A multiwavelength consensus on the main sequence of star-forming galaxies at z ∼ 2

scientific article

A multiwavelength consensus on the main sequence of star-forming galaxies at z ∼ 2 is …
instance of (P31):
scholarly articleQ13442814

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P819ADS bibcode2014MNRAS.443...19R
P818arXiv ID1406.1189
P356DOI10.1093/MNRAS/STU1110
P724Internet Archive IDarxiv-1406.1189

P50authorEmanuele DaddiQ56547981
Paola SantiniQ56550798
Giulia RodighieroQ56550799
Carlotta GruppioniQ56555893
Stefano BertaQ59675173
John D. SilvermanQ59675243
Dieter LutzQ62520019
Alberto FranceschiniQ68004078
Emeric Le Floc'hQ112583617
Francesca PozziQ112767807
Giovanni ZamoraniQ56555897
Benjamin MagnelliQ57079160
Giovanni CresciQ57315066
Daichi KashinoQ58914130
Ivano BaronchelliQ58914629
Paola AndreaniQ58916811
P2093author name stringA. Cimatti
A. Renzini
P. Popesso
H. Domínguez Sánchez
C. Mancini
P2860cites workThe Luminosity Function and Stellar Evolution.Q29013440
The Cosmic Evolution Survey (COSMOS): OverviewQ56567287
The evolving interstellar medium of star-forming galaxies since z = 2 as probed by their infrared spectral energy distributionsQ57710870
GOODS-Herschel measurements of the dust attenuation of typical star-forming galaxies at high redshift: observations of ultraviolet-selected galaxies at z ~ 2Q57710901
GOODS–Herschel: an infrared main sequence for star-forming galaxiesQ57710922
Comparison of star formation rates from Hα and infrared luminosity as seen byHerschelQ58035496
Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the schechter functionQ58035604
Mid- and far-infrared luminosity functions and galaxy evolution from multiwavelengthSpitzerobservations up toz ~ 2.5Q58035622
The impact of evolving infrared spectral energy distributions of galaxies on star formation rate estimatesQ58217207
Galaxy stellar mass assembly between 0.2 < z < 2 from the S-COSMOS surveyQ58489782
The COSMOS-WIRCam near-infrared imaging survey. I. BzK-selected passive and star-forming galaxy candidates at z {>~} 1.4Q58489794
Star formation and dust obscuration at z {approx} 2: galaxies at the dawn of downsizingQ58489833
Star formation rates and masses of z∼ 2 galaxies from multicolour photometryQ58490180
Star formation and mass assembly in high redshift galaxiesQ58907872
The FMOS-COSMOS survey of star-forming galaxies at z ~ 1.6. I. H{alpha}-based star formation rates and dust extinctionQ58908469
Galaxy structure and mode of star formation in the SFR-mass plane from z ~ 2.5 to z ~ 0.1Q58908687
The star formation history of mass-selected galaxies in the COSMOS fieldQ58908730
Multiwavelength Study of Massive Galaxies at z∼2. I. Star Formation and Galaxy GrowthQ58909666
The Population of BzK-selected ULIRGs at z ~ 2Q58909728
Star Formation in AEGIS Field Galaxies since z = 1.1: The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-forming GalaxiesQ58910042
The lesser role of starbursts in star formation at z = 2Q58910727
A New Photometric Technique for the Joint Selection of Star‐forming and Passive Galaxies at 1.4 ≲z≲ 2.5Q58910816
PACS Evolutionary Probe (PEP) – A Herschel key programQ58911973
The first Herschel view of the mass-SFR link in high-z galaxiesQ58912008
The star-formation rates of 1.5 < z < 2.5 massive galaxiesQ58912010
The SINS survey: SINFONI integral field spectroscopy of z ~ 2 star-forming galaxiesQ58912032
The SINS survey: modeling the dynamics of z ~ 2 galaxies and the high-z Tully-Fisher relationQ58912046
The reversal of the star formation-density relation in the distant universeQ58912075
Panchromatic spectral energy distributions ofHerschelsourcesQ58916322
P433issue1
P407language of work or nameEnglishQ1860
P921main subjectstar-forming galaxyQ109101277
P1104number of pages12
P304page(s)19–30
P577publication date2014-07-08
P1433published inMonthly Notices of the Royal Astronomical SocietyQ1536490
P1476titleA multiwavelength consensus on the main sequence of star-forming galaxies at z ∼ 2
P478volume443

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cites work (P2860)
Q58983738ALMA observations of cold molecular gas in AGN hosts at z ∼ 1.5 – evidence of AGN feedback?
Q58911833CO excitation of normal star-forming galaxies out to z = 1.5 as regulated by the properties of their interstellar medium
Q58911797Dust attenuation inz~ 1 galaxies fromHerscheland 3D-HST Hαmeasurements
Q58908178Dust properties of Lyman-break galaxies at z ~ 3
Q58908131Effect of the star formation histories on the SFR-M∗relation at z ≥ 2
Q46298043Galaxy evolution. Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang
Q56550194On the nature of Hα emitters atz∼ 2 from the HiZELS survey: physical properties, Lyα escape fraction and main sequence
Q58982060Physical properties of AGN host galaxies as a probe of supermassive black hole feeding mechanisms
Q58911812Satellite content and quenching of star formation in galaxy groups at z ~ 1.8
Q58908272Star formation and quenching among the most massive galaxies at z ∼ 1.7
Q58916839The KMOS Deep Survey (KDS) – I. Dynamical measurements of typical star-forming galaxies at z ≃ 3.5
Q57088385The SCUBA-2 Cosmology Legacy Survey: galaxies in the deep 850 μm survey, and the star-forming ‘main sequence’
Q58492565The evolving relation between star formation rate and stellar mass in the VIDEO survey sincez = 3
Q58035331The evolving star formation rate: M⋆relation and sSFR since z ≃ 5 from the VUDS spectroscopic survey
Q58911805The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV and [OII]λ3727 luminosities

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