A dataset provided by the European Space Agency

Name: Unveiling the emission processes of the radio-loud NLS1 galaxy PKS2004-447
Published: 2013-11-07T00:00:00Z

Proposal ID	069453
Title	Unveiling the emission processes of the radio-loud NLS1 galaxy PKS2004-447
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0694530101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0694530201
DOI	https://doi.org/10.5270/esa-amsxvin
Principal Investigator, PI	Mrs Annika Kreikenbohm
Abstract	We propose XMM-Newton observations of the radio- and gamma-ray loud narrow lineSeyfert 1 (RL-NLS1) galaxy PKS2004-447 as part of a five-month multiwavelengthmonitoring program. We will pin down the X-ray continuum model with two deepXMM-Newton observations and use monthly Swift ToO observations to monitor theX-ray light curve of the X-Ray spectrum between the two deep exposures. Togetherwith guaranteed simultaneous radio and gamma-ray data from the TANAMI programand Fermi/LAT, these observations will yield a dynamic SED for a key object froma new type of high-energy emitting extragalactic objects. PKS2004-447 is one outof only a handful of gamma-bright RL-NLS1 galaxies and plays a key role in thiselusive sample because it shows intruiging optical, X-ray, and radio properties.
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 Properties of flat-spectrum radio-loud narrow-line Seyfert 1 galaxies \|Foschini, L., Berton, M., et al. \| A&A \| 575-13 \| 2015 \| 2015A&A...575A..13F \| http://ui.adsabs.harvard.edu/#abs/2015A&A...575A..13F Investigating powerful jets in radio-loud narrow-line Seyfert 1s \|Orienti, M., D.Ammando, F., et al. \| MNRAS \| 453-4037 \| 2015 \| 2015MNRAS.453.4037O \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.453.4037O The gamma-ray emitting radio-loud narrow-line Seyfert 1 galaxy PKS 2004-447. I. The X-ray View \|Kreikenbohm, A., Schulz, R., et al. \| A&A \| 585-91 \| 2016 \| 2016A&A...585A..91K \| http://ui.adsabs.harvard.edu/#abs/2016A&A...585A..91K 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 AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda, J., Guainazzi, M., \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S General Physical Properties of Gamma-Ray-emitting Narrow-line Seyfert 1 Galaxies \|Paliya, Vaidehi S., Parker, M. L., et al. \| ApJ \| 872-169 \| 2019 \| 2019ApJ...872..169P \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...872..169P 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 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2012-05-01T05:32:38Z/2012-10-19T08:27:16Z
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	2013-11-07T00:00:00Z
Keywords	"dynamic sed", "tanami program", "XMM-Newton", "xray continuum model", "xmm newton", "gamma ray data", "radio properties", "emission processes", "key role", "elusive sample", "XMM", "p2004 447", "xray spectrum", "intruiging optical", "monthly swift", "deep xmm newton", "key object", "five month multiwavelength", "xray light curve"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mrs Annika Kreikenbohm, 2013, 'Unveiling the emission processes of the radio-loud NLS1 galaxy PKS2004-447', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-amsxvin