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

被引:61
作者
Duncan, K. J. [1 ]
Sabater, J. [2 ]
Rottgering, H. J. A. [1 ]
Jarvis, M. J. [3 ]
Smith, D. J. B. [4 ]
Best, P. N. [2 ]
Callingham, J. R. [5 ]
Cochrane, R. [2 ]
Croston, J. H. [6 ]
Hardcastle, M. J. [4 ]
Mingo, B. [6 ]
Morabito, L. [3 ]
Nisbet, D. [2 ]
Prandoni, I. [7 ]
Shimwell, T. W. [1 ,5 ]
Tasse, C. [8 ]
White, G. J. [6 ,9 ]
Williams, W. L. [4 ]
Alegre, L. [2 ]
Chyzy, K. T. [10 ]
Gurkan, G. [11 ]
Hoeft, M. [12 ]
Kondapally, R. [2 ]
Mechev, A. P. [1 ]
Miley, G. K. [1 ]
Schwarz, D. J. [13 ]
van Weeren, R. J. [1 ]
机构
[1] Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands
[2] Royal Observ, Inst Astron, SUPA, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland
[3] Univ Oxford, Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England
[4] Univ Hertfordshire, Sch Phys Astron & Math, Ctr Astrophys Res, Coll Lane, Hatfield AL10 9AB, Herts, England
[5] ASTRON, Netherlands Inst Radio Astron, Postbus 2, NL-7990 AA Dwingeloo, Netherlands
[6] Open Univ, Sch Phys Sci, Walton Hall, Milton Keynes MK7 6AA, Bucks, England
[7] INAF, Ist Radioastron, Via Gobetti 101, I-40129 Bologna, Italy
[8] Univ Paris Diderot, CNRS, Observ Paris, GEPI, 5 Pl Jules Jansse, F-92190 Meudon, France
[9] Rutherford Appleton Lab, Space Sci & Technol Dept, Didcot OX11 0NL, Oxon, England
[10] Jagiellonian Univ, Astron Observ, Ul Orla 171, PL-30244 Krakow, Poland
[11] CSIRO Astron & Space Sci, POB 1130, Bentley, WA 6102, Australia
[12] Thuringer Landessternwarte TLS, Sternwarte 5, D-07778 Tautenburg, Germany
[13] Univ Bielefeld, Fak Phys, Postfach 100131, D-33501 Bielefeld, Germany
基金
英国科学技术设施理事会; 美国国家科学基金会; 美国国家航空航天局;
关键词
radio continuum: galaxies; galaxies: active; galaxies: distances and redshifts; GALAXIES;
D O I
10.1051/0004-6361/201833562
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 (10(h)45(m)00(s) < right ascension < 15(h)30(m)00(s) and 45 degrees 00'00 '' < declination < 57 degrees 00'00 '') with a median sensitivity of 71 mu Jy beam(-1) and a resolution of 6 ''. In this paper we present photometric redshifts (photo-z) for 94.4% of optical sources over this region that are detected in the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) 3 pi steradian survey. Combining the Pan-STARRS optical data with mid-infrared photometry from the Wide-field Infrared Survey Explorer, we estimate photo-zs using a novel hybrid photometric redshift methodology optimised to produce the best possible performance for the diverse sample of radio continuum selected sources. For the radio-continuum detected population, we find an overall scatter in the photo-z of 3.9% and an outlier fraction (vertical bar Z(phot) - Z(spec)vertical bar/(1 + Z(spec)) > 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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页数:17
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