activity
20082017
most citedThe Baryon Oscillation Spectroscopic Survey of SDSS-III

2.1k citations · 8.3k across the 20 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

13 papers · 1 filter

astro-ph.CO2014★ 89 cited

Observations of environmental quenching in groups in the 11 Gyr since z=2.5: different quenching for central and satellite galaxies

Tomer Tal, Avishai Dekel, Pascal Oesch +16

We present direct observational evidence for star formation quenching in galaxy groups in the redshift range 0<z<2.5. We utilize a large sample of nearly 6000 groups, selected by f…

astro-ph.CO2013★ 181 cited

CANDELS+3D-HST: compact SFGs at z~2-3, the progenitors of the first quiescent galaxies

G. Barro, S. M. Faber, P. G. Perez-Gonzalez +32

We analyze the star-forming and structural properties of 45 massive (log(M/Msun)>10) compact star-forming galaxies (SFGs) at 2<z<3 to explore whether they are progenitors of compac…

astro-ph.CO2013★ 33 cited

Galaxy environments over cosmic time: the non-evolving radial galaxy distributions around massive galaxies since z=1.6

Tomer Tal, Pieter G. van Dokkum, Marijn Franx +3

We present a statistical study of the environments of massive galaxies in four redshift bins between z=0.04 and z=1.6, using data from the Sloan Digital Sky Survey (SDSS) and the N…

astro-ph.CO2012★ 2.1k cited

The Baryon Oscillation Spectroscopic Survey of SDSS-III

Kyle S. Dawson, David J. Schlegel, Christopher P. Ahn +162

The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger volume than the…

astro-ph.CO2012★ 699 cited

3D-HST: A wide-field grism spectroscopic survey with the Hubble Space Telescope

Gabriel Brammer, Pieter van Dokkum, Marijn Franx +27

We present 3D-HST, a near-infrared spectroscopic Treasury program with the Hubble Space Telescope for studying the processes that shape galaxies in the distant Universe. 3D-HST pro…

astro-ph.CO2012★ 39 cited

Observations of dark and luminous matter: the radial distribution of satellite galaxies around massive red galaxies

Tomer Tal, David A. Wake, Pieter G. van Dokkum

We study the projected radial distribution of satellite galaxies around more than 28,000 Luminous Red Galaxies (LRGs) at 0.28<z<0.40 and trace the gravitational potential of LRG gr…

astro-ph.CO2011★ 117 cited

First Results from the 3D-HST Survey: The Striking Diversity of Massive Galaxies at z>1

Pieter G. van Dokkum, Gabriel Brammer, Mattia Fumagalli +26

We present first results from the 3D-HST program, a near-IR spectroscopic survey performed with the Wide Field Camera 3 on the Hubble Space Telescope. We have used 3D-HST spectra t…

astro-ph.CO2011★ 38 cited

Mass growth and mergers: direct observations of the luminosity function of LRG satellite galaxies out to z=0.7 from SDSS and BOSS images

Tomer Tal, David A. Wake, Pieter G. van Dokkum +4

We present a statistical study of the luminosity functions of galaxies surrounding luminous red galaxies (LRGs) at average redshifts <z>=0.34 and <z>=0.65. The luminosity functions…

astro-ph.CO2011★ 495 cited

The NEWFIRM Medium-band Survey: Photometric Catalogs, Redshifts and the Bimodal Color Distribution of Galaxies out to z~3

Katherine E. Whitaker, Ivo Labbe, Pieter G. van Dokkum +15

We present deep near-infrared (NIR) medium-bandwidth photometry over the wavelength range 1-1.8 microns in the All-wavelength Extended Groth strip International Survey (AEGIS) and…

astro-ph.CO2011★ 81 cited

The faint stellar halos of massive red galaxies from stacks of more than 42000 SDSS LRG images

Tomer Tal, Pieter van Dokkum

We study the properties of massive galaxies at an average redshift of z~0.34 through stacking more than 42000 images of Luminous Red Galaxies from the Sloan Digital Sky Survey. Thi…

astro-ph.CO2009★ 818 cited

The Growth of Massive Galaxies Since z=2

Pieter G. van Dokkum, Katherine E. Whitaker, Gabriel Brammer +11

We study the growth of massive galaxies from z=2 to the present using data from the NEWFIRM Medium Band Survey. The sample is selected at a constant number density of n=2x10^-4 Mpc…

astro-ph.CO2009

Searching for a Gravitational Heating Signature in Nearby Luminous Ellipticals

Tomer Tal, Pieter G. van Dokkum, Jeffrey D. P. Kenney

We present a new deep optical study of a luminosity limited sample of nearby elliptical galaxies, attempting to observe the effects of gravitational interactions on the ISM of thes…

astro-ph.CO2009★ 271 cited

The Frequency of Tidal Features Associated with Nearby Luminous Elliptical Galaxies from a Statistically Complete Sample

Tomer Tal, Pieter G. van Dokkum, Jenica Nelan +1

We present a deep broadband optical imaging study of a complete sample of luminous elliptical galaxies (M_B<-20) at distances 15 Mpc - 50 Mpc, selected from the Tully catalog of ne…