Introduction to high-energy gamma-ray astronomy

Bernard Degrange; Gérard Fontaine

doi:10.1016/j.crhy.2015.07.003

Introduction to high-energy gamma-ray astronomy
[Introduction à l'astronomie gamma de haute énergie]

Bernard Degrange ¹ ; Gérard Fontaine ¹

¹ Laboratoire Leprince-Ringuet, École polytechnique, CNRS/IN2P3, Université Paris-Saclay, 91128 Palaiseau cedex, France

Comptes Rendus. Physique, Volume 16 (2015) no. 6-7, pp. 587-599.

Résumé
Abstract

Le présent numéro est le premier de deux volumes consacrés à l'astronomie gamma de haute énergie au-dessus de 100 MeV, qui a considérablement progressé au cours des vingt dernières années. Cet article expose les motivations à la base de cette recherche, présente les articles de ces deux fascicules et fournit une brève introduction historique au domaine.

The present issue is the first of a two-volume review devoted to gamma-ray astronomy above 100 MeV, which has witnessed considerable progress over the last 20 years. The motivations for research in this area are explained, the follow-on articles of these two issues are introduced and a brief history of the field is given.

Publié le : 2015-08-01

DOI : 10.1016/j.crhy.2015.07.003

Keywords: Cosmic rays, Non-thermal radiation, High-energy gamma rays, Space-borne detectors, Ground-based detectors
Mot clés : Rayons cosmiques, Rayonnement non thermique, Rayons gamma de haute énergie, Détecteurs en satellite, Détecteurs au sol

Affiliations des auteurs :

Bernard Degrange ¹ ; Gérard Fontaine ¹

¹ Laboratoire Leprince-Ringuet, École polytechnique, CNRS/IN2P3, Université Paris-Saclay, 91128 Palaiseau cedex, France

@article{CRPHYS_2015__16_6-7_587_0,
     author = {Bernard Degrange and G\'erard Fontaine},
     title = {Introduction to high-energy gamma-ray astronomy},
     journal = {Comptes Rendus. Physique},
     pages = {587--599},
     publisher = {Elsevier},
     volume = {16},
     number = {6-7},
     year = {2015},
     doi = {10.1016/j.crhy.2015.07.003},
     language = {en},
}

TY  - JOUR
AU  - Bernard Degrange
AU  - Gérard Fontaine
TI  - Introduction to high-energy gamma-ray astronomy
JO  - Comptes Rendus. Physique
PY  - 2015
SP  - 587
EP  - 599
VL  - 16
IS  - 6-7
PB  - Elsevier
DO  - 10.1016/j.crhy.2015.07.003
LA  - en
ID  - CRPHYS_2015__16_6-7_587_0
ER  -

%0 Journal Article
%A Bernard Degrange
%A Gérard Fontaine
%T Introduction to high-energy gamma-ray astronomy
%J Comptes Rendus. Physique
%D 2015
%P 587-599
%V 16
%N 6-7
%I Elsevier
%R 10.1016/j.crhy.2015.07.003
%G en
%F CRPHYS_2015__16_6-7_587_0

Bernard Degrange; Gérard Fontaine. Introduction to high-energy gamma-ray astronomy. Comptes Rendus. Physique, Volume 16 (2015) no. 6-7, pp. 587-599. doi : 10.1016/j.crhy.2015.07.003. https://comptes-rendus.academie-sciences.fr/physique/articles/10.1016/j.crhy.2015.07.003/

Bibliographie
Cité par

[1] V. Hess Phys. Z., 13 (1912), pp. 1084-1091

[2] M.S. Longair, Cambridge University Press, Cambridge, UK (2011), pp. 493-496

[3] A. Aab et al. Astrophys. J., 794 (2014), p. 172

[4] A. Abdo et al. Astrophys. J., 708 (2010), p. 1254

[5] F. Aharonian et al. Astrophys. J., 696 (2009)

[6] M. Lemoine; G. Pelletier C. R. Physique, 16 (2015), pp. 628-640 ( in this issue )

