[PDF] Top 20 Dust attenuation in galaxies up to redshift ≃ 2

... spectroscopic redshift between 0.95 and 2.2 and no X ray detection. In this redshift range we have more than ten photometric bands available in the UV rest-frame and a good sampling around 2175 ˚ ... See full document

... star-forming galaxies during the peak epoch of galaxy formation grew through smooth accretion of cold gas triggering internal star formation pro- cesses (Kereˇs et ...star-forming galaxies, (Noeske et ... See full document

... We fi rst binned a subset of the eBOSS galaxy sample based on the age of the template that produced the best- fi t model. Objects were chosen with best- fi tting templates of zero line fl ux to identify a passively evolving ... See full document

... of galaxies in the local Universe where photometric information in the UV and IR as well as measurements of key spec- tral lines such as H α and H β are ...Section 2, we describe the various surveys and ... See full document

... Conventional wisdom places this dusty population at z ∼ 2.5 ( Chapman et al. 2005; Simpson et al. 2014 ) , but recent work by Riechers et al. ( 2013 ) , Dowell et al. ( 2014 ) , Asboth et al. ( 2016 ) , and ( Ivison et ... See full document

... We are almost ready to calculate the Fisher matrix elements using Equation 4.19, but we need to comment first on one additional complication. The issue relates to the continuum foreground, which is significantly larger ... See full document

... GHz dust continuum and [CII] ...GHz dust continuum and [CII] emission of the SMGs are resolved in our observations and the 345 GHz dust continuum sizes of the sources are listed in Table 2 and ... See full document

... of galaxies and consequently manifest in the relative strengths of fi ne structure emission ...the dust that drives their extreme far-IR luminosities also makes observations at optical and near-IR ... See full document

... several galaxies individually we would be unable to determine the differential magnification on a case by case ...individual galaxies may have quite substantial differential magnification ... See full document

... the galaxies that lie on the red sequence are predominantly passively evolving, old ...star-forming galaxies ( with A V ~ 1 3 – ) exhibit colors similar to those expected from quenched, passively evolving ( ... See full document

... five galaxies with detected Lyman continuum ...these galaxies have among the lowest best- fit star-formation rate and below average dust ...leaking galaxies and thus their E(B − V ) and star- ... See full document

... and dust are locked into stars during the star and planet formation process (or- ange points) then the model dust masses match the observed val- ues for 11/26 ...the dust masses of the major- ity of ... See full document

... reality, galaxies are unlikely to be closed systems ...for galaxies at a fixed gas-phase oxygen abundance (Gallazzi et ...high redshift provide further indirect evidence that inflows are required, ... See full document

... of galaxies for the thermodynamics and chemistry of the gas, for the dynamics of the accretion in dense star-forming clouds, and for the attenuation of UV/blue radiation and its re-emission in the ... See full document

... whether galaxies have reionized the Universe, it is perhaps more interesting to un- derstand which galaxies have been the most important to do ...in galaxies is likely very bi- modal and dependent on ... See full document

... Table 2 indicates that only 15 per cent of our green sam- ple would be considered early type and 25 per cent late type (if we assume the S0/Sa class corresponds to the indeterminate-types in the Galaxy Zoo ...of ... See full document

... of galaxies in the COSMOS field (Scoville et ...∼ 2 deg 2 ) for the effects of the large- scale structure to be discernible, with a minimal cosmic ...of galaxies and their stellar mass on the ... See full document

... analysis. In fact, Diaferio et al. (1999a) show that the two point correlation function of the mock catalogues agrees quite well with the CfA2S function. As expected, the Minkowski functionals are able to extract more ... See full document

... the redshift evolution of essentially all ions is sensitive to (i) the increase in the total mass density of metals towards lower redshifts due to on- going star formation, (ii) the propagation of enrich- ment ... See full document

... earliest galaxies at redshift z ∼ 10 (see, ...early galaxies began to develop the orderly, regular morphological structures with which we are familiar in the local ...∼ 2 − 3 (when the ... See full document