Research lines: Galaxy clusters and their evolution through imaging, strong lensing and SZ signatures. Machine learning techniques to exploit large imaging surveys.
Current projects: Imaging surveys like VST-ATLAS and the Chilean U-band extension (UVAS). Follow up of SZ galaxy clusters. Quasars behind Clusters (QbC). Red-Sequence Cluster Surveys. MOONS Extragalactic Survey.
Research lines: Multi-wavelength studies of AGN structure, distant star-forming galaxies, and extragalactic transients
Looking to sponsor postdocs who can be incorporated into the following projects:
VLT/MOONS Extragalactic Survey - PUC is a member of the instrument team and PUC-MOONS team members (incl. Bauer, Treister, Barrientos, Padilla, Vanzi) are taking part in an SDSS-like guaranteed-time sky survey to acquire 0.6-1.8um spectra for >200,000 galaxies at z~1.5. PUC will be involved in the planning, observing, reduction and analysis of the spectra, and lead AGN and z>6 galaxy characterization programs. Sponsored postdocs would take part in the assembly of these samples (including new observations with Chilean facilities) and early commissioning campaigns.
LSST AGN and transients - PUC faculty Bauer and Treister are members of the LSST AGN working group and are involved in much of the preparatory work required to identify and study the AGNs that will be probed by LSST. At the moment the AGN working group is focusing on the Deep Drilling fields to generate effective truth tables to use with the fully sky survey. More generally, Bauer is involved in the development of the ALERCE broker for ZTF, HAT-PI, LSST, etc. Sponsored postdocs would take part in preparatory work (optimization of search algorithms, assembly of these samples, optimization of follow-up, etc), as well as help with the commissioning data and follow-up campaigns.
ALMA studies of AGNs and SMGs - Bauer is PI of ongoing programs to observe dusty star forming galaxies in the Frontier Fields and CDF-S survey regions, as well as co-I in several other surveys and individual studies. Sponsor postdocs with interferometry expertise would work on proprietary and archival data to place useful constraints on distant obscured star formation and black hole accretion.
X-ray studies of AGNs and extragalactic transients - Sponsored postdocs would exploit archive and new X-ray observations to test and probe AGN, TDEs, SNe, ULXs, and other objects.
Research lines: stellar structure and evolution; pulsating stars; variable stars and their use as tracers of Galactic structure, formation and evolution; extraction and classification of variable stars in large surveys; globular star clusters. A list of publications can be found at https://tinyurl.com/y5fccxdo. Currently involved in a variety of large-scale surveys, such as Catalina, VVV(X), and LSST. Postdoctoral candidates with an interest in exploring the synergies among these and other ongoing surveys, such as Gaia and TESS, are especially encouraged to apply. E-mail address for questions: firstname.lastname@example.org or email@example.com.
Research lines: stellar dynamics of galaxies and star clusters; stellar structure and evolution; stellar rotation; Milky Way and Local Group stellar populations; wide binaries
Looking for postdocs who could join and take the lead on any of the following projects:
Dynamical modeling (Jeans and discrete Schwarzchild) of the resolved stellar populations of nearby galaxies and star clusters (luminous and dark mass content and distribution, central black holes). Projects within the HSTPROMO collaboration.
Search and characterization of debris from the Magellanic Clouds using deep optical and near-infrared data wide field data.
Based on products of surveys such as APOGEE (as member of SDSS-IV), RAVE, K2, Gaia, TESS, etc., my team works on problems such as: the census of 2nd generation stars in the Galactic field, the rotational evolution of low-mass stars, rotation and lithium in red giants, gyrochronology, age determination of field stars, and others.
Gaia wide binaries and applications: wide binary formation channels, chemical tagging, the initial-to-final mass relation for white dwarfs, rotational evolution of low-mass stars, gyrochronology, halo dark matter constraints, testing gravity at the low acceleration regime, statistics of hierarchical triples, double white dwarfs with distant tertiaries as progenitors of type Ia supernovae, moving groups, wide binaries in other galaxies, etc.
Research lines: Observational studies of bright SN based on spectrophotometric evolution and polarization spectra, with special interest on luminous or subluminous Type Ia SNe. Theoretical studies of these events in collaboration with long term visiting professor Stephane Blondin. Empirical methods of distance estimation using SNe, with emphasis on Type II events. Intensive follow up of transients at early time using a dedicated, automated, 0.5m telescope.
Research lines: Galactic centre astrophysics; protoplanetary discs and planet–disc interactions; supermassive black hole binaries; star formation and dynamics in galactic nuclei.
Max Planck Partner Group on Galactic Centre Astrophysics: JC leads this group, established in collaboration with MPE in Garching. We are interested in gas dynamics, stellar winds, black hole accretion, stellar dynamics and star formation in the region around Sgr A*.
We are part of the Millennium Nucleus on Planet Formation (NPF), together with astronomers in nearby Valparaíso. At PUC we're mostly interested in modelling dust and gas dynamics, circumbinary and perturbed discs, and the effects of accretion feedback from growing planets.
We are also interested in massive black hole binaries, their interaction with accretion discs and background stars, and their decay due to gravitational wave emission.
For more details, please check our group website.
Research lines: CMB observations and instrumentation, CMB science, mm-wave extragalactic sources, SZ galaxy clusters.
Simons Observatory: participate in the design, field setup and first observations using the new generation of CMB experiments.
