Stefano Ettori
INAF
468 Papers
6.2K Citations
Stefano Ettori is an academic researcher from INAF. The author has contributed to research in topics: Galaxy cluster & Galaxy. The author has an hindex of 81, co-authored 428 publications. Previous affiliations of Stefano Ettori include University of Wollongong & University of Cambridge.
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Papers
The Cluster HEritage project with XMM-Newton: Mass Assembly and Thermodynamics at the Endpoint of structure formation - I. Programme overview
M. Arnaud,Stefano Ettori,G. W. Pratt,M. Rossetti,Dominique Eckert,F. Gastaldello,Raphael Gavazzi,Scott T. Kay,Lorenzo Lovisari,Lorenzo Lovisari,Ben J Maughan,Etienne Pointecouteau,Mauro Sereno,I. Bartalucci,I. Bartalucci,Annalisa Bonafede,Annalisa Bonafede,Hervé Bourdin,Rossella Cassano,R. T. Duffy,A. Iqbal,S. Maurogordato,E. Rasia,Jack Sayers,F. Andrade-Santos,Herve Aussel,David J. Barnes,R. Barrena,R. Barrena,Stefano Borgani,S. Burkutean,Nicolas Clerc,P. S. Corasaniti,P. S. Corasaniti,Jean-Charles Cuillandre,S. De Grandi,M. De Petris,Klaus Dolag,Klaus Dolag,Megan Donahue,A. Ferragamo,Massimo Gaspari,Massimo Gaspari,Simona Ghizzardi,Myriam Gitti,Myriam Gitti,Chris P. Haines,Mathilde Jauzac,Melanie Johnston-Hollitt,Christine Jones,Florian Kéruzoré,A. M. C. LeBrun,A. M. C. LeBrun,F. Mayet,Pasquale Mazzotta,Jean-Baptiste Melin,S. Molendi,Mario Nonino,Nobuhiro Okabe,S. Paltani,L. Perotto,Sandrine Pires,Mario Radovich,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,L. Salvati,L. Salvati,A. Saro,Barbara Sartoris,G. Schellenberger,Alina Streblyanska,Alina Streblyanska,Paula Tarrío,Paolo Tozzi,Keiichi Umetsu,R. F. J. van der Burg,R. F. J. van der Burg,Franco Vazza,Franco Vazza,Tiziana Venturi,Gustavo Yepes,S. Zarattini,S. Zarattini +82 more
TL;DR: The Cluster HEritage project with XMM-Newton -Mass Assembly and Thermodynamics at the Endpoint of structure formation (CHEX-MATE) is a three-mega-second multi-year Heritage Programme to obtain X-ray observations of a minimally-biased, signal-to-noise-limited sample of 118 galaxy clusters detected by Planck through the Sunyaev-Zeldovich effect.
The XMM Cluster Outskirts Project (X-COP)
Dominique Eckert,Stefano Ettori,Etienne Pointecouteau,Etienne Pointecouteau,S. Molendi,Stéphane Paltani,C. Tchernin +6 more
TL;DR: The XMM-Newton Cluster Outskirts Project (X-COP) as discussed by the authors targets the outer regions of a sample of 13 massive clusters in the redshift range 0.04-0.1 at uniform depth.
70
X-Ray Morphological Analysis of the Planck ESZ Clusters
Lorenzo Lovisari,William R. Forman,Christine Jones,Stefano Ettori,Felipe Andrade-Santos,Monique Arnaud,J. Démoclès,Gabriel W. Pratt,Scott W. Randall,Ralph P. Kraft +9 more
TL;DR: In this article, the authors determined eight morphological parameters for the Planck Early Sunyaev-Zeldovich (ESZ) objects observed with XMM-Newton and found that two parameters, concentration and centroid-shift, are the best to distinguish between relaxed and disturbed systems.
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Mass distribution in the core of MACS J1206: robust modeling from an exceptionally large sample of central multiple images
G. B. Caminha,Claudio Grillo,Piero Rosati,Massimo Meneghetti,Amata Mercurio,Stefano Ettori,Italo Balestra,Andrea Biviano,Keiichi Umetsu,E. Vanzella,M. Annunziatella,M. Bonamigo,C. Delgado-Correal,Marisa Girardi,Marco Lombardi,Mario Nonino,Barbara Sartoris,Paolo Tozzi,Matthias Bartelmann,Larry Bradley,Karina Caputi,Dan Coe,Holland C. Ford,Raphael Gobat,Marc Postman,Stella Seitz,Adi Zitrin +26 more
TL;DR: In this article, a strong lensing analysis of the galaxy cluster MACS J1206.2-0847 (MACS 1206), at z=0.44, using deep spectroscopy from CLASH-VLT and VLT/MUSE archival data in combination with imaging from the Cluster Lensing and Supernova survey with Hubble, is presented.
The morphologies and alignments of gas, mass, and the central galaxies of clash clusters of galaxies
Megan Donahue,Stefano Ettori,Elena Rasia,Elena Rasia,Jack Sayers,Adi Zitrin,Massimo Meneghetti,G. Mark Voit,Sunil Golwala,Nicole G. Czakon,Gustavo Yepes,Alessandro Baldi,Anton M. Koekemoer,Marc Postman +13 more
TL;DR: In this paper, the authors used weak and strong lensing to measure the distribution of matter within a sample of 25 clusters, 20 of which were deemed to be "relaxed" based on their X-ray morphology and alignment with the Brightest Cluster Galaxy.