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A. Iovino
Researcher at INAF
Publications - 428
Citations - 40120
A. Iovino is an academic researcher from INAF. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 94, co-authored 423 publications receiving 37563 citations. Previous affiliations of A. Iovino include ASTRON & University of Insubria.
Papers
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The VIMOS-VLT deep survey: the group catalogue
TL;DR: In this paper, a complete catalog of optical galaxy groups identified in the purely flux-limited (17.5 ≤ IAB ≤ 24.0) VIMOS-VLT deep redshift Survey (VVDS) is presented.
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VVDS-SWIRE - Clustering evolution from a spectroscopic sample of galaxies with redshift 0.2 < z < 2.1 selected from Spitzer IRAC 3.6 μm and 4.5 μm photometry
S. de la Torre,O. Le Fevre,S. Arnouts,Luigi Guzzo,Duncan Farrah,A. Iovino,Carol J. Lonsdale,Carol J. Lonsdale,B. Meneux,S. J. Oliver,A. Pollo,I. Waddington,D. Bottini,Fan Fang,B. Garilli,V. Le Brun,D. Maccagni,J. P. Picat,Roberto Scaramella,Marco Scodeggio,David L. Shupe,Jason Surace,L. Tresse,G. Vettolani,A. Zanichelli,C. Adami,S. Bardelli,M. Bolzonella,A. Cappi,Stephane Charlot,Paolo Ciliegi,T. Contini,Sylvie Foucaud,P. Franzetti,I. Gavignaud,Olivier Ilbert,F. Lamareille,H. J. McCracken,Bruno Marano,Christian Marinoni,A. Mazure,R. Merighi,Stéphane Paltani,R. Pello,Lucia Pozzetti,Mario Radovich,G. Zamorani,E. Zucca,M. Bondi,Angela Bongiorno,Jarle Brinchmann,Olga Cucciati,Olga Cucciati,Yannick Mellier,Paola Merluzzi,S. Temporin,Daniela Vergani,C. J. Walcher +57 more
TL;DR: In this article, the authors used the projected two-point correlation function w_p(r_p) to study the three dimensional clustering properties of galaxies detected at 3.6-4.5 μm, across the whole redshift range explored.
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Dust Absorption and the Cosmic UV Flux Density
TL;DR: In this paper, the authors studied the evolution of the galaxy UV luminosity density as a function of redshift in the Hubble Deep Field North (HDF-N) and estimated the amount of energy absorbed by dust and hidden from optical observations.
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Properties and environment of radio-emitting galaxies in the VLA-zCOSMOS survey
S. Bardelli,Eva Schinnerer,Vernesa Smolčić,G. Zamorani,E. Zucca,M. Mignoli,C. Halliday,K. Kovac,Paolo Ciliegi,Karina Caputi,Anton M. Koekemoer,Angela Bongiorno,M. Bondi,Micol Bolzonella,Daniela Vergani,Lucia Pozzetti,C. M. Carollo,Thierry Contini,Jean-Paul Kneib,O. Le Fevre,S. J. Lilly,Vincenzo Mainieri,Alvio Renzini,Marco Scodeggio,Graziano Coppa,Olga Cucciati,S. de la Torre,L. de Ravel,P. Franzetti,B. Garilli,A. Iovino,P. Kampczyk,C. Knobel,F. Lamareille,J. F. Le Borgne,V. Le Brun,Christian Maier,R. Pello,Y. Peng,Enrique Perez-Montero,Enrique Perez-Montero,E. Ricciardelli,John D. Silverman,Masayuki Tanaka,Lidia Tasca,Laurence Tresse,Ummi Abbas,D. Bottini,A. Cappi,Paolo Cassata,Andrea Cimatti,Luigi Guzzo,Alexie Leauthaud,D. Maccagni,Christian Marinoni,H. J. McCracken,P. Memeo,B. Meneux,P. Oesch,Cristiano Porciani,Roberto Scaramella,Peter Capak,D. B. Sanders,Nick Scoville,Yoshi Taniguchi,Knud Jahnke +65 more
TL;DR: In this paper, the authors investigated the properties and the environment of radio sources with optical counterparts from the combined VLA-COSMOS and============πεγγγεγε ε −1 −4.5 µm infrared color-specific star-formation plane, from which they extracted the corresponding control samples.
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The VIMOS Public Extragalactic Redshift Survey (VIPERS). Measuring nonlinear galaxy bias at z~0.8
C. Di Porto,E. Branchini,J. Bel,Federico Marulli,M. Bolzonella,O. Cucciati,S. de la Torre,B. R. Granett,Luigi Guzzo,Christian Marinoni,L. Moscardini,U. Abbas,C. Adami,Stephane Arnouts,D. Bottini,A. Cappi,Jean Coupon,I. Davidzon,G. De Lucia,A. Fritz,P. Franzetti,M. Fumana,B. Garilli,O. Ilbert,A. Iovino,J. Krywult,V. Le Brun,O. Le Fevre,D. Maccagni,Katarzyna Małek,H. J. McCracken,L. Paioro,M. Polletta,A. Pollo,Marco Scodeggio,L. A. M. Tasca,Rita Tojeiro,D. Vergani,A. Zanichelli,Angela Burden,A. Marchetti,Davide Martizzi,Yannick Mellier,Robert C. Nichol,John A. Peacock,Will J. Percival,Matteo Viel,M. Wolk,G. Zamorani +48 more
TL;DR: In this article, the authors used the first release of the VImos Public Extragalactic Redshift Survey of galaxies (VIPERS) of ~50,000 objects to measure the bias relation between galaxies and mass in the redshift range z=[0.5, 1.1].