2010ApJ...710..828A

Query : 2010ApJ...710..828A

2010ApJ...710..828A - Astrophys. J., 710, 828-835 (2010/February-2)

Search for very high energy gamma-ray emission from pulsar-pulsar wind nebula systems with the MAGIC telescope.

ANDERHUB H., ANTONELLI L.A., ANTORANZ P., BACKES M., BAIXERAS C., BALESTRA S., BARRIO J.A., BASTIERI D., BECERRA GONZALEZ J., BECKER J.K., BEDNAREK W., BERGER A.K., BERNARDINI E., BILAND A., BOCK R.K., BONNOLI G., BORDAS P., BORLA TRIDON D., BOSCH-RAMON V., BOSE D., BRAUN I., BRETZ T., BRITZGER D., CAMARA M., CARMONA E., CAROSI A., COLIN P., COMMICHAU S., CONTRERAS J.L., CORTINA J., COSTADO M.T., COVINO S., DAZZI F., DE ANGELIS A., DE CEA DEL POZO E., DE LOS REYES R., DE LOTTO B., DE MARIA M., DE SABATA F., DELGADO MENDEZ C., DOMINGUEZ A., DOMINIS PRESTER D., DORNER D., DORO M., ELSAESSER D., ERRANDO M., FERENC D., FERNANDEZ E., FIRPO R., FONSECA M.V., FONT L., GALANTE N., GARCIA LOPEZ R.J., GARCZARCZYK M., GAUG M., GODINOVIC N., GOEBEL F., HADASCH D., HERRERO A., HILDEBRAND D., HOHNE-MONCH D., HOSE J., HRUPEC D., HSU C.C., JOGLER T., KLEPSER S., KRANICH D., LA BARBERA A., LAILLE A., LEONARDO E., LINDFORS E., LOMBARDI S., LONGO F., LOPEZ M., LORENZ E., MAJUMDAR P., MANEVA G., MANKUZHIYIL N., MANNHEIM K., MARASCHI L., MARIOTTI M., MARTINEZ M., MAZIN D., MEUCCI M., MIRANDA J.M., MIRZOYAN R., MIYAMOTO H., MOLDON J., MOLES M., MORALEJO A., NIETO D., NILSSON K., NINKOVIC J., ORITO R., OYA I., PAOLETTI R., PAREDES J.M., PASANEN M., PASCOLI D., PAUSS F., PEGNA R.G., PEREZ-TORRES M.A., PERSIC M., PERUZZO L., PRADA F., PRANDINI E., PUCHADES N., PULJAK I., REICHARDT I., RHODE W., RIBO M., RICO J., RISSI M., ROBERT A., RUGAMER S., SAGGION A., SAITO T.Y., SALVATI M., SANCHEZ-CONDE M., SATALECKA K., SCALZOTTO V., SCAPIN V., SCHWEIZER T., SHAYDUK M., SHORE S.N., SIERPOWSKA-BARTOSIK A., SILLANPAA A., SITAREK J., SOBCZYNSKA D., SPANIER F., SPIRO S., STAMERRA A., STARK L.S., SURIC T., TAKALO L., TAVECCHIO F., TEMNIKOV P., TESCARO D., TESHIMA M., TORRES D.F., TURINI N., VANKOV H., WAGNER R.M., ZABALZA V., ZANDANEL F., ZANIN R., ZAPATERO J. and COGNARD I.

Abstract (from CDS):

The MAGIC collaboration has searched for high-energy gamma-ray emission of some of the most promising pulsar candidates above an energy threshold of 50 GeV, an energy not reachable up to now by other ground-based instruments. Neither pulsed nor steady gamma-ray emission has been observed at energies of 100 GeV from the classical radio pulsars PSR J0205+6449 and PSR J2229+6114 (and their nebulae 3C58 and Boomerang, respectively) and the millisecond pulsar PSR J0218+4232. Here, we present the flux upper limits for these sources and discuss their implications in the context of current model predictions.

Abstract Copyright: ∼

Journal keyword(s): gamma rays: stars - methods: observational - pulsars: individual (PSR J0205+6449, PSR J2229+6114, PSR J0218+4232) - telescopes

Simbad objects: 33

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Number of rows : 33
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 SNR G119.5+10.2 SNR 00 06.6 +72 47           ~ 268 1
2 PSR J0030+0451 Psr 00 30 27.42348 +04 51 39.7144           ~ 596 1
3 PSR J0034-05 Psr 00 34 21.8281 -05 34 36.620           ~ 201 0
4 SNR G130.7+03.1 SNR 02 05 35.73 +64 49 41.3           ~ 661 4
5 PSR J0205+6449 Psr 02 05 37.92 +64 49 42.8           ~ 268 1
6 PSR J0218+42 Psr 02 18 06.3604 +42 32 17.365           ~ 365 2
7 3C 66A BLL 02 22 39.6114771888 +43 02 07.799534304   15.71 15.21 14.5   ~ 942 2
8 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
9 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
10 PSR B0613-02.0 Psr 06 13 43.977070 -02 00 47.34294           ~ 319 1
11 PSR J0633+1746 Psr 06 33 54.153 +17 46 12.91           ~ 1308 0
12 PSR B0656+14 Psr 06 59 48.18800 +14 14 19.2000   24.85 24.90     ~ 943 1
13 PSR J0751+1807 Psr 07 51 09.1539 +18 07 38.335           ~ 316 1
14 NAME Vela SNR 08 34.0 -45 50           ~ 1331 2
15 PSR J1012+5307 Psr 10 12 33.4345449600 +53 07 02.548542576     19.5     DA 419 1
16 PSR J1025-07 Psr 10 24 38.6991893112 -07 19 19.045523388     19.81 18.78 18.00 ~ 286 1
17 NAME Boomerang Nebula pA* 12 44 46.0915042296 -54 31 13.329460776       13.06   ~ 74 0
18 PSR B1257+12 Psr 13 00 03.1075 +12 40 55.155           ~ 546 1
19 PSR B1706-44 Psr 17 09 42.62000 -44 29 12.0000     13.30     ~ 670 1
20 PSR J1740+1000 Psr 17 40 25.91 +10 00 06.0           ~ 110 0
21 PSR J1744-1134 Psr 17 44 29.4220844 -11 34 54.801320           ~ 323 1
22 PSR J1824-2452A Psr 18 24 32.009 -24 52 11.10           ~ 529 2
23 PSR B1823-13 Psr 18 26 13.06 -13 34 48.1           ~ 460 1
24 SNR G021.5-00.9 SNR 18 33 33.612 -10 34 07.69           ~ 490 1
25 PSR J1843-1113 Psr 18 43 41.260405 -11 13 31.10310           ~ 86 0
26 PSR J1846-0258 Psr 18 46 24.75 -02 58 29.6           ~ 388 2
27 PSR J1913+1011 Psr 19 13 20.341 +10 11 22.97           ~ 84 0
28 PSR J1930+1852 Psr 19 30 30.13 +18 52 14.1           ~ 110 1
29 PSR B1937+21.4 Psr 19 39 38.560096 +21 34 59.13552           ~ 1142 0
30 PSR B1951+32 Psr 19 52 58.181 +32 52 40.98           ~ 615 2
31 PSR J1959+2048 Psr 19 59 36.7643141520 +20 48 14.896407996   21.08 20.16 19.53 18.79 G: 854 3
32 NAME Boomerang PWN G106.6+2.9 SNR 22 27 50.9 +61 02 54           ~ 52 1
33 PSR J2229+6114 Psr 22 29 05.262 +61 14 08.48           ~ 252 2

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