scholarly journals Spectral energy distributions for galaxies in high-redshift clusters – II. 0016 + 16 at z = 0.54

1985 ◽  
Vol 217 (2) ◽  
pp. 239-264 ◽  
Author(s):  
Richard S. Ellis ◽  
Warrick J. Couch ◽  
Iain MacLaren ◽  
David C. Koo
2000 ◽  
Vol 17 (1) ◽  
pp. 56-71 ◽  
Author(s):  
Paul J. Francis ◽  
Matthew T. Whiting ◽  
Rachel L. Webster

AbstractWe present quasi-simultaneous multi-colour optical/near-IR photometry for 157 radio selected quasars, forming an unbiassed sub-sample of the Parkes Flat-Spectrum Sample. Data are also presented for 12 optically selected QSOs, drawn from the Large Bright QSO Survey. The spectral energy distributions of the radio- and optically-selected sources are quite different. The optically selected QSOs are all very similar: they have blue spectral energy distributions curving downwards at shorter wavelengths. Roughly 90% of the radio-selected quasars have roughly power-law spectral energy distributions, with slopes ranging from Fv∝v0 to Fv∝v−2. The remaining 10% have spectral energy distributions showing sharp peaks: these are radio galaxies and highly reddened quasars. Four radio sources were not detected down to magnitude limits of H ∼ 19·6. These are probably high redshift (z > 3) galaxies or quasars. We show that the colours of our red quasars lie close to the stellar locus in the optical: they will be hard to identify in surveys such as the Sloan Digital Sky Survey. If near-IR photometry is added, however, the red power-law sources can be clearly separated from the stellar locus: IR surveys such as 2MASS should be capable of finding these sources on the basis of their excess flux in the K-band.


1994 ◽  
Vol 108 ◽  
pp. 374 ◽  
Author(s):  
Jill Bechtold ◽  
Martin Elvis ◽  
Fabrizio Fiore ◽  
Olga Kuhn ◽  
Roc M. Cutri ◽  
...  

1994 ◽  
Author(s):  
Jill Bechtold ◽  
Roc Cutri ◽  
Marcia Rieke ◽  
Martin Elvis ◽  
Fabrizio Fiore ◽  
...  

2020 ◽  
Vol 500 (3) ◽  
pp. 2859-2860
Author(s):  
A S G Robotham ◽  
S Bellstedt ◽  
C del P Lagos ◽  
J E Thorne ◽  
L J Davies ◽  
...  

Sign in / Sign up

Export Citation Format

Share Document