Radio luminosity histogram for our sample
Radio Sources in the COSMOS Field: Star Forming Properties of High Luminosity Radio Sources
... redshift radio galaxy ...the sample properties are con- sistent with predictions for the low frequency radio ...compare radio and IR star formation rate (SFR) tracers on a large sample ...
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Radio sources in the 6dFGS: Local luminosity functions at 1.4 GHz for star-forming galaxies and radio-loud AGN
... whose radio optical identification is ...shows our hand classification of 6dFGS-NVSS candi- ...component radio sources with position offset between 30 arcsec and 40 ...NVSS radio sources at ...
21
Counting quasar–radio source pairs to derive the millijansky radio luminosity function and clustering strength to z = 3.5.
... Small radio samples with complete spectroscopic coverage con- strain the bright end of the RLF at high z (Dunlop & Peacock 1990 ; Willott et ...fluxes radio sources are found up to high-redshift ( z ∼ ...
9
Relation between dust and radio luminosity in optically selected early type galaxies
... clear radio emission does not seem to be a very good discrim- inator between SBs and ...of our objects have measured nuclear Hα fluxes or upper limits (Tran, private communication), and standard ...
8
GAMA/WiggleZ: The 1.4GHz radio luminosity functions of high- and low-excitation radio galaxies and their redshift evolution to z=0.75
... able number of objects in estimating the completeness, while in high density regions we obtain a finer more local sampling of the completeness. The completeness in this plane is shown in Figure 3. Each galaxy is assigned ...
18
The bivariate K-band-submillimetre luminosity functions of the local HRS galaxy sample
... SDSS sample by Cross & Driver (2002), Ball et ...fficient. Our approach is fundamentally di fferent from previous works deal- ing with the bivariate ...
8
Neural-network selection of high-redshift radio quasars, and the luminosity function at z ∼ 4
... 4.1 Spectroscopy of the 15 NN-selected candidates At the time, none of the 15 QSO candidates selected by our NN had spectra available in the literature. Therefore, long-slit spectra of all 15 were obtained with ...
19
An Investigation into the Effects of Luminosity on the Mid-Infrared Spectral Energy Distributions of Radio-quiet Quasars
... the luminosity at 8 m in luminous ...2006). Our focus on type 1 quasars has reduced the effect of option (1) to the extent ...a luminosity dependence of dust grain size, composition, and ...
8
LOFAR/H-ATLAS: The low-frequency radio luminosity - star-formation rate relation
... LOFAR flux densities of the SFGs measured using the forced photometry method for this work. incorporates the ‘bootstrap’ process described by H16 that corrects for LOFAR beam model uncertainties, but it is carried out at ...
20
GAMA/WiggleZ: the 1.4 GHz radio luminosity functions of high- and low-excitation radio galaxies and their redshift evolution to z = 0.75
... 3.1 Estimating the completeness The overall spectroscopic completeness is given by the number of targets for which we obtained a spectrum of sufficient qual- ity to make a reliable redshift measurement divided by the ...
16
A new sample of giant radio galaxies from the WENSS survey. II. A multi-frequency radio study of a complete sample: Properties of the radio lobes and their environment
... for our subsample of 3CR sources is obtained for a maximum angle of 43 ◦ between the plane of the sky and the line of ...sub- sample are radio galaxies, this agrees with the orientation dependent ...
30
Unveiling the Milky Way: A New Technique for Determining the Optical Color and Luminosity of Our Galaxy
... allowing our Galaxy to be compared directly to objects measured in extragalactic ...a sample of Milky Way analog galaxies designed to reproduce the best Galactic M and M ˙ measurements, including all ...
19
Galaxy And Mass Assembly (GAMA): the 325 MHz radio luminosity function of AGN and star-forming galaxies.
... the radio sources to their optical ...the sample properties and show how the spectral indices of the sources vary as a function of luminosity and ...present our RLFs, and determine the ...
16
The XXL Survey : XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations.
... see Fig. 16 from Smolˇci´c et al. 2017a or Fig. 1 from Delvec- chio et al. 2017 for details). We created the redshift histogram of this dataset. Then we examined the same dataset with an addi- tional threshold ...
12
Does the evolution of the radio luminosity function of star-forming galaxies match that of the star-formation rate function?
... focus our paper and to clarify several ...lution radio surveys, by PRIN–INAF 2012 ‘Looking into the dust- obscured phase of galaxy formation through cosmic zoom lenses in the Herschel Astrophysical Large ...
12
Radio halos in a mass-selected sample of galaxy clusters
... diffuse radio emission in the NVSS images, in these cases, we reprocessed the NVSS datasets, aiming at producing better images, with rms noise ∼2 times below the nominal NVSS rms ...cases. Our analysis led ...
162
Radio properties of a complete sample of nearby groups of galaxies
... affect our age estimate, lowering the break frequency and therefore the estimated ...the radio, but the fact that the lobes have high sur- face brightnesses and smooth surface brightness distributions ...
337
A sample of 669 ultra steep spectrum radio sources to find high redshift radio galaxies
... of our three USS samples in logarithmic histograms ...TN sample coin- cides with that of the WN, its flat end part falls off much ...MP sample, the same effect is less pronounced, though still ...
31
The Sizes of Candidate z~9-10 Galaxies: Confirmation of the Bright CANDELS Sample and Relation with Luminosity and Mass.
... We note that the IRAC-red interlopers are about equally numerous as sources in our z ∼ 9 – 10 sample. Without information from deep Spitzer /IRAC imaging on these sources, they could constitute a serious ...
10
Radio and optical observations of a complete sample of E and SO galaxies
... calculated using 0.5 magnitude bins, and the error bars are given by /n for each bin. The area covered by the UGC is taken as 20668 deg.2. The relationship between N(m) and m must be interpreted with some subtlety, since ...
365