About: Sobczyńska, Dorota

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Attributs	Valeurs
type	Person
sameAs	Sobczyńska, Dorota
name	Sobczynska, D.
familyName	Sobczynska Sobczyńska
Given name	D.
is relates of	http://hub.abes.fr/edp/periodical/aa/2012/volume_539/issue_2012/aa18668-11/authorship/134 http://hub.abes.fr/edp/periodical/aa/2014/volume_564/issue_2014/aa22951-13/authorship/132 http://hub.abes.fr/edp/periodical/aa/2015/volume_576/issue_2015/aa24216-14/authorship/132 http://hub.abes.fr/edp/periodical/aa/2010/volume_517/issue_2010/aa13461-09/authorship/132 http://hub.abes.fr/edp/periodical/aa/2011/volume_530/issue_2011/aa16497-11/authorship/122 http://hub.abes.fr/edp/periodical/aa/2012/volume_540/issue_2012/aa18166-11/authorship/130 http://hub.abes.fr/edp/periodical/aa/2012/volume_544/issue_2012/aa17827-11/authorship/130 http://hub.abes.fr/edp/periodical/aa/2014/volume_567/issue_2014/aa23364-14/authorship/135 http://hub.abes.fr/edp/periodical/aa/2014/volume_572/issue_2014/aa24254-14/authorship/133 http://hub.abes.fr/edp/periodical/aa/2014/volume_573/issue_2014/aa22906-13/authorship/132 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is Author of	Discovery of VHE γ-ray emission from the BL Lacertae object B3 2247+381 with the MAGIC telescopes Detection of very-high energy γ-ray emission from NGC 1275 by the MAGIC telescopes Phase-resolved energy spectra of the Crab pulsar in the range of 50-400 GeV measured with the MAGIC telescopes MAGIC observations of the giant radio galaxy M 87 in a low-emission state between 2005 and 2007 Discovery of VHE γ-rays from the blazar 1ES 1215+303 with the MAGIC telescopes and simultaneous multi-wavelength observations MAGIC Observations and multiwavelength properties of the quasar 3C 279 in 2007 and 2009 Observations of the magnetars 4U 0142+61 and 1E 2259+586 with the MAGIC telescopes The simultaneous low state spectral energy distribution of 1ES 2344+514 from radio to very high energies Discovery of TeV γ-ray emission from the pulsar wind nebula 3C 58 by MAGIC MAGIC search for VHE γ-ray emission from AE Aquarii in a multiwavelength context MAGIC observations of MWC 656, the only known Be/BH system MAGIC upper limits to the VHE gamma-ray flux of 3C 454.3 in high emission state Simultaneous multi-frequency observation of the unknown redshift blazar PG 1553+113 in March-April 2008 Search for an extended VHE γ-ray emission from Mrk 421 and Mrk 501 with the MAGIC Telescope Contemporaneous observations of the radio galaxy NGC 1275 from radio to very high energy γ-rays MAGIC long-term study of the distant TeV blazar PKS 1424+240 in a multiwavelength context MAGIC gamma-ray and multi-frequency observations of flat spectrum radio quasar PKS 1510−089 in early 2012 Multiwavelength observations of Mrk 501 in 2008 Very high-energy γ-ray observations of novae and dwarf novae with the MAGIC telescopes Teraelectronvolt pulsed emission from the Crab Pulsar detected by MAGIC MAGIC observations of the February 2014 flare of 1ES 1011+496 and ensuing constraint of the EBL density Mechanism of hadron-nucleus soft collisions in the Geometrical Two-Chain Model Mrk 421 active state in 2008: the MAGIC view, simultaneous multi-wavelength observations and SSC model constrained MAGIC reveals a complex morphology within the unidentified gamma-ray source HESS J1857+026 First broadband characterization and redshift determination of the VHE blazar MAGIC J2001+439 First characterization of the emission behavior of Mrk 421 from radio to very high-energy gamma rays with simultaneous X-ray polarization measurements Insights into the broadband emission of the TeV blazar Mrk 501 during the first X-ray polarization measurements A fast, very-high-energy γ-ray flare from BL Lacertae during a period of multi-wavelength activity in June 2015 Statistics of VHE γ-rays in temporal association with radio giant pulses from the Crab pulsar MAGIC very large zenith angle observations of the Crab Nebula up to 100 TeV Broadband characterisation of the very intense TeV flares of the blazar 1ES 1959+650 in 2016 Testing two-component models on very high-energy gamma-ray-emitting BL Lac objects VHE gamma-ray detection of FSRQ QSO B1420+326 and modeling of its enhanced broadband state in 2020

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