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MAGIC observations of variable very-high-energy gamma-ray emission from PKS1510-089 during May 2015 outburst. / MAGIC and Fermi-LAT Collaborations.

35th International Cosmic Ray Conference, ICRC 2017. 2017. (Proceedings of Science).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Research › peer-review

Harvard

MAGIC and Fermi-LAT Collaborations 2017, MAGIC observations of variable very-high-energy gamma-ray emission from PKS1510-089 during May 2015 outburst. in 35th International Cosmic Ray Conference, ICRC 2017. Proceedings of Science, 35th International Cosmic Ray Conference, ICRC 2017, Bexco, Busan, Korea, Republic of, 10/07/17.

APA

MAGIC and Fermi-LAT Collaborations (2017). MAGIC observations of variable very-high-energy gamma-ray emission from PKS1510-089 during May 2015 outburst. In 35th International Cosmic Ray Conference, ICRC 2017 (Proceedings of Science).

Vancouver

MAGIC and Fermi-LAT Collaborations. MAGIC observations of variable very-high-energy gamma-ray emission from PKS1510-089 during May 2015 outburst. In 35th International Cosmic Ray Conference, ICRC 2017. 2017. (Proceedings of Science).

Author

MAGIC and Fermi-LAT Collaborations. / MAGIC observations of variable very-high-energy gamma-ray emission from PKS1510-089 during May 2015 outburst. 35th International Cosmic Ray Conference, ICRC 2017. 2017. (Proceedings of Science).

BibTeX

@inproceedings{913747feb7ad4ab3926ea350084ce5ac,
title = "MAGIC observations of variable very-high-energy gamma-ray emission from PKS1510-089 during May 2015 outburst",
abstract = "PKS1510-089 is a flat spectrum radio quasar located at a redshift of 0.36. It is one of only a few such sources detected in very-high-energy (VHE, >100 GeV) gamma rays. Though PKS1510-089 is highly variable at GeV energies, until recently no variability has been observed in the VHE band. In 2015 May PKS1510-089 showed a high state in optical and in the GeV range. A VHE gamma-ray flare was detected with MAGIC at that time, showing the first instance of VHE gamma-ray flux variability on the time scale of days in this source. We will present the MAGIC results from this observation, discuss their temporal and spectral properties in the multi-wavelength context and present modelling of such emission in the external Compton scenario.",
author = "{MAGIC and Fermi-LAT Collaborations} and Julian Sitarek and Gonz{\'a}lez, {Josefa Becerra} and Ramazani, {Vandad Fallah} and Elina Lindfors and Giovanna Pedaletti and Fabrizio Tavecchio and Acosta, {Monica Vazquez} and Stefan Larsson and Kiran Baliyan and Navpreet Kaur and Sameer and Svetlana Jorstad and Claudia Raiteri",
note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives 4.0 International License (CC BY-NC-ND 4.0).; 35th International Cosmic Ray Conference, ICRC 2017 ; Conference date: 10-07-2017 Through 20-07-2017",
year = "2017",
language = "English",
series = "Proceedings of Science",
publisher = "Sissa Medialab Srl",
booktitle = "35th International Cosmic Ray Conference, ICRC 2017",

}

RIS

TY - GEN

T1 - MAGIC observations of variable very-high-energy gamma-ray emission from PKS1510-089 during May 2015 outburst

AU - MAGIC and Fermi-LAT Collaborations

AU - Sitarek, Julian

AU - González, Josefa Becerra

AU - Ramazani, Vandad Fallah

AU - Lindfors, Elina

AU - Pedaletti, Giovanna

AU - Tavecchio, Fabrizio

AU - Acosta, Monica Vazquez

AU - Larsson, Stefan

AU - Baliyan, Kiran

AU - Kaur, Navpreet

AU - Sameer,

AU - Jorstad, Svetlana

AU - Raiteri, Claudia

N1 - Publisher Copyright: © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives 4.0 International License (CC BY-NC-ND 4.0).

PY - 2017

Y1 - 2017

N2 - PKS1510-089 is a flat spectrum radio quasar located at a redshift of 0.36. It is one of only a few such sources detected in very-high-energy (VHE, >100 GeV) gamma rays. Though PKS1510-089 is highly variable at GeV energies, until recently no variability has been observed in the VHE band. In 2015 May PKS1510-089 showed a high state in optical and in the GeV range. A VHE gamma-ray flare was detected with MAGIC at that time, showing the first instance of VHE gamma-ray flux variability on the time scale of days in this source. We will present the MAGIC results from this observation, discuss their temporal and spectral properties in the multi-wavelength context and present modelling of such emission in the external Compton scenario.

AB - PKS1510-089 is a flat spectrum radio quasar located at a redshift of 0.36. It is one of only a few such sources detected in very-high-energy (VHE, >100 GeV) gamma rays. Though PKS1510-089 is highly variable at GeV energies, until recently no variability has been observed in the VHE band. In 2015 May PKS1510-089 showed a high state in optical and in the GeV range. A VHE gamma-ray flare was detected with MAGIC at that time, showing the first instance of VHE gamma-ray flux variability on the time scale of days in this source. We will present the MAGIC results from this observation, discuss their temporal and spectral properties in the multi-wavelength context and present modelling of such emission in the external Compton scenario.

UR - http://www.scopus.com/inward/record.url?scp=85046057223&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:85046057223

T3 - Proceedings of Science

BT - 35th International Cosmic Ray Conference, ICRC 2017

T2 - 35th International Cosmic Ray Conference, ICRC 2017

Y2 - 10 July 2017 through 20 July 2017

ER -

ID: 88427656