The LOFAR two metre sky survey data release 2: probabilistic spectral source classifications and faint radio source demographics

A. B. Drake*, D. J.B. Smith, M. J. Hardcastle, P. N. Best, R. Kondapally, M. I. Arnaudova, S. Das, S. Shenoy, K. J. Duncan, H. J.A. Röttgering, C. Tasse

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract / Description of output

We present an analysis of 152 355 radio sources identified in the second data release of the LOFAR Two Metre Sky Survey (LoTSS-DR2) with Sloan Digital Sky Survey (SDSS) spectroscopic redshifts in the range <tex-math id="TM0001" notation="LaTeX">$0.00 /lt z /lt 0.57$</tex-math>. Using Monte Carlo simulations, we determine the reliability of each source exhibiting an excess in radio luminosity relative to that predicted from their H <tex-math id="TM0002" notation="LaTeX">$/alpha$</tex-math> emission, and, for a subset of 124 023 sources we combine this measurement with a full BPT analysis. Using these two independent diagnostics, we determine the reliability of each source hosting a supermassive black hole of high or low Eddington-scaled accretion rate, and combine the measurements to determine the reliability of sources belonging to each of four physical classes of objects: star-forming galaxies (SFGs), radio-quiet active galactic nuclei (RQAGN), and high- or low-excitation radio galaxies (HERGs or emission-line LERGs). The result is a catalogue that enables user-defined samples of radio sources with a reliability threshold suited to their science goal, for example prioritizing purity or completeness. Here, we select high-confidence samples of radio sources (>90 per cent reliability) to report: 38 588 radio-excess AGNs in the LoTSS-DR2 sample (362 HERGs, and 12 648 emission-line LERGs), together with 38 729 SFGs, and 18 726 RQAGN. We validate these results through comparison to literature using independent emission-line measurements, and to widely adopted WISE photometric selection techniques. While our use of SDSS spectroscopy limits our current analysis to <tex-math id="TM0003" notation="LaTeX">$/sim 4$</tex-math> per cent of the LoTSS-DR2 catalogue, our method is directly applicable to data from the forthcoming WEAVE-LOFAR survey, which will obtain over a million spectra of 144 MHz selected sources.

Original languageEnglish
Pages (from-to)1107-1126
Number of pages20
JournalMonthly Notices of the Royal Astronomical Society
Volume534
Issue number2
Early online date11 Sept 2024
DOIs
Publication statusPublished - 1 Oct 2024

Keywords / Materials (for Non-textual outputs)

  • catalogues
  • galaxies: active
  • galaxies: evolution
  • galaxies: star formation
  • radio continuum: galaxies

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