This paper presents stellar mass functions and i-band luminosity functions for Sloan Digital Sky Survey (SDSS) galaxies at $i 10^{11.4}$ between $0.2 <z <0.7$, with completeness falling significantly at redshifts higher than 0.7, and at lower masses. Large photometric datasets will be available in the near future (DECaLS, DES, Euclid), so this, and similar techniques will become increasingly useful in order to fully utilise this data
HG, ZZ, and IZ were supported by NSF grant AST-0907947. ZZ was partially supported by NSF grant AST-...
International audienceContext. The next generation of galaxy surveys will provide cluster catalogues...
International audienceObtaining large samples of galaxy clusters is important for cosmology: cluster...
This paper presents stellar mass functions and i-band luminosity functions for Sloan Digital Sky Sur...
International audienceWe measure the stellar mass function (SMF) and stellar mass density of galaxie...
We measure the redshift-dependent luminosity function and the comoving radial density of galaxies in...
In this thesis I investigate galaxy evolution by measuring the luminosity functions of galaxies acro...
We propose a novel method to constrain the missing fraction of galaxies using galaxy clustering meas...
We present baryon acoustic oscillation (BAO) scale measurements determined from the clustering of 1....
Citation: Howlett, C., Ross, A. J., Samushia, L., Percival, W. J., & Manera, M. (2015). The clusteri...
© 2019. The American Astronomical Society. All rights reserved. We measured evolution of the K-band ...
A clean measurement of the evolution of the galaxy cluster mass function can significantly improve o...
We study the evolution of star-forming galaxies with 10 10 M ⊙ < M ∗ < 10 11.6 M ⊙ over the redshift...
HG, ZZ, and IZ were supported by NSF grant AST-0907947. ZZ was partially supported by NSF grant AST-...
International audienceContext. The next generation of galaxy surveys will provide cluster catalogues...
International audienceObtaining large samples of galaxy clusters is important for cosmology: cluster...
This paper presents stellar mass functions and i-band luminosity functions for Sloan Digital Sky Sur...
International audienceWe measure the stellar mass function (SMF) and stellar mass density of galaxie...
We measure the redshift-dependent luminosity function and the comoving radial density of galaxies in...
In this thesis I investigate galaxy evolution by measuring the luminosity functions of galaxies acro...
We propose a novel method to constrain the missing fraction of galaxies using galaxy clustering meas...
We present baryon acoustic oscillation (BAO) scale measurements determined from the clustering of 1....
Citation: Howlett, C., Ross, A. J., Samushia, L., Percival, W. J., & Manera, M. (2015). The clusteri...
© 2019. The American Astronomical Society. All rights reserved. We measured evolution of the K-band ...
A clean measurement of the evolution of the galaxy cluster mass function can significantly improve o...
We study the evolution of star-forming galaxies with 10 10 M ⊙ < M ∗ < 10 11.6 M ⊙ over the redshift...
HG, ZZ, and IZ were supported by NSF grant AST-0907947. ZZ was partially supported by NSF grant AST-...
International audienceContext. The next generation of galaxy surveys will provide cluster catalogues...
International audienceObtaining large samples of galaxy clusters is important for cosmology: cluster...