[PDF] Top 20 The Size Evolution of Star-forming Galaxies since z ~ 7 Using ZFOURGE
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The Size Evolution of Star-forming Galaxies since z ~ 7 Using ZFOURGE
... . ZFOURGE takes advantage of the near-IR medium-band fi lters J1, J2, J3, Hs, and Hl on the FourStar instrument ( Persson et ...< z < ...declining star formation rate with t = 10 Myr to 10 ... See full document
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The Differential Size Growth of Field and Cluster Galaxies at z = 2.1 Using the ZFOURGE Survey
... gas-rich star- forming galaxies are found preferentially in low density environments while gas-poor quiescent galaxies are found in the highest density ...and star formation contribute ... See full document
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The production and escape of Lyman-Continuum radiation from star-forming galaxies at z {sim} 2 and their redshift evolution
... at z > 7 ...that galaxies may indeed have provided the ionizing photons to reionize the Universe ...at z ∼ 5 is consistent with the derived emissivity from galaxies (Choudhury et ... See full document
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The production and escape of Lyman Continuum radiation from star forming galaxies at z~2 and their redshift evolution
... to z ∼ 1. However, at higher redshifts, our photo-z uncertainties are large enough that they probably wash out extremely dense ...beyond z & ...(the size of COSMOS field) and how the ... See full document
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The production and escape of Lyman Continuum radiation from star forming galaxies at z~2 and their redshift evolution
... of galaxies as a function of their UV luminosity (lumi- nosity functions) at z > 7 ...at z ∼ 2− 3), and a steepening of the faint-end slope with increasing red- shift (see for example the ... See full document
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The growth of typical star forming galaxies and their super massive black holes across cosmic time since z~2
... typical star- forming ...selected galaxies below the X-ray detection limit and recover much lower black hole accre- tion ...same size of the stacking area, making sure these would fall outside ... See full document
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An Empirically Calibrated Model for Interpreting the Evolution of Galaxies during the Reionization Era
... simple star formation model whose goal is to interpret the emerging body of observational data of star-forming galaxies at z k ...the star formation activity within dark matter ... See full document
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Angular momentum evolution of galaxies over the past 10 Gyr:a MUSE and KMOS dynamical survey of 400 star forming galaxies from z=0 3 to 1 7
... the galaxies; see Stott et ...targets using the Magellan Multi- object Infra-Red Spectrograph ( MMIRS ) to search for and mea- sure the Hα flux of each target, and then carried out follow-up observations ... See full document
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The structural and size evolution of star forming galaxies over the last 11 Gyrs
... true evolution of galaxies we need to ac- count for any observational bias that may affect our observed ...its evolution with red- shift, the strongest bias could come from cosmological sur- face ... See full document
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ZFOURGE catalogue of AGN candidates: an enhancement of 160-μm-derived star formation rates in active galaxies to z = 3.2
... in star formation activity over inactive ...Fig. 7, this population is found to be exclusively hosted by quenched galaxies, which exhibit a lower level of star formation ac- tivity than their ... See full document
13
Star-forming galaxies at the Cosmic Dawn
... at z ∼ 4 − 7 with UV luminosity function (LF) determinations to derive star formation rate (SFR) functions at z ∼4, 5, 6 and ...well-established z ∼ 4 − 7 UV LFs, UV-continuum ... See full document
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One Plane for All: Massive Star-forming and Quiescent Galaxies Lie on the Same Mass Fundamental Plane at z ~ 0 and z ~ 0.7
... and star-forming galaxies exist within the same 3D space, they still populate different regions of that ...of galaxies from one population may alter galaxy structures and dynamics and must do ... See full document
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Evolution of Star forming Galaxies from z=0 7 to 1 2 with eBOSS Emission line Galaxies
... the evolution of the star-forming galaxies without assuming any redshift dependency in the model parame- ters, which may distort the high-redshift results in order to fit the low-redshift ... See full document
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The Evolution of the Fractions of Quiescent and Star-forming Galaxies as a Function of Stellar Mass Since z = 3: Increasing Importance of Massive, Dusty Star-forming Galaxies in the Early Universe
... dSF galaxies, more sophisticated techniques to estimate the dust obscuration and level of star formation will be necessary to improve the presented ... See full document
6
The growth of the central region by acquisition of counterrotating gas in star forming galaxies
... red galaxies with little star formation, gas and stars are counter-rotating, demonstrating the importance of external gas acquisition in these ...blue, star-forming galaxies are rare, ... See full document
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ZFOURGE catalogue of AGN candidates: an enhancement of 160-μm-derived star formation rates in active galaxies to z = 3.2
... and evolution of galaxies over cosmic ...the star-formation activity of galaxies ...massive galaxies in simulations by heating or driving out gas to suppress star- ...trigger ... See full document
16
Extreme conditions in the molecular gas of lensed star-forming galaxies at z ~ 3
... high-excitation galaxies with large linewidths are not necessarily associated with high AGN contributions and galaxies with large AGN contribu- tions do not display necessarily large linewidths (Rosenberg ... See full document
6
The Interstellar Medium in [O III]-selected Star-forming Galaxies at z ~ 3.2
... UV-selected galaxies and Ly α emitters at the same epoch and fi nd that the [ O III ] -based selection does not appear to show any systematic bias in the selection of star-forming ...with ... See full document
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OMEGA – OSIRIS Mapping of Emission line Galaxies in A901/2: II Environmental influence on integrated star formation properties and AGN activity
... performed using the OSIRIS Offline Pipeline software (OOPs; Ederoclite ...the galaxies, a pattern that is more apparent when the images are ...(2015). Using this method, the sky subtraction was ... See full document
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A multiwavelength exploration of the [C II]/IR ratio in H ATLAS/GAMA galaxies out to z = 0 2
... EI acknowledges funding from CONICYT FONDECYT postdoc- toral project No:3130504. RJI, LD and SM acknowledge support from the European Research Council in the form of Advanced Inves- tigator programme, COSMICISM. CF ... See full document
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