[7] A. Abramowski; et al.; HESS collaboration Science, 347 (2015) no. 6220, p. 406

[8] I.A. Grenier; A.K. Harding C. R. Physique, 16 (2015), pp. 641-660 ( in this issue )

[9] J.W. Hewitt; M. Lemoine-Goumard C. R. Physique, 16 (2015), pp. 674-685 ( in this issue )

[10] G. Dubus C. R. Physique, 16 (2015), pp. 661-673 ( in this issue )

[11] M. Su; C. van Eldik C. R. Physique, 16 (2015), pp. 686-703 ( in this issue )

[12] S. Ohm, to be published in a forthcoming dossier of C. R. Physique, continuation of the present one, 2016.

[13] C. Dermer, B. Giebels, to be published in a forthcoming dossier of C. R. Physique, continuation of the present one, 2016.

[14] F. Piron, to be published in a forthcoming dossier of C. R. Physique, continuation of the present one, 2016.

[15] D. Horns, A. Jacholkowska, to be published in a forthcoming dossier of C. R. Physique, continuation of the present one, 2016.

[16] G. Bertone; D. Hooper; J. Silk Phys. Rep., 405 (2005), p. 279

[17] F. Halzen; E. Zas; J.M. Mac Gibbon; T.C. Weekes Nature, 353 (1991), p. 807

[18] P. Brun and J. Cohen-Tanugi, to be published in a forthcoming dossier of C. R. Physique, continuation of the present one, 2016.

[19] G. Amelino-Camelia et al. Nature, 395 (1998), p. 525

[20] G. Raffelt; L. Stodolsky Phys. Rev. D, 37 (1988), p. 1237

[21] R. Giacconi; H. Gurski; F. Paolini; B. Rossi; R. Giacconi; H. Gurski; J.R. Waters Nature, 9 (1962), p. 439

[22] B. Degrange; M. Punch C. R. Acad. Sci. Paris, Ser. IV, 2 (2000), p. 189

[23] D.J. Thompson C. R. Physique, 16 (2015), pp. 600-609 ( in this issue )

[24] M. de Naurois; D. Mazin C. R. Physique, 16 (2015), pp. 610-627 ( in this issue )

[25] J. Knödlseder, to be published in a forthcoming dossier of C. R. Physique, continuation of the present one, 2016.

[26] W.L. Kraushaar et al. Astrophys. J., 177 (1972), p. 341

[27] C.E. Fichtel et al. Astrophys. J., 198 (1975), p. 163

[28] B. Swanenburg et al. Astrophys. J. Lett., 243 (1981)

[29] G. Kanbach et al. Space Sci. Rev., 49 (1988), p. 69

[30] R.C. Hartman et al. Astrophys. J. Suppl. Ser., 123 (1999), p. 79

[31] M. Ackermann et al. Astrophys. J., 697 (2009), p. 1071

[32] M. Tavani et al. Astron. Astrophys., 502 (2009), p. 995

[33] P.L. Nolan et al. Astrophys. J. Suppl. Ser., 199 (2012), p. 31

[34] F. Acero et al. Astrophys. J. Suppl. Ser., 218 (2015), p. 23

[35] R.W. Klebesadel; I.B. Strong; R.A. Olson Astrophys. J., 182 (1973)

[36] Y. Kaneko et al. Astrophys. J. Suppl. Ser., 166 (2006), p. 298

[37] J. van Paradijs et al. Nature, 386 (1997), p. 686

[38] N.R. Tanvir et al. Nature, 461 (2009), p. 1254

[39] K. Hurley et al. Nature, 372 (1994), p. 652

[40] C. Meegan et al. Astrophys. J., 702 (2009), p. 791

[41] M. Ackermann et al. Astrophys. J. Suppl. Ser., 209 (2013), p. 11

[42] M. Ackermann et al. Science, 343 (2014), p. 42

[43] P.A. Cherenkov C. R. (Dokl.) Acad. Sci. URSS, 2 (1934), p. 451

[44] I. Frank; I. Tamm C. R. (Dokl.) Acad. Sci. URSS, 14 (1937), p. 109

[45] P.M.S. Blackett Phys. Soc. Gassiot Committee report 34, 1948

[46] W. Galbraith; J.V. Jelley Nature, 171 (1953), pp. 349-350

[47] A.E. Chudakov; N.M. Nesterova Il Nuovo Cimento, 8 (1958) no. Suppl. 2, pp. 606-611

