A dataset provided by the European Space Agency

Name 055624
Title X-ray properties of nearby isolated Ellipticals
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556240501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556240601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556240701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556240801

DOI 10.5270/esa-ys0dt65
Author Dr Elisabetta Memola
Description We propose to investigate the intrinsic properties of the hot interstellar-medium in early-type galaxies. For this purpose we have chosen a well selected sample of isolated, optically similar, nearby, elliptical galaxies to minimize the influence of external factors such as the presence of a group or different luminous masses. Three objects already studied show the full range of Lx-Lb scatter observed in larger, heterogeneous samples. With this proposal we request 5 additional objects that will complete the small, but homogeneous sample of bright Ellipticals.
Publication Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive . Clerc, N., Sadibekova, T., et all. . MNRAS . 423-3561 . 2012 . 2012MNRAS.423.3561C ,
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 ,
SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV . Clerc, N., Merloni, A., et all. . MNRAS . 463-4490 . 2016 . 2016MNRAS.463.4490C ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation . Molham, Mona, Clerc, Nicolas, et all. . MNRAS . 494-161 . 2020 . 2020MNRAS.494..161M ,
Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks . Kosiba, Matej, Lieu, Maggie, et all. . MNRAS . 496-4141 . 2020 . 2020MNRAS.496.4141K ,
SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release . Clerc, N., Kirkpatrick, C. C., et all. . MNRAS . 497-3976 . 2020 . 2020MNRAS.497.3976C ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-06-03T08:07:27Z/2009-02-26T12:26:42Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2010-03-26T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-03-26T00:00:00Z, 055624, 17.56_20190403_1200. https://doi.org/10.5270/esa-ys0dt65