Man

Iván Andrés Lacerna Zambrano

profesor asistente

Universidad de Atacama

Copiapó, Chile

Líneas de Investigación


Elliptical galaxies; Large-scale environment properties such as two-halo conformity and assembly bias; Formation and evolution of galaxies

Educación

  •  Astrofísica, PONTIFICIA UNIVERSIDAD CATOLICA DE CHILE. Chile, 2012
  •  Astronomía, PONTIFICIA UNIVERSIDAD CATOLICA DE CHILE. Chile, 2005

Experiencia Académica

  •   profesor asistente Full Time

    UNIVERSIDAD DE ATACAMA

    Copiapó, Chile

    2019 - A la fecha

Experiencia Profesional

  •   investigador postdoctoral Full Time

    UNIVERSIDAD CATOLICA DEL NORTE

    Antofagasta, Chile

    2018 - 2019

  •   investigador postdoctoral Full Time

    Instituto Milenio de Astrofísica

    Santiago, Chile

    2017 - 2018

  •   Investigador postdoctoral Part Time

    Centro de Astroingeniería, Pontificia Universidad Católica de Chile

    Santiago, Chile

    2014 - 2016

  •   Support astronomer and telescope operator at MPG/ESO 2.2m telescope Part Time

    Max Planck Institute for Astronomy

    Observatorio La Silla, Chile

    2014 - 2016

  •   Astronomer for the operations of APOGEE-2 South Other

    Sloan Digital Sky Survey

    Observatorio Las Campanas, Chile

    2016 - 2019

  •   investigador postdoctoral Full Time

    Universidad Nacional Autónoma de México

    Ciudad de México, México

    2012 - 2014

  •   Deputy Lead Observer for the operations of APOGEE-2 South Other

    Sloan Digital Sky Survey IV

    Observatorio Las Campanas, Chile

    2018 - 2019


 

Article (48)

The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
An iterative method to deblend AGN-Host contributions for Integral Field spectroscopic observations
A comparative analysis of the chemical compositions of Gaia-Enceladus/Sausage and Milky Way satellites using APOGEE
SDSS-IV MaNGA: The Effect of Stellar Mass and Halo Mass on the Assembly Histories of Satellite Galaxies
The Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-V
The evolution of radial gradients of MaNGA quiescent elliptical galaxies: inside-out quenching or outer mass growth?
The H i content of red geyser galaxies
Infrared variability of young solar analogues in the Lagoon Nebula
New insights into the Triangulum Australis supercluster of galaxies
On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
SDSS IV MaNGA: visual morphological and statistical characterization of the DR15 sample
SDSS-IV MaNGA: How the Stellar Populations of Passive Central Galaxies Depend on Stellar and Halo Mass
SDSS-IV MaNGA: Identification and multiwavelength properties of Type-1 AGN in the DR15 sample
The differences between mass- and light-derived structural parameters over time for MaNGA elliptical galaxies
The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data
APOGEE Chemical Abundance Patterns of the Massive Milky Way Satellites
Signatures of Inflowing Gas in Red Geyser Galaxies Hosting Radio Active Galactic Nuclei
Homogeneous analysis of globular clusters from the APOGEE survey with the BACCHUS code - II. The Southern clusters and overview
Metallicity and alpha-Element Abundance Gradients along the Sagittarius Stream as Seen by APOGEE
SDSS-IV MaNGA: Global and local stellar population properties of elliptical galaxies
The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra
The Lazy Giants: APOGEE Abundances Reveal Low Star Formation Efficiencies in the Magellanic Clouds
The manifestation of secondary bias on the galaxy population from IllustrisTNG300
SDSS-IV MaNGA=> Environmental Dependence of the Mgb/< Fe >-sigma(*) Relation for Nearby Galaxies
SDSS-IV MaNGA=> Inside-out versus Outside-in Quenching of Galaxies in Different Local Environments
SDSS-IV MaNGA=> signatures of halo assembly in kinematically misaligned galaxies
The evolution of assembly bias
The Fifteenth Data Release of the Sloan Digital Sky Surveys=> First Release of MaNGA-derived Quantities, Data Visualization Tools, and Stellar Library
Field spheroid-dominated galaxies in a Lambda-CDM Universe
Galactic conformity measured in semi-analytic models
SDSS IV MaNGA=> Dependence of Global and Spatially Resolved SFR-M-* Relations on Galaxy Properties
SDSS-IV MaNGA=> constraints on the conditions for star formation in galaxy discs
The dependence of mass and environment on the secular processes of AGNs in terms of morphology, colour, and specific star-formation rate
The Fourteenth Data Release of the Sloan Digital Sky Survey=> First Spectroscopic Data from the Extended Baryon Oscillation Spectroscopic Survey and from the Second Phase of the Apache Point Observatory Galactic Evolution Experiment
The less significant role of large-scale environment than optical AGN in nearby, isolated elliptical galaxies
SDSS-IV MaNGA-resolved Star Formation and Molecular Gas Properties of Green Valley Galaxies=> A First Look with ALMA and MaNGA
Sloan Digital Sky Survey IV=> Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
The 13th Data Release of the Sloan Digital Sky Survey=> First Spectroscopic Data from the SDSS-IV Survey Mapping Nearby Galaxies at Apache Point Observatory
Evolution of Balmer jump selected galaxies in the ALHAMBRA survey
Isolated elliptical galaxies in the local Universe
Central galaxies in different environments=> Do they have similar properties?
The growth of galactic bulges through mergers in Lambda cold dark matter haloes revisited - II. Morphological mix evolution
The nature of assembly bias - III. Observational properties
GALAXY CLUSTERS IN THE LINE OF SIGHT TO BACKGROUND QUASARS. III. MULTI-OBJECT SPECTROSCOPY
The nature of assembly bias - II. Halo spin
The nature of assembly bias - I. Clues from a Lambda CDM cosmology
THE GLOBULAR CLUSTER NGC 5286. II. VARIABLE STARS
Galaxy clusters in the line of sight to background quasars - II. Environmental effects on the sizes of baryonic halo sizes