[48] G. Cocconi Moscow (1960), pp. 309-311

[49] G.T. Zatsepin; A.E. Chudakov J. Exp. Theor. Phys., 41 (1961), pp. 655-656

[50] T.C. Weekes Paris (1981), pp. 34-37

[51] A.M. Hillas La Jolla, CA (1985), pp. 445-448

[52] T.C. Weekes et al. Astrophys. J., 342 (1989), pp. 379-395

[53] J.M. Bonnet-Bidaud; G. Chardin Phys. Rep., 170 (1988) no. 6, pp. 325-404

[54] P. Goret et al. Astron. Astrophys., 270 (1993), pp. 401-406

[55] P. Baillon et al. Astropart. Phys., 1 (1993), pp. 341-355

[56] E. Paré et al. Nucl. Instrum. Methods A, 490 (2002), pp. 71-89

[57] M. de Naurois Astrophys. J., 566 (2002), pp. 343-357

[58] D.M. Gingrich et al. IEEE Trans. Nucl. Sci., 52 (2005), pp. 2977-2985

[59] F. Arqueros et al. Astropart. Phys., 17 (2002), pp. 293-318

[60] T. Tümer et al. Astropart. Phys., 11 (1999), pp. 271-273

[61] M. Punch et al. Nature, 358 (1992), pp. 477-478

[62] T. Hara et al. Nucl. Instrum. Methods A, 332 (1993), pp. 300-309

[63] P. Armstrong et al. Exp. Astron., 9 (1999), pp. 51-80

[64] A. Daum et al. Astropart. Phys., 8 (1997), pp. 1-11

[65] A. Barrau et al. Nucl. Instrum. Methods A, 416 (1998), pp. 278-292

[66] S. Le Bohec et al. Nucl. Instrum. Methods A, 416 (1998), pp. 425-437

[67] A. Djannati-Atai et al. Kruger (1997)

[68] H. Kubo et al. New Astron. Rev., 48 (2004), pp. 323-329

[69] C. Stegmann; et al.; J. Bolmont et al. Nucl. Instrum. Methods A, AIP Conf. Proc., vol. 1505 (2012), p. 194-57

[70] J. Aleksic et al. Astropart. Phys., 35 (2012), pp. 435-448

[71] D.B. Kieda et al. Rio de Janeiro (2013) | arXiv

[72] B.S. Acharya et al. Astropart. Phys., 43 (2013), pp. 3-18

[73] A.A. Abdo et al. Nucl. Phys. B, Proc. Suppl., 151 (2006), pp. 101-107

[74] A.U. Abeysekara et al. Astropart. Phys., 50–52 (2013), pp. 26-32

[75] http://tevcat.uchicago.edu (TeVCat database)

[76] D.J. Fegan Nucl. Instrum. Methods A, 662 (2012), p. S2-S11

[77] E. Lorenz; R. Wagner Eur. Phys. J. H, 37 (2012), pp. 459-513

[78] A.M. Hillas Astropart. Phys., 43 (2013), pp. 19-43

Cité par Sources :

Commentaires - Politique

Ces articles pourraient vous intéresser

Ground-based detectors in very-high-energy gamma-ray astronomy

Mathieu de Naurois; Daniel Mazin

C. R. Phys (2015)

The future of gamma-ray astronomy

Jürgen Knödlseder

C. R. Phys (2016)

Active galactic nuclei at gamma-ray energies

Charles Dennison Dermer; Berrie Giebels

C. R. Phys (2016)