activity
19982016
most citedThe 3D power spectrum of galaxies from the SDSS

1.8k citations · 4.6k across the 33 of their papers we have counts for

collaborators

33 papers

astro-ph.GA2016★ 48 cited

On the Star Formation Properties of Void Galaxies

Crystal M. Moorman, Jackeline Moreno, Amanda White +4

We measure the star formation properties of two large samples of galaxies from the SDSS in large-scale cosmic voids on time scales of 10 Myr and 100 Myr, using H emission line s…

astro-ph.GA2015★ 30 cited

Spectral Properties of Galaxies in Void Regions

Chenxu Liu, Danny Pan, Lei Hao +3

We present a study of spectral properties of galaxies in underdense large-scale structures, voids. Our void galaxy sample (75,939 galaxies) is selected from the Sloan Digital Sky S…

astro-ph.GA2015★ 32 cited

The Optical Luminosity Function of Void Galaxies in the SDSS and ALFALFA Surveys

Crystal M. Moorman, Michael S. Vogeley, Fiona Hoyle +3

We measure the r-band galaxy luminosity function (LF) across environments over the redshift range 0<<0.107 using the SDSS. We divide our sample into galaxies residing in large s…

astro-ph.CO2015★ 5 cited

An observational detection of the bridge effect of void filaments

Junsup Shim, Jounghun Lee, Fiona Hoyle

The bridge effect of void filaments is a phrase coined by Park & Lee (2009b) to explain the correlations found in a numerical experiment between the luminosity of the void galaxies…

astro-ph.CO2014★ 5 cited

An observational signal of the void shape correlation and its link to the cosmic web

Jounghun Lee, Fiona Hoyle

The shapes of cosmic voids are prone to distortions by the external tidal forces since their low-densities imply a lower internal resistance. This susceptibility of the void shapes…

astro-ph.GA2014★ 49 cited

The HI Mass Function and Velocity Width Function of Void Galaxies in the Arecibo Legacy Fast ALFA Survey

Crystal M. Moorman, Michael S. Vogeley, Fiona Hoyle +3

We measure the HI mass function (HIMF) and velocity width function (WF) across environments over a range of masses , and profile widths $1.3\log(km…