TeV γ-ray observations of the young synchrotron-dominated SNRs G1.9+0.3 and G330.2+1.0 with H.E.S.S.

A. Abramowski; F. Aharonian; F. Ait Benkhali; A. G. Akhperjanian; E. Angüner; G. Anton; S. Balenderan; Agnès Balzer; A. Barnacka; Y. Becherini; J. Becker Tjus; K. Bernlöhr; E. Birsin; E. Bissaldi; J. Biteau; M. Böttcher; C. Boisson; J. Bolmont; P. Bordas; J. Brucker; F. Brun; P. Brun; T. Bulik; S. Carrigan; S. Casanova; M. Cerruti; P. M. Chadwick; R. Chalme-Calvet; R. C. G. Chaves; A. Cheesebrough; M. Chrétien; S. Colafrancesco; G. Cologna; J. Conrad; C. Couturier; Y. Cui; M. Dalton; M. K. Daniel; I. D. Davids; B. Degrange; C. Deil; P. Dewilt; H. J. Dickinson; A. Djannati-Ataï; W. Domainko; L. O'C. Drury; G. Dubus; K. Dutson; J. Dyks; M. Dyrda; T. Edwards; K. Egberts; P. Eger; P. Espigat; C. Farnier; S. Fegan; F. Feinstein; M. V. Fernandes; D. Fernandez; A. Fiasson; G. Fontaine; A. Förster; M. Füssling; M. Gajdus; Y. A. Gallant; T. Garrigoux; G. Giavitto; B. Giebels; J. F. Glicenstein; M. -H. Grondin; M. Grudzińska; S. Häffner; J. Hahn; J. Harris; G. Heinzelmann; G. Henri; G. Hermann; O. Hervet; A. Hillert; J. A. Hinton; W. Hofmann; P. Hofverberg; M. Holler; D. Horns; A. Jacholkowska; C. Jahn; M. Jamrozy; M. Janiak; F. Jankowsky; I. Jung; M. A. Kastendieck; K. Katarzyński; U. Katz; S. Kaufmann; B. Khélifi; Michel Kieffer; S. Klepser; D. Klochkov; W. Kluźniak; T. Kneiske; D. Kolitzus; Nu. Komin; K. Kosack; S. Krakau; F. Krayzel; P. P. Krüger; H. Laffon; G. Lamanna; J. Lefaucheur; A. Lemière; M. Lemoine-Goumard; J. -P. Lenain; D. Lennarz; T. Lohse; A. Lopatin; C. -C. Lu; V. Marandon; Alexandre Marcowith; R. Marx; G. Maurin; N. Maxted; M. Mayer; T. J. L. Mccomb; J. Méhault; P. J. Meintjes; U. Menzler; M. Meyer; R. Moderski; M. Mohamed; Emmanuel Moulin; T. Murach; C. L. Naumann; M. de Naurois; J. Niemiec; S. J. Nolan; L. Oakes; S. Ohm; E. de Oña Wilhelmi; B. Opitz; M. Ostrowski; I. Oya; M. Panter; R. D. Parsons; M. Paz Arribas; N. W. Pekeur; G. Pelletier; J. Perez; P. -O. Petrucci; B. Peyaud; S. Pita; H. Poon; G. Pühlhofer; M. Punch; A. Quirrenbach; S. Raab; M. Raue; A. Reimer; O. Reimer; Matthieu Renaud; R. de Los Reyes; F. Rieger; L. Rob; C. Romoli; S. Rosier-Lees; G. Rowell; B. Rudak; C. B. Rulten; V. Sahakian; D. A. Sanchez; A. Santangelo; R. Schlickeiser; F. Schüssler; A. Schulz; U. Schwanke; S. Schwarzburg; S. Schwemmer; H. Sol; G. Spengler; F. Spies; Ł. Stawarz; R. Steenkamp; C. Stegmann; F. Stinzing; K. Stycz; I. Sushch; A. Szostek; J. -P. Tavernet; T. Tavernier; A. M. Taylor; R. Terrier; M. Tluczykont; C. Trichard; K. Valerius; C. van Eldik; B. van Soelen; George Vasileiadis; C. Venter; A. Viana; P. Vincent; H. J. Völk; F. Volpe; M. Vorster; T. Vuillaume; S. J. Wagner; P. Wagner; M. Ward; M. Weidinger; Q. Weitzel; R. White; A. Wierzcholska; P. Willmann; A. Wörnlein; D. Wouters; V. Zabalza; M. Zacharias; A. Zajczyk; A. A. Zdziarski; A. Zech; H. -S. Zechlin

doi:10.1093/mnras/stu459

Journal Articles Monthly Notices of the Royal Astronomical Society Year : 2014

TeV γ-ray observations of the young synchrotron-dominated SNRs G1.9+0.3 and G330.2+1.0 with H.E.S.S.

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A. Abramowski

Function : Author

F. Aharonian

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PersonId : 755280
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F. Ait Benkhali

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A. G. Akhperjanian

Function : Author

E. Angüner

Function : Author

G. Anton

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S. Balenderan

Function : Author

Agnès Balzer

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A. Barnacka

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Y. Becherini

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J. Becker Tjus

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K. Bernlöhr

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E. Birsin

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E. Bissaldi

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J. Biteau

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Laboratoire Leprince-Ringuet

M. Böttcher

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C. Boisson

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Laboratoire Univers et Théories

J. Bolmont

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Laboratoire de Physique Nucléaire et de Hautes Énergies

P. Bordas

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J. Brucker

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F. Brun

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P. Brun

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Institut de Recherches sur les lois Fondamentales de l'Univers

T. Bulik

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S. Carrigan

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S. Casanova

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M. Cerruti

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P. M. Chadwick

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R. Chalme-Calvet

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Laboratoire de Physique Nucléaire et de Hautes Énergies

