The LOFAR Two-metre Sky Survey (LoTSS) III. First Data Release: optical/IR identifications and value-added catalogue
W. L. Williams, M. J. Hardcastle, P. N. Best, J. Sabater, J. H., Croston, K. J. Duncan, T. W. Shimwell, H. J. A. R\"ottgering, D. Nisbet, G., G\"urkan, L. Alegre, R. K. Cochrane, A. Goyal, C. L. Hale, N. Jackson, M., Jamrozy, R. Kondapally, M. Kunert-Bajraszewska, V. H. Mahatma

TL;DR
The paper presents the first data release of the LoTSS survey, including a comprehensive catalogue of over 318,000 radio sources with optical/IR identifications, achieved through combined statistical and visual classification methods.
Contribution
It introduces a detailed methodology for associating radio sources with optical/IR counterparts and provides a large, publicly available value-added catalogue for the first LoTSS data release.
Findings
73% of sources have optical/IR identifications
Over 318,000 radio sources catalogued
Combined statistical and visual classification methods used
Abstract
The LOFAR Two-metre Sky Survey (LoTSS) is an ongoing sensitive, high-resolution 120-168 MHz survey of the Northern sky with diverse and ambitious science goals. Many of the scientific objectives of LoTSS rely upon, or are enhanced by, the association or separation of the sometimes incorrectly catalogued radio components into distinct radio sources, and the identification and characterisation of the optical counterparts to these sources. Here we present the source associations and optical and/or IR identifications for sources in the first data release, which are made using a combination of statistical techniques and visual association and identification. We document in detail the colour- and magnitude-dependent likelihood ratio method used for statistical identification as well as the Zooniverse project, called LOFAR Galaxy Zoo, used for the visual classification. We describe the process…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena · Astronomical Observations and Instrumentation
