Man

Julie Beth Nantais

Profesora Asistente

Universidad Andrés Bello

Las Condes, Chile

Líneas de Investigación


Globular Clusters in Spiral Galaxies; High Redshift Galaxy Clusters; Galaxy Formation and Evolution; Large Scale Structures; Observational Cosmology

Educación

  •  Astronomy, HARVARD UNIVERSITY. Estados Unidos, 2010
  •  Astronomy, HARVARD UNIVERSITY. Estados Unidos, 2004
  •  Physics and Astronomy, UNIV.OF MASSACHUSETTS AMHERST. Estados Unidos, 2002

Experiencia Académica

  •   Profesora asistente Full Time

    UNIVERSIDAD ANDRES BELLO

    Ciencias Exactas

    Santiago, Chile

    2014 - A la fecha

  •   Investigadora Postdoctoral Other

    UNIVERSIDAD DE CONCEPCION

    Ciencias Físicas y Matemáticas

    Concepción, Chile

    2010 - 2014

Experiencia Profesional

  •   Profesora asistente Full Time

    Universidad Andrés Bello

    Santiago, Chile

    2014 - A la fecha


 

Article (33)

The GOGREEN and GCLASS surveys: first data release
The GOGREEN survey: Internal dynamics of clusters of galaxies at redshift 0.9-1.4
An Extremely Massive Quiescent Galaxy at z=3.493: Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models
The GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0 z 1.4 and the complex nature of satellite quenching
The GOGREEN survey: post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z > 1
The GOGREEN survey: the environmental dependence of the star-forming galaxy main sequence at 1.0 z 1.5
The GOGREEN survey: the environmental dependence of the star-forming galaxy main sequence at 1.0 < z < 1.5
The H alpha star formation main sequence in cluster and field galaxies at z similar to 1.6
Resolving CO (2-1) in z similar to 1.6 Gas-rich Cluster Galaxies with ALMA: Rotating Molecular Gas Disks with Possible Signatures of Gas Stripping
The Rest-frame H-band Luminosity Function of Red-sequence Galaxies in Clusters at 1.0 < Z < 1.3
The Evolution of Environmental Quenching Timescales to z ~1.6=> Evidence for Dynamically Driven Quenching of the Cluster Galaxy Population
ALMA Observations of Gas-rich Galaxies in z ? 1.6 Galaxy Clusters=> Evidence for Higher Gas Fractions in High-density Environments
ALMA Observations of Gas-Rich Galaxies in z~1.6 Galaxy Clusters=> Evidence for Higher Gas Fractions in High-Density Environments
Discovery of Ram-pressure Stripped Gas around an Elliptical Galaxy in Abell 2670
Discovery of Ram-pressure Stripped Gas around an Elliptical Galaxy in Abell 2670
Evidence for strong evolution in galaxy environmental quenching efficiency between z = 1.6 and z = 0.9
Evidence for strong evolution in galaxy environmental quenching efficiency between z = 1.6 and z = 0.9
Galaxy Merger Candidates in High-redshift Cluster Environments
Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I=> Survey description
Weak lensing magnification of SpARCS galaxy clusters
Stellar mass function of cluster galaxies at z ~ 1.5=> evidence for reduced quenching efficiency at high redshift
EVIDENCE FOR THE UNIVERSALITY OF PROPERTIES OF RED-SEQUENCE GALAXIES IN X-RAY- AND RED-SEQUENCE-SELECTED CLUSTERS AT z similar to 1
DISCOVERY OF A RICH CLUSTER AT z=1.63 USING THE REST-FRAME 1.6 mu m "STELLAR BUMP SEQUENCE" METHOD
Morphology with light profile fitting of confirmed cluster galaxies at z = 0.84
Star-forming fractions and galaxy evolution with redshift in rich X-ray-selected galaxy clusters
The importance of major mergers in the build up of stellar mass in brightest cluster galaxies at z=1
Evidence for significant growth in the stellar mass of brightest cluster galaxies over the past 10 billion years
THE GEMINI CLUSTER ASTROPHYSICS SPECTROSCOPIC SURVEY (GCLASS): THE ROLE OF ENVIRONMENT AND SELF-REGULATION IN GALAXY EVOLUTION AT z similar to 1
Hubble Space Telescope Photometry of Globular Clusters in M81
Nearby Spiral Galaxy Globular Cluster Systems II: Globular Cluster Metallicities in NGC 300
Spectroscopy of M81 Globular Clusters
Star Cluster Candidates in M81
Nearby Spiral Globular Cluster Systems. I. Luminosity Functions

ConferencePaper (1)

Early-type galaxy formation: Understanding the role of the environment

Proyecto (5)

The Galaxy Nature-Nurture Problem Across Mass and Time
Star Formation in Galaxy Clusters: Does Environment Matter Before Quenching?
El Problema "Gallina o Huevo" de Galaxias Tipo Temprano y Formación de Cúmulos
Cúmulos de Galaxias=> Más Allá de la Edad de Oro
THE CESSATION OF STAR FORMATION IN EARLY-TYPE GALAXIES IN CLUSTERS
18
Julie Nantais

Profesora Asistente

Ciencias Físicas

Universidad Andrés Bello

Las Condes, Chile

13
Ricardo Demarco

Profesor Titular

Ciencias Físicas

Universidad Andrés Bello

Talcahuano, Chile

2
Pierluigi Cerulo

Profesor asistente

Ingeniería Informática y Ciencias de la COmputación

Universidad de Concepción

Concepción, Chile

1
Yara Jaffé

Prof. Adjunto

Instituto de Fisica y Astronomia

Universidad de Valparaiso

Valparaiso, Chile

1
Luis Barrientos

Associate Professor, Director

Institute of Astrophysics

PONTIFICIA UNIVERSIDAD CATOLICA DE CHILE

Santiago, Chile