1ES 2344+514 Multi-wavelength stud (MAGIC Collaboration, 2020)

In the present work, we report on the observations of a VHE {gamma}-ray are of 1ES 2344+514 in August 2016, detected by FACT (First G-APD Cherenkov Telescope), and followed up by many instruments, including the MAGIC (Major Atmospheric Gamma Imaging Cherenkov) telescopes, the Fermi-LAT (Large Area Telescope), Swift-XRT and Swift-UVOT, TCS (Telescope Carlos Sanchez), KAIT (Katzman Automatic Imaging Telescope), KVA (Kungliga Vetenskapsakademien), Stella, LX-200, AZT-8, NOT (Nordic Optical Telescope) IAC80 and OVRO (Owens Valley Radio Observatory). We collected a dataset from simultaneous and quasisimultaneous MWL observations of a flaring state. FACT and MAGIC are both IACT devoted to the study of VHE {gamma} rays. It is worth to note that, for this source, the combination of Fermi-LAT and MAGIC data for the first time offers an unprecedented characterisation of the IC peak during a flaring state. Other data underlying this article will be shared on reasonable request to the corresponding authors.

Source http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/MNRAS/496/3912
Related Identifier https://ui.adsabs.harvard.edu/abs/2020MNRAS.496.3912M
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_datacite&identifier=ivo://CDS.VizieR/J/MNRAS/496/3912
Creator MAGIC Collaboration, Acciari V.A., Ansoldi S., et al.
Publisher CDS
Contributor International Virtual Observatory Alliance (IVOA)
Publication Year 2021
Rights public
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Format text/xml+votable
Version 30-Jun-2020
Discipline Galactic and extragalactic Astronomy