A dataset provided by the European Space Agency

Name: Joint Chandra/XMM-Newton Observation of NGC1407/1400 complex
Published: 2013-02-04T00:00:00Z

Proposal ID	067960
Title	Joint Chandra/XMM-Newton Observation of NGC1407/1400 complex
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0679600101
DOI	https://doi.org/10.5270/esa-5qs7y7z
Principal Investigator, PI	Ms Yuanyuan Su
Abstract	The nearby dark group centered on NGC 1407 is notable for a nearby bright galaxy(NGC 1400) with a velocity differing by at least 1200 km/s. This large velocitydifference, plus controversy over these two galaxiesa?? respective distances,hasled to a wide range of mass estimates for this group. Our analysis of XMM-Newtondata reveals an extended region of enhanced surface brightness near NGC 1400which may be a cold front. We also find that the hottest regions lie betweenNGC 1400 and 1407, suggesting that their atmospheres are colliding. We propose..text on Chandra cut .. a 30 ks XMM pointing covering the east side of NGC1407 to obtain a complete temperature map as well as a total group mass profile.
Publications	Joint XMM-Newton and Chandra Observations of the NGC 1407/1400 Complex: A Tail of an Early-Type Galaxy and a Tale of a Nearby Merging Group \|Su, Yuanyuan, Gu, Liyi, et al. \| ApJ \| 786-152 \| 2014 \| 2014ApJ...786..152S \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786..152S 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 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	2012-01-15T03:38:51Z/2012-01-15T13:04:05Z
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	2013-02-04T00:00:00Z
Keywords	"ngc 1400", "mass profile", "NGC1407", "XMM-Newton", "enhanced surface brightness", "xmm newton", "ngc 1407", "galaxya ??", "[... text", "chandra cut ...]", "1200 km", "XMM", "complete temperature map", "nearby dark", "1400 complex", "hottest region lie", "wide range", "velocity differing", "respective distances", "cold front"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Ms Yuanyuan Su, 2013, 'Joint Chandra/XMM-Newton Observation of NGC1407/1400 complex', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-5qs7y7z