Applying Observational Methods to Images of a Simulated High-Redshift Universe

Mathematics – Logic

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Flexible Image Transport (FITS) images produced from numerical cosmological simulations of dark and baryonic matter are analyzed using Source Extractor (SExtractor), a tool frequently used in observational image analysis. The goal is to assist the interpretation of simulation by better understanding how simulation data might appear in the observational domain.
The simulation model, based on Gadget-2 (Springel and Hernquist, 2003) includes gas heating, cooling and star formation. The stellar components of the model are processed by the Bruzual-Charlot (BC03) stellar population models to produce SEDs (Spectral Energy Distributions). These are then folded with different infrared filters, including selected filters from WFC3 and the proposed Near Infrared Camera (NIRCam) for the James Webb Space Telescope (JWST). The simulation data are taken at different redshifts from z 4 to 11, re-sized according to their comoving distances, converted to FITS format files and combined with noise to simulate instrument and background effects. The images are then analyzed with SExtractor to find groupings which are identified as galaxies or galaxy building blocks. Photometry is performed on these objects using SExtractor to extract luminosity functions in the emitted rest frames. Initially, minimal noise levels are used to allow fine details of the model to be "observed.” More realistic sky background levels are then added to estimate the effect of artifacts of observation.
We use these models to predict the faint-end Schechter slope evolution alpha(z). We compare these models to the most recent Hathi et al. (2010, ApJ, 720, 1708 ) data, and find good agreement in the faint end slope evolution: predicted alpha (7>z>5) = -1.7 to -1.8, observed alpha (z>5) = -1.75 .

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Applying Observational Methods to Images of a Simulated High-Redshift Universe does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Applying Observational Methods to Images of a Simulated High-Redshift Universe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Applying Observational Methods to Images of a Simulated High-Redshift Universe will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1205483

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.