Photo.png_thumb90

Christopher Paul Haines

Assistant Professor

Universidad de Atacama

Copiapó, Chile

Líneas de Investigación


(1) Cluster galaxy evolution and the impact of environmental processes on star-formation activity in galaxies (2) Assembly of massive galaxy clusters (3) Galaxy evolution

Educación

  •  Astrophysics, UNIVERSITY OF CENTRAL LANCASHIRE. Reino Unido, 2001
  •  Physics, UNIVERSITY OF CAMBRIDGE. Reino Unido, 1997

Experiencia Académica

  •   Assistant Professor Full Time

    UNIVERSIDAD DE ATACAMA

    Copiapó, Chile

    2019 - At present

  •   Post-doctoral researcher Full Time

    Osservatorio Astronomico de Brera

    Milan, Italia

    2015 - 2018

  •   Post-doctoral researcher Full Time

    UNIVERSIDAD DE CHILE

    Santiago, Chile

    2013 - 2015

  •   Post-doctoral researcher Full Time

    UNIVERSITY OF ARIZONA

    Tucson, Estados Unidos

    2011 - 2012

  •   Post-doctoral researcher Full Time

    UNIVERSITY OF BIRMINGHAM

    Birmingham, Reino Unido

    2007 - 2011

  •   Post-doctoral researcher Full Time

    Osservatorio Astronomico de Capodimonte

    Napoles, Italia

    2002 - 2007

Experiencia Profesional

  •   Assistant Professor Full Time

    Universidad de Atacama

    Copiapó, Chile

    2019 - At present


 

Article (72)

