Gabriel AltayDepartment of PhysicsCarnegie Mellon University 8416 Wean Hall 5000 Forbes Avenue Pittsburgh, PA, 15224 USA
Email: gabriel.altay@gmail.com
Publications
SoftwareObservational LinksNational Radio Astronomy Observatory (NRAO) National Optical Astronomy Observatory (NOAO) National Solar Observatory (NSO) Murchison Widefield Array (MWA) Atacama Cosmology Telescope (ACT) South African Large Telescope (SALT) NASA/IPAC Extragalactic Database (NED) US National Virtual Observatory (NVO) NASA's Wilkinson Microwave Anisotropy Probe (WMAP) NASA's Legacy Archive for Microwave Background Data Analysis (LAMBDA) All-wavelength Extended Groth strip International Survey (AEGIS) Sloan Digital Sky Survey (SDSS) Sloan Digital Sky Survey - SkyServer (SDSS SkyServer) The Space Telescope Science Institute (STScI) Large Synoptic Survey Telescope (LSST) NASA's High Energy Astrophysics Science Archive Research Center (HEASARC)
Learning On Your Own!Astro 2010 Decadal Review |
Welcome to my research website. I've gathered together some things here that
are useful to me. Some of them may be useful for you as well. I'm currently
a graduate student in the
physics department of
Carnegie Mellon University
working under the guidance of
Rupert Croft .
The physics department is affiliated with the
Bruce and Astrid McWilliams Center for Cosmology
which brings together researchers in particle physics, astrophysics,
computer science, and statistics.
Research InterestsSPHRAYI am developing a radiative transfer code called SPHRAY. It ray traces through Smoothed Particle Hydrodynamics (SPH) density fields without griding the particles and so can preserve the symmetries and resolution of an SPH run. I have applied it to reionization simulations using 5123 particles sampled with hundreds of millions of rays. You can learn more about the code at the SPHRAY home page or by reading the SPHRAY code paper which is becoming slightly dated as the code evolves but contains a nice overview of the fundamental solution method. 21 cm CosmologyMany groups (see the observational links below) are preparing to observe the 21 cm signal from neutral hydrogen in the Universe before, during and after reionization. I would like to use SPHRAY (or any other software that proves to be a useful tool) to help connect 21 cm maps to the underlying cosmological density field. Lyman Systems
Lyman prefixed objects, namely Lyman-&alpha forests, Lyman limit systems
(LLSs), damped Lyman-&alpha systems (DLAs), and Lyman break galaxies (LBGs)
give us
many ways to gain information about cosmology, the intergalactic medium (IGM),
and active galaxies. I'm interested in squeezing more information out of
observations of these systems using simulations that track the ionization and
temperature state of gas in the presence of a realistic UV field that varies
in time and space.
Black Hole Galaxy Coevolution
Many galaxies, including our own, are believed to harbor super massive black holes at
their center. I am interested in exploring the feedback processes associated with
active galactic nuclei and their host galaxies both numerically (by exploring coupling
mechanisms using hydrodynamic simulations) and observationally (through SZ and lensing measurements)
Paper Organizer
I organize the papers I've read or am trying to read using a web service
called citeulike. Here is a
link
to my library.
Generally Useful LinksSoftware Installation Notes (Intel Fortran Compiler, MPICH2, FFTW) SQL searchable Millennium Simulation Database Fundamental Constants from NIST My Movies
Links to some movies I've made of my most recent reionization simulations.
grid_032_2fps.mp4 grid_064_3fps.mp4 grid_128_5fps.mp4 grid_256_5fps.mp4 grid_256_10fps.mp4 part_512_10fps.mp4 part_512_20fps.mp4 part_512_30fps.mp4 |
Page last modified: 21 Jul, 2008.