scholarly journals A search for high-redshift quasars among GB/FIRST flat-spectrum radio sources

1998 ◽  
Vol 297 (4) ◽  
pp. 1115-1122 ◽  
Author(s):  
I. M. Hook ◽  
R. H. Becker ◽  
R. G. McMahon ◽  
R. L. White
2014 ◽  
Vol 10 (S313) ◽  
pp. 231-235
Author(s):  
Leah K. Morabito ◽  
Adam Deller ◽  
J. B. R. Oonk ◽  
Huub Röttgering ◽  
George Miley

AbstractThe correlation between radio spectral steepness and redshift has been successfully used to find high redshift (z ⩾ 2) radio galaxies, but the origin of this relation is unknown. The ultra-steep spectra of high-z radio sources make them ideally suited for studies with the Low Band Antenna of the new Low Frequency Array, which covers 10–80 MHz and has baselines up to about 1300 km. As part of an ongoing survey, we use the longest baselines to map the low-frequency (< 70 MHz) spatial distributions along the jets of 5 bright extended steep spectrum high-z radio sources. From this, we will determine whether the spectra change over these spatially resolved sources, thereby constraining particle acceleration processes. We present early results from our low-frequency survey of ultra-steep spectrum radio galaxies. The first low frequency long baseline images of these objects are presented.


2000 ◽  
Vol 143 (2) ◽  
pp. 303-333 ◽  
Author(s):  
C. De Breuck ◽  
W. van Breugel ◽  
H. J.A. Röttgering ◽  
G. Miley

2002 ◽  
Vol 199 ◽  
pp. 217-218 ◽  
Author(s):  
H. Andernach ◽  
O.V. Verkhodanov ◽  
N.V. Verkhodanova

We used radio source catalogues accessible from the CATS database to establish radio continuum spectra for decametric radio sources in the UTR-2 catalogue. In an attempt to find further candidates for high-redshift radio galaxies, we searched the FIRST and NVSS surveys for counterparts of a sample of UTR sources with ultra-steep radio spectra (USS, α ≤ −1.2, S ∼ vα). We derived accurate positions and sizes for 23 of these USS sources. The search for optical counterparts from the APM (object) and DSS (image) databases, as well as infrared and X—ray identifications of these UTR sources are in progress.


1996 ◽  
Vol 106 ◽  
pp. 247 ◽  
Author(s):  
K. C. Chambers ◽  
G. K. Miley ◽  
W. J. M. van Breugel ◽  
M. A. R. Bremer ◽  
J.-S. Huang ◽  
...  

2013 ◽  
Vol 22 (12) ◽  
pp. 1350089 ◽  
Author(s):  
PRABHAKAR TIWARI ◽  
PANKAJ JAIN

We present a detailed statistical analysis of the alignment of polarizations of radio sources at high redshift. This study is motivated by the puzzling signal of alignment of polarizations from distant quasars at optical frequencies. We use a coordinate invariant measure of dispersion to test for alignment of polarizations of widely separated sources. The data from JVAS/CLASS 8.4 GHz surveys are used for our study. We find that the data set with polarization flux greater than 1 mJy shows a significant signal of alignment at distance scales of order 150 Mpc. The significance of alignment decreases as we go to larger distances. In contrast the data set with polarization flux less than 1 mJy does not show significant alignment at short distances. However this set, as well as the full data sample, shows a very significant signal at large distances of order 500–850 Mpc. Due to the presence of relatively large error in the low polarization sample, this signal needs to be tested further with more refined data. We also study the signal by imposing a cut on the error in polarization. We find that the significance of alignment increases with decrease in fractional error. We are unable to attribute our results to known sources of bias. We discuss a possible physical explanation of our results.


1996 ◽  
Vol 175 ◽  
pp. 561-562
Author(s):  
P.A. Shaver ◽  
J.V. Wall ◽  
K.I. Kellermann ◽  
C. Jackson ◽  
M.R. Hawkins

An upper limit on the space density of quasars at z > 5 is obtained independent of any optical magnitude limit, from the complete identification of a large sample of flat-spectrum radio sources. This upper limit is below the observed space density at z ≃ 2 − 3, showing that the turnover in space density is real and not merely due to obscuration.


2014 ◽  
Vol 569 ◽  
pp. A52 ◽  
Author(s):  
V. Singh ◽  
A. Beelen ◽  
Y. Wadadekar ◽  
S. Sirothia ◽  
C. H. Ishwara-Chandra ◽  
...  

1999 ◽  
Vol 515 (2) ◽  
pp. 558-566 ◽  
Author(s):  
David B. Shaffer ◽  
K. I. Kellermann ◽  
T. J. Cornwell
Keyword(s):  

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