Indirect search for dark matter in M 31 with the CELESTE experiment

J. Lavalle; H. Manseri; A. Jacholkowska; E. Brion; R. Britto; P. Bruel; J. Bussons Gordo; D. Dumora; E. Durand; E. Giraud; B. Lott; F. Münz; E. Nuss; F. Piron; T. Reposeur; D. A. Smith

doi:10.1051/0004-6361:20054340

Indirect search for dark matter in M 31 with the CELESTE experiment

J. Lavalle
, H. Manseri
, A. Jacholkowska
, E. Brion
, R. Britto
, P. Bruel
, J. Bussons Gordo
, D. Dumora
, E. Durand
, E. Giraud
, B. Lott
, F. Münz
, E. Nuss
, F. Piron
, T. Reposeur
, D. A. Smith

Laboratoire Univers et Particules de Montpellier
Aix-Marseille Université
Ip Paris
Université Paris-Sud
Collège de France

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

Résumé

Context. If dark matter is made of neutralinos, annihilation of such Majorana particles should produce high energy cosmic rays, especially in galaxy halo high density regions like galaxy centres. Aims. M 31 (Andromeda) is our nearest neighbour spiral galaxy, and both its high mass and its low distance make it a source of interest for the indirect search for dark matter through γ-ray detection. Methods. The ground based atmospheric Cherenkov telescope CELESTE observed M 31 from 2001 to 2003, in the mostly unexplored energy range 50-500 GeV. Results. These observations provide an upper limit on the flux above 50 GeV around 10^-10 cm^-2 s^-1 in the frame of supersymmetric dark matter, and more generally on any gamma emission from M 31.

langue originale	Anglais
Pages (de - à)	1-8
Nombre de pages	8
journal	Astronomy and Astrophysics
Volume	450
Numéro de publication	1
Les DOIs	https://doi.org/10.1051/0004-6361:20054340
état	Publié - 1 janv. 2006

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10.1051/0004-6361:20054340

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@article{3e661549c5334b68bb5b26e3347ea48a,

title = "Indirect search for dark matter in M 31 with the CELESTE experiment",

abstract = "Context. If dark matter is made of neutralinos, annihilation of such Majorana particles should produce high energy cosmic rays, especially in galaxy halo high density regions like galaxy centres. Aims. M 31 (Andromeda) is our nearest neighbour spiral galaxy, and both its high mass and its low distance make it a source of interest for the indirect search for dark matter through γ-ray detection. Methods. The ground based atmospheric Cherenkov telescope CELESTE observed M 31 from 2001 to 2003, in the mostly unexplored energy range 50-500 GeV. Results. These observations provide an upper limit on the flux above 50 GeV around 10-10 cm-2 s-1 in the frame of supersymmetric dark matter, and more generally on any gamma emission from M 31.",

keywords = "Cosmology: dark matter, Galaxies: spiral, Gamma ray: observations",

author = "J. Lavalle and H. Manseri and A. Jacholkowska and E. Brion and R. Britto and P. Bruel and Gordo, \{J. Bussons\} and D. Dumora and E. Durand and E. Giraud and B. Lott and F. M{\"u}nz and E. Nuss and F. Piron and T. Reposeur and Smith, \{D. A.\}",

year = "2006",

month = jan,

day = "1",

doi = "10.1051/0004-6361:20054340",

language = "English",

volume = "450",

pages = "1--8",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

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}

TY - JOUR

T1 - Indirect search for dark matter in M 31 with the CELESTE experiment

AU - Lavalle, J.

AU - Manseri, H.

AU - Jacholkowska, A.

AU - Brion, E.

AU - Britto, R.

AU - Bruel, P.

AU - Gordo, J. Bussons

AU - Dumora, D.

AU - Durand, E.

AU - Giraud, E.

AU - Lott, B.

AU - Münz, F.

AU - Nuss, E.

AU - Piron, F.

AU - Reposeur, T.

AU - Smith, D. A.

PY - 2006/1/1

Y1 - 2006/1/1

N2 - Context. If dark matter is made of neutralinos, annihilation of such Majorana particles should produce high energy cosmic rays, especially in galaxy halo high density regions like galaxy centres. Aims. M 31 (Andromeda) is our nearest neighbour spiral galaxy, and both its high mass and its low distance make it a source of interest for the indirect search for dark matter through γ-ray detection. Methods. The ground based atmospheric Cherenkov telescope CELESTE observed M 31 from 2001 to 2003, in the mostly unexplored energy range 50-500 GeV. Results. These observations provide an upper limit on the flux above 50 GeV around 10-10 cm-2 s-1 in the frame of supersymmetric dark matter, and more generally on any gamma emission from M 31.

AB - Context. If dark matter is made of neutralinos, annihilation of such Majorana particles should produce high energy cosmic rays, especially in galaxy halo high density regions like galaxy centres. Aims. M 31 (Andromeda) is our nearest neighbour spiral galaxy, and both its high mass and its low distance make it a source of interest for the indirect search for dark matter through γ-ray detection. Methods. The ground based atmospheric Cherenkov telescope CELESTE observed M 31 from 2001 to 2003, in the mostly unexplored energy range 50-500 GeV. Results. These observations provide an upper limit on the flux above 50 GeV around 10-10 cm-2 s-1 in the frame of supersymmetric dark matter, and more generally on any gamma emission from M 31.

KW - Cosmology: dark matter

KW - Galaxies: spiral

KW - Gamma ray: observations

U2 - 10.1051/0004-6361:20054340

DO - 10.1051/0004-6361:20054340

M3 - Article

AN - SCOPUS:33645822534

SN - 0004-6361

VL - 450

SP - 1

EP - 8

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 1

ER -

Indirect search for dark matter in M 31 with the CELESTE experiment

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