The Complete ATLAS Radio Luminosity Function
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 ...
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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 ...
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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 z and ...
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Herschel ATLAS/GAMA: how does the far IR luminosity function depend on galaxy group properties?
... a function of group mass and redshift are consistent between these two methods, but the results from the direct method are less noisy, so we use the direct method for most of our ...
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The Evolution QSOs—The Optical Luminosity Function
... optical luminosity function which fits the observed QSO optical luminosity function, is ...optical luminosity function are also determined. A complete understanding of the ...
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Galaxy And Mass Assembly (GAMA): the 325 MHz radio luminosity function of AGN and star-forming galaxies.
... higher luminosity. Radio-loud AGN samples selected at lower frequency are not as likely to detect sig- nificant numbers of sources with beamed cores, as at lower fre- quency the lobes of galaxies should ...
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Upgrade of the ATLAS Hadronic Tile Calorimeter for the High Luminosity LHC
... of ATLAS TileCal for HL-LHC is nearly complete, where essentially all parts of the system have been prototyped and tested with other parts of the ...the ATLAS pit by the end of ...
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An Observational Determination of the Bolometric Quasar Luminosity Function
... more complete census of obscured quasars, and sample much fainter luminosities and wider (∼ 4 − 5 dex) luminosity ranges, but are measured from much smaller sur- vey areas ...quasar luminosity in a ...
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An Observational Determination of the Bolometric Quasar Luminosity Function
... more complete census of obscured quasars, and sample much fainter luminosities and wider (∼ 4 − 5 dex) luminosity ranges, but are measured from much smaller sur- vey areas ...quasar luminosity in a ...
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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 ...
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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 ...
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A Physical Model for the Luminosity Function of High‐Redshift Quasars
... THEORETICAL LUMINOSITY FUNCTIONS We discuss two models for the high-redshift quasar lumi- nosity function that are based on the Press-Schechter (1974) mass function of dark matter halos (including ...
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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 ( ...
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Luminosity Function of White Dwarfs in the Local Disk and Halo
... The degenerate star ratio, if complete, ought to be somewhat lower since a larger effective interval of the mass function has formed white dwarfs in the halo po[r] ...
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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 ...total luminosity L of such an object is a measurement of its total energy ...
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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 ...
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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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The 2dF Galaxy Redshift survey : the bJ-band galaxy luminosity function and survey selection function.
... the luminosity function depends on spectral ...selection function of the ...the luminosity function, including that from the Sloan Digital Sky Survey ...mated luminosity ...
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Improved luminosity determination in pp collisions at √s=7 TeV using the ATLAS detector at the LHC
... Tile luminosity algorithm measures PMT currents for selected cells in a region near | η | ≈ ...a function of the luminosity are ...the luminosity measured by the LUCID_EventOR algorithm in a ...
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