activity
20022019
most citedEAZY: A Fast, Public Photometric Redshift Code

1.9k citations · 3.7k across the 33 of their papers we have counts for

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Showing astro-ph.COShow all

10 papers · 1 filter

astro-ph.CO2011★ 13 cited

A study of the color diversity around maximum light in Type Ia supernovae

Regis Cartier, Francisco Forster, Paolo Coppi +5

From a sample of 12 well-observed Type Ia supernovae, we find clear evidence of correlations between early phase (U-B), (V-R), and (V-I) colors and the velocity shifts of the [Fe I…

astro-ph.CO2010★ 79 cited

The Sudden Death of the Nearest Quasar

Kevin Schawinski, Daniel A. Evans, Shanil Virani +13

Galaxy formation is significantly modulated by energy output from supermassive black holes at the centers of galaxies which grow in highly efficient luminous quasar phases. The tim…

astro-ph.CO2010★ 5 cited

Overview of EXIST mission science and implementation

J. Grindlay, N. Gehrels, J. Bloom +14

The Energetic X-ray Imaging Survey Telescope (EXIST) is designed to i) use the birth of stellar mass black holes, as revealed by cosmic Gamma-Ray Bursts (GRBs), as probes of the ve…

astro-ph.CO2010★ 3 cited

Black hole growth and host galaxy morphology

Kevin Schawinski, C. Megan Urry, Shanil Virani +11

We use data from large surveys of the local Universe (SDSS+Galaxy Zoo) to show that the galaxy-black hole connection is linked to host morphology at a fundamental level. The fracti…

astro-ph.CO2010★ 195 cited

Galaxy Zoo: The fundamentally different co-evolution of supermassive black holes and their early- and late-type host galaxies

Kevin Schawinski, C. Megan Urry, Shanil Virani +18

We use data from the Sloan Digital Sky Survey and visual classifications of morphology from the Galaxy Zoo project to study black hole growth in the nearby Universe (z < 0.05) and…

astro-ph.CO2009

The EXIST view of Super-Massive Black Holes in the Universe

Roberto Della Ceca, Gabriele Ghisellini, Gianpiero Tagliaferri +9

With its large collection area, broad-band energy coverage from optical/NIR (0.3 to 2.2 micron) to soft/hard X-ray (0.1-600 keV), all-sky monitoring capability, and on-board follow…