A dataset provided by the European Space Agency

Name: X-ray study of a double-source-plane gravitational lensing system Eye of Horus
Published: 2019-01-19T23:00:00Z

Proposal ID	080079
Title	X-ray study of a double-source-plane gravitational lensing system Eye of Horus
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800790101
DOI	https://doi.org/10.5270/esa-bcveav8
Principal Investigator, PI	Dr Yuto Ichinohe
Abstract	Double-source-plane (DSP) gravitational lensing systems offer a variety ofcosmological/astrophysical information, although they are rare. We discoveredthe DSP lens Eye of Horus in the Subaru HSC survey Program, and our follow-upspectroscopy makes this system the only DSP lens to date with spectroscopicconfirmation of both source redshifts. Recently, we have found two massiveclusters in the lens plane, likely affecting the lens potential. In order todisentangle the complex environment to exploit this unique system, we propose a40 ksec XMM observation of the system, which will allow us to determineaccurately the clusters. X-ray centroids, potential shapes, and individual gasthermodynamic properties, providing valuable priors for detailed lens modeling.
Publications	X-ray study of the double source plane gravitational lens system Eye of Horus observed with XMM-Newton \|Tanaka, Keigo, Tsuji, Ayumi, et al. \| MNRAS \| 491-3411 \| 2020 \| 2020MNRAS.491.3411T \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.491.3411T 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2018-01-06T06:26:13Z/2018-01-06T19:46:13Z
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	2019-01-19T23:00:00Z
Keywords	"massive cluster", "spectroscopic confirmation", "XMM", "astrophysical information", "xray centroids", "potential shapes", "lens plane", "spectroscopy makes", "valuable priors", "dsp lens", "source redshifts", "lens modeling", "x ray", "dsp lens eye", "lens potential"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Yuto Ichinohe, 2019, 'X-ray study of a double-source-plane gravitational lensing system Eye of Horus', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-bcveav8