Man

Valentino Gaston Gonzalez Corvalan

Profesor Asistente

UNIVERSIDAD DE CHILE

Santiago, Chile

Líneas de Investigación


Galaxy Formation and Evolution; Stellar Population Modeling of Distant Galaxies; Stellar Mass Buildup of the Universe

Educación

  •  Licenciatura en Ciencias mencion Astronomia, UNIVERSIDAD DE CHILE. Chile, 2005
  •  Master of Science, Astronomy, UNIVERSITY OF CALIFORNIA, SANTA CRUZ. Estados Unidos, 2009
  •  Philosophy Doctorate, Astronomy, UNIVERSITY OF CALIFORNIA, SANTA CRUZ. Estados Unidos, 2012

Experiencia Académica

  •   Profesor Asistente Full Time

    UNIVERSIDAD DE CHILE

    2015 - A la fecha

Experiencia Profesional

  •   Postdoctoral Researcher

    University of California Riverside

    Estados Unidos

    2012 - 2015


 

Article (41)

LATIS: The Ly alpha Tomography IMACS Survey
The high-redshift SFR M relation is sensitive to the employed star formation rate and stellar mass indicators: towards addressing the tension between observations and simulations
An Evolving and Mass-dependent sigma sSFR-M(* )Relation for Galaxies
The GREATS H beta plus [O III] luminosity function and galaxy properties at z similar to 8: walking the way of JWST
The Hubble Legacy Field GOODS-S Photometric Catalog
Rotation in [C II]-emitting gas in two galaxies at a redshift of 6.8
A Comprehensive Study of Ly alpha Emission in the High-redshift Galaxy Population
The evolution of the star formation rate function in the EAGLE simulations: a comparison with UV, IR and H alpha observations from z similar to 8 to z similar to 0
The Rest-frame Optical (900nm) Galaxy Luminosity Function at z similar to 4-7: Abundance Matching Points to Limited Evolution in the M-STAR/M-HALO Ratio at z >= 4
A REMARKABLY LUMINOUS GALAXY AT Z=11.1 MEASURED WITH HUBBLE SPACE TELESCOPE GRISM SPECTROSCOPY
HOW LYMAN ALPHA EMISSION DEPENDS ON GALAXY STELLAR MASS
REST-FRAME OPTICAL EMISSION LINES IN z similar to 3.5 LYMAN-BREAK-SELECTED GALAXIES: THE UBIQUITY OF UNUSUALLY HIGH [O III]/H beta RATIOS AT 2 Gyr
z greater than or similar to 7 GALAXIES WITH RED SPITZER/IRAC [3.6]-[4.5] COLORS IN THE FULL CANDELS DATA SET: THE BRIGHTEST-KNOWN GALAXIES AT z similar to 7-9 AND A PROBABLE SPECTROSCOPIC CONFIRMATION AT z=7.48
A SPECTROSCOPIC REDSHIFT MEASUREMENT FOR A LUMINOUS LYMAN BREAK GALAXY AT z=7.730 USING KECK/MOSFIRE
ULTRADEEP IRAC IMAGING OVER THE HUDF AND GOODS-SOUTH: SURVEY DESIGN AND IMAGING DATA RELEASE
UV LUMINOSITY FUNCTIONS AT REDSHIFTS z similar to 4 TO z similar to 10: 10,000 GALAXIES FROM HST LEGACY FIELDS
Evidence for Ubiquitous High-equivalent-width Nebular Emission in z ~ 7 Galaxies: Toward a Clean Measurement of the Specific Star-formation Rate Using a Sample of Bright, Magnified Galaxies
SLOW EVOLUTION OF THE SPECIFIC STAR FORMATION RATE AT z > 2: THE IMPACT OF DUST, EMISSION LINES, AND A RISING STAR FORMATION HISTORY
THE MOST LUMINOUS z similar to 9-10 GALAXY CANDIDATES YET FOUND: THE LUMINOSITY FUNCTION, COSMIC STAR-FORMATION RATE, AND THE FIRST MASS DENSITY ESTIMATE AT 500 Myr*
TRACING THE MASS GROWTH AND STAR FORMATION RATE EVOLUTION OF MASSIVE GALAXIES FROM Z similar to 6 TO Z similar to 1 IN THE HUBBLE ULTRA-DEEP FIELD
