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

14
Ricardo Demarco

Profesor Asociado

Astronomia

UNIVERSIDAD DE CONCEPCION, DEPARTAMENTO DE ASTRONOMIA

Concepcion, 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