Redshift survey
The 2dF Galaxy Redshift Survey: galaxy luminosity functions per spectral type
... Up until now the greatest obstacle faced when attempt- ing to determine how the LF varied with different galaxy properties was the fact that one was required to divide al- ready small data sets, thereby losing much of ...
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The VIMOS Public Extragalactic Redshift Survey (VIPERS) On the recovery of the count in cell probability distribution function
... We compare three methods to measure the count-in-cell probability density function of galaxies in a spectroscopic redshift survey. From this comparison we found that, when the sampling is low (the average ...
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The VIMOS Public Extragalactic Redshift Survey (VIPERS) Environmental effects shaping the galaxy stellar mass function
... We aim to provide new clues in this context, exploiting the VIMOS Public Extragalactic Redshift Survey (VIPERS, Guzzo et al. 2014) to search for environmental effects between z 1 and z 0.5. As shown in a ...
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The 2dF Galaxy Redshift Survey: the amplitudes of fluctuations in the 2dFGRS and the CMB, and implications for galaxy biasing
... Galaxy Redshift Survey (2dFGRS) has now mea- sured over 210 000 galaxy redshifts and is the largest existing galaxy redshift survey (Colless et ...
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The VIMOS Public Extragalactic Redshift Survey (VIPERS) : galaxy segregation inside filaments at z ≃ 0 7
... We present the first quantitative detection of large-scale filamentary structure at z ' 0.7 in the large cosmological volume probed by the VIMOS Public Extragalactic Redshift Survey (VIPERS). We use ...
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The VIMOS Public Extragalactic Redshift Survey (VIPERS) The coevolution of galaxy morphology and colour to z ~ 1
... shift Survey (VIPERS; Guzzo & The Vipers Team 2013) ful- fills these requirements over the redshift range ...spectroscopic redshift survey which provides, on one hand, a unique combination ...
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The VIMOS Public Extragalactic Redshift Survey (VIPERS) : unbiased clustering estimate with VIPERS slit assignment
... multiple survey realisations are generated shifting the original VIPERS spectroscopic mask over the underlying parent catalogue (red ...new survey realisation is generated shifting the ‘extended’ ...
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Window Effect in the Power Spectrum Analysis of a Galaxy Redshift Survey
... LRGs. The data reduction is the same as that described in Refs. [19,20,29,30]. In this subsection, we show general features of the window function of the LRG sample. In our approach, division of the full sample into ...
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The VIMOS Public Extragalactic Redshift Survey (VIPERS) Star formation history of passive red galaxies
... separate the red- and blue-type galaxy populations within the VIPERS dataset were already discussed by Fritz et al. (2014). In this work we focus on a sample of passive red galaxies with the lowest possible contamination ...
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The SAMI galaxy survey : the cluster redshift survey, target selection and cluster properties
... of the resolved properties of galaxies spanning a range in mass, in combination with a detailed description of the galaxy environment. The ongoing Sydney-AAO Multi-Object Integral field spectrograph Galaxy Survey ...
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The power spectrum from the angular distribution of galaxies in the CFHTLS Wide fields at redshift ~0 7
... Legacy Survey. With the redshift distributions measured with a preliminary ∼14 000 spectroscopic redshifts from the VIMOS Public Extragalactic Redshift Survey (VIPERS), we deproject the ...
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Photometric redshifts for the next generation of deep radio continuum surveys - I. Template fitting
... photometric redshift estimates are at least as accurate are those radio sources which are also identified as luminous X-ray sources or host dust obscured ...photometric redshift estimates than the ...
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CF-HiZELS, an ~ 10 deg2 emission-line survey with spectroscopic follow-up: Hα, [O III] + Hβ and [O II] luminosity functions at z = 0.8, 1.4 and 2.2
... We note that this finding could be important to also interpret any overdensity of star-forming galaxies detected at this or at even higher redshift. Without a careful analysis of the full galaxy pop- ulation, one ...
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The Dark Energy Survey Y1 Supernova Search: Survey Strategy Compared to Forecasts and the Photometric Type Ia Sn Volumetric Rate
... large redshift range. The Dark Energy Survey, projected to find thousands of high signal-to- noise light curves from z = 0 to z = ...broad redshift supernova sample when compared to ...
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The ALMA Redshift 4 Survey (AR4S). I. The massive end of the z 4 main sequence of galaxies
... ALMA Redshift 4 Survey (AR4S 1 ), a complete survey of massive galaxies in the Hubble Space Telescope (HST) CANDELS fields at z ∼ 4 with the ALMA ...
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De Lucia, Gabriella (2004): Evolution of Galaxies in Clusters. Dissertation, LMU München: Fakultät für Physik
... The coefficients of the fit and the corresponding errors are determined using a bootstrap method over 100 Monte Carlo realizations. Both the slope and the zero– point are allowed to vary. In Table 6.1 we report the ...
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Slicing COSMOS with SC4K:the evolution of typical Lya emitters and the Lya escape fraction from z~2 to z~6
... Sources with weak emission lines or with low EWs may be missed by our selection criteria, causing the measured num- ber density of sources to be underestimated. To estimate the line flux completeness we follow Sobral et ...
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Photoreflectance spectroscopy of GaInSbBi and AlGaSbBi quaternary alloys
... transition with increasing In and Bi contents, whereas the AlGaSbBi layers show redshift with increasing Bi and decreasing Al content. The temperature induced narrowing of the band gap in GaInSbBi and AlGaSbBi ...
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Photoreflectance spectroscopy of GaInSbBi and AlGaSbBi quaternary alloys
... transition with increasing In and Bi contents, whereas the AlGaSbBi layers show redshift with increasing Bi and decreasing Al content. The temperature induced narrowing of the band gap in GaInSbBi and AlGaSbBi ...
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Static and Dynamic Components of the Redshift
... cosmological redshift may be cumulatively due to the expansion of the universe and the tired light pheno- ...Ia redshift data using one parameter than the standard ΛCDM model with two ...of redshift ...
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