Cosmic star-formation history
P Madau, M Dickinson - Annual Review of Astronomy and …, 2014 - annualreviews.org
Over the past two decades, an avalanche of new data from multiwavelength imaging and
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …
Fitting the integrated spectral energy distributions of galaxies
J Walcher, B Groves, T Budavári, D Dale - Astrophysics and Space …, 2011 - Springer
Fitting the spectral energy distributions (SEDs) of galaxies is an almost universally used
technique that has matured significantly in the last decade. Model predictions and fitting …
technique that has matured significantly in the last decade. Model predictions and fitting …
[HTML][HTML] GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with∼ 4,000,000 Galaxies at z∼ 2–7: Galaxy–AGN Transition, Star Formation Efficiency, and …
We present new measurements of rest-UV luminosity functions and angular correlation
functions from 4,100,221 galaxies at z∼ 2–7 identified in the Subaru/Hyper Suprime-Cam …
functions from 4,100,221 galaxies at z∼ 2–7 identified in the Subaru/Hyper Suprime-Cam …
UV luminosity functions at redshifts z∼ 4 to z∼ 10: 10,000 galaxies from HST legacy fields
RJ Bouwens, GD Illingworth, PA Oesch… - The Astrophysical …, 2015 - iopscience.iop.org
ABSTRACT The remarkable Hubble Space Telescope (HST) data sets from the CANDELS,
HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the …
HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the …
How do galaxies get their gas?
D Kereš, N Katz, DH Weinberg… - Monthly Notices of the …, 2005 - academic.oup.com
We examine the temperature history of gas accreted by forming galaxies in smoothed
particle hydrodynamics simulations. About half of the gas follows the track expected in the …
particle hydrodynamics simulations. About half of the gas follows the track expected in the …
[HTML][HTML] Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey
O Ilbert, S Arnouts, HJ Mccracken, M Bolzonella… - Astronomy & …, 2006 - aanda.org
Aims. We present and release photometric redshifts for a uniquely large and deep sample of
522286 objects with in the Canada-France Hawaii Telescope Legacy Survey …
522286 objects with in the Canada-France Hawaii Telescope Legacy Survey …
Cosmos photometric redshifts with 30-bands for 2-deg2
COSMOS PHOTOMETRIC REDSHIFTS WITH 30-BANDS FOR 2-deg2 - IOPscience Skip to
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content IOP Science home Accessibility Help Search Journals Journals list Browse more than …
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 …