[PDF] Top 20 A massive, quiescent galaxy at a redshift of z = 3.717

... of galaxy formation and possibly our standard model of cold dark matter halo assembly are needed to explain the rapid formation, and sudden and deep quenching, of massive galaxies in the very early Universe ... See full document

... The brightening and magnifying effects from strong grav- itational lensing are a powerful tool that permit us to study high-redshift galaxies with better signal-to-noise ratio (S/N) and higher spatial resolution ... See full document

... between galaxy density - either on average or within a central region - and stellar populations and ongoing star formation ...high redshift we are limited to ...high redshift where observations probe ... See full document

... from z ∼ 2 to z ∼ ...at z ∼ 2 is a hybrid environmental density and stellar mass ranking ...since z ∼ 2, and BCG progenitors are mainly late-type galaxies, exhibiting less concentrated ... See full document

... The situation has been improved in the local Universe by the advent of large systematic surveys designed to obtain high signal- to-noise ratio (SNR) continuum spectroscopy. These data are more strongly constraining on ... See full document

... cluster galaxy formation, one needs to identify the galaxy popu- lations residing in young ...high redshift have identified signifi- cant galaxy overdensities ...of massive ‘red and ... See full document

... at z = 4, at least among massive ...from z = 4 to the present day, that is, over at least 90% of the cosmic ...the massive end of the z = 4 galaxy ... See full document

... that quiescent galaxies have effective radii that are a factor ∼ 4 smaller than those of low-redshift quiescent galaxies of similar mass, and have no excess flux at large ...a galaxy can create ... See full document

... more massive galaxies being closer to filaments as indicated by the shift in the median values of the two PDFs (downward ...our massive (M ∗ ≥ 10 ...most massive star-forming galaxies being closer to ... See full document

... for quiescent galaxies. However, there is a weak trend at each redshift for star-forming galaxies such that velocity dispersion decreases slightly for rounder ...at z ∼ ...measuring galaxy ... See full document

... host-galaxy redshift of ...host galaxy redshift of ...a massive, low- SFR host ...this galaxy are expected to be SNe ...highest redshift SN Ia with a spectroscopic ... See full document

... as massive as those of control galaxies of the same stellar ...more massive black holes seem to trigger radio jets more easily, but as this boost in halo mass is independent of radio luminosity, the authors ... See full document

... with redshift as (1 + z) 2−5 ...the galaxy, which makes this method prone to system- ...+ z) −4 , which can lead to a biased identification of faint merger-specific features as a function of ... See full document

... ( z − K, K - [ ...SFR, redshift, stellar mass, and their relationship to other galaxy ...comparison quiescent galaxy and less FIR luminous star- forming galaxy samples that are ... See full document

... times. For instance, by tracing the gas dynamics, the Tully- Fisher relation (Tully & Fisher 1977), which links the angular momentum of the parent DM halo of a disk galaxy with the luminosity/mass of its ... See full document

... a galaxy, which is assumed to be a triaxial ax- isymmetric system with diffuse dust and dense molecular clouds, in which stars are ...of galaxy properties from quiescent to star- burst and span an A ... See full document

... and quiescent galaxies segre- gate themselves particularly well in the NUV − r versus r − K ...by massive galaxies with a variety of morphologies probably transiting from the star-forming to the ... See full document

... With a very similar characteristic stellar mass of log(M/M ⊙ ) ∼ 10.4 − 10.5, a space density 6-7 times higher at ∼ 6 − 7 × 10 −5 Mpc −3 but an observable timescale up to an order of magnitude longer, the ... See full document

... improving redshift estimates through spectroscopy ( largely due to the impact of the more neutral IGM on the prevalence of Ly α emission in z > ...of z ∼ 5 – 8 galaxies over the GOODS-N and ... See full document

... and 1.0 mm, respectively) and CO (5–4) flux and velocity, created by S15, using the lensing model by Dye et al. (2015). This model was used in the image plane with the semilinear inversion method (Warren & Dye 2003) ... See full document