The LOFAR Two-metre Sky Survey IV. First Data Release: Photometric redshifts and rest-frame magnitudes

Duncan, Kenneth J, Sabater, J., Röttgering, H. J. A., Jarvis, M. J., Smith, D. J. B., Best, P. N., Callingham, J. R., Cochrane, R., Croston, J. H., Hardcastle, M. J., Mingo, B., Morabito, L., Nisbet, D., Prandoni, I., Shimwell, T. W., Tasse, C., White, G. J., Williams, W. L., Alegre, L., Chyży, K. T., Gürkan, G., Hoeft, M., Kondapally, R., Mechev, A. P., Miley, G. K., Schwarz, D. J. and Weeren, R. J. van (2018) The LOFAR Two-metre Sky Survey IV. First Data Release: Photometric redshifts and rest-frame magnitudes. ISSN 0004-6361
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The LOFAR Two-metre Sky Survey (LoTSS) is a sensitive, high-resolution 120-168 MHz survey of the Northern sky. The LoTSS First Data Release (DR1) presents 424 square degrees of radio continuum observations over the HETDEX Spring Field (10h45m00s $ 0.15$) of 7.9%. We also find that, at a given redshift, there is no strong trend in photo-$z$ quality as a function of radio luminosity. However there are strong trends as a function of redshift for a given radio luminosity, a result of selection effects in the spectroscopic sample and/or intrinsic evolution within the radio source population. Additionally, for the sample of sources in the LoTSS First Data Release with optical counterparts, we present rest-frame optical and mid-infrared magnitudes based on template fits to the consensus photometric (or spectroscopic when available) redshift.

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