SIMBAD references

2009A&A...493..467A - Astronomy and Astrophysics, volume 493467-469 (2009/1-2)

MAGIC observations of PG1553+113 during a multiwavelength campaign in July 2006.

ALBERT J., ALIU E., ANDERHUB H., ANTORANZ P., BAIXERAS C., BARRIO J.A., BARTKO H., BASTIERI D., BECKER J.K., BEDNAREK W., BERDYUGIN A., BERGER K., BIGONGIARI C., BILAND A., BOCK R.K., BORDAS P., BOSCH-RAMON V., BRETZ T., BRITVITCH I., CAMARA M., CARMONA E., CHILINGARIAN A., COMMICHAU S., CONTRERAS J.L., CORTINA J., COSTADO M.T., CURTEF V., DANIELYAN V., DAZZI F., DE ANGELIS A., DELGADO C., DE LOS REYES R., DE LOTTO B., DORNER D., DORO M., ERRANDO M., FAGIOLINI M., FERENC D., FERNANDEZ E., FIRPO R., FONSECA M.V., FONT L., FUCHS M., GALANTE N., GARCIA-LOPEZ R.J., GARCZARCZYK M., GAUG M., GOEBEL F., HAKOBYAN D., HAYASHIDA M., HENGSTEBECK T., HERRERO A., HOEHNE D., HOSE J., HSU C.C., HUBER S., JACON P., JOGLER T., KOSYRA R., KRANICH D., KRITZER R., LAILLE A., LINDFORS E., LOMBARDI S., LONGO F., LOPEZ M., LORENZ E., MAJUMDAR P., MANEVA G., MANNHEIM K., MARIOTTI M., MARTINEZ M., MAZIN D., MERCK C., MEUCCI M., MEYER M., MIRANDA J.M., MIRZOYAN R., MIZOBUCHI S., MORALEJO A., NIETO D., NILSSON K., NINKOVIC J., ONA-WILHELMI E., OTTE N., OYA I., PANNIELLO M., PAOLETTI R., PASANEN M., PASCOLI D., PAUSS F., PEGNA R., PERSIC M., PERUZZO L., PICCIOLI A., PRANDINI E., PUCHADES N., RAYMERS A., RICO J., RHODE W., RICO J., RISSI M., ROBERT A., RUEGAMER S., SAGGION A., SAITO T.Y., SANCHEZ A., SARTORI P., SCALZOTTO V., SCAPIN V., SCHMITT R., SCHWEIZER T., SHAYDUK M., SHINOZAKI K., SHORE S.N., SIDRO N., SILLANPAEAE A., SOBCZYNSKA D., SPANIER F., STAMERRA A., STARK L.S., TAKALO L., TEMNIKOV P., TESCARO D., TESHIMA M., TORRES D.F., TURINI N., VANKOV H., VENTURINI A., VITALE V., WAGNER R.M., WIBIG T., WITTEK W., ZANDANEL F., ZANIN R. and ZAPATERO J.

Abstract (from CDS):

The active galactic nucleus PG1553+113 was observed by the MAGIC telescope in July 2006 during a multiwavelength campaign, in which telescopes in the optical, X-ray, and very high energies participated. Although the MAGIC data were affected by strong atmospheric absorption (calima), they were analyzed after applying a correction. In 8.5h, a signal was detected with a significance of 5.0σ. The integral flux above 150GeV was (2.6±0.9)x10–7ph/s/m. By fitting the differential energy spectrum with a power law, a spectral index of -4.1±0.3 was obtained.

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Journal keyword(s): gamma rays: observations - galaxies: active - galaxies: BL Lacertae objects: individual: PG1553+113

Simbad objects: 1

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