Man

Paolo Cassata

Assistant professor

Universidad de Valparaiso

Valparaiso, Chile

Líneas de Investigación


Galaxy evolution; mass-assembly and SFRD; structure of passive early-type galaxies at high redshift; automatic tools for morphological analysis of high-z galaxies; spectroscopy of high redshift galaxies; Lyman? emitters; observational cosmology.

Educación

  •  Astronomy, UNIVERSITA DEGLI STUDI DI PADOVA. Italia, 2006
  •  Astronomy, UNIVERSITA DEGLI STUDI DI PADOVA. Italia, 2002

Experiencia Académica

  •   PhD Student Full Time

    UNIVERSITA DEGLI STUDI DI PADOVA

    Scienze Matematiche Fisiche e Naturali

    Padova, Italia

    2003 - 2005

  •   Postdoc Full Time

    INAF-IASF Milano

    Milano, Chile

    2006 - 2006

  •   Postdoc Full Time

    Laboratoire d'astrophysique de Marseille

    Marseille, Francia

    2006 - 2008

  •   Postdoc Full Time

    UNIV.OF MASSACHUSETTS AMHERST

    Amherst, Massachusetts, Estados Unidos

    2008 - 2011

  •   Postdoc Full Time

    Laboratoire d'Astrophysique de Marseille

    Marseille, Francia

    2011 - 2014

  •   Assistant professor Full Time

    UNIVERSIDAD DE VALPARAISO

    Ciencias

    Valparaiso, Chile

    2014 - A la fecha

Experiencia Profesional

  •   Postdoc Full Time

    Laboratoire d'Astrophysique de Marseille

    Marseille, Francia

    2011 - 2014

  •   Postdoc Full Time

    University of Massachusetts

    Amherst, Massachusetts, Estados Unidos

    2008 - 2011

  •   Postdoc Full Time

    Laboratoire d'Astrophysique de Marseille

    Marseille, Francia

    2006 - 2008

  •   Postdoc Full Time

    INAF-IASF Milano

    Milano, Italia

    2006 - 2006

Formación de Capital Humano


= Phd thesis supervisor, student Rosamaria Carraro, "The growth of supermassive black holes in galaxies: co-evolution and regulation of the star formation activity", since august 2015
= Phd thesis supervisor, student Hugo Méndez Hérnandez, PhD thesis supervisor, “a multiphase view of the gas content of galaxies at z~2”, since march 2015
= supervisor of the postdoc Romain Thomas, Gemini-CONICYT project “A multi-wavelength approach to identify the mechanisms that regulate star-formation in high-z galaxies”, June 2015 - June 2017
= Phd thesis co-supervisor, student Pin-Wei Wang, “Star formation rate and the assemblyof galaxies in the early universe”, January 2011 - June 2014
= Senior Thesis co-supervisor, student Francesco Valentino, “The dependence of the mass-size relation of early-type galaxies at redshift 0.2 < z < 1”, October 2012 - June 2013
= Mentor for the internship at the Laboratoire d’Astrophysique de Marseille (LAM), student Francesco Valentino, “The dependence of the mass-size relation of early-type galaxies at redshift 0.2 < z < 1”, July 2012 - September 2012
= Support for LAM graduate students Romain Thomas, Bin- Wei Wang, Anna Durkalec, July 2011 - June 2014
= Senior Thesis supervisor, student Peter Panka, “An Upper Limit to the Dry Merger Fraction from z=0 to z=1”, September 2010-June 2011
= Mentor for the University of Massachusetts REU summer program, student Peter Panka, “An Upper Limit to the Dry Merger Fraction from z=0 to z=1”, Summer 2010
= Mentor for the University of Massachusetts REU summer program, student Peter Panka, “The size distribution of massive early-type galaxies in SDSS as a function of the wavelength”, Summer 2009
= Support for University of Massachusetts graduate students Christina Williams, Yicheng Guo, Bomee Lee, Jul 2008 - Jun 2011
= Mentor and support for LAM master student Yann Boehler, Spring 2007



 

Article (26)

