The james webb space telescope
JP Gardner, JC Mather, M Clampin, R Doyon… - Space Science …, 2006 - Springer
Abstract The James Webb Space Telescope (JWST) is a large (6.6 m), cold (< 50 K), infrared
(IR)-optimized space observatory that will be launched early in the next decade into orbit …
(IR)-optimized space observatory that will be launched early in the next decade into orbit …
Weak gravitational lensing
M Bartelmann, P Schneider - Physics Reports, 2001 - Elsevier
We review theory and applications of weak gravitational lensing. After summarising
Friedmann–Lemaı̂tre cosmological models, we present the formalism of gravitational …
Friedmann–Lemaı̂tre cosmological models, we present the formalism of gravitational …
A critical assessment of photometric redshift methods: a CANDELS investigation
T Dahlen, B Mobasher, SM Faber… - The Astrophysical …, 2013 - iopscience.iop.org
We present results from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy
Survey (CANDELS) photometric redshift methods investigation. In this investigation, the …
Survey (CANDELS) photometric redshift methods investigation. In this investigation, the …
Bayesian photometric redshift estimation
N Benitez - The Astrophysical Journal, 2000 - iopscience.iop.org
Photometric redshifts are quickly becoming an essential tool of observational cosmology,
although their utilization is somewhat hindered by certain shortcomings of the existing …
although their utilization is somewhat hindered by certain shortcomings of the existing …
Measuring and modelling the redshift evolution of clustering: the Hubble Deep Field North
S Arnouts, S Cristiani, L Moscardini… - Monthly Notices of …, 1999 - academic.oup.com
The evolution of galaxy clustering from z= 0 to z≃ 4.5 is analysed using the angular
correlation function and the photometric redshift distribution of galaxies brighter than I AB …
correlation function and the photometric redshift distribution of galaxies brighter than I AB …
Photometric redshifts based on standard SED fitting procedures
M Bolzonella, JM Miralles, R Pelló - Arxiv preprint astro-ph/0003380, 2000 - arxiv.org
In this paper we study the accuracy of photometric redshifts computed through a standard
SED fitting procedure, where SEDs are obtained from broad-band photometry. We present …
SED fitting procedure, where SEDs are obtained from broad-band photometry. We present …
The nature of high-redshift galaxies
RS Somerville, JR Primack… - Monthly Notices of the …, 2001 - academic.oup.com
Using semi-analytic models of galaxy formation set within the cold dark matter (CDM)
merging hierarchy, we investigate several scenarios for the nature of the high-redshift) …
merging hierarchy, we investigate several scenarios for the nature of the high-redshift) …
Power spectrum tomography with weak lensing
W Hu - The Astrophysical Journal, 1999 - iopscience.iop.org
Upcoming weak lensing surveys on wide fields will provide the opportunity to reconstruct the
structure along the line of sight tomographically by employing photometric redshift …
structure along the line of sight tomographically by employing photometric redshift …
Photometric redshift analysis in the Dark Energy Survey science verification data
C Sánchez, M Carrasco Kind, H Lin… - Monthly Notices of …, 2014 - academic.oup.com
We present results from a study of the photometric redshift performance of the Dark Energy
Survey (DES), using the early data from a Science Verification period of observations in late …
Survey (DES), using the early data from a Science Verification period of observations in late …
PHAT: PHoto-z accuracy testing
H Hildebrandt, S Arnouts, P Capak… - Astronomy & …, 2010 - aanda.org
Context. Photometric redshifts (photo-z's) have become an essential tool in extragalactic
astronomy. Many current and upcoming observing programmes require great accuracy of …
astronomy. Many current and upcoming observing programmes require great accuracy of …