R. C. G. Chaves

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A. Cheesebrough

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M. Chrétien

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S. Colafrancesco

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G. Cologna

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J. Conrad

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C. Couturier

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Y. Cui

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M. Dalton

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FERMI

M. K. Daniel

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I. D. Davids

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B. Degrange

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C. Deil

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P. Dewilt

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H. J. Dickinson

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A. Djannati-Ataï

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APC - Astrophysique des Hautes Energies

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L. O'C. Drury

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K. Dutson

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J. Dyks

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M. Dyrda

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T. Edwards

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K. Egberts

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P. Eger

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P. Espigat

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AstroParticule et Cosmologie

C. Farnier

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S. Fegan

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F. Feinstein

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A. Fiasson

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G. Fontaine

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A. Förster

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M. Füssling

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M. Gajdus

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Y. A. Gallant

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T. Garrigoux

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J. F. Glicenstein

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M. -H. Grondin

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M. Grudzińska

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S. Häffner

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J. Hahn

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J. Harris

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G. Heinzelmann

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G. Henri

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G. Hermann

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O. Hervet

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J. A. Hinton

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M. Janiak

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D. Klochkov

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W. Kluźniak

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T. Kneiske

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D. Kolitzus

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Nu. Komin

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K. Kosack

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S. Krakau

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F. Krayzel

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P. P. Krüger

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H. Laffon

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G. Lamanna

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J. Lefaucheur

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A. Lemière

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A. Lopatin

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V. Marandon

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N. Maxted

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M. Mayer

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T. J. L. Mccomb

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J. Méhault

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P. J. Meintjes

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U. Menzler

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M. Meyer

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R. Moderski

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M. Mohamed

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Emmanuel Moulin

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M. de Naurois

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J. Niemiec

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G. Pelletier

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J. Perez

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P. -O. Petrucci

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B. Peyaud

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S. Pita

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H. Poon

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Ł. Stawarz

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R. Steenkamp

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C. Stegmann

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F. Stinzing

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T. Tavernier

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A. M. Taylor

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George Vasileiadis

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H. J. Völk

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F. Volpe

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M. Vorster

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T. Vuillaume

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S. J. Wagner

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P. Wagner

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M. Weidinger

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Q. Weitzel

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A. Wörnlein

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D. Wouters

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V. Zabalza

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M. Zacharias

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A. A. Zdziarski

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A. Zech

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Laboratoire Univers et Théories

H. -S. Zechlin

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Abstract

The non-thermal nature of the X-ray emission from the shell-type supernova remnants (SNRs) G1.9+0.3 and G330.2+1.0 is an indication of intense particle acceleration in the shock fronts of both objects. This suggests that the SNRs are prime candidates for very-high-energy (VHE; E $>$ 0.1 TeV) {\gamma}-ray observations. G1.9+0.3, recently established as the youngest known SNR in the Galaxy, also offers a unique opportunity to study the earliest stages of SNR evolution in the VHE domain. The purpose of this work is to probe the level of VHE {\gamma}-ray emission from both SNRs and use this to constrain their physical properties. Observations were conducted with the H.E.S.S. (High Energy Stereoscopic System) Cherenkov telescope array over a more than six-year period spanning 2004-2010. The obtained data have effective livetimes of 67 h for G1.9+0.3 and 16 h for G330.2+1.0. The data are analyzed in the context of the multi-wavelength observations currently available and in the framework of both leptonic and hadronic particle acceleration scenarios. No significant {\gamma}-ray signal from G1.9+0.3 or G330.2+1.0 was detected. Upper limits (99% confidence level) to the TeV flux from G1.9+0.3 and G330.2+1.0 for the assumed spectral index {\Gamma} = 2.5 were set at 5.6 $\times$ 10$^{-13}$ cm$^{-2}$ s$^{-1}$ above 0.26 TeV and 3.2 $\times$ 10$^{-12}$ cm$^{-2}$ s$^{-1}$ above 0.38 TeV, respectively. In a one-zone leptonic scenario, these upper limits imply lower limits on the interior magnetic field to B$_{\mathrm{G1.9}}$ $\gtrsim$ 11 {\mu}G for G1.9+0.3 and to B$_{\mathrm{G330}}$ $\gtrsim$ 8 {\mu}G for G330.2+1.0. In a hadronic scenario, the low ambient densities and the large distances to the SNRs result in very low predicted fluxes, for which the H.E.S.S. upper limits are not constraining.

Domains

Physics [physics] Astrophysics [astro-ph] High Energy Astrophysical Phenomena [astro-ph.HE] Sciences of the Universe [physics] Astrophysics [astro-ph] High Energy Astrophysical Phenomena [astro-ph.HE]

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Submitted on : Tuesday, April 8, 2014-3:43:59 PM

Last modification on : Wednesday, February 1, 2023-6:44:10 PM

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in2p3-00975408 , version 1 (08-04-2014)

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HAL Id : in2p3-00975408 , version 1
ARXIV : 1404.1613
BIBCODE : 2014MNRAS.441..790H
DOI : 10.1093/mnras/stu459

Cite

A. Abramowski, F. Aharonian, F. Ait Benkhali, A. G. Akhperjanian, E. Angüner, et al.. TeV γ-ray observations of the young synchrotron-dominated SNRs G1.9+0.3 and G330.2+1.0 with H.E.S.S.. Monthly Notices of the Royal Astronomical Society, 2014, 441 (1), pp.790-799. ⟨10.1093/mnras/stu459⟩. ⟨in2p3-00975408⟩

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TeV γ-ray observations of the young synchrotron-dominated SNRs G1.9+0.3 and G330.2+1.0 with H.E.S.S.

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