PACS Evolutionary Probe (PEP) – A Herschel key program
A&A, 532 (2011) A90
Published online: 2011-07-28
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The PEP survey: evidence for intense star-forming activity in the majority of radio-selected AGN atz≳ 1
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KMOS3D: DYNAMICAL CONSTRAINTS ON THE MASS BUDGET IN EARLY STAR-FORMING DISKS*
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HOW ACCURATE ARE INFRARED LUMINOSITIES FROM MONOCHROMATIC PHOTOMETRIC EXTRAPOLATION?
Zesen Lin, Guanwen Fang and Xu KongThe Astronomical Journal 152 (6) 191 (2016)
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GAS FRACTION AND DEPLETION TIME OF MASSIVE STAR-FORMING GALAXIES AT z ∼ 3.2: NO CHANGE IN GLOBAL STAR FORMATION PROCESS OUT TO z > 3
E. Schinnerer, B. Groves, M. T. Sargent, A. Karim, P. A. Oesch, B. Magnelli, O. LeFevre, L. Tasca, F. Civano, P. Cassata and V. SmolčićThe Astrophysical Journal 833 (1) 112 (2016)
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THE COSMOS2015 CATALOG: EXPLORING THE 1 < z < 6 UNIVERSE WITH HALF A MILLION GALAXIES
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AGNfitter: A BAYESIAN MCMC APPROACH TO FITTING SPECTRAL ENERGY DISTRIBUTIONS OF AGNs
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HELP: star formation as a function of galaxy environment withHerschel
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Compact radio cores in radio-quiet active galactic nuclei
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Characterizing elusive, faint dusty star-forming galaxies: a lensed, optically undetected ALMA galaxy atz ~ 3.3
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Measures of galaxy dust and gas mass withHerschelphotometry and prospects for ALMA
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The spatially resolved dynamics of dusty starburst galaxies in az ∼ 0.4 cluster: beginning the transition from spirals to S0s
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Dust attenuation inz~ 1 galaxies fromHerscheland 3D-HST Hαmeasurements
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X-ray observations of dust obscured galaxies in theChandradeep field south
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REST-FRAME OPTICAL EMISSION LINES IN FAR-INFRARED-SELECTED GALAXIES AT z < 1.7 FROM THE FMOS-COSMOS SURVEY
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DUSTY STARBURSTS AND THE FORMATION OF ELLIPTICAL GALAXIES: A SCUBA-2 SURVEY OF Az= 1.46 CLUSTER
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Combining physical galaxy models with radio observations to constrain the SFRs of high-z dusty star-forming galaxies
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The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV and [OII]λ3727 luminosities
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SHARDS: A GLOBAL VIEW OF THE STAR FORMATION ACTIVITY ATz∼ 0.84 andz∼ 1.23
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The spectral energy distribution of the redshift 7.1 quasar ULAS J1120+0641
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COMBINED CO AND DUST SCALING RELATIONS OF DEPLETION TIME AND MOLECULAR GAS FRACTIONS WITH COSMIC TIME, SPECIFIC STAR-FORMATION RATE, AND STELLAR MASS
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Galaxy-wide outflows inz~ 1.5 luminous obscured quasars revealed through near-IR slit-resolved spectroscopy
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Star formation and quenching among the most massive galaxies at z ∼ 1.7
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COLDz: KARL G. JANSKY VERY LARGE ARRAY DISCOVERY OF A GAS-RICH GALAXY IN COSMOS
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Infrared-faint radio sources remain undetected at far-infrared wavelengths
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Compton thick AGN in the XMM-COSMOS survey
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X-shooter reveals powerful outflows in z ∼ 1.5 X-ray selected obscured quasi-stellar objects
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Trident: A three-pronged galaxy survey
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The composite nature of Dust-Obscured Galaxies (DOGs) atz ∼ 2–3 in the COSMOS field – I. A far-infrared view
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THE FMOS-COSMOS SURVEY OF STAR-FORMING GALAXIES AT z ∼ 1.6. III. SURVEY DESIGN, PERFORMANCE, AND SAMPLE CHARACTERISTICS
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Satellite content and quenching of star formation in galaxy groups atz~ 1.8
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The far-infrared/radio correlation and radio spectral index of galaxies in the SFR–M∗plane up toz~2
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ARE THE BULK OFz> 2HERSCHELGALAXIES PROTO-SPHEROIDS?
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Evolution of the dust emission of massive galaxies up toz= 4 and constraints on their dominant mode of star formation
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Mapping the average AGN accretion rate in the SFR–M* plane for Herschel★-selected galaxies at 0 < z ≤ 2.5
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