Atacama Cosmology Telescope: the new AdvACT dataset will cover 40% of the sky with unprecedented sensitivity and resolution, allowing for state of the are studies of CMB physics, galaxy clusters through tSZ and kSZ, CMB lensing, and B-mode search for primordial GW.
CLASS experiment: new W-band receivers have been installed, entering its scientific CMB observation phase. We participate from several aspects of the experiment, which will provide an independent measurement of primordial B-modes at large angular scales.
Drone-based antenna calibrators: we are developing mm-wave sources that can be flown on drones to measure the antenna response of CMB telescopes, including beam shape, polarization, sidelobes and bandpass calibration.
Research lines: Extragalactic Astronomy. Low surface brightness galaxies - Ultra diffuse galaxies. Properties of the galaxy distribution. Infrared extragalactic astronomy.
Current and potential projects:
A detailed study of the giant low surface brightness galaxy Malin 1.
Diffuse galaxies in Fornax and intracluster light (in collaboration with Thomas Puzia and team).
Formation and evolution of low surface brightness galaxies in the cosmic web, using simulations (in collaboration with Nelson Padilla).
Galaxy populations in the UVAS survey (in collaboration with Leopoldo Infante and Felipe Barrientos).
Formation of gigantic spiral arms in low surface brightness galaxies (in collaboration with Chanda Jog, India).
A detailed study of low surface brightness galaxies in the SDSS, in particular those edge-on spirals.
Research lines: Astrochemistry, prestellar cores, photo-dominated regions and protoplanetary disks.
- Chemistry in protoplanetary disks
- Complex organic molecules in PDRs
- Wide-field spectral-imaging of giant molecular clouds (ORION-B IRAM-30m Large Program http://iram.fr/~pety/ORION-B/)
Research lines: Discovery and characterization of extrasolar planets.
Current projects: HATSouth (http://hatsouth.org), CHAT (http://chat.hatsurveys.org), HATPI (http://hatpi.org), ACCESS (survey of transmission spectra with IMACS/Magellan)
Research lines: galaxy formation, structure formation, cosmology
Understanding the relation between dark matter haloes and galaxies via HOD and SHAM phenomenological models of clustering, and semi-analytic and hydro simulations.
Members of the GALFORM collaboration, studying effects of different merger tree codes, improving the treatment of angular momentum of galaxies.
SDSS-IV surveys eBOSS (cosmology via clustering measurements, bivariate functions for galaxy formation), MANGA (inhomogeneities in SF in galaxies)
Preparations for LSST with the Dark Energy Science Collaboration (DESC) constructing mock catalogues for survey design.
Research lines: formation and evolution of galaxies, galaxy scaling relations and morphologies, star cluster systems and stellar populations, population synthesis models, stellar content of the Milky Way (see also https://goo.gl/gajsd).
Current projects: Our group is leading the following large surveys:
Coma Cluster Core Project (C3PO)
Next Generation Fornax Survey (NGFS)
Survey of Centaurus A's Baryonic Structures (SCABS)
Next Generation Virgo Survey - Infrared (NGVS-IR)
GeMS/GSAOI Galactic Globular Cluster Survey (G4CS)
Panchromatic High-Resolution Spectroscopic Survey of LG Star Clusters
VIMOS Virgo Cluster Survey - The Baryonic Angular Momentum Content of Galaxy Halos
We have numerous projects related to the exploitation of these datasets as well as their follow-up projects that the candidate postdoctoral fellows could lead and/or fuse with their expertise. Our group has also recently commissioned a new H-alpha filter on DECam at CTIO, which opens various interesting follow-up opportunities for postdoctoral projects.
Research lines: High-energy astrophysics, neutron stars, stellar magnetic fields, high-energy gamma-ray emission, large-scale structure (group web site: http://www2.astro.puc.cl/answers/)
Very high energy gamma ray emission from dark matter decay/annihilation, pulsars, and other sources, prospects for the Cherenkov Telescope Array (CTA)
Neutron stars with stable magnetic field configurations or crust "mountains" as sources of continuous gravitational waves
Magnetic field evolution in neutron stars
Neutron star reheating processes: modeling of thermal evolution and spectral energy distribution, observational constraints from HST UV/optical observations of old pulsars
Pulsar and magnetar glitches & starquakes: phenomenology and modeling
Physical models of fast radio bursts
Gravitational collapse of superclusters of galaxies: constraints from the Shapley Supercluster
Research lines: Supermassive black hole growth, multiwavelength extragalactic surveys, galaxy mergers
Multiwavelength (ALMA, optical and near-IR IFUs, mid-IR imaging, X-rays) observations of AGN in major galaxy mergers. Member of the MODA (Multiwavelength Observations of Dual AGN) collaboration.
High redshift, z>5, AGN surveys. Formation of the first supermassive black hole seeds. Gas contents of high redshift AGN with ALMA.
High energy census of supermassive black holes. Member of the BASS collaboration.
AGN population synthesis models and studies of AGN structure.
Research lines: Old stellar populations in the Milky Way, with special emphasis in the Galactic bulge.
- High spatial resolution study of the Nuclear Bulge
- Chemical abundances and kinematics in the Galactic bulge with APOGEE, and in preparation for MOONS.
- Proper motions in the Galactic bulge and disk, from VVV and VVVX data. 3D kinematics + metallicity for bulge field stars.
- Search and confirmation of new star clusters.