A dataset provided by the European Space Agency

Name: Constraining the nature of PMN J1603-4904-is it a gamma-loud young radio galaxyquestionMark
Published: 2014-10-02T00:00:00Z

Proposal ID	072470
Title	Constraining the nature of PMN J1603-4904-is it a gamma-loud young radio galaxy?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724700101
DOI	https://doi.org/10.5270/esa-xhv6l0c
Principal Investigator, PI	Mrs Cornelia Mueller
Abstract	We request a 35ksec XMM observation of the gamma-ray emitting compact symmetricradio source PMNJ1603-4904 as a crucial part of the first simultaneous radio togamma-ray campaign on this object. Constraining the X-ray spectrum of thecompact radio source is needed to properly model the broadband SED, which isessential for understanding the physical nature of this unusual object. TheSwift detection allows no spectral modeling of its very faint X-ray counterpart,hence, precise spectral investigations with XMM are strongly required.PMNJ1603-4904 is one of the few young radio galaxy candidates associated with abright gamma-ray source, thus it plays a key role in investigating theunderlying emission mechanism of newly born active galaxies.
Publications	Redshifted Fe Kalpha line from the unusual gamma-ray source PMN J1603-4904 \|Muller, C., Krauss, F., et al. \| A&A \| 574-117 \| 2015 \| 2015A&A...574A.117M \| http://ui.adsabs.harvard.edu/#abs/2015A&A...574A.117M 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 Investigating source confusion in PMN J1603-4904 \|Krauss, F., Kreter, M., et al. \| A&A \| 610-8 \| 2018 \| 2018A&A...610L...8K \| http://ui.adsabs.harvard.edu/#abs/2018A&A...610L...8K 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 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	2013-09-17T18:16:51Z/2013-09-18T05:56:51Z
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	2014-10-02T00:00:00Z
Keywords	"pmn j1603 4904", "broadband sed", "gamma ray campaign", "precise spectral investigations", "XMM", "xray spectrum", "properly model", "emission mechanism", "pmnj1603 4904", "born active galaxy", "key role", "swift detection allows", "compact radio source", "faint xray counterpart", "spectral modeling", "radiogalaxy candidates", "gamma loud", "radiogalaxy ?."
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mrs Cornelia Mueller, 2014, 'Constraining the nature of PMN J1603-4904-is it a gamma-loud young radio galaxyquestionMark', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xhv6l0c