A massive galaxy in its core formation phase three billion years after the Big Bang

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A massive galaxy in its core formation phase three billion years after the Big Bang is …
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scholarly articleQ13442814

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P819ADS bibcode2014Natur.513..394N
P818arXiv ID1406.3350
P6179Dimensions Publication ID1025415492
P356DOI10.1038/NATURE13616
P8608Fatcat IDrelease_pvtwmaai55b65cdaplmvwaobgm
P724Internet Archive IDarxiv-1406.3350
P698PubMed publication ID25162527
P5875ResearchGate publication ID263126747

P50authorHans-Walter RixQ109227
Marijn FranxQ15638035
Arjen van der WelQ56547474
Elisabete da CunhaQ56548884
Joel LejaQ57570207
Gabriel BrammerQ58914496
Rachel BezansonQ59404758
Pieter van DokkumQ59671631
Erica NelsonQ59672159
Katherine WhitakerQ59676274
Rosalind SkeltonQ60043814
Natascha M. Förster SchreiberQ72044124
Stijn WuytsQ72044290
Ivelina MomchevaQ100711748
Allison R KirkpatrickQ114369308
P2093author name stringLinda Tacconi
P2860cites workGalactic Stellar and Substellar Initial Mass FunctionQ29010804
The Global Schmidt Law in Star‐forming GalaxiesQ55954221
Keck-I MOSFIRE spectroscopy of compact star-forming galaxies at z >~ 2: high velocity dispersions in progenitors of compact quiescent galaxiesQ56547473
Submillimeter Galaxies atz∼ 2: Evidence for Major Mergers and Constraints on Lifetimes, IMF, and CO‐H2Conversion FactorQ56556101
The Origin of the Mass‐Metallicity Relation: Insights from 53,000 Star‐forming Galaxies in the Sloan Digital Sky SurveyQ56608299
Passively Evolving Early‐Type Galaxies at 1.4 ≲z≲ 2.5 in the Hubble Ultra Deep FieldQ57602999
GOODS-Herschel: impact of active galactic nuclei and star formation activity on infrared spectral energy distributions at high redshiftQ57710859
GOODS–Herschel: an infrared main sequence for star-forming galaxiesQ57710922
Hubble Space Telescope and Spitzer Imaging of Red and Blue Galaxies at z ∼ 2.5: A Correlation between Size and Star Formation Activity from Compact Quiescent Galaxies to Extended Star‐forming GalaxiesQ57768304
CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy SurveyQ58474370
CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey--The Hubble Space Telescope observations, imaging data products, and mosaicsQ58474373
3D-HST+CANDELS: the evolution of the galaxy size-mass distribution since z = 3Q58492573
The Size Evolution of Galaxies sincez∼3: Combining SDSS, GEMS, and FIRESQ58492606
The progenitors of the compact early-type galaxies at high redshiftQ58908448
Galaxy structure and mode of star formation in the SFR-mass plane from z ~ 2.5 to z ~ 0.1Q58908687
The Chandra Deep Field North Survey. XIII. 2 Ms Point-Source CatalogsQ58909751
ALMA reveals a warm and compact starburst around a heavily obscured supermassive black hole at z = 4.75Q58910672
GMASS ultradeep spectroscopy of galaxies at z ~ 2 II. Superdense passive galaxies: how did they form and evolve?Q58910766
PACS Evolutionary Probe (PEP) – A Herschel key programQ58911973
The SINS survey: SINFONI integral field spectroscopy of z ~ 2 star-forming galaxiesQ58912032
Submillimeter galaxies as progenitors of compact quiescent galaxiesQ58913634
3D-HST WFC3-selected photometric catalogs in the five CANDELS/3D-HST fields: photometry, photometric redshifts, and stellar massesQ59723515
Dense cores in galaxies out to z = 2.5 in SDSS, UltraVISTA, and the five 3D-HST/CANDELS fieldsQ59723519
Massive and newly dead: discovery of a significant population of galaxies with high-velocity dispersions and strong Balmer lines at z ~ 1.5 from deep Keck spectra and HST/WFC3 imagingQ59727145
Strong nebular line ratios in the spectra of z ~ 2-3 star forming galaxies: first results from KBSS-MOSFIREQ59784005
Velocity dispersions and dynamical masses for a large sample of quiescent galaxies at z > 1: improved measures of the growth in mass and sizeQ59818305
3D-HST: a wide-field grism spectroscopic survey with the Hubble Space TelescopeQ59938952
A simple model to interpret the ultraviolet, optical and infrared emission from galaxiesQ59938957
Keck spectroscopy of z > 1 field spheroidals: dynamical constraints on the growth rate of red "Nuggets"Q59969809
Confirmation of the compactness of a z = 1.91 quiescent galaxy with Hubble space telescope's wide field camera 3Q60023506
Confirmation of the Remarkable Compactness of Massive Quiescent Galaxies at z ~ 2.3: Early-Type Galaxies Did not Form in a Simple Monolithic CollapseQ60310812
AMAZE. I. The evolution of the mass-metallicity relation at z>3Q62622443
H{alpha} observations of a large sample of galaxies at z ~ 2: implications for star formation in high-redshift galaxiesQ66710378
Stellar kinematics of z ~ 2 galaxies and the inside-out growth of quiescent galaxiesQ68124589
A high stellar velocity dispersion for a compact massive galaxy at redshift z = 2.186Q68145452
An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z = 2.2Q68488454
Weak homology of elliptical galaxiesQ68511004
Star formation in galaxies along the Hubble sequenceQ68643149
High-mass X-ray binaries as a star formation rate indicator in distant galaxiesQ68701832
Toy models for galaxy formation versus simulationsQ68738272
The two phases of galaxy formationQ68986573
The NEWFIRM Medium-Band Survey: photometric catalogs, redshifts, and the bimodal color distribution of galaxies out to z ~ 3Q69007416
A K_S_ and IRAC selection of high-redshift extremely red objectsQ69029643
Wet disc contraction to galactic blue nuggets and quenching to red nuggetsQ69079533
Exploring the chemical link between local ellipticals and their high-redshift progenitorsQ69206211
P433issue7518
P407language of work or nameEnglishQ1860
P921main subjectBig BangQ323
P304page(s)394–397
P577publication date2014-08-27
P1433published inNatureQ180445
P1476titleA massive galaxy in its core formation phase three billion years after the Big Bang
P478volume513

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cites work (P2860)
Q58916875Evidence for wide-spread active galactic nucleus-driven outflows in the most massive z ~ 1-2 star-forming galaxies
Q59818290Rotating Starburst Cores in Massive Galaxies at z = 2.5
Q59818289The KMOS3D Survey: Rotating Compact Star-forming Galaxies and the Decomposition of Integrated Line Widths

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