A dataset provided by the European Space Agency

Name: Probing the X-ray - TeV connection in the BLLac 1ES 0229+200
Published: 2010-09-08T00:00:00Z

Proposal ID	060421
Title	Probing the X-ray - TeV connection in the BLLac 1ES 0229+200
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604210201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604210301
DOI	https://doi.org/10.5270/esa-vlw5bzn
Principal Investigator, PI	Mrs Sarah Kaufmann
Abstract	Simultaneous observations with the high sensitive telescopes XMM-Newton andH.E.S.S. are an important tool to shed light on the identification of theemission processes and the particle acceleration in the jet of active galacticnuclei. We request two 20ks observations during 2 consecutive XMM-Newtonrevolutions, which will maximize the simultaneous X-ray-TeV coverage, on thehigh energy peaked BL Lac object 1ES 0229+200. This source was detected up to 10TeV and is besides 1ES 1426+428 the only source with z greater than 0.1 that hasbeen measured up to this high energy. Therefore this source is well suited forprobing known emission models and for deriving conclusions about theextragalactic background light.
Publications	Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y 1ES 0229+200: an extreme blazar with a very high minimum Lorentz factor \|Kaufmann, S., Wagner, S. J., et al. \| A&A \| 534-130 \| 2011 \| 2011A&A...534A.130K \| http://ui.adsabs.harvard.edu/#abs/2011A&A...534A.130K The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Hard X-Ray-selected AGNs in Low-mass Galaxies from the NuSTAR Serendipitous Survey \|Chen, C.-T. J., Brandt, W. N., et al. \| ApJ \| 837-48 \| 2017 \| 2017ApJ...837...48C \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...837...48C The NuSTAR Extragalactic Surveys: X-Ray Spectroscopic Analysis of the Bright Hard-band Selected Sample \|Zappacosta, L., Comastri, A., et al. \| ApJ \| 854-33 \| 2018 \| 2018ApJ...854...33Z \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...854...33Z Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Study of X-Ray Intraday Variability of HBL Blazars Based on Observations Obtained with XMM-Newton \|Devanand, P. U., Gupta, Alok C., et al. \| ApJ \| 939-80 \| 2022 \| 2022ApJ...939...80D \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...939...80D From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2009-08-21T00:46:11Z/2009-08-23T08:19:22Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2010-09-08T00:00:00Z
Keywords	"besides 1es 1426", "emission models", "XMM", "xray tev coverage", "xray tev connection", "shed light", "deriving conclusions", "active galactic nuclei", "emission processes", "XMM-Newton", "particle acceleration", "bllac 1es 0229", "extragalactic background light"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mrs Sarah Kaufmann, 2010, 'Probing the X-ray - TeV connection in the BLLac 1ES 0229+200', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-vlw5bzn