Discovery of SN 1006 in VHE gamma-rays by H.E.S.S.

M. Naumann-Godó; M. Beilicke; D. Hauser; M. Lemoine-Goumard; M. De Naurois

doi:10.1063/1.3076666

Discovery of SN 1006 in VHE gamma-rays by H.E.S.S.

M. Naumann-Godó
, M. Beilicke
, D. Hauser
, M. Lemoine-Goumard
, M. De Naurois

Ip Paris
Washington University in St. Louis
Max-Planck-Institut für Kernphysik
Landessternwarte Heidelberg
UMR 5797
Universités Paris VI and VII

Résultats de recherche: Contribution à un journal › Article de conférence › Revue par des pairs

4 Citations (Scopus)

Résumé

Recent theoretical predictions of the TeV-luminosity of SN 1006 under various scenarii are only a factor of 2 to 3 below the previously published H.E.S.S. upper limit, thus motivating further in-depth observations of this source. After analysing more than 100 hours of accumulated H.E.S.S. data a signal associated with the remnant of SN 1006 has finally been detected. The measured gamma-ray flux is of order 1% that detected from the Crab Nebula, consistent with the previously established H.E.S.S. upper limit. The new results and morphological comparisons with X-ray data on this source is presented at the conference.

langue originale	Anglais
Pages (de - à)	304-307
Nombre de pages	4
journal	AIP Conference Proceedings
Volume	1085
Les DOIs	https://doi.org/10.1063/1.3076666
état	Publié - 1 janv. 2009
Modification externe	Oui
Evénement	4th International Meeting on High Energy Gamma-Ray Astronomy - Heidelberg, Allemagne Durée: 7 juil. 2008 → 11 juil. 2008

Accès au document

10.1063/1.3076666

Contient cette citation

@article{80e0fa8528d543a0b5b6b3d563d0ed76,

title = "Discovery of SN 1006 in VHE gamma-rays by H.E.S.S.",

abstract = "Recent theoretical predictions of the TeV-luminosity of SN 1006 under various scenarii are only a factor of 2 to 3 below the previously published H.E.S.S. upper limit, thus motivating further in-depth observations of this source. After analysing more than 100 hours of accumulated H.E.S.S. data a signal associated with the remnant of SN 1006 has finally been detected. The measured gamma-ray flux is of order 1\% that detected from the Crab Nebula, consistent with the previously established H.E.S.S. upper limit. The new results and morphological comparisons with X-ray data on this source is presented at the conference.",

keywords = "Gamma rays, Morphology, SN 1006, Supernova remnants",

author = "M. Naumann-God{\'o} and M. Beilicke and D. Hauser and M. Lemoine-Goumard and \{De Naurois\}, M.",

year = "2009",

month = jan,

day = "1",

doi = "10.1063/1.3076666",

language = "English",

volume = "1085",

pages = "304--307",

journal = "AIP Conference Proceedings",

issn = "0094-243X",

publisher = "American Institute of Physics",

note = "4th International Meeting on High Energy Gamma-Ray Astronomy ; Conference date: 07-07-2008 Through 11-07-2008",

}

TY - JOUR

T1 - Discovery of SN 1006 in VHE gamma-rays by H.E.S.S.

AU - Naumann-Godó, M.

AU - Beilicke, M.

AU - Hauser, D.

AU - Lemoine-Goumard, M.

AU - De Naurois, M.

PY - 2009/1/1

Y1 - 2009/1/1

N2 - Recent theoretical predictions of the TeV-luminosity of SN 1006 under various scenarii are only a factor of 2 to 3 below the previously published H.E.S.S. upper limit, thus motivating further in-depth observations of this source. After analysing more than 100 hours of accumulated H.E.S.S. data a signal associated with the remnant of SN 1006 has finally been detected. The measured gamma-ray flux is of order 1% that detected from the Crab Nebula, consistent with the previously established H.E.S.S. upper limit. The new results and morphological comparisons with X-ray data on this source is presented at the conference.

AB - Recent theoretical predictions of the TeV-luminosity of SN 1006 under various scenarii are only a factor of 2 to 3 below the previously published H.E.S.S. upper limit, thus motivating further in-depth observations of this source. After analysing more than 100 hours of accumulated H.E.S.S. data a signal associated with the remnant of SN 1006 has finally been detected. The measured gamma-ray flux is of order 1% that detected from the Crab Nebula, consistent with the previously established H.E.S.S. upper limit. The new results and morphological comparisons with X-ray data on this source is presented at the conference.

KW - Gamma rays

KW - Morphology

KW - SN 1006

KW - Supernova remnants

U2 - 10.1063/1.3076666

DO - 10.1063/1.3076666

M3 - Conference article

AN - SCOPUS:63849085200

SN - 0094-243X

VL - 1085

SP - 304

EP - 307

JO - AIP Conference Proceedings

JF - AIP Conference Proceedings

T2 - 4th International Meeting on High Energy Gamma-Ray Astronomy

Y2 - 7 July 2008 through 11 July 2008

ER -

Discovery of SN 1006 in VHE gamma-rays by H.E.S.S.

Résumé

Accès au document

Empreinte digitale

Contient cette citation