A dataset provided by the European Space Agency

Name: XMM-Newton Observations of Southern Radio Loud AGN
Published: 2013-04-24T00:00:00Z

Proposal ID	067433
Title	XMM-Newton Observations of Southern Radio Loud AGN
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674330201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674330301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674330401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674330501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674330601
DOI	https://doi.org/10.5270/esa-0ga0zuq
Principal Investigator, PI	Prof Joern Wilms
Abstract	We request XMM-Newton observations of five southern radio-loud AGN which arepart of our radio VLBI monitoring campaign TANAMI. Even though all five sourcesare detected with Fermi, apart from ROSAT All Sky Survey data no observations inthe 1-10 keV band exist with any modern X-ray telescope.
Publications	TANAMI blazars in the IceCube>; PeV-neutrino fields \|Krauss F. Kadler M. et al. \| A&A \| 566-7 \| 2014 \| 2014A&A...566L...7K \| http://ui.adsabs.harvard.edu/#abs/2014A&A...566L...7K 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 The TANAMI Multiwavelength Program: Dynamic spectral energy distributions of southern blazars \|Krauss F. Wilms J. et al. \| A&A \| 591-130 \| 2016 \| 2016A&A...591A.130K \| http://ui.adsabs.harvard.edu/#abs/2016A&A...591A.130K Peak of spectral energy distribution plays an important role in intra-day variability of blazars? \|Gupta Alok C. Kalita Nibedita et al. \| MNRAS \| 462-1508 \| 2016 \| 2016MNRAS.462.1508G \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.462.1508G 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 Signature of inverse Compton emission from blazars \|Gaur Haritma Mohan Prashanth et al. \| MNRAS \| 473-3638 \| 2018 \| 2018MNRAS.473.3638G \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.473.3638G 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 Intra-Day Flux Distributions of Blazars Using XMM-Newton Satellite \|Wani Kiran Gaur Haritma \| Univ \| 8-578 \| 2022 \| 2022Univ....8..578W \| http://ui.adsabs.harvard.edu/#abs/2022Univ....8..578W The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2012-02-11T11:27:07Z/2012-04-02T07:03:45Z
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	2013-04-24T00:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "XMM-Newton", "campaign tanami", "sky survey data", "radio vlbi", "xmm newton", "kev band exist", "ROSAT", "modern xray telescope"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Joern Wilms, 2013, 'XMM-Newton Observations of Southern Radio Loud AGN', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0ga0zuq