Crab pulsar 50-400GeV light curve

DOI

The Crab pulsar is the only astronomical pulsed source detected at very high energy (VHE, E>100GeV) gamma rays. The emission mechanism of VHE pulsation is not yet fully understood, although several theoretical models have been proposed. In order to test new models, we measured the light curve and the spectra of the Crab pulsar with high precision by means of deep observations. We analyzed 135h of selected MAGIC data taken between 2009 and 2013 in stereoscopic mode. In order to discuss the spectral shape in connection with lower energies, 5.5 years of Fermi-LAT data were also analyzed

Identifier
DOI http://doi.org/10.26093/cds/vizier.35659012
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/565/L12
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/565/L12
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/565/L12
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/565/L12
Provenance
Creator Aleksic J.; Saito T.Y.; Zanin R.; Bonnefoy S.; Hirotani K.,Ansoldi S.; Antonelli L.A.; Antoranz P.; Babic A.; Bangale P.,Barres de Almeida U.; Barrio J.A.; Becerra Gonzalez J.; Bednarek W.,Bernardini E.; Biasuzzi B.; Biland A.; Blanch O.; Bonnoli G.; Borracci F.,Bretz T.; Carmona E.; Carosi A.; Colin P.; Colombo E.; Contreras J.L.,Cortina J.; Covino S.; Da Vela P.; Dazzi F.; De Angelis A.; De Caneva G.,De Lotto B.; Delgado Mendez C.; Doert M.; Dominis Prester D.; Dorner D.,Doro M.; Einecke S.; Eisenacher D.; Elsaesser D.; Farina E.; Ferenc D.,Fidalgo D.; Fonseca M.V.; Font L.; Frantzen K.; Fruck C.; Garcia Lopez R.J.,Garczarczyk M.; Garrido Terrats D.; Gaug M.; Godinovic N.,Gonzalez Munoz A.; Gozzini S.R.; Hadasch D.; Hayashida M.; Herrera J.,Herrero A.; Hildebrand D.; Hose J.; Hrupec D.; Idec W.; Kadenius V.,Kellermann H.; Kodani K.; Konno Y.; Krause J.; Kubo H.; Kushida J.,La Barbera A.; Lelas D.; Lewandowska N.; Lindfors E.; Lombardi S.; Lopez M.,Lopez-Coto R.; Lopez-Oramas A.; Lorenz E.; Lozano I.; Makariev M.,Mallot K.; Maneva G.; Mankuzhiyil N.; Mannheim K.; Maraschi L.; Marcote B.,Mariotti M.; Martinez M.; Mazin D.; Menzel U.; Miranda J.M.; Mirzoyan R.,Moralejo A.; Munar-Adrover P.; Nakajima D.; Niedzwiecki A.; Nilsson K.,Nishijima K.; Noda K.; Nowak N.; Orito R.; Overkemping A.; Paiano S.,Palatiello M.; Paneque D.; Paoletti R.; Paredes J.M.; Paredes-Fortuny X.,Partini S.; Persic M.; Prada Moroni P.G.; Prandini E.; Preziuso S.,Puljak I.; Reinthal R.; Rhode W.; Ribo M.; Rico J.; Rodriguez Garcia J.,Rugamer S.; Saggion A.; Saito K.; Satalecka K.; Scalzotto V.; Scapin V.,Schultz C.; Schweizer T.; Shore S.N.; Sillanpaa A.; Sitarek J.; Snidaric I.,Sobczynska D.; Spanier F.; Stamatescu V.; Stamerra A.; Steinbring T.,Storz J.; Strzys M.; Sun S.; Suric T.; Takalo L.; Takami H.; Tavecchio F.,Temnikov P.; Terzic T.; Tescaro D.; Teshima M.; Thaele J.; Tibolla O.,Torres D.F.; Toyama T.; Treves A.; Uellenbeck M.; Vogler P.; Wagner R.M.
Publisher CDS
Publication Year 2014
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysical Processes; Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy