Academicos


Leonardo Bronfman - Profesor Titular
Ph.D. en Astrofísica, 1986, U. de Columbia,EEUU.
Línea de Investigación: Nubes Moleculares, Formación Estelar, Estructura Galáctica.
Teléfono: 56 (2) 2 977 1113
E-mail: leo[at]das.uchile.cl

Áreas de Interes


My main line of research is the large scale distribution and the physical properties of molecular clouds and regions of massive star formation in the Milky Way. I carry on large scale surveys of the millimeter and sub millimeter line and continuum emission to determine statistically the physical properties of the gas and dust involved in the formation of massive stars. The most interesting regions from these large data bases are selected for individual studies, at the highest resolution and sensitivity available, to unveil the fairly unknown earliest phases of massive star formation.


Luis Campusano - Profesor Titular
Ph.D. en Astrofísica, 1992, U. de Toulousse, Francia.
Línea de Investigación: Cuasares, Cosmología.
Teléfono: 56 (2) 2 977 1100
E-mail: luis[at]das.uchile.cl

Áreas de Interes


Astrónomo Visitante de los observatorios: Interamericano de Cerro Tololo (Chile), Las Campanas (Carnegie Institution of Washington, Chile), La Silla (ESO, Chile) y Paranal (ESO, Chile).
Ha pertenecido a diversos directorios: del Observatorio Astronómico Gemini (2002-2007), de la Sociedad Chilena de Astronomía (2008, y de 2010 a la fecha). Y Director de la Oficina Conicyt para Proyecto Astronómico Gemini, Conicyt (2000-2006) y el Primer Director del Programa de Astronomía de Conicyt (2006 - 2007). En 2010 se desempeña como Profesor Visitante de la Yale University, New Haven.


Simón Casassus - Profesor Titular
Ph.D. en Astrofísica, 1999, U. de Oxford, Reino Unido.
Línea de Investigación: Nebulosas Planetarias, Formación Estelar.
Teléfono: 56 (2) 2 977 1137
E-mail: simon[at]das.uchile.cl
Webpage: http://www.das.uchile.cl/~simon/

Áreas de Interes


I am involved in the study of interstellar and circumstellar media. My areas of interests are:
1. The emission mechanisms at cm-wavelengths as diagnostics of the ISM, motivated by the discovery of a new component of radio continuum emission, presumably due to `spinning dust’. This work is mostly based on observations with the CBI radio-interformeter.
2. The nature of the cm-wave continuum in planetary nebulae (PNe).
3. The heterogeneity of the ISM on 100pc scales, using ¹²C/¹³C as tracer of the mixing of stellar yields. This work is based on optical high-resolution spectroscopy of molecular absorption lines.
4. High-resolution IR spectroscopy of planetary nebulae (PNe) aimed at constraining isotopic ratios throught the hyper-fine structure of ionic emission lines.


Edgardo Costa - Profesor Titular
Lic. en Astronomía, 1978, U. de Chile.
Línea de Investigación: Astrometría: Paralajes - Movimientos Propios - Cinemática del Grupo Local, Cúmulos Abiertos - Estructura Espiral.
Teléfono: 56 (2) 2 977 1116
E-mail: costa[at]das.uchile.cl

Áreas de Interes


El profesor Costa ha dictado un importante número de materias en la Universidad de Chile, dentro de los que se encuentran (en pre y postgrado): Astronomía General, Astronomía Experimental, Laboratorio de Astronomía, en otros.


Andrés Escala - Profesor Asistente
Ph.D., 2004, Yale University, EEUU.
Doctor en Ciencias, 2004, Universidad de Chile.
Línea de Investigación: Theoretical Astrophysics/Numerical Simulations, Massive Black Hole Mergers and Growth, Star and Galaxy Formation.
Teléfono: 56 (2) 2 977 1134
E-mail: aescala[at]das.uchile.cl

Áreas de Interes


My research interests spans in a broad range of topics in theoretical astrophysics, using both analytical and numerical (SPH and AMR techniques) approaches. My current interests are: BH Mergers, BH Growth and Star/Galaxy Formation.


