E-resources
-
Aleksić, J; Antonelli, L. A; Backes, M; Barrio, J. A; Bastieri, D; Becerra González, J; Bednarek, W; Berdyugin, A; Berger, K; Bernardini, E; Blanch, O; Boller, A; Borla Tridon, D; Carmona, E; Carosi, A; Colin, P; Colombo, E; Cortina, J; Cossio, L; Dazzi, F; De Angelis, A; De Cea del Pozo, E; De Lotto, B; Delgado Mendez, C; Doert, M; Domínguez, A; Dominis Prester, D; Dorner, D; Elsaesser, D; Ferenc, D; Font, L; Fruck, C; García López, R. J; Giavitto, G; Godinović, N; Herrero, A; Hildebrand, D; Hose, J; Hrupec, D; Huber, B; Klepser, S; Krause, J; Lelas, D; Leonardo, E; Lindfors, E; Lombardi, S; Makariev, M; Maneva, G; Mankuzhiyil, N; Mannheim, K; Maraschi, L; Mazin, D; Meucci, M; Moralejo, A; Nieto, D; Oya, I; Paneque, D; Pasanen, M; Pauss, F; Perez-Torres, M. A; Pilia, M; Pochon, J; Prada, F; Prada Moroni, P. G; Puljak, I; Rhode, W; Ribó, M; Rico, J; Rügamer, S; Saggion, A; Saito, K; Saito, T. Y; Salvati, M; Satalecka, K; Scalzotto, V; Scapin, V; Schultz, C; Schweizer, T; Shore, S. N; Sitarek, J; Sobczynska, D; Spanier, F; Spiro, S; Stamerra, A; Storz, J; Strah, N; Surić, T; Temnikov, P; Tescaro, D; Teshima, M; Thom, M; Tibolla, O; Treves, A; Vankov, H; Wagner, R. M; Zabalza, V; Zandanel, F; Zanin, R; Wood, D. L; Buson, S
Astrophysical journal. Letters, 03/2011, Volume: 730, Issue: 1Journal Article
Very high energy (VHE) Delta *g-ray emission from the flat spectrum radio quasar (FSRQ) PKS 1222+21 (4C 21.35, z = 0.432) was detected with the MAGIC Cherenkov telescopes during a short observation (~0.5 hr) performed on 2010 June 17. The MAGIC detection coincides with high-energy MeV/GeV Delta *g-ray activity measured by the Large Area Telescope (LAT) on board the Fermi satellite. The VHE spectrum measured by MAGIC extends from about 70 GeV up to at least 400 GeV and can be well described by a power-law dN/dE E -- Delta *G with a photon index Delta *G = 3.75 ? 0.27stat ? 0.2syst. The averaged integral flux above 100 GeV is (4.6 ? 0.5) X 10--10 cm--2 s--1 (~1 Crab Nebula flux). The VHE flux measured by MAGIC varies significantly within the 30 minute exposure implying a flux doubling time of about 10 minutes. The VHE and MeV/GeV spectra, corrected for the absorption by the extragalactic background light (EBL), can be described by a single power law with photon index 2.72 ? 0.34 between 3 GeV and 400 GeV, and is consistent with emission belonging to a single component in the jet. The absence of a spectral cutoff constrains the Delta *g-ray emission region to lie outside the broad-line region, which would otherwise absorb the VHE Delta *g-rays. Together with the detected fast variability, this challenges present emission models from jets in FSRQs. Moreover, the combined Fermi/LAT and MAGIC spectral data yield constraints on the density of the EBL in the UV-optical to near-infrared range that are compatible with recent models.
Author
Shelf entry
Permalink
- URL:
Impact factor
Access to the JCR database is permitted only to users from Slovenia. Your current IP address is not on the list of IP addresses with access permission, and authentication with the relevant AAI accout is required.
Year | Impact factor | Edition | Category | Classification | ||||
---|---|---|---|---|---|---|---|---|
JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
Select the library membership card:
If the library membership card is not in the list,
add a new one.
DRS, in which the journal is indexed
Database name | Field | Year |
---|
Links to authors' personal bibliographies | Links to information on researchers in the SICRIS system |
---|
Source: Personal bibliographies
and: SICRIS
The material is available in full text. If you wish to order the material anyway, click the Continue button.