A dataset provided by the European Space Agency

Name 040001
Title The Abell 3395-Abell 3391 Filament in the Horologium Supercluster
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400010201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400010301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400010501

DOI 10.5270/esa-lgewewj
Author Dr Mark Henriksen
Description We will use the spectro-spatial capability of XMM to map the hot gas of the entire Abell 3395-Abell 3391 region of the Horologium supercluster. In particular, we will: (1) measure the baryon fraction for clusters, groups, and filamentary gas, (2) make temperature, pressure, and entropy maps to search for the merger and infall signatures of the complex Abell 3395 3-body system, (3) construct a dynamical model of the Abell 3395-Abell 3391 filament using the X-ray measured masses combined with the galaxy kinematical parameters obtained from Horologium Consortium collaborators, and (4) work with Horologium Consortium members on a multi-waveband analysis of galaxy evolution in the context of large-scale structure formation.
Publication HIFLUGCS: Galaxy cluster scaling relations between X-ray luminosity, gas mass, cluster radius, and velocity dispersion . Zhang, Y.-Y., Andernach, H., et all. . A&A . 526-105 . 2011 . 2011A&A...526A.105Z ,
The Swift Burst Alert Telescope Perspective on Non-thermal Emission in HIFLUGCS Galaxy Clusters . Wik, Daniel R., Sarazin, Craig L., et all. . ApJ . 748-67 . 2012 . 2012ApJ...748...67W ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
Intracluster Medium of the Merging Cluster A3395 . Lakhchaura, Kiran, Singh, K. P., et all. . ApJ . 743-78 . 2011 . 2011ApJ...743...78L ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
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 ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . ...,
The cool-core bias in X-ray galaxy cluster samples. I. Method and application to HIFLUGCS . Eckert, D., Molendi, S., . A&A . 526-79 . 2011 . 2011A&A...526A..79E ,
Characterization of Intracluster Medium Temperature Distributions of 62 Galaxy Clusters with XMM-Newton . Frank, K. A., Peterson, J. R., et all. . ApJ . 764-46 . 2013 . 2013ApJ...764...46F ,
A volume-limited sample of X-ray galaxy groups and clusters - I. Radial entropy and cooling time profiles . Panagoulia, E. K., Fabian, A. C., . MNRAS . 438-2341 . 2014 . 2014MNRAS.438.2341P ,
Automatic Classification of Time-variable X-Ray Sources . Lo, Kitty K., Farrell, Sean, et all. . ApJ . 786-20 . 2014 . 2014ApJ...786...20L ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
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 ,
XMM-Newton and Chandra cross-calibration using HIFLUGCS galaxy clusters . Systematic temperature differences and cosmological impact . Schellenberger, G., Reiprich, T. H., et all. . A&A . 575-30 . 2015 . 2015A&A...575A..30S ,
Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters . Xiao, Weike, Chen, Chen, et all. . MNRAS . 432-41 . 2013 . 2013MNRAS.432L..41X ,
A volume-limited sample of X-ray galaxy groups and clusters - II. X-ray cavity dynamics . Panagoulia, E. K., Fabian, A. C., et all. . MNRAS . 444-1236 . 2014 . 2014MNRAS.444.1236P ,
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 ,
HIFLUGCS: X-ray luminosity-dynamical mass relation and its implications for mass calibrations with the SPIDERS and 4MOST surveys . Zhang, Yu-Ying, Reiprich, Thomas H., et all. . A&A . 599-138 . 2017 . 2017A&A...599A.138Z ,
HICOSMO - cosmology with a complete sample of galaxy clusters - I. Data analysis, sample selection and luminosity-mass scaling relation . Schellenberger, G., Reiprich, T. H., . MNRAS . 469-3738 . 2017 . 2017MNRAS.469.3738S ,
X-Ray Morphological Analysis of the Planck ESZ Clusters . Lovisari, Lorenzo, Forman, William R., et all. . ApJ . 846-51 . 2017 . 2017ApJ...846...51L ,
HICOSMO: cosmology with a complete sample of galaxy clusters - II. Cosmological results . Schellenberger, G., Reiprich, T. H., . MNRAS . 471-1370 . 2017 . 2017MNRAS.471.1370S ,
Anisotropy of the galaxy cluster X-ray luminosity-temperature relation . Migkas, Konstantinos, Reiprich, Thomas H., . A&A . 611-50 . 2018 . 2018A&A...611A..50M ,
Chandra and XMM-Newton Observations of the Abell 3395-Abell 3391 Intercluster Filament . Alvarez, Gabriella E., Randall, Scott W., et all. . ApJ . 858-44 . 2018 . 2018ApJ...858...44A ,
The XMM Cluster Survey: Present status and latest results . Viana, P. T. P., Mehrtens, N., et all. . AN . 334-462 . 2013 . 2013AN....334..462V ,
The Galaxy Cluster Mass Scale and Its Impact on Cosmological Constraints from the Cluster Population . Pratt, G. W., Arnaud, M., et all. . SSRv . 215-25 . 2019 . 2019SSRv..215...25P ,
Physical properties of the X-ray gas as a dynamical diagnosis for galaxy clusters . Lagana, T. F., Durret, F., . MNRAS . 484-2807 . 2019 . 2019MNRAS.484.2807L ,
The Fornax3D project: Tracing the assembly history of the cluster from the kinematic and line-strength maps . Iodice, E., Sarzi, M., et all. . A&A . 627-136 . 2019 . 2019A&A...627A.136I ,
Testing emergent gravity on galaxy cluster scales . Tamosiunas, Andrius, Bacon, David, et all. . JCAP . 5-53 . 2019 . 2019JCAP...05..053T ,
Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline . Hollowood, Devon L., Jeltema, Tesla, et all. . ApJS . 244-22 . 2019 . 2019ApJS..244...22H ,
Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters . Palmese, A., Annis, J., et all. . MNRAS . 493-4591 . 2020 . 2020MNRAS.493.4591P ,
X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton . Lovisari, Lorenzo, Schellenberger, Gerrit, et all. . ApJ . 892-102 . 2020 . 2020ApJ...892..102L ,
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 ,
TESS observations of southern ultrafast rotating low-mass stars . Ramsay, Gavin, Doyle, J. Gerry, . MNRAS . 497-2320 . 2020 . 2020MNRAS.497.2320R ,
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 2007-01-24T12:30:29Z/2007-04-06T11:59:47Z
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 2008-04-20T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-04-20T00:00:00Z, 040001, 17.56_20190403_1200. https://doi.org/10.5270/esa-lgewewj