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Z Relation (z + relation)
Selected AbstractsThe K - z diagram of FIRST radio sources identified in the Boötes and Cetus fieldsASTRONOMISCHE NACHRICHTEN, Issue 8 2009K. El Bouchefry Abstract This paper presents the Hubble diagram (K - z relation) for FIRST (Faint Images of the Radio Sky at 20 cm) radio sources identified in the Boötes and Cetus fields. The correlation between the K magnitude of the FIRST-NDWFS sample and the photometric redshifts found to be linear. The dispersion about the best fit line is given by 1.53 for the whole sample and 0.75 at z > 1. The paper also presents a composite K - z diagram of FIRST radio sources and low-frequency selected radio samples with progressively fainter flux-density limits (3CRR, 6C, 7CRS and the EIS-NVSS sample). The majority of FIRST radio sources lie fainter than the no evolution curve (3 L* galaxies) probably highlighting the fact that the galaxy luminosity is correlated with the radio power (© 2009 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim) [source] Identifications of FIRST radio sources in the NOAO Deep Wide-Field SurveyASTRONOMISCHE NACHRICHTEN, Issue 6 2007K. El Bouchefry Abstract In this paper we present the results of an optical and near infrared identification of 514 radio sources from the FIRST survey (Faint Images of the Radio Sky Survey at Twenty centimetres) with a flux-density limit of 1 mJy in the NOAO Deep Wide-Field Survey (NDWFS) Boötes field. Using optical (Bw, R, I) and K band data with approximate limits of Bw , 25.5 mag, R , 25.8 mag, I , 25.5 mag and K , 19.4 mag, optical counterparts have been identified for 378 of 514 FIRST radio sources. This corresponds to an identification rate of 34% in four bands (BwRIK), 60% in optical bands (BwRI) and 74% in the I band. Photometric redshifts for these sources have been computed using the hyperz code. The inclusion of quasar template spectra in hyperz is investigated. We note that the photometric data are, in many cases, best matched to templates with very short star-formation timescales and the inferred ages of identified galaxies depend strongly on the assumptions about the star-formation timescale. The redshifts obtained are fairly consistent with those expected from the K - z relation for brighter radio sources but there is more scatter in the K - z diagram at z < 1. (© 2007 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim) [source] Permeability of the continental crust: dynamic variations inferred from seismicity and metamorphismGEOFLUIDS (ELECTRONIC), Issue 1-2 2010S. E. INGEBRITSEN Geofluids (2010) 10, 193,205 Abstract The variation of permeability with depth can be probed indirectly by various means, including hydrologic models that use geothermal data as constraints and the progress of metamorphic reactions driven by fluid flow. Geothermal and metamorphic data combine to indicate that mean permeability (k) of tectonically active continental crust decreases with depth (z) according to log k , ,14,3.2 log z, where k is in m2 and z in km. Other independently derived, crustal-scale k,z relations are generally similar to this power-law curve. Yet there is also substantial evidence for local-to-regional-scale, transient, permeability-generation events that entail permeabilities much higher than these mean k,z relations would suggest. Compilation of such data yields a fit to these elevated, transient values of log k , ,11.5,3.2 log z, suggesting a functional form similar to that of tectonically active crust, but shifted to higher permeability at a given depth. In addition, it seems possible that, in the absence of active prograde metamorphism, permeability in the deeper crust will decay toward values below the mean k,z curves. Several lines of evidence suggest geologically rapid (years to 103 years) decay of high-permeability transients toward background values. Crustal-scale k,z curves may reflect a dynamic competition between permeability creation by processes such as fluid sourcing and rock failure, and permeability destruction by processes such as compaction, hydrothermal alteration, and retrograde metamorphism. [source] The evolution of the cluster X-ray scaling relations in the Wide Angle ROSAT Pointed Survey sample at 0.6 < z < 1.0MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Issue 2 2006B. J. Maughan ABSTRACT The X-ray properties of a sample of 11 high-redshift (0.6 < z < 1.0) clusters observed with Chandra and/or XMM,Newton are used to investigate the evolution of the cluster scaling relations. The observed evolution in the normalization of the L,T, M,T, Mg,T and M,L relations is consistent with simple self-similar predictions, in which the properties of clusters reflect the properties of the Universe at their redshift of observation. Under the assumption that the model of self-similar evolution is correct and that the local systems formed via a single spherical collapse, the high-redshift L,T relation is consistent with the high- z clusters having virialized at a significantly higher redshift than the local systems. The data are also consistent with the more realistic scenario of clusters forming via the continuous accretion of material. The slope of the L,T relation at high redshift (B= 3.32 ± 0.37) is consistent with the local relation, and significantly steeper than the self-similar prediction of B= 2. This suggests that the same non-gravitational processes are responsible for steepening the local and high- z relations, possibly occurring universally at z, 1 or in the early stages of the cluster formation, prior to their observation. The properties of the intracluster medium at high redshift are found to be similar to those in the local Universe. The mean surface-brightness profile slope for the sample is ,= 0.66 ± 0.05, the mean gas mass fractions within R2500(z) and R200(z) are 0.069 ± 0.012 and 0.11 ± 0.02, respectively, and the mean metallicity of the sample is 0.28 ± 0.11 Z,. [source] | ||||||||||