[PDF] Top 20 THE REDSHIFT AND NATURE OF AzTEC/COSMOS 1: A STARBURST GALAXY AT z = 4.6∗
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THE REDSHIFT AND NATURE OF AzTEC/COSMOS 1: A STARBURST GALAXY AT z = 4.6∗
... mag, and a stellar mass of M ∗ = (1.5 ± 0.2) × 10 11 M (see the top panel in Figure ...using the Maraston et ...some of the free parameters may be poorly parameterized in young ... See full document
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UNVEILING THE NATURE OF SUBMILLIMETER GALAXY SXDF 850 6
... obtained at the VLA. Our new SMA detection finds that the submillimeter emission coincides with the brightest radio emission that is found ∼8 north of the coordinates determined ... See full document
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Deep 1.1 mm-wavelength imaging of the GOODS-S field by AzTEC/ASTE – II. Redshift distribution and nature of the submillimetre Galaxy Population
... in the rest-frame UV and op- tical bands? And how do they fit into the larger population of high- redshift galaxies identified in those more traditional bands? Opti- cal/UV size, ... See full document
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First simultaneous optical/near infrared imaging of an X ray selected, high redshift cluster of galaxies with GROND The galaxy population of XMMU J0338 7+0030 at z=1 1
... checked the reliability of the publicly available transmission functions of the GROND dichroic filters uploaded into le Phare by comparing the distributions of the ... See full document
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ALMA Observations of Gas rich Galaxies in z ~ 1 6 Galaxy Clusters: Evidence for Higher Gas Fractions in High density Environments
... above the scaling relation mass limit of 10 10 M ☉ . For each of these seven non-detections, we create a 400 km s − 1 ( the average FWHM of the detected sample ) ... See full document
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Discovery of the X ray selected galaxy cluster XMMU J0338 8+0021 at z=1 49
... to the median redshift. This allows us to confirm the presence of a bound system of, at least, 7 galaxies with a me- dian redshift of z = 1 ...Using ... See full document
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The composite nature of Dust Obscured Galaxies (DOGs) at z ∼ 2–3 in the COSMOS field – I A far infrared view
... in the photodissociation regions (PDR) component and/or variation in the intensity of the field is responsible for the bluer colour of these bright DOGs, by comparing to ... See full document
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A SPITZER SELECTED GALAXY CLUSTER AT z=1 62
... bands), the UKIRT Infrared Deep Survey–Ultra-Deep Survey (UKIDSS–UDS, JK bands), and from the Spitzer Public UDS survey ...density of galaxies at z ≈ 1.6 that is >20σ above ... See full document
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The x ray luminous galaxy cluster population at 0 9 < z less than or similar to 1 6 as revealed by the XMM Newton Distant Cluster Project
... estimates at z < ∼ 0.9, given a sufficiently accurate galaxy evolution ...clusters at z > 0.9 the color-based redshift reliability decreases rapidly due to ... See full document
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AzTEC 1.1-mm images of 16 radio galaxies at 0.5 < z < 5.2 and a quasar at z = 6.3
... starting at 2σ and increasing linearly by 1 σ . Bars indicate the orientation of the radio source, where ...Most of the active galaxies in our sample have been ... See full document
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Bright strongly lensed galaxies at redshift z similar to 6 7 behind the clusters abell 1703 and CL0024+16
... determine the intrinsic properties of the high-redshift galaxy candidates identified in our search, it is necessary to model the effect of gravitational lensing on these ... See full document
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The X ray luminous galaxy cluster XMMU J1007 4+1237 at z=1 56 The dawn of starburst activity in cluster cores
... high- z radio galaxies have been reported for a number of z > 1 systems ...origin of their diffuse emission can in principle contribute to the measured flux or even mimic ... See full document
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SPT CL J0205 5829: A z=1 32 EVOLVED MASSIVE GALAXY CLUSTER IN THE SOUTH POLE TELESCOPE SUNYAEV ZEL'DOVICH EFFECT SURVEY
... part of a larger program to follow up clusters identified in the SPT ...for the confirmation and study of high-redshift SPT clusters such as SPT-CL J0205 − 5829 where the ... See full document
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On the accuracy of the high redshift cluster luminosity function
... that the true probability distributions of photometric redshifts are often highly non-Gaussian, and that secondary maxima or ex- tended wings might change the accuracy of photometric ... See full document
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On the evolution of environmental and mass properties of strong lens galaxies in COSMOS
... set of stellar masses using the Bayesian code described in Bundy et ...made of the observed galaxy spectral energy distribution (SED) and its redshift, is referenced to a ... See full document
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Scaling relations of the colour detected cluster RzCS 052 at z=1 016 and some other high redshift clusters
... using the European Photon Imaging Camera (EPIC) instrument (Jansen et ...with the thin filter. After flares filtering, the good exposure time is ∼13 ks for the MOSes (Turner et ...2001), ... See full document
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The lack of star formation gradients in galaxy groups up to z ~ 1 6
... one of the best-studied extragalactic fields in the sky ...wavelengths. The smaller Chandra Deep Field South (CDFS, α = 03h32m25s , δ = 27 o 49 m 58 s ), in the central part of ... See full document
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The VLT LBG Redshift Survey III The clustering and dynamics of Lyman break galaxies at z similar to 3
... from the Steidel et al. (2003) survey meant the authors could not solve for both the bulk motion and the veloc- ity dispersion, which are degenerate, severely limiting the scope ... See full document
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The color bimodality in galaxy clusters since z to 0 9
... comparison of local and high-redshift clusters of galaxies is a powerful tool for constraining theories of structure forma- tion and cosmological world ...models. The ... See full document
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The representative XMM Newton cluster structure survey (REXCESS) of an X ray luminosity selected galaxy cluster sample
... assessing the relia- bility with which the cluster fluxes have been determined in the RASS ...take the fluxes determined by Böhringer et ...with the growth curve analysis method for a ... See full document
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