ConferencePaper (1)

Assembly bias: Clues from a ?CDM cosmology

Correction (1)

The H i content of red geyser galaxies (vol 519, pg 3312, 2023)
3
Sandro Villanova

Associate Profesor

Astronomy

UNIVERSIDAD DE CONCEPCION, DEPTO DE ASTRONOMIA

Concepcion, Chile

1
Douglas Geisler

Full Professor

Astronomy

UNIVERSIDAD DE CONCEPCION, DEPTO DE ASTRONOMIA

Concepcion, Chile

1
Nelson Padilla

Profesor Titular

Astrophysics

Universidad Católica de Chile

Santiago, Chile

2
Ricardo Munoz

Associate Professor

Astronomy

Universidad de Chile

Santiago, Chile

1
Médéric Boquien

Académico

Vicerrectoría de Investigación

UNIVERSIDAD DE ANTOFAGASTA

Antofagasta, Chile

2
Amelia Stutz

Associate Professor

Astronomy

UNIVERSIDAD DE CONCEPCION

Concepcion, Chile

2
Christian Nitschelm

Full professor

Sciences

Universidad de Antofagasta

Antofagasta, Chile

1
Eduardo Unda

Director

Universidad de Antofagasta

Antofagasta, Chile

3
José Fernández

Assistant Professor

Universidad de Atacama

Copiapo, Chile

1
Antonela Monachesi

Associate Professor

Astronomía

Universidad de La Serena

La Serena, Chile

3
Antonio Montero

Profesor Adjunto

Physics

Universidad Técnica Federico Santa María

Santiago, Chile

2
Christian Moni Bidin

Director

Vicerrectoría de Investigación y Desarrollo Tecnológico

Universidad Católica del Norte

Antofagasta, Chile

3
Maria Artale

Profesor Asistente

Departamento de Física y Astronomía

Universidad Andrés Bello

Santiago, Chile

1
Lorena Hernandez

Postdoc

Universidad de Valparaíso

Valparaiso, Chile

25
Iván Lacerna

profesor asistente

Instituto de Astronomía y Ciencias Planetarias

Universidad de Atacama

Copiapó, Chile

1
Camila Ordenes

Postdoc

PUC - Mas

Santiago, Chile