Analogues of primeval galaxies two billion years after the Big Bang
Corrigendum: Analogues of primeval galaxies two billion years after the Big Bang
Hidden starbursts and active galactic nuclei at 0 < z < 4 from the Herschel*-VVDS-CFHTLS-D1 field: Inferences on coevolution and feedback (vol 572, A90, 2014)
Morphology Dependence of Stellar Age in Quenched Galaxies at Redshift similar to 1.2: Massive Compact Galaxies Are Older than More Extended Ones
New constraints on the average escape fraction of Lyman continuum radiation in z similar to 4 galaxies from the VIMOS Ultra Deep Survey (VUDS)
The extended epoch of galaxy formation: Age dating of similar to 3600 galaxies with 2 < z < 6.5 in the VIMOS Ultra-Deep Survey
The VIMOS Ultra Deep Survey first data release: Spectra and spectroscopic redshifts of 698 objects up to z(spec) similar to 6 in CANDELS
VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies with 2.5 < z < 5.5 and the colour selection of high-redshift galaxies
A high definition view of the COSMOS Wall at z similar to 0.73
Effect of the star formation histories on the SFR-M-* relation at z >= 2
GAS FRACTION AND DEPLETION TIME OF MASSIVE STAR-FORMING GALAXIES AT z similar to 3.2: NO CHANGE IN GLOBAL STAR FORMATION PROCESS OUT TO z > 3
Size evolution of star-forming galaxies with 2 < z < 4.5 in the VIMOS Ultra-Deep Survey
The VIMOS Ultra Deep Survey: Ly alpha emission and stellar populations of star- forming galaxies at 2 < z < 2.5
Evolution of clustering length, large-scale bias, and host halo mass at 2 < z < 5 in the VIMOS Ultra Deep Survey (VUDS)
Narrowband selected high-redshift galaxy candidates contaminated by lower redshift [OIII] ultra-strong emitter line galaxies
Stellar mass to halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z similar or equal to 3
The evolving star formation rate: M-star relation and sSFR since z similar or equal to 5 from the VUDS spectroscopic survey
The host galaxies of X- ray selected active galactic nuclei to z=2.5: Structure, star formation, and their relationships from CANDELS and Herschel/PACS
THE INTERSTELLAR MEDIUM AND FEEDBACK IN THE PROGENITORS OF THE COMPACT PASSIVE GALAXIES AT z similar to 2
The VIMOS Ultra-Deep Survey (VUDS): fast increase in the fraction of strong Lyman-alpha emitters from z=2 to z=6
Discovery of a rich proto-cluster at z=2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS)
LY alpha FOREST TOMOGRAPHY FROM BACKGROUND GALAXIES: THE FIRST MEGAPARSEC-RESOLUTION LARGE-SCALE STRUCTURE MAP AT Z > 2
THE PROGENITORS OF THE COMPACT EARLY-TYPE GALAXIES AT HIGH REDSHIFT
VIMOS Ultra-Deep Survey (VUDS): Witnessing the assembly of a massive cluster at z similar to 3.3
The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35 016 galaxies and AGN out to z similar to 6.7 selected with 17.5 <= i(AB) <= 24.75
The Optical Spectra of 24 μm Galaxies in the COSMOS Field. I. Spitzer MIPS Bright Sources in the zCOSMOS‐Bright 10k Catalog
1
Franz Bauer

Associate Professor

Instituto de Astrofisica

PONTIFICÍA UNIVERSIDAD CATÓLICA DE CHILE, DEPARTAMENTO DE ASTRONOMÍA Y ASTROFÍSICA

Santiago, Chile

1
Isabelle JARRY

Directora Licenciatura en Astronomía

Ciencias Físicas

UNIVERSIDAD ANDRES BELLO,

Santiago, Chile

26
Paolo Cassata

Assistant professor

Fisica y Astronomia

Universidad de Valparaiso

Valparaiso, Chile

12
Ricardo Amorin

Associate Professor (Académico)

Fisica y Astronomia

Universidad de La Serena

La Serena, Chile

3
LUCIA GUAITA

Faculty

Universidad Andrés Bello

santiago, Chile