output
20022009
most citedMeasurement of the Cosmic Ray e+ plus e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope

911 citations

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20 papers · 1 filter

astro-ph.CO200921 cited

Multi-wavelength properties of Spitzer-selected starbursts at z~2

N. Fiolet, A. Omont, M. Polletta +17

A complete sample of 33 sources believed to be starbursts ("5.8micron-peakers") was selected in the (0.5 sq. deg.) J1046+56 field with selection criteria F_(24micron)>400muJy, the…

astro-ph.CO2009

Kinematic and Structural Evolution of Field and Cluster Spiral Galaxies

Bodo L. Ziegler, Elif Kutdemir, Cristiano Da Rocha +3

To understand the processes that build up galaxies we investigate the stellar structure and gas kinematics of spiral and irregular galaxies out to redshift 1. We target 92 galaxies…

astro-ph.CO200985 cited

Warm Molecular Hydrogen in the Galactic Wind of M82

S. Veilleux, D. S. N. Rupke, R. Swaters

We report the detection of a complex of extraplanar warm H_2 knots and filaments extending more than ~3 kpc above and below the galactic plane of M82, roughly coincident with the w…

astro-ph.CO2009292 cited

The Black Hole Mass, Stellar M/L, and Dark Halo in M87

Karl Gebhardt, Jens Thomas

We model the dynamical structure of M87 (NGC4486) using high spatial resolution long-slit observations of stellar light in the central regions, two-dimensional stellar light kinema…

astro-ph.CO200993 cited

The evolution of early and late type galaxies in the COSMOS up to z~1.2

Maurilio Pannella, Armin Gabasch, Yuliana Goranova +6

The Cosmic Evolution Survey (COSMOS) allows for the first time a highly significant census of environments and structures up to redshift one, as well as a full morphological descri…

astro-ph.CO200948 cited

Color Distributions, Number and Mass Densities of Massive Galaxies at 1.5 < z < 3: Comparing Observations with Merger Simulations

Stijn Wuyts, Marijn Franx, Thomas J. Cox +9

We present a comparison between the observed color distribution, number and mass density of massive galaxies at 1.5 < z < 3 and a model by Hopkins et al. that relates the quasar an…