Ricardo Finger - Profesor Asistente
Ph.D. en Ingenieria Eléctrica, 2013, U. de Chile, CHILE.
Licenciado en Física, 2004, U. de Chile, Chile
Línea de Investigación: Instrumentación Astronómica, Receptores Heterodinos, Procesamiento digital de señales, materiales.
Teléfono: 56 (2) 2 977 1150
E-mail: rfinger[at]das.uchile.cl

Áreas de Interes


I enjoy doing engineering and science. I have worked in telecommunications, technology integration, scientific research and scientific-technological projects. My expertise is mostly in laboratory work doing physics and astronomical instrumentation, as well as on-field commissioning of astronomical instruments. I am now mostly involved in instrumentation project engineering and management, as well as doing research on millimeter/sub-millimeter receivers, high speed radio-astronomy digital signal processing and getting into galactic astronomy.


Guido Garay - Profesor Titular
Ph.D. en Astronomía, 1983, U. de Harvard, EEUU.
Línea de Investigación: Medio Interestelar, Formación Estelar.
Teléfono: 56 (2) 2 977 1140-41
E-mail: guido[at]das.uchile.cl

Áreas de Interes


My research focus primarely on the study of a range of phenomena that are associated with the early stages of massive star formation: compact regions of ionized gas, massive and dense molecular cores, ionized jets, bipolar molecular outflows, and accretion disks. The goal is to determine the physical characteristics and dynamics of these objects in order to get a deeper understanding of how massive stars are formed and evolve. To accomplish this, I carry out single dish and interferometric observations at millimeter and centimeter wavelengths.


Mario Hamuy - Profesor Titular
Ph.D. en Astronomía, 2001, U. de Arizona, EEUU.
Línea de Investigación: Supernovas, Cosmología.
Teléfono: 56 (2) 2 977 1101
E-mail: mhamuy[at]das.uchile.cl
Webpage: http://www.das.uchile.cl/~mhamuy/

Áreas de Interes


I am interested in the study of supernovae. I am the principal investigator of the Millennium Center for Supernova Studies (MCSS), which includes 5 professors, 4 postdocs, 4 PhD students and more than 10 undergraduates. Our activities involve a nearby supernova search program (CHASE) using the PROMPT robotic telescopes located at Cerro Tololo, the development of our own 50 cm robotic telescope, and photometric and spectroscopic followup of selected supernovae. The main goal of the MCSS is the study of the physics of supernovae and their use as distance indicators.


Eduardo Hardy - Profesor Adjunto
Ph.D. en Astronomía, 1976, U. of Indiana, EEUU.
Línea de Investigación: Galaxias, Poblaciones Estelares, Cosmología.
E-mail: ehardy[at]das.uchile.cl

Áreas de Interes


Galaxies, Stellar Populations, Cosmology.
Representante en Chile, Associated Universities Inc., National Radio.


James Jenkins - Profesor Asistente
Ph.D., en Astronomía, 2007., U. de Hertfordshire, Reino Unido.
Línea de Investigación: Enanas café, Sistemas planetarios, Astrofísica Estelar, Planetas Extrasolares.
Teléfono: 56 (2) 2 977 1125
E-mail: jjenkins[at]das.uchile.cl
Webpage: http://www.das.uchile.cl/~jjenkins/

Áreas de Interes


I am PI of a long term effort to discover and characterise benchmark extrasolar planets (aka. exoplanets) in the southern hemisphere. The main goal is to detect short period transiting planets around bright stars where follow-up ground and space-based analysis can lead to further breakthroughs into the physics of exoplanetary atmospheres. In addition, we also aim to study and detect the lowest mass planets, down into the Earth-mass regime. We employ the radial-velocity technique to detect such systems, utilising instruments such as the HARPS spectrograph. HARPS is shown to be stable down to around 80cm/s in the long term on real stars and we aim to make use of such precision to detect planets down into the low mass rocky regime.


Paulina Lira - Profesora Asociado
Ph.D., en Astronomía, 1999., U. de Edimburgo, Reino Unido.
Línea de Investigación: Galaxias Activas, Galaxias.
Teléfono: 56 (2) 2 977 1138
E-mail: plira[at]das.uchile.cl

Áreas de Interes


I am mostly interested in AGN, at low and high redshift. We are trying to understand the variability properties of a large sample of AGN using the QUEST optical camera and NIR data from the UltraVista and VIDEO surveys. Also, we are following a small sample of local well known Seyferts using the SMARTS telecopes to determine their optical and NIR light curves. I'm also interested in the obscuration properties of AGN and we are studying the dusty torus for a well defined sample of nearby Seyferts using IR imaging in the 1-10 um range and with ALMA in the near future. Finally, I'm also interested in the feedback mechanisms operating in AGN and powerfull starburst, for which we are starting a program trying to determine the presence of large scale winds in nearby ULIRGs and high-redshift galaxies and in binary Black Holes, which can be searched using spectropolarimetric observations.


Sebastián López - Profesor Asociado
Ph.D. en Astronomía, 1999, U. of Hamburg, Alemania.
Línea de Investigación: Medio intergaláctico, Lentes gravitacionales.
Teléfono: 56 (2) 2 977 1135
E-mail: slopez[at]das.uchile.cl
Webpage: http://www.das.uchile.cl/~slopez/.

Áreas de Interes


I study the Intergalactic Medium and its interplay with galaxy formation and evolution. Absorption line spectra of distant QSO and GRB Afterglows allows one to probe the IGM over all along the Hubble time and over 10 orders of magnitude in HI column density, from the Ly-alpha forest through the damped Ly-alpha galaxies. Currently I am leading the ESO Large Programme "Quasars and their absorption lines: a legacy survey of the high redshift universe". Besides, I am interested in gravitational lensing, in galaxy clusters, and also in astrophysical tests of fundamental physical constants. Finally, I am also quite interested in finding new applications of probability and statistics to astrophysical problems. My personal web-page can be found here: http://www.das.uchile.cl/~slopez/.


Diego Mardones - Profesor Asociado
Ph.D. en Astronomía, 1998, U. de Harvard, EEUU.
Línea de Investigación: Formación estelar.
Teléfono: 56 (2) 2 977 1143
E-mail: dmardones[at]das.uchile.cl

Áreas de Interes


I am interested in studying all aspects of the star formation process itself. In particular in the closest low mass star forming regions in the southern hemisphere such as Chamaeleon, Lupus, Corona Australis and in mid-distance southern massive star forming regions in the first galactic quadrant.


José Maza - Profesor Titular
Ph.D., en Astronomía, 1979, U. de Toronto, Canada.
Premio Nacional de Ciencias 1999.
Línea de Investigación: Supernovas, Energía oscura, Galaxias Seyfert, Cuasares, Telescopía robótica.
Teléfono: 56 (2) 2 977 1102
E-mail: jmaza[at]das.uchile.cl

Áreas de Interes





René Méndez - Profesor Asociado
Ph.D., en Astronomía, 1995, Yale University, EEUU.
Línea de Investigación: Estructura Galáctica, Cinemática y Dinamica Estelar, Astrometría.
Teléfono: 56 (2) 2 977 1117
E-mail: rmendez[at]das.uchile.cl
Webpage: http://www.das.uchile.cl/~rmendez/

Áreas de Interes


My research focuses on the use of state-of-the-art, high-accuracy, astrometric techniques on digital detectors to address various problems of astrophysical interest, using also other complementary tools such as optical and near-IR photometry, numerical (Monte-Carlo type) simulations, and Galactic structure models. My specific topics of interest include:

• Studies of the solar neighborhood (within ~30 pc of the Sun): How complete is our census of the solar vicinity, especially in the southern hemisphere? What is the shape of luminosity function, especially for low mass stars? What is the space-density of nearby low-mass stellar systems?
• Galactic Structure and Kinematics: Comparisons between star-count models and observations. What are the global Galactic structural parameters? What is the nature of the Galactic thick-disk? What is the extent and shape of the Galactic Halo? What is the nature of dark-matter?
• Satellite Galaxies of the Milky Way: Dynamical status through their present-day positions, radial velocity and proper-motions. The relationship between star-formation episodes in these galaxies and their orbital properties. The Milky Way Gravitational potential at great distances from the Galactic Center (> 50 000 pc).
• Currently I am involved in the NPARSEC program (acronyms for NTT Parallaxes of Southern Extremely Cool Objects), led by Dr. Richard Smart at the Osservatorio Astronomico di Torino in Italy, and which is a major ESO Large Program that will perform high precision astrometric observations on ~100 nights over the next 3 years with the near-IR instrument SOFI at the ESO-La Silla NTT 3.5m telescope, for a sample of about 60 L and T-type nearby brown dwarfs. (see http://parsec.oato.inaf.it/nparsec.php) to obtain their trigonometric parallaxes with an expected accuracy of 2 milli-arc-seconds, or less.


Ricardo Muñoz - Profesor Asistente
Ph.D. Astronomía, 2008, Universidad de Virginia, EEUU.
Línea de Investigación: Galaxia esferoidales enanas, Materia oscura, Estructura del halo galactico, Nubes de Magallanes.
Teléfono: 56 (2) 2 977 1133
E-mail: rmunoz[at]das.uchile.cl

Áreas de Interes


My current interests are focused primarily on the evolution of dwarf galaxies (particularly dwarf spheroidal galaxies) and their interactions with our Milky Way. My work involves observational and computational (N-body simulations) studies of these systems aimed at understanding the role that Galactic tides play in shaping their properties. Dwarf spheroidal galaxies are the faintest and possibly the darkest (most dark-matter dominated) kind of galaxies in the universe. Besides being interesting systems in their own right, they provide us with significant constraints on current cosmological models and can potentially teach us something about the nature of dark matter.


Patricio Rojo - Profesor Asistente
Ph.D. Astronomía, 2006, Cornell University, EEUU.
Línea de Investigación: Planetas extrasolares, Asteroides del Sistema Solar, Poblaciones Estelares.
Teléfono: 56 (2) 2 977 1136
E-mail: projo[at]das.uchile.cl

Áreas de Interes


I study both extrasolar planets and minor bodies of the Solar System using ground based telescopes. In the former area, I specialize in exoatmospheric characterization through the study of high-precision transmission and/or emission spectra during transit or occultation, respectively.
I am also interested in targeted radial velocity exoplanet surveys and in the photometric monitoring of transit events to detect temporal variation. I also participate in minor body surveys and binary characterization. Other areas of research include stellar populations in the solar neighbourhood.


Mónica Rubio - Profesora Titular
Ph.D. en Astrofísica, 1992, U. de París, Francia.
Línea de Investigación: Nubes de Magallanes, Medio Interestelar, Nubes Moleculares, Formación Estelar.
Teléfono: 56 (2) 2 977 1111
E-mail: mrubio[at]das.uchile.cl

Áreas de Interes


My main stream research is the study of the properties and physical conditions of molecular clouds in the LMC and SMC, and its relation to massive star formation. The LMC and SMC offer a unique laboratory to perform this study. Their proximity and their different conditions of the ISM, constitute very good systems to study the formation of molecular clouds and the star formation process in low metallicty environments. The results of these investigations can give important clues to these processes in the early universe, where the abundance of heavier elements and the content of dust was much lower.


Maria Teresa Ruíz - Profesora Titular
Ph.D. en Astrofí,sica, 1975, U. de Princeton, EEUU.
Premio Nacional de Ciencias 1997.
Línea de Investigación: Enanas Blancas, Estrellas cercanas, Cúmulos Estelares.
Teléfono: 56 (2) 2 977 1115
E-mail: mtruiz[at]das.uchile.cl

Áreas de Interes