[PDF] Top 20 Unveiling the Physical Conditions in Star-Forming Galaxies at the Peak of Galaxy Assembly

... of star formation his- tory in determining galaxy scaling relations requires data for galaxies spanning the full range of plausible star formation histories at a given ...Evolved ... See full document

... imaging, galaxies located further away from the redshift corresponding to the peak of the response curve will have larger intrinsic line ...in galaxies with larger intrinsic [O II ] flux are likely ... See full document

... SF galaxies, at lower frequencies we would expect a population of flatter spectrum sources to shift the median spectral index above α = ...a peak flux density below the survey limit, but their total flux ... See full document

... of galaxy assembly is one of the key goals of modern ...because galaxies form and evolve under the in fluence of a variety of competing baryonic processes, the effects of which are dif ficult to ...for ... See full document

... pair galaxies is only significantly altered when the pair ratio is close to 1, otherwise we observe the same galaxies as we would in an unpaired ...minor galaxy in a pair is greatly affected by its ... See full document

... of physical properties based on these photometric redshifts, first estimating galaxy stellar ...the galaxy luminosity into stellar ...The physical parameter called “stellar mass” in this paper ... See full document

... of galaxies and in different conditions within a galaxy, both in the optical and in the molecular wavelength range, through the use of IFS, observed diagnostics and models ...nearby galaxies ... See full document

... gas conditions due to degeneracies between the line ratio and model parameter ...mean physical conditions in each galaxy by comparing the observations to the model parameter ... See full document

... in galaxies in pairs and their parent ...emission-line galaxies as Star Forming, Seyfert, LINER, composite spectra between LINER and Seyfert or between Star Forming and Seyfert ... See full document

... detected galaxies at z > 3.5: the radio galaxies 8C1909+722 and ...submillimetre-selected galaxies (SMGs) near the first of these at SNRs of ...such galaxies, made possible by AKARI’s ... See full document

... on galaxy SFRs for the star-forming ...early-type galaxies that are the largest contributor to the suppression in SFR at high ...for star-forming galaxies shows no change ... See full document

... local star formation history as traced by Hα emitters contained within photometrically selected GAMA ...faint star forming galaxies at higher–z (z < ... See full document

... SF galaxies (grey filled symbols) shows higher values at higher masses than the GAMA blue SMF as a result of the contribution from the photometrically classified red SF ...SF galaxies is shown in the right ... See full document

... dwarf galaxies and H I clouds are the trig- gering mechanism of their strong SF activity (L´opez-S´anchez 2010 ; L´opez-S´anchez et ...of star-forming galaxies in pairs taken from the Sloan ... See full document

... all galaxies are on their first approach and that they have not had previous passes, which would affect their ...if galaxies have already had one or more passes prior to the observation epoch, as such we ... See full document

... other galaxies, observations of ordered magnetic fields show coherent orientations parallel to galactic disks and along spiral arms or transitioning from parallel to vertical in the halo of edge-on ... See full document

... on star formation and particle physics I worked full time with astrophysicists ...of galaxy clusters using cosmological dark matter ...of galaxies in the early ... See full document

... 1.2 The Star Formation Rate The star formation rate is the total mass of stars formed per year, often given as solar masses per year. The usual way to estimate such a rate is to derive it from monochromatic ... See full document

... of galaxy formation in a CDM universe, the properties of disc galaxies are determined by the relationship between dark matter and ...a galaxy is spiral or ... See full document

... of the low-CO rotational lines even at low metallicity and they are fully concomitant with CO line emission (Gerin & Phillips 2000; Papadopoulos et al. 2004; Alaghband-Zadeh et al. 2013). The positive K-correction of the ... See full document