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19962021
most citedSpectroscopic Needs for Imaging Dark Energy Experiments: Photometric Redshift Training and Calibration

97 citations · 223 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2021★ 7 cited

CLMM: a LSST-DESC Cluster weak Lensing Mass Modeling library for cosmology

M. Aguena, C. Avestruz, C. Combet +22

We present the v1.0 release of CLMM, an open source Python library for the estimation of the weak lensing masses of clusters of galaxies. CLMM is designed as a standalone toolkit o…

astro-ph.CO2019★ 1 cited

Measuring the Hubble Constant Near and Far in the Era of ELT's

Rachael L. Beaton, Simon Birrer, Ian Dell'Antonio +7

Many of the fundamental physical constants in Physics, as a discipline, are measured to exquisite levels of precision. The fundamental constants that define Cosmology, however, are…

astro-ph.CO2013★ 97 cited

Spectroscopic Needs for Imaging Dark Energy Experiments: Photometric Redshift Training and Calibration

J. Newman, A. Abate, F. Abdalla +58

Large sets of objects with spectroscopic redshift measurements will be needed for imaging dark energy experiments to achieve their full potential, serving two goals:_training_, i.e…

astro-ph.CO2010★ 24 cited

Empirical optical k-Corrections for redshifts <= 0.7

Eduard Westra, Margaret J. Geller, Michael J. Kurtz +2

The Smithsonian Hectospec Lensing Survey (SHELS) is a magnitude limited spectroscopically complete survey for R<=21.0 covering 4 square degrees. SHELS provides a large sample (15,5…

astro-ph2004★ 15 cited

The Brera Multi-scale Wavelet HRI Cluster Survey: I Selection of the Sample and Number Counts

A. Moretti, L. Guzzo, S. Campana +7

We describe the construction of the Brera Multi-scale Wavelet (BMW) HRI Cluster Survey, a deep sample of serendipitous X-ray selected clusters of galaxies based on the ROSAT HRI ar…

astro-ph1996★ 79 cited

Galaxy Dark Matter: Galaxy-Galaxy Lensing in the Hubble Deep Field

Ian P. Dell'Antonio, J. Anthony Tyson

In this Letter we present calibrated observations of the average mass of galaxies with 22< I < 25 in the Hubble Deep Field. We measure the mean mass profile using the statistical g…