scholarly article | Q13442814 |
P819 | ADS bibcode | 2014MNRAS.443...19R |
P818 | arXiv ID | 1406.1189 |
P356 | DOI | 10.1093/MNRAS/STU1110 |
P724 | Internet Archive ID | arxiv-1406.1189 |
P50 | author | Emanuele Daddi | Q56547981 |
Paola Santini | Q56550798 | ||
Giulia Rodighiero | Q56550799 | ||
Carlotta Gruppioni | Q56555893 | ||
Stefano Berta | Q59675173 | ||
John D. Silverman | Q59675243 | ||
Dieter Lutz | Q62520019 | ||
Alberto Franceschini | Q68004078 | ||
Emeric Le Floc'h | Q112583617 | ||
Francesca Pozzi | Q112767807 | ||
Giovanni Zamorani | Q56555897 | ||
Benjamin Magnelli | Q57079160 | ||
Giovanni Cresci | Q57315066 | ||
Daichi Kashino | Q58914130 | ||
Ivano Baronchelli | Q58914629 | ||
Paola Andreani | Q58916811 | ||
P2093 | author name string | A. Cimatti | |
A. Renzini | |||
P. Popesso | |||
H. Domínguez Sánchez | |||
C. Mancini | |||
P2860 | cites work | The Luminosity Function and Stellar Evolution. | Q29013440 |
The Cosmic Evolution Survey (COSMOS): Overview | Q56567287 | ||
The evolving interstellar medium of star-forming galaxies since z = 2 as probed by their infrared spectral energy distributions | Q57710870 | ||
GOODS-Herschel measurements of the dust attenuation of typical star-forming galaxies at high redshift: observations of ultraviolet-selected galaxies at z ~ 2 | Q57710901 | ||
GOODS–Herschel: an infrared main sequence for star-forming galaxies | Q57710922 | ||
Comparison of star formation rates from Hα and infrared luminosity as seen byHerschel | Q58035496 | ||
Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the schechter function | Q58035604 | ||
Mid- and far-infrared luminosity functions and galaxy evolution from multiwavelengthSpitzerobservations up toz ~ 2.5 | Q58035622 | ||
The impact of evolving infrared spectral energy distributions of galaxies on star formation rate estimates | Q58217207 | ||
Galaxy stellar mass assembly between 0.2 < z < 2 from the S-COSMOS survey | Q58489782 | ||
The COSMOS-WIRCam near-infrared imaging survey. I. BzK-selected passive and star-forming galaxy candidates at z {>~} 1.4 | Q58489794 | ||
Star formation and dust obscuration at z {approx} 2: galaxies at the dawn of downsizing | Q58489833 | ||
Star formation rates and masses of z∼ 2 galaxies from multicolour photometry | Q58490180 | ||
Star formation and mass assembly in high redshift galaxies | Q58907872 | ||
The FMOS-COSMOS survey of star-forming galaxies at z ~ 1.6. I. H{alpha}-based star formation rates and dust extinction | Q58908469 | ||
Galaxy structure and mode of star formation in the SFR-mass plane from z ~ 2.5 to z ~ 0.1 | Q58908687 | ||
The star formation history of mass-selected galaxies in the COSMOS field | Q58908730 | ||
Multiwavelength Study of Massive Galaxies at z∼2. I. Star Formation and Galaxy Growth | Q58909666 | ||
The Population of BzK-selected ULIRGs at z ~ 2 | Q58909728 | ||
Star Formation in AEGIS Field Galaxies since z = 1.1: The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-forming Galaxies | Q58910042 | ||
The lesser role of starbursts in star formation at z = 2 | Q58910727 | ||
A New Photometric Technique for the Joint Selection of Star‐forming and Passive Galaxies at 1.4 ≲z≲ 2.5 | Q58910816 | ||
PACS Evolutionary Probe (PEP) – A Herschel key program | Q58911973 | ||
The first Herschel view of the mass-SFR link in high-z galaxies | Q58912008 | ||
The star-formation rates of 1.5 < z < 2.5 massive galaxies | Q58912010 | ||
The SINS survey: SINFONI integral field spectroscopy of z ~ 2 star-forming galaxies | Q58912032 | ||
The SINS survey: modeling the dynamics of z ~ 2 galaxies and the high-z Tully-Fisher relation | Q58912046 | ||
The reversal of the star formation-density relation in the distant universe | Q58912075 | ||
Panchromatic spectral energy distributions ofHerschelsources | Q58916322 | ||
P433 | issue | 1 | |
P407 | language of work or name | English | Q1860 |
P921 | main subject | star-forming galaxy | Q109101277 |
P1104 | number of pages | 12 | |
P304 | page(s) | 19–30 | |
P577 | publication date | 2014-07-08 | |
P1433 | published in | Monthly Notices of the Royal Astronomical Society | Q1536490 |
P1476 | title | A multiwavelength consensus on the main sequence of star-forming galaxies at z ∼ 2 | |
P478 | volume | 443 |
Q58983738 | ALMA observations of cold molecular gas in AGN hosts at z ∼ 1.5 – evidence of AGN feedback? |
Q58911833 | CO excitation of normal star-forming galaxies out to z = 1.5 as regulated by the properties of their interstellar medium |
Q58911797 | Dust attenuation inz~ 1 galaxies fromHerscheland 3D-HST Hαmeasurements |
Q58908178 | Dust properties of Lyman-break galaxies at z ~ 3 |
Q58908131 | Effect of the star formation histories on the SFR-M∗relation at z ≥ 2 |
Q46298043 | Galaxy evolution. Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang |
Q56550194 | On the nature of Hα emitters atz∼ 2 from the HiZELS survey: physical properties, Lyα escape fraction and main sequence |
Q58982060 | Physical properties of AGN host galaxies as a probe of supermassive black hole feeding mechanisms |
Q58911812 | Satellite content and quenching of star formation in galaxy groups at z ~ 1.8 |
Q58908272 | Star formation and quenching among the most massive galaxies at z ∼ 1.7 |
Q58916839 | The KMOS Deep Survey (KDS) – I. Dynamical measurements of typical star-forming galaxies at z ≃ 3.5 |
Q57088385 | The SCUBA-2 Cosmology Legacy Survey: galaxies in the deep 850 μm survey, and the star-forming ‘main sequence’ |
Q58492565 | The evolving relation between star formation rate and stellar mass in the VIDEO survey sincez = 3 |
Q58035331 | The evolving star formation rate: M⋆relation and sSFR since z ≃ 5 from the VUDS spectroscopic survey |
Q58911805 | The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV and [OII]λ3727 luminosities |
Search more.