'Redshift distribution' presentation slideshows

Small Galaxy Groups Clustering and the Evolution of Galaxy Clustering

914 views • 73 slides

Large-Scale Structure in the DEEP2 Galaxy Redshift Survey

Large-Scale Structure in the DEEP2 Galaxy Redshift Survey. Jeffrey Newman Lawrence Berkeley National Laboratory. And The DEEP2 Team.

625 views • 46 slides

The Evolution of the Luminosity Function in Semi-Analytic models

The Evolution of the Luminosity Function in Semi-Analytic models. Bruno Henriques. Simon White, Gerard Lemson, Peter Thomas, Roderick Overzier, Qi Guo, Claudia Maraston. Henriques, Maraston, Monaco, et al., Astro-ph: 1009.1392. Henriques, et al., 2011, in prep. Guo et al. 2010. Stars.

500 views • 40 slides

DESpec survey strategy : realistic mock catalogue and target selection

DESpec survey strategy : realistic mock catalogue and target selection. Stephanie Jouvel , Filipe Abdalla , Huan Lin, James Annis , Richard Kron 22 jun 2011. PLAN : Investigate DESpec survey strategy. Build realistic Mock Catalogues of the DES + VISTA survey

543 views • 38 slides

511 views • 34 slides

...digerendo la pizza...

390 views • 29 slides

Neutrino from GRBs and hypernova remnants

425 views • 29 slides

Outline: Introduction Cosmological applications Systematics Summary

Cosmological studies with Weak Lensing Effects Zuhui Fan Dept. of Astronomy, Peking University. Outline: Introduction Cosmological applications Systematics Summary. Introduction Gravitational lensing effects arise from the light deflection by the intervening structures.

388 views • 27 slides

The Optically Unbiased GRB Host (TOUGH) sample

The Optically Unbiased GRB Host (TOUGH) sample. TOUGH 1: Survey Design and Catalogues (Hjorth et al.). TOUGH 2: Fundamental Properties (Malesani et al.). TOUGH 3: Redshift Distribution (Jakobsson et al.). TOUGH 4: Ly ? Emitters (Milvang-Jensen et al.).

301 views • 16 slides

SDSS spectra were used with the Hubble law to create a map

SDSS spectra were used with the Hubble law to create a map. This is an AGN Spectral Energy Distribution (SED). We are picking quasars since they outshine their host galaxy. Color. But redshift as well as temperature affects the color of a galaxy?. Resdshift : 1+z= l o/ l e. 8.

283 views • 15 slides

by Fidy A. RAMAMONJISOA MSc Project University of the Western Cape

Modelling radio galaxies in simulations: CMB contaminants and SKA / Meerkat sources. by Fidy A. RAMAMONJISOA MSc Project University of the Western Cape. Supervisor : Prof Catherine Cress. SKA 4 th annual Bursary Conference, Stellenbosch Institute for Advanced Study 03/12/09.

296 views • 14 slides

A Survey for Large Separation Lensing Among 9100 FIRST Quasars

A Survey for Large Separation Lensing Among 9100 FIRST Quasars. 1,2. 2. 4. 1. 3. 1- School of Physics and Astronomy and Wise Observatory, Tel-Aviv University, Tel-Aviv 69978, Israel 2-Max-Planck-Institut f?r Astronomie, K ? nigstuhl 17, D-69117 Heidelberg, Germany

115 views • 4 slides