Abstract. Using 1.4 GHz ATCA & VLA images with 5.5 GHz ATCA data, we present a sample of 12 bent-tailed galaxies over the 4 deg2 area of the Chandra Deep Field South (CDFS). We find 10 new sources, one of which is possibly the highest red-shift bent-tailed galaxy detected at z ∼ 2. Key words. Extended radio sources—head–tail galaxies. 1. CDFS bent-tailed galaxies Bent-tailed sources are found almost exclusively in rich clusters of galaxies in the local Universe (z ≤ 1), and their curvature is believed to result of interaction Figure 1. Bent-tailed sources detected in the CDFS field; Radio contours at 1.4 (ATCA – blue, VLA – red) and 5.5 (ATCA – black) GHz overlaid on optical images from the SWIRE and DSS. Countours begin at 3σ and incre...
<p>To probe the earliest eras of cluster formation, we need to find clusters with a variety of morph...
We present X-ray source catalogs for the ≈7 Ms exposure of the Chandra Deep Field-South (CDF-S), whi...
The sub-mJy radio population is a mixture of active systems, that is star-forming galaxies (SFGs) an...
Using 1. 4 GHz ATCA & VLA images with 5. 5 GHz ATCA data, we present a sample of 12 bent-tailed ...
Using the 1.4 GHz Australia Telescope Large Area Survey, supplemented by the 1.4 GHz Very Large Arra...
Using the 1.4 GHz Australia Telescope Large Area Survey, supplemented by the 1.4 GHz Very Large Arra...
Open AccessWe report the serendipitous detection of a Wide-Angle Tail (WAT) radio galaxy at 240 and ...
Building a map of galaxy cluster evolution requires clusters spanning a range of redshifts, masses, ...
We are conducting a survey of distant clusters of galaxies (0.5 < z < 3.0) using bent, double-lobed ...
Thesis (Ph.D.)--Boston University PLEASE NOTE: Boston University Libraries did not receive an Autho...
We present a new image of the 9.0 GHz radio emission from the extended Chandra Deep Field South. A t...
Bent tail radio sources (BTRSs) are radio galaxies which have jets that show a characteristic C‐sha...
Clusters of galaxies are the most massive and large gravitationally bounded systems in the whole Uni...
Bent-double radio sources can act as tracers for clusters of galaxies. We present imaging and spectr...
We present a list of candidate tailed radio galaxies using the TIFR GMRT Sky Survey Alternative Data...
<p>To probe the earliest eras of cluster formation, we need to find clusters with a variety of morph...
We present X-ray source catalogs for the ≈7 Ms exposure of the Chandra Deep Field-South (CDF-S), whi...
The sub-mJy radio population is a mixture of active systems, that is star-forming galaxies (SFGs) an...
Using 1. 4 GHz ATCA & VLA images with 5. 5 GHz ATCA data, we present a sample of 12 bent-tailed ...
Using the 1.4 GHz Australia Telescope Large Area Survey, supplemented by the 1.4 GHz Very Large Arra...
Using the 1.4 GHz Australia Telescope Large Area Survey, supplemented by the 1.4 GHz Very Large Arra...
Open AccessWe report the serendipitous detection of a Wide-Angle Tail (WAT) radio galaxy at 240 and ...
Building a map of galaxy cluster evolution requires clusters spanning a range of redshifts, masses, ...
We are conducting a survey of distant clusters of galaxies (0.5 < z < 3.0) using bent, double-lobed ...
Thesis (Ph.D.)--Boston University PLEASE NOTE: Boston University Libraries did not receive an Autho...
We present a new image of the 9.0 GHz radio emission from the extended Chandra Deep Field South. A t...
Bent tail radio sources (BTRSs) are radio galaxies which have jets that show a characteristic C‐sha...
Clusters of galaxies are the most massive and large gravitationally bounded systems in the whole Uni...
Bent-double radio sources can act as tracers for clusters of galaxies. We present imaging and spectr...
We present a list of candidate tailed radio galaxies using the TIFR GMRT Sky Survey Alternative Data...
<p>To probe the earliest eras of cluster formation, we need to find clusters with a variety of morph...
We present X-ray source catalogs for the ≈7 Ms exposure of the Chandra Deep Field-South (CDF-S), whi...
The sub-mJy radio population is a mixture of active systems, that is star-forming galaxies (SFGs) an...