A dataset provided by the European Space Agency

Name 060428
Title A combined X-ray and SZ study of the ICM in the low mass cluster XLSSC 006
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604280101

DOI 10.5270/esa-xd7qi0i
Author Dr Florian Pacaud
Description We propose a deep observation of the z=0.43, T=5 keV galaxy cluster XLSSC 006. Its Sunyaev- Zel.dovich (SZ) signature was detected with high signal to noise at 150 GHz by the APEX-SZ instrument. This makes XLSSC 006 the coolest cluster ever detected in SZ. Combining our well resolved SZ map with a high sensitivity XMM observation will permit to derive for the first time the gas temperature profile from a deprojection of the SZ and X-ray surface brightness out to at least 0.8xr500. This will further enable us to estimate the average temperature of the RzCS 059, a red sequence selected cluster at z=0.9 and add two interesting points in the scaling relations for low mass systems. Possible other X-ray detections could also be correlated to less significant SZ decrements visible in the field.
Publication 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 ,
The XXL Survey. I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme . Pierre, M., Pacaud, F., et all. . A&A . 592-1 . 2016 . 2016A&A...592A...1P ,
The XXL Survey. II. The bright cluster sample: catalogue and luminosity function . Pacaud, F., Clerc, N., et all. . A&A . 592-2 . 2016 . 2016A&A...592A...2P ,
The XXL Survey. III. Luminosity-temperature relation of the bright cluster sample . Giles, P. A., Maughan, B. J., et all. . A&A . 592-3 . 2016 . 2016A&A...592A...3G ,
The XXL Survey . IV. Mass-temperature relation of the bright cluster sample . Lieu, M., Smith, G. P., et all. . A&A . 592-4 . 2016 . 2016A&A...592A...4L ,
The XXL Survey. VI. The 1000 brightest X-ray point sources . Fotopoulou, S., Pacaud, F., et all. . A&A . 592-5 . 2016 . 2016A&A...592A...5F ,
The XXL Survey. VII. A supercluster of galaxies at z = 0.43 . Pompei, E., Adami, C., et all. . A&A . 592-6 . 2016 . 2016A&A...592A...6P ,
The XXL Survey. VIII. MUSE characterisation of intracluster light in a z ~ 0.53 cluster of galaxies . Adami, C., Pompei, E., et all. . A&A . 592-7 . 2016 . 2016A&A...592A...7A ,
The XXL Survey. XIII. Ba...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-08-10T11:30:36Z/2009-08-11T15:59:32Z
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 2010-09-10T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-09-10T00:00:00Z, 060428, 17.56_20190403_1200. https://doi.org/10.5270/esa-xd7qi0i