[PDF] Top 20 Evolution of galaxy size-stellar mass relation from the Kilo-Degree Survey

... lower mass bin, they look almost ...larger mass bin at low-z, which goes along the direc- tion of previous finding in local samples ...all mass (and increasing with it) and redshift, except possibly ... See full document

... the galaxy environment in GAMA Galaxy Groups Catalogue (G3C) using a volume-limited galaxy sample from the Kilo Degree Survey Data Release ...the relation between ... See full document

... Observations from precursor surveys such as the Dark Energy Survey (DES), the Kilo Degree Survey (KiDS), and the Hyper Suprime Cam Survey (HSC) – in combination with CMB and ... See full document

... The size evolution of massive quiescent galaxies is one of the open problems in ...fixed stellar mass, the average size of quiescent galaxies has increased by a factor of a few between ... See full document

... halo mass between groups and clusters has been interpreted in terms of a varying efficiency of the star forma- tion with the total mass of the system ...low stellar mass fraction, of the order ... See full document

... with mass-weighted sizes, which are typically smaller than luminosity-weighted (see Appendix ...the size-mass relation. Nonetheless, at fixed stellar mass, we observe the spread ... See full document

... expanded Galaxy and Mass Assembly (GAMA) survey phase II visual morphology sample and the large-scale bulge and disc decomposition analysis of Lange et ...new stellar mass function fits ... See full document

... merger mass ratio, the timing of mergers, and the gas ...of galaxy formation, when the in-situ component generally settles down in a flattened rotating disk component (Rodriguez-Gomez et ...in size ... See full document

... We can predict, using the virial theorem, how the points would lie if the scatter is intrinsic, i.e., due to variations in the galaxy structure. This line is shown in Figure 4(c), and we see that the galaxies lie ... See full document

... probe galaxy build-up from z = 4 out to z = 8, aiming to improve on the limiting factors dis- cussed above, with a goal of providing robust constraints on the GSMFs of galaxies at 4 < z < ...data ... See full document

... the size evolution of a mass-complete ( log ( M * / M e )> 10 ) sample of star-forming galaxies over redshifts z = 1 – 7, selected from the FourStar Galaxy Evolution ... See full document

... galaxies from the ‘Evolution and Assembly of GaLaxies and their Environments’ (EAGLE; Schaye et ...0 galaxy stellar mass function, galaxy stellar mass–black hole ... See full document

... gas from the IGM, every galaxy has an internal channel for replenishing the reservoir of gas in the interstellar medium (ISM), namely the shedding of mass by the stellar populations ...their ... See full document

... Tully-Fisher relation (Tully & Fisher 1977) links the rotational velocity of galaxies to their absolute magni- tude, which is, in turn, proportional to stellar ...low mass galaxies have ... See full document

... forms: from galaxies displaying two strong ‘grand design’ arms to those with many ‘flocculent’ ...measurements from Galaxy Zoo ...photometry from GALEX and WISE to measure the rates and ... See full document

... of stellar mass in the universe can be traced by measuring the star formation rate density (SFRD) as a function of ...a galaxy? Ongoing star formation reveals itself mainly in three effects (see ... See full document

... the relation between γ and the observable image ellipticities, yielding significant biases in all weak lensing ...mean mass density of the Universe – the convergence part in the optical tidal equation (see, ... See full document

... ranges from 0 to 10 −18 erg s −1 cm −2 Å −1 ...tenth degree polynomial from 3836 to 5873 Å in the observed frame and subtracting the result from the corresponding science exposures prior to ... See full document

... obtained from jackknife resampling, with each pointing being a jackknife ...away from the diagonal shows that the level of catastrophic failures in the redshifts is low, and provides confidence in the ... See full document

... There is general agreement that feedback is the way to solve these problems [15, 16]. Two methods are commonly used. One is kinetic feedback that adds velocity kicks to gas particles to remove them from the inner ... See full document