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Enrichetta Iodice
Researcher at Astronomical Observatory of Capodimonte
Publications - 95
Citations - 1695
Enrichetta Iodice is an academic researcher from Astronomical Observatory of Capodimonte. The author has contributed to research in topics: Galaxy & Fornax Cluster. The author has an hindex of 20, co-authored 74 publications receiving 1255 citations. Previous affiliations of Enrichetta Iodice include INAF & European Southern Observatory.
Papers
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Journal ArticleDOI
The Fornax Deep Survey (FDS) with the VST: III. Low Surface Brightness (LSB) dwarfs and Ultra Diffuse Galaxies (UDGs) in the center of the Fornax cluster
Aku Venhola,Reynier Peletier,Eija Laurikainen,H. Salo,Thorsten Lisker,Enrichetta Iodice,Massimo Capaccioli,G. A. Verdoes Kleijn,Edwin A. Valentijn,Steffen Mieske,M. Hilker,C. Wittman,G. Van de Venn,Aniello Grado,Marilena Spavone,Michele Cantiello,Nicola R. Napolitano,Maurizio Paolillo,Jesús Falcón-Barroso +18 more
TL;DR: In this paper, a 2D Sersic model fitting with GALFIT was used to classify low surface brightness (LSB) galaxies in nearby clusters and analyzed their distribution and orientations in the cluster, and studied their colors.
Journal ArticleDOI
The Fornax Deep Survey with VST. III. Low surface brightness dwarfs and ultra diffuse galaxies in the center of the Fornax cluster
Aku Venhola,Aku Venhola,Reynier Peletier,Eija Laurikainen,Heikki Salo,Thorsten Lisker,Enrichetta Iodice,Massimo Capaccioli,Gijs Verdois Kleijn,Edwin A. Valentijn,Steffen Mieske,M. Hilker,Carolin Wittmann,Glenn van de Ven,A. Grado,Marilena Spavone,Michele Cantiello,Nicola R. Napolitano,Maurizio Paolillo,Maurizio Paolillo,Jesús Falcón-Barroso,Jesús Falcón-Barroso +21 more
TL;DR: In this paper, a 2D Sersic model fitting with GALFIT was used to identify low surface brightness (LSB) galaxies in the Fornax Deep Survey (FDS) images.
Journal ArticleDOI
The Fornax Deep Survey with the VST. IV. A size and magnitude limited catalog of dwarf galaxies in the area of the Fornax cluster
Aku Venhola,Reynier Peletier,Eija Laurikainen,Heikki Salo,Enrichetta Iodice,Steffen Mieske,M. Hilker,Carolin Wittmann,Thorsten Lisker,Maurizio Paolillo,Maurizio Paolillo,Michele Cantiello,Joachim Janz,Joachim Janz,Marilena Spavone,Raffaele D'Abrusco,Glenn van de Ven,Glenn van de Ven,Nicola R. Napolitano,Gijs Verdoes Kleijn,Natasha Maddox,Massimo Capaccioli,A. Grado,Edwin A. Valentijn,Jesús Falcón-Barroso,Jesús Falcón-Barroso,L. Limatola +26 more
TL;DR: The Fornax Deep Survey (FDS) dwarf galaxy catalog as discussed by the authors was used to study the galaxies down to r'-band magnitude m(r') approximate to 21 mag (M-r' approximate to -10.5 mag), which opens a new parameter regime to investigate the evolution of dwarf galaxies in the cluster environment.
Journal ArticleDOI
The Fornax Deep Survey (FDS) with the VST: IV. A size and magnitude limited catalog of dwarf galaxies in the area of the Fornax cluster
Aku Venhola,Reynier Peletier,Eija Laurikainen,Heikki Salo,Enrichetta Iodice,Steffen Mieske,Michael Hilker,Carolin Wittmann,Thorsten Lisker,Maurizio Paolillo,Michele Cantiello,Joachim Janz,Marilena Spavone,Raffaele D'Abrusco,Glenn van de Ven,Nicola R. Napolitano,Gijs Verdoes Kleijn,Natasha Maddox,Massimo Capaccioli,Aniello Grado,Edwin A. Valentijn,Jesús Falcón-Barroso,Luca Limatola +22 more
TL;DR: The Fornax Deep Survey (FDS) dwarf galaxy catalog as mentioned in this paper contains 14,095 galaxies and reaches its 50% completeness limit at magnitude M$r'}$ = -10.5 mag and surface brightness $\bar{\mu}_{e,r'}) = 26 mag arcsec-2.
Journal ArticleDOI
VEGAS: A VST Early-type GAlaxy Survey. II. Photometric study of giant ellipticals and their stellar halos
Marilena Spavone,Massimo Capaccioli,Massimo Capaccioli,Nicola R. Napolitano,Enrichetta Iodice,Aniello Grado,Luca Limatola,Andrew Cooper,Michele Cantiello,Michele Cantiello,Duncan A. Forbes,Maurizio Paolillo,Pietro Schipani +12 more
TL;DR: In this article, the authors investigate the photometric properties of six massive early type galaxies (ETGs) in the VEGAS sample (NGC 1399, NGC 3923 and NGC 4365), out to extremely low surface brightness levels, with the goal of characterizing the global structure of their light profiles for comparison to state-of-theart galaxy formation models.