LoCuSS: exploring the connection between local environment, star formation, and dust mass in Abell 1758
A few StePS forward in unveiling the complexity of galaxy evolution: light-weighted stellar ages of intermediate-redshift galaxies with WEAVE
Detection of anti-correlation of hot and cold baryons in galaxy clusters
Forming One of the Most Massive Objects in the Universe: The Quadruple Merger in Abell 1758
LoCuSS: scaling relations between galaxy cluster mass, gas, and stellar content
Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.2 less than or similar to z less than or similar to 0.9
Slow-then-rapid quenching as traced by tentative evidence for enhanced metallicities of cluster galaxies at z similar to 0.2 in the slow quenching phase
The VIMOS Public Extragalactic Redshift Survey (VIPERS) Environment-size relation of massive passive galaxies at 0.5 <= z <= 0.8
A 3D Voronoi+Gapper Galaxy Cluster Finder in Redshift Space to z ? 0.2. II. An Abundant Cluster Population Dominated by Late-type Galaxies Unveiled
An Interacting Galaxy Pair at the Origin of a Light Echo
Cosmic dance in the Shapley Concentration Core I. A study of the radio emission of the BCGs and tailed radio galaxies
LoCuSS: pre-processing in galaxy groups falling into massive galaxy clusters at z=0.2
LoCuSS=> The infall of X-ray groups on to massive clusters
Shapley Supercluster Survey: Mapping the filamentary network connecting the clusters
The VIMOS Public Extragalactic Redshift Survey (VIPERS) AGN feedback in [NeV] emitters
The VIMOS Public Extragalactic Redshift Survey (VIPERS) The complexity of galaxy populations at 0.4 z 1.3 revealed with unsupervised machine-learning algorithms
A 3D Voronoi+Gapper Galaxy Cluster Finder in Redshift Space to z~0.2 I=> An Algorithm Optimized for the 2dFGRS
Galaxy cluster luminosities and colours, and their dependence on cluster mass and merger state
Galaxy evolution in merging clusters: The passive core of the "Train Wreck" cluster of galaxies, A520
The Complete Local Volume Groups Sample - I. Sample selection and X-ray properties of the high-richness subsample
The VIMOS Public Extragalactic Redshift Survey (VIPERS) Downsizing of the blue cloud and the influence of galaxy size on mass quenching over the last eight billion years
The VIMOS Public Extragalactic Redshift Survey (VIPERS) Star formation history of passive red galaxies
The VIMOS Public Extragalactic Redshift Survey (VIPERS) The coevolution of galaxy morphology and colour to z similar to 1
The VIMOS Public Extragalactic Redshift Survey (VIPERS) The distinct build-up of dense and normal massive passive galaxies
BUDHIES - III=> the fate of H I and the quenching of galaxies in evolving environments
Dry Merger Rate and Post-merger Fraction in the Coma Cluster Core
Early Science with the Large Millimeter Telescope: COOL BUDHIES I - a pilot study of molecular and atomic gas at z similar or equal to 0.2
LoCuSS=> exploring the selection of faint blue background galaxies for cluster weak-lensing
Shapley Supercluster Survey=> ram-pressure stripping versus tidal interactions in the Shapley supercluster
y LoCuSS: Testing hydrostatic equilibrium in galaxy clusters
A Herschel Study of 24um-Selected AGNs and Their Host Galaxies
GLACE survey=> OSIRIS/GTC tuneable filter H&#945; imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. I. Survey presentation, TF data reduction techniques, and catalogue
LoCuSS=> The Slow Quenching of Star Formation in Cluster Galaxies and the Need for Pre-processing
Shapley Supercluster Survey: construction of the photometric catalogues and i-band data release
THE RELATION BETWEEN LUMINOUS AGNs AND STAR FORMATION IN THEIR HOST GALAXIES
LoCuSS: the near-infrared luminosity and weak-lensing mass scaling relation of galaxy clusters
Shapley Supercluster Survey: Galaxy evolution from filaments to cluster cores
Star formation activity and gas stripping in the Cluster Projected Phase-Space (CPPS)
Star formation in the massive cluster merger Abell 2744
LoCuSS=> The Steady Decline and Slow Quenching of Star Formation in Cluster Galaxies over the Last Four Billion Years
ACCESS - V. Dissecting ram-pressure stripping through integral-field spectroscopy and multiband imaging
The drivers of AGN activity in galaxy clusters: AGN fraction as a function of mass and environment
A WEAK-LENSING AND NEAR-INFRARED STUDY OF A3192: DISASSEMBLING A RICHNESS CLASS 3 ABELL CLUSTER
LoCuSS: A DYNAMICAL ANALYSIS OF X-RAY ACTIVE GALACTIC NUCLEI IN LOCAL CLUSTERS
THE RELATION BETWEEN COOL CLUSTER CORES AND HERSCHEL-DETECTED STAR FORMATION IN BRIGHTEST CLUSTER GALAXIES
ACCESS - II. A complete census of star formation in the Shapley supercluster - UV and IR luminosity functions
ACCESS - III. The nature of star formation in the Shapley supercluster
ACCESS - IV. The quenching of star formation in a cluster population of dusty S0s
The evolution of dwarf galaxies in the Coma supercluster
ACCESS: NIR luminosity function and stellar mass function of galaxies in the Shapley supercluster environment
LoCuSS: A Herschel view of obscured star formation in Abell 1835
LoCuSS: connecting the dominance and shape of brightest cluster galaxies with the assembly history of massive clusters
LoCuSS: Probing galaxy transformation physics with Herschel
LoCuSS: Shedding new light on the massive lensing cluster Abell 1689-the view from Herschel
Star formation, starbursts and quenching across the Coma supercluster
LoCuSS: luminous infrared galaxies in the merging cluster Abell 1758 at z=0.28
LoCuSS: THE MID-INFRARED BUTCHER-OEMLER EFFECT
On the origin of the scatter around the Fundamental Plane: correlations with stellar population parameters
The Clowes-Campusano Large Quasar Group Survey. I. GALEX Selected Sample of Lyman Break Galaxies at z~1
Global properties of the rich cluster ABCG 209 at z similar to 0.2. Spectroscopic and photometric catalogue
The SDSS-GALEX viewpoint of the truncated red sequence in field environments at z similar to 0
THE SDSS-UKIDSS FUNDAMENTAL PLANE OF EARLY-TYPE GALAXIES
The different physical mechanisms that drive the star formation histories of giant and dwarf galaxies
Weak lensing mass reconstruction of the galaxy cluster Abell 209
Shapley optical survey - I. Luminosity functions in the supercluster environment
Shapley Optical Survey - II. The effect of environment on the colour-magnitude relation and galaxy colours
The different environmental dependencies of star formation for giant and dwarf galaxies
New insights into the structure of early-type galaxies: the Photometric Plane at z similar to 0.3
Detection of 20-30 h(-1) Mpc-scale galaxy structures embedded in 100 h(-1) Mpc-scale structures of quasars and MgII absorbers at z similar or equal to 0.8 and z similar or equal to 1.2
Galaxy evolution in the environment of ABCG 209
Transformations of galaxies in the environments of the cluster ABCG 209 at z similar to 0.2
The galaxy environment of a quasar at z = 1.226=> a possible cluster merger
58
Christopher Haines

Assistant Professor

Instituto de Astronomía y Ciencias Planetarias

Universidad de Atacama

Copiapó, Chile

1
Nancy Hitschfeld

Full Professor

Computer Science

UNIVERSIDAD DE CHILE , DEPTO CIENCIAS COMPUTACION

Santiago, Chile

1
Lorenzo Morelli

Profesor

Instituto de astronomia y ciencias planetarias

Universidad de Atacama

Copiapo, Chile

1
Yara Jaffé

Prof. Adjunto

Instituto de Fisica y Astronomia

Universidad de Valparaiso

Valparaiso, Chile