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19972026
most citedOverview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory

1.7k citations · 48.1k across the 484 of their papers we have counts for

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Showing 2011Show all

15 papers · 1 filter

astro-ph.CO2011★ 96 cited

Stellar metallicity of star-forming galaxies at z ~ 3

Veronica Sommariva, Filippo Mannucci, Giovanni Cresci +5

The stellar metallicity is a direct measure of the amount of metals present in a galaxy, as a large part of the metals lie in its stars. In this paper we investigate new stellar me…

astro-ph.CO2011★ 41 cited

The metallicity properties of zCOSMOS galaxies at 0.2<z<0.8

Giovanni Cresci, Filippo Mannucci, Veronica Sommariva +3

We study the metallicity properties of galaxies in the zCOSMOS sample between 0.2<z<0.8. At z<0.46, where Ha and [NII] are detected, we find the same dependence of metallicity on s…

astro-ph.CO2011★ 13 cited

FIR measurements of Ly- emitters at z1.0: dust attenuation from PACS-\emph{Herschel}

I. Oteo, A. Bongiovanni, A. M. Pérez García +24

One remaining open question regarding the physical properties of Ly emitters (LAEs) is their dust content and its evolution with redshift. The variety of results is large and wi…

astro-ph.CO2011★ 17 cited

Chemical properties in the most distant radio galaxy

Kenta Matsuoka, Tohru Nagao, Roberto Maiolino +2

We present a deep optical spectrum of TN J0924-2201, the most distant radio galaxy at z = 5.19, obtained with FOCAS on the Subaru Telescope. We successfully detect, for the first t…

astro-ph.CO2011★ 417 cited

On Star Formation Rates and Star Formation Histories of Galaxies out to z ~ 3

Stijn Wuyts, Natascha M. Forster Schreiber, Dieter Lutz +23

We compare multi-wavelength SFR indicators out to z~3 in GOODS-South. Our analysis uniquely combines U-to-8um photometry from FIREWORKS, MIPS 24um and PACS 70, 100, and 160um photo…

astro-ph.CO2011★ 22 cited

Is GRB 050904 at z=6.3 absorbed by dust?

G. Stratta, S. Gallerani, R. Maiolino

Claim of dust extinction for this GRB has been debated in the past. We suggest that the discrepant results occur primarily because most of previous studies have not simultaneously…

astro-ph.CO2011★ 503 cited

PACS Evolutionary Probe (PEP) - A Herschel Key Program

D. Lutz, A. Poglitsch, B. Altieri +35

Deep far-infrared photometric surveys studying galaxy evolution and the nature of the cosmic infrared background are a key strength of the Herschel mission. We describe the scienti…

astro-ph.CO2011★ 104 cited

The impact of evolving infrared spectral energy distributions of galaxies on star formation rate estimates

R. Nordon, D. Lutz, R. Genzel +27

We combine Herschel-PACS data from the PEP program with Spitzer 24 um and 16 um photometry and ultra deep IRS mid-infrared spectra, to measure the mid- to far-infrared spectral ene…

astro-ph.CO2011★ 30 cited

The PEP survey: clustering of infrared-selected galaxies and structure formation at z~2 in the GOODS South

M. Magliocchetti, P. Santini, G. Rodighiero +23

ABRIDGED-This paper presents the first direct estimate of the 3D clustering properties of far-infrared sources up to z~3. This has been possible thanks to the Pacs Evolutionary Pro…

astro-ph.CO2011★ 566 cited

Massive molecular outflows and negative feedback in ULIRGs observed by Herschel-PACS

E. Sturm, E. González-Alfonso, S. Veilleux +13

Mass outflows driven by stars and active galactic nuclei are a key element in many current models of galaxy evolution. They may produce the observed black hole-galaxy mass relation…

astro-ph.CO2011★ 5 cited

Sub-millimeter Detected z~2 Radio-quiet QSOs: Accurate Redshifts, Black Hole Masses, and Inflow/Outflow Velocities

Gustavo Orellana, Neil M. Nagar, Kate G. Isaac +5

We present near-IR spectroscopy of a sample of luminous (Lbol >10^14 Lsun), sub-millimeter-detected, dusty (M_dust~10^9 Msun), radio-quiet QSOs at z~2. We measure the redshift, wid…

astro-ph.CO2011★ 65 cited

Enhanced [CII] emission in a z=4.76 submillimetre galaxy

Carlos De Breuck, Roberto Maiolino, Paola Caselli +3

We present the detection of bright [CII] emission in the z=4.76 submillimetre galaxy LESS J033229.4-275619 using the Atacama Pathfinder EXperiment. This represents the highest reds…

astro-ph.IM2011★ 7 cited

ORIGIN: Metal Creation and Evolution from the Cosmic Dawn

J. W. den Herder, L. Piro, T. Ohashi +156

ORIGIN is a proposal for the M3 mission call of ESA aimed at the study of metal creation from the epoch of cosmic dawn. Using high-spectral resolution in the soft X-ray band, ORIGI…

astro-ph.CO2011★ 58 cited

The effect of environment on star forming galaxies at redshift 1 - First insight from PACS

P. Popesso, G. Rodighiero, A. Saintonge +4

We use deep 70, 100 and 160 um observations taken with PACS, the Photodetector Array Camera and Spectrometer on board of Herschel, as part of the PACS Evolutionary Probe (PEP) guar…

astro-ph.CO2011★ 4 cited

Optical-NIR spectra of quasars close to reionization (z~ 6)

V. D'Odorico, G. Cupani, S. Cristiani +14

X-shooter, with its characteristics of resolution, spectral coverage and efficiency, provides a unique opportunity to obtain spectra of the highest-redshift quasars (z ~ 6) that wi…