activity
20022026
most citedThe Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package

7.7k citations · 26.1k across the 145 of their papers we have counts for

collaborators
Showing 2008Show all

11 papers · 1 filter

astro-ph2008★ 154 cited

The environments of starburst and post-starburst galaxies at z=0.4-0.8

Bianca M. Poggianti, Alfonso Aragon-Salamanca, Dennis Zaritsky +16

Post-starburst (E+A or k+a) spectra, characterized by their exceptionally strong Balmer lines in absorption and the lack of emission lines, belong to galaxies in which the star for…

astro-ph2008★ 221 cited

Galaxy Zoo: Disentangling the Environmental Dependence of Morphology and Colour

Ramin A. Skibba, Steven P. Bamford, Robert C. Nichol +10

We analyze the environmental dependence of galaxy morphology and colour with two-point clustering statistics, using data from the Galaxy Zoo, the largest sample of visually classif…

astro-ph2008★ 49 cited

Galaxy Zoo: Chiral correlation function of galaxy spins

Anze Slosar, Kate Land, Steven Bamford +9

Galaxy Zoo is the first study of nearby galaxies that contains reliable information about the spiral sense of rotation of galaxy arms for a sizeable number of galaxies. We measure…

astro-ph2008★ 45 cited

Revealing components of the galaxy population through nonparametric techniques

Steven P. Bamford, Alex L. Rojas, Robert C. Nichol +4

The distributions of galaxy properties vary with environment, and are often multimodal, suggesting that the galaxy population may be a combination of multiple components. The behav…

astro-ph2008★ 3 cited

Galaxy And Mass Assembly (GAMA)

Simon P. Driver, the GAMA team

The GAMA survey aims to deliver 250,000 optical spectra (3--7Ang resolution) over 250 sq. degrees to spectroscopic limits of r_{AB} <19.8 and K_{AB}<17.0 mag. Complementary imaging…

astro-ph2008★ 155 cited

The relation between star formation, morphology and local density in high redshift clusters and groups

Bianca M. Poggianti, Vandana Desai, Rose Finn +17

We investigate how the [OII] properties and the morphologies of galaxies in clusters and groups at z=0.4-0.8 depend on projected local galaxy density, and compare with the field at…