when the new component is ejected from the 43 GHz VLBA core and the studied SED models fit the data well. However, the fast HE γ-ray variability requires that within the modelled large emitting region, more compact regions must exist. Lastly, we suggest that these observed signatures would be most naturally explained by a turbulent plasma flowing at a relativistic speed down the jet and crossing a standing conical shock.

Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Contributing Organization:
MAGIC Collaboration; AGILE Collaboration; Fermi-LAT Collaboration
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1356441
Journal Information:
Astronomy and Astrophysics, Vol. 569; ISSN 0004-6361
Publisher:
EDP SciencesCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 67 works
Citation information provided by
Web of Science

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Cited By (39)

Polarization angle swings in blazars: The case of 3C 279 journal April 2016
Detection of very high energy gamma-ray emission from the gravitationally lensed blazar QSO B0218+357 with the MAGIC telescopes journal November 2016
Multiwavelength observations of a VHE gamma-ray flare from PKS 1510−089 in 2015 journal July 2017
Luminous and high-frequency peaked blazars: the origin of the γ -ray emission from PKS 1424+240 journal October 2017
Detection of the blazar S4 0954+65 at very-high-energy with the MAGIC telescopes during an exceptionally high optical state journal September 2018
Detection of persistent VHE gamma-ray emission from PKS 1510–089 by the MAGIC telescopes during low states between 2012 and 2017 journal November 2018
Long-term optical monitoring of TeV emitting blazars: I. Data analysis⋆ journal December 2018
A fast, very-high-energy γ -ray flare from BL Lacertae during a period of multi-wavelength activity in June 2015 journal March 2019
The most powerful flaring activity from the NLSy1 PMN J0948+0022 journal November 2014
FBQS J1644+2619: multiwavelength properties and its place in the class of γ-ray emitting Narrow Line Seyfert 1s journal January 2018
Multifrequency study of the gamma-ray flaring BL Lacertae object PKS 2233–148 in 2009–2012 journal November 2018
On the origin of gamma-rays in Fermi blazars: beyondthe broad-line region journal May 2018
Jet kinematics of the quasar 4C+21.35 from observations with the KaVA very long baseline interferometry array journal April 2019
Multiwavelength Picture of the Blazar S5 0716+714 during Its Brightest Outburst journal November 2016
Blazar Optical Polarimetry: Current Progress in Observations and Theories journal October 2019
Relativistic Jets in Gamma-Ray-Emitting Narrow-Line Seyfert 1 Galaxies journal November 2019
Kinematics of Parsec-scale Jets of Gamma-Ray Blazars at 43 GHz within the VLBA-BU-BLAZAR Program journal September 2017
Blazar Spectra with Hard-sphere-like Acceleration of Electrons journal June 2018
On the Multiwavelength Emission from CTA 102 journal August 2018
Characterizing the Gamma-Ray Variability of the Brightest Flat Spectrum Radio Quasars Observed with the Fermi LAT journal May 2019
Ejection of Double Knots from the Radio Core of PKS 1510–089 during the Strong Gamma-Ray Flares in 2015 journal May 2019
Two-zone Emission Modeling of PKS 1510-089 during the High State of 2015 journal September 2019
Multiwavelength picture of the blazar S5 0716+714 during its brightest outburst text January 2016
The most powerful flaring activity from the NLSy1 PMN J0948+0022 text January 2015
Detection of very high energy gamma-ray emission from the gravitationally lensed blazar QSO B0218+357 with the MAGIC telescopes text January 2016
Detection of persistent VHE gamma-ray emission from PKS 1510-089 by the MAGIC telescopes during low states between 2012 and 2017 text January 2018
Multiwavelength Picture of the Blazar S5 0716+714 during Its Brightest Outburst text January 2016
Multiwavelength observations of a VHE gamma-ray flare from PKS 1510-089 in 2015 text January 2016
Luminous and high-frequency peaked blazars: the origin of the $\gamma$-ray emission from PKS 1424+240 text January 2017
Detection of the blazar S4 0954+65 at very-high-energy with the MAGIC telescopes during an exceptionally high optical state text January 2018
Multiwavelength observations of a VHE gamma-ray flare from PKS 1510−089 in 2015 text January 2017
Polarization angle swings in blazars: The case of 3C 279 text January 2016
Multiwavelength observations of a VHE gamma-ray flare from PKS 1510-089 in 2015 text January 2016
Multiwavelength picture of the blazar S5 0716+714 during its brightest outburst text January 2017
FBQS J1644+2619: multiwavelength properties and its place in the class of gamma-ray emitting Narrow Line Seyfert 1s text January 2018
On the origin of gamma rays in Fermi blazars: beyond the broad line region text January 2018
On the multi-wavelength Emission from CTA 102 text January 2018
Multi-frequency study of the gamma-ray flaring BL Lac object PKS 2233-148 in 2009-2012 text January 2018
Ejection of Double knots from the radio core of PKS 1510--089 during the strong gamma-ray flares in 2015 text January 2019

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