English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We present optical spectroscopy, near‐infrared (mostly  K ‐band) and radio (151‐MHz and 1.4‐GHz) imaging of the first complete region (TOOT00) of the TexOx‐1000 (TOOT) redshift survey of radio sources. The 0.0015‐sr (∼5 deg 2 ) TOOT00 region is selected from pointed observations of the Cambridge Low‐Frequency Survey Telescope at 151 MHz at a flux density limit of ≃100 mJy, approximately five times fainter than the 7C Redshift Survey (7CRS), and contains 47 radio sources. We have obtained 40 spectroscopic redshifts (∼85 per cent completeness). Adding redshifts estimated for the seven other cases yields a median redshift   z  med ∼ 1.25 . We find a significant population of objects with Fanaroff–Riley type I (FRI) like radio structures at radio luminosities above both the low‐redshift FRI/II break and the break in the radio luminosity function. The redshift distribution and subpopulations of TOOT00 are broadly consistent with extrapolations from the 7CRS/6CE/3CRR data sets underlying the SKADS Simulated Skies Semi‐Empirical Extragalactic Data base, S 3 ‐SEX.

The TexOx‐1000 redshift survey of radio sources I: the TOOT00 region