UV-CONTINUUM SLOPES OF > 4000 z similar to 4-8 GALAXIES FROM THE HUDF/XDF, HUDF09, ERS, CANDELS-SOUTH, AND CANDELS-NORTH FIELDS
A REST-FRAME OPTICAL VIEW ON z similar to 4 GALAXIES. I. COLOR AND AGE DISTRIBUTIONS FROM DEEP IRAC PHOTOMETRY OF THE IUDF10 AND GOODS SURVEYS
Photometric Constraints on the Redshift of z ~ 10 Candidate UDFj-39546284 from Deeper WFC3/IR+ACS+IRAC Observations over the HUDF
PROBING THE DAWN OF GALAXIES AT z similar to 9-12: NEW CONSTRAINTS FROM HUDF12/XDF AND CANDELS DATA
THE HST EXTREME DEEP FIELD (XDF): COMBINING ALL ACS AND WFC3/IR DATA ON THE HUDF REGION INTO THE DEEPEST FIELD EVER
THE SPECTRAL ENERGY DISTRIBUTIONS OF z similar to 8 GALAXIES FROM THE IRAC ULTRA DEEP FIELDS: EMISSION LINES, STELLAR MASSES, AND SPECIFIC STAR FORMATION RATES AT 650 MYR
EXPANDED SEARCH FOR z similar to 10 GALAXIES FROM HUDF09, ERS, AND CANDELS DATA: EVIDENCE FOR ACCELERATED EVOLUTION AT z > 8?
THE BRIGHT END OF THE ULTRAVIOLET LUMINOSITY FUNCTION AT z similar to 8: NEW CONSTRAINTS FROM CANDELS DATA IN GOODS-SOUTH
THE EVOLUTION OF MASS-SIZE RELATION FOR LYMAN BREAK GALAXIES FROM z=1 to z=7
THE REST-FRAME UV-TO-OPTICAL COLORS AND SPECTRAL ENERGY DISTRIBUTIONS OF z similar to 4-7 GALAXIES
UV-CONTINUUM SLOPES AT z similar to 4-7 FROM THE HUDF09+ERS+CANDELS OBSERVATIONS: DISCOVERY OF A WELL-DEFINED UV COLOR-MAGNITUDE RELATIONSHIP FOR z >= 4 STAR-FORMING GALAXIES
A candidate redshift z approximate to 10 galaxy and rapid changes in that population at an age of 500 Myr
EVOLUTION OF GALAXY STELLAR MASS FUNCTIONS, MASS DENSITIES, AND MASS-TO-LIGHT RATIOS FROM z similar to 7 TO z similar to 4
ULTRAVIOLET LUMINOSITY FUNCTIONS FROM 132 z similar to 7 AND z similar to 8 LYMAN-BREAK GALAXIES IN THE ULTRA-DEEP HUDF09 AND WIDE-AREA EARLY RELEASE SCIENCE WFC3/IR OBSERVATIONS
DISCOVERY OF z similar to 8 GALAXIES IN THE HUBBLE ULTRA DEEP FIELD FROM ULTRA-DEEP WFC3/IR OBSERVATIONS
STAR FORMATION RATES AND STELLAR MASSES OF z=7-8 GALAXIES FROM IRAC OBSERVATIONS OF THE WFC3/IR EARLY RELEASE SCIENCE AND THE HUDF FIELDS
THE STELLAR MASS DENSITY AND SPECIFIC STAR FORMATION RATE OF THE UNIVERSE AT z similar to 7
ULTRADEEP INFRARED ARRAY CAMERA OBSERVATIONS OF SUB-L* z similar to 7 AND z similar to 8 GALAXIES IN THE HUBBLE ULTRA DEEP FIELD: THE CONTRIBUTION OF LOW-LUMINOSITY GALAXIES TO THE STELLAR MASS DENSITY AND REIONIZATION
z similar to 7 GALAXY CANDIDATES FROM NICMOS OBSERVATIONS OVER THE HDF-SOUTH AND THE CDF-SOUTH AND HDF-NORTH GOODS FIELDS
An infrared study of the double nucleus in NGC3256
The Calán-Yale Deep Extragalactic Research (CYDER) Survey: Optical Properties and Deep Spectroscopy of Serendipitous X-Ray Sources

Proyecto (1)

HIGH REDSHIFT GALAXY EVOLUTION=> ROBUST STELLAR MASSES AND THE ROLE OF NEBULAR EMISSION LINES.
37
Valentino Gonzalez

Profesor Asistente

UNIVERSIDAD DE CHILE

Santiago, Chile

4
Guillermo Blanc

Adjunct Professor

Astronomía

UNIVERSIDAD DE CHILE

Santiago, Chile

1
Nicolas Tejos

Associate Professor

Pontificia Universidad Católica de Valparaíso

Curauma, Chile

1
Sebastian Lopez

Associate Professor

DEPARTAMENTO DE ASTRONOMIA

Santiago, Chile

1
Paulina Lira

Associate Professor

Astronomía

Universidad de Chile

Santiago, Chile