A dataset provided by the European Space Agency

Name: Explaining the soft X-ray emission in narrow-line radio-loud galaxies
Published: 2020-05-20T22:00:00Z

Proposal ID	082212
Title	Explaining the soft X-ray emission in narrow-line radio-loud galaxies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0822120401
DOI	https://doi.org/10.5270/esa-g0s9518
Principal Investigator, PI	Dr Laura Di Gesu
Abstract	We propose to observe the bright quasar 3C 234 for 240 ks using the RGS as primeinstrument. This observation will provide the first deep high-resolutionspectrum ever obtained of a narrow-line radio-loud AGN. This will allow us toget unprecedented insights on the longstanding debate about the origin of thesoft X-ray emission in radio-loud type 2 AGN.
Publications	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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2019-04-25T21:49:42Z/2019-04-26T22:14:42Z
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	2020-05-20T22:00:00Z
Keywords	"prime instrument", "resolution spectrum", "radio loud type", "soft xray emission"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Laura Di Gesu, 2020, 'Explaining the soft X-ray emission in narrow-line radio-loud galaxies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-g0s9518