Total radio luminosity function for ATLAS
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 ...
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Does the evolution of the radio luminosity function of star-forming galaxies match that of the star-formation rate function?
... between radio continuum luminosity and star formation rate (SFR) is of crucial importance to make reliable predictions for the forthcoming ultra- deep radio surveys and to allow a full exploitation ...
12
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
Neural-network selection of high-redshift radio quasars, and the luminosity function at z ∼ 4
... optical luminosity function (LF) of radio-loud QSOs at z ∼ 4, and also the LF of the total QSO population and its comoving ...the radio-loud fraction at high z is similar to that at low ...
19
Herschel ATLAS/GAMA: how does the far IR luminosity function depend on galaxy group properties?
... Our stacking method for measuring the CLF in groups involves subtracting the estimated local background density of galaxies from the total projected counts, which means that our results might be affected by how we ...
18
ATLAS Future Plans: Upgrade and the Physics with High Luminosity
... the ATLAS trigger and data acqui- sition is motivated by the desire to maintain low p T thresh- olds for isolated electrons and muons with increasing lu- minosity in order to maximize the physics acceptance for ...
6
Galaxy And Mass Assembly (GAMA): the 325 MHz radio luminosity function of AGN and star-forming galaxies.
... The structure of this paper is as follows. In Section 2, we outline the GAMA survey and the GMRT data used in this study. In Sec- tion 3, we explain the technique to match the radio sources to their optical ...
16
An Observational Determination of the Bolometric Quasar Luminosity Function
... break luminosity and faint-end slope out to z ∼ ...on luminosity, a single bolometric QLF self-consistently reproduces the observed QLFs in all bands and at all redshifts for which we compile ...this ...
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An Observational Determination of the Bolometric Quasar Luminosity Function
... break luminosity and faint-end slope out to z ∼ ...on luminosity, a single bolometric QLF self-consistently reproduces the observed QLFs in all bands and at all redshifts for which we compile ...this ...
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Radio Sources in the COSMOS Field: Star Forming Properties of High Luminosity Radio Sources
... 2.6 Summary and Conclusions Different studies determining the evolution of the SFR density over cosmic times have employed a range of SFR tracers. Yet many of these commonly used tracers are calibrated on local sample of ...
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Cosmic evolution of radio sources in ATLAS
... my radio luminosity function data when I became hopelessly stuck and helped me to un- derstand RLFs and (finally!) construct them ...in ATLAS paper from the bin and convinced me that it was ...
213
Cosmic evolution of radio sources in ATLAS
... my radio luminosity function data when I became hopelessly stuck and helped me to un- derstand RLFs and (finally!) construct them ...in ATLAS paper from the bin and convinced me that it was ...
17
Measuring the quasar luminosity function below the detection threshold
... SKADS radio-quiet al- though there are deviations at the bright end, where the SKADS radio-quiet population rapidly drops off compared to the reconstructed ...into radio-loud and radio-quiet ( ...
93
Revisiting the luminosity function of single halo white dwarfs
... dwarf luminosity function and that obtained with our reference model, for which the ratio of non-DA white dwarfs is ...ical luminosity function and even ...the luminosity bins close to ...
10
The ATLAS-SPT radio survey of cluster galaxies
... 1.4 Radio Telescopes Our knowledge about astrophysical processes is based on observations of the electromagnetic radiation they ...The total luminosity L of such an object is a measurement of its ...
330
Evolution of the stellar mass function and infrared luminosity function of galaxies since z = 1.2
... K-band luminosity function and stellar mass function (SMF) for red and blue galaxies at z ...of total galaxy light, photometric redshift, and absolute ...K-band luminosity density for ...
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Luminosity determination in pp collisions at √s = 8 TeV using the ATLAS detector at the LHC
... the ATLAS detec- tor [12] and are primarily used to monitor radiation con- ditions in the experimental ...calibrated luminosity measurements, the total num- ber of pixel clusters observed in each ...
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The faint end of the 250μm luminosity function at z< 0 5
... In addition, large and deep spectroscopic surveys such as EU- CLID and DESI will further improve the quality of photometric redshift. Acknowledgements. P.N. acknowledges the support of the Royal Society through the award ...
6
Radio sources in the 6dFGS: Local luminosity functions at 1.4 GHz for star-forming galaxies and radio-loud AGN
... ACKNOWLEDGEMENTS We would like to thank the Anglo-Australian Observatory staff at the UK Schmidt Telescope and the entire 6dFGS team for ensuring the success of the 6dFGS. We thank D. Heath Jones for providing early ...
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Remnant radio-loud AGN in the Herschel-ATLAS field
... the total flux density at 150 MHz (the exact frequency for the measurement of a core flux density is unimportant, since the cores of radio- loud AGN are expected to be flat spectrum out to high frequencies ...
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