S. Zarattini
University of Padua
12 Papers
170 Citations
S. Zarattini is an academic researcher from University of Padua. The author has contributed to research in topics: Galaxy & Galaxy cluster. The author has an hindex of 8, co-authored 12 publications. Previous affiliations of S. Zarattini include Paris Diderot University & Spanish National Research Council.
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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 nature and nurture of bars and disks
Jairo Méndez-Abreu,Jairo Méndez-Abreu,Ruben Sanchez-Janssen,J. A. L. Aguerri,J. A. L. Aguerri,Enrico Maria Corsini,Enrico Maria Corsini,S. Zarattini,S. Zarattini,S. Zarattini +9 more
TL;DR: In this paper, the authors derived the bar fraction in three different environments ranging from the field to Virgo and Coma clusters, covering an unprecedentedly large range of galaxy luminosities (or, equivalently, stellar masses).
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Fossil groups origins II. Unveiling the formation of the brightest group galaxies through their scaling relations
Jairo Méndez-Abreu,J. A. L. Aguerri,R. Barrena,Ruben Sanchez-Janssen,W. Boschin,N. Castro-Rodriguez,Enrico Maria Corsini,C. del Burgo,Elena D'Onghia,Marisa Girardi,Jorge Iglesias-Páramo,Nicola R. Napolitano,José M. Vílchez,S. Zarattini +13 more
TL;DR: In this article, the authors analyzed the near-infrared photometric and structural properties of a sample of 20 BGGs present in FGs in order to better understand their formation mechanisms.
The nature and nurture of bars and disks
Jairo Méndez-Abreu,Jairo Méndez-Abreu,Ruben Sanchez-Janssen,J. A. L. Aguerri,J. A. L. Aguerri,Enrico Maria Corsini,Enrico Maria Corsini,S. Zarattini,S. Zarattini,S. Zarattini +9 more
TL;DR: In this paper, the authors derived the bar fraction in three different environments ranging from the field to Virgo and Coma Clusters, covering an unprecedentedly large range of galaxy luminosities (or, equivalently, stellar masses).
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Fossil Groups Origins III. Characterization of the sample and observational properties of fossil systems
S. Zarattini,R. Barrena,Marisa Girardi,N. Castro-Rodriguez,W. Boschin,J. A. L. Aguerri,J. Mendez-Abreu,Ruben Sanchez-Janssen,Cristina Catalán-Torrecilla,Enrico Maria Corsini,C. del Burgo,Elena D'Onghia,N. Herrera-Ruiz,Jorge Iglesias-Páramo,E. Jimenez Bailon,M. Lozada Muñoz,Nicola R. Napolitano,José M. Vílchez +17 more
TL;DR: In this article, an extensive observational program to characterize a sample of 34 fossil group candidates spanning a broad range of physical properties was carried out and 15 candidates turned out to be fossil systems.