MIGHTEE: Multi-wavelength counterparts in the COSMOS field

In this paper, we combine the Early Science radio continuum data from the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) Survey, with optical and near-infrared data and release the cross-matched catalogues. The radio data used in this work covers 0.86 deg2 of the COSMOS field,...

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Main Authors: Whittam, I.H., Prescott, M., Hale, C.L., Jarvis, M.J., Heywood, I., An, F., Glowacki, Marcin, Maddox, N., Marchetti, L., Morabito, L.K., Adams, N.J., Bowler, R.A.A., Hatfield, P.W., Varadaraj, R.G., Collier, J., Frank, B., Taylor, A.R., Santos, M.G., Vaccari, M., Afonso, J., Ao, Y., Delhaize, J., Knowles, K., Kolwa, S., Randriamampandry, S.M., Randriamanakoto, Z., Smirnov, O., Smith, D.J.B., White, S.V.
Format: Journal Article
Published: 2024
Online Access:http://purl.org/au-research/grants/arc/DP210102103
http://hdl.handle.net/20.500.11937/94776
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author Whittam, I.H.
Prescott, M.
Hale, C.L.
Jarvis, M.J.
Heywood, I.
An, F.
Glowacki, Marcin
Maddox, N.
Marchetti, L.
Morabito, L.K.
Adams, N.J.
Bowler, R.A.A.
Hatfield, P.W.
Varadaraj, R.G.
Collier, J.
Frank, B.
Taylor, A.R.
Santos, M.G.
Vaccari, M.
Afonso, J.
Ao, Y.
Delhaize, J.
Knowles, K.
Kolwa, S.
Randriamampandry, S.M.
Randriamanakoto, Z.
Smirnov, O.
Smith, D.J.B.
White, S.V.
author_facet Whittam, I.H.
Prescott, M.
Hale, C.L.
Jarvis, M.J.
Heywood, I.
An, F.
Glowacki, Marcin
Maddox, N.
Marchetti, L.
Morabito, L.K.
Adams, N.J.
Bowler, R.A.A.
Hatfield, P.W.
Varadaraj, R.G.
Collier, J.
Frank, B.
Taylor, A.R.
Santos, M.G.
Vaccari, M.
Afonso, J.
Ao, Y.
Delhaize, J.
Knowles, K.
Kolwa, S.
Randriamampandry, S.M.
Randriamanakoto, Z.
Smirnov, O.
Smith, D.J.B.
White, S.V.
author_sort Whittam, I.H.
building Curtin Institutional Repository
collection Online Access
description In this paper, we combine the Early Science radio continuum data from the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) Survey, with optical and near-infrared data and release the cross-matched catalogues. The radio data used in this work covers 0.86 deg2 of the COSMOS field, reaches a thermal noise of 1.7 μJy beam-1 and contains 6102 radio components. We visually inspect and cross-match the radio sample with optical and near-infrared data from the Hyper Suprime-Cam (HSC) and UltraVISTA surveys. This allows the properties of active galactic nuclei and star-forming populations of galaxies to be probed out to z ≈ 5. Additionally, we use the likelihood ratio method to automatically cross-match the radio and optical catalogues and compare this to the visually cross-matched catalogue. We find that 94 per cent of our radio source catalogue can be matched with this method, with a reliability of 95 per cent. We proceed to show that visual classification will still remain an essential process for the cross-matching of complex and extended radio sources. In the near future, the MIGHTEE survey will be expanded in area to cover a total of ∼20 deg2; thus the combination of automated and visual identification will be critical. We compare the redshift distribution of SFG and AGN to the SKADS and T-RECS simulations and find more AGN than predicted at z ∼1.
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institution Curtin University Malaysia
institution_category Local University
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publishDate 2024
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spelling curtin-20.500.11937-947762024-05-07T08:48:39Z MIGHTEE: Multi-wavelength counterparts in the COSMOS field Whittam, I.H. Prescott, M. Hale, C.L. Jarvis, M.J. Heywood, I. An, F. Glowacki, Marcin Maddox, N. Marchetti, L. Morabito, L.K. Adams, N.J. Bowler, R.A.A. Hatfield, P.W. Varadaraj, R.G. Collier, J. Frank, B. Taylor, A.R. Santos, M.G. Vaccari, M. Afonso, J. Ao, Y. Delhaize, J. Knowles, K. Kolwa, S. Randriamampandry, S.M. Randriamanakoto, Z. Smirnov, O. Smith, D.J.B. White, S.V. In this paper, we combine the Early Science radio continuum data from the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) Survey, with optical and near-infrared data and release the cross-matched catalogues. The radio data used in this work covers 0.86 deg2 of the COSMOS field, reaches a thermal noise of 1.7 μJy beam-1 and contains 6102 radio components. We visually inspect and cross-match the radio sample with optical and near-infrared data from the Hyper Suprime-Cam (HSC) and UltraVISTA surveys. This allows the properties of active galactic nuclei and star-forming populations of galaxies to be probed out to z ≈ 5. Additionally, we use the likelihood ratio method to automatically cross-match the radio and optical catalogues and compare this to the visually cross-matched catalogue. We find that 94 per cent of our radio source catalogue can be matched with this method, with a reliability of 95 per cent. We proceed to show that visual classification will still remain an essential process for the cross-matching of complex and extended radio sources. In the near future, the MIGHTEE survey will be expanded in area to cover a total of ∼20 deg2; thus the combination of automated and visual identification will be critical. We compare the redshift distribution of SFG and AGN to the SKADS and T-RECS simulations and find more AGN than predicted at z ∼1. 2024 Journal Article http://hdl.handle.net/20.500.11937/94776 10.1093/mnras/stad3307 http://purl.org/au-research/grants/arc/DP210102103 http://creativecommons.org/licenses/by/4.0/ fulltext
spellingShingle Whittam, I.H.
Prescott, M.
Hale, C.L.
Jarvis, M.J.
Heywood, I.
An, F.
Glowacki, Marcin
Maddox, N.
Marchetti, L.
Morabito, L.K.
Adams, N.J.
Bowler, R.A.A.
Hatfield, P.W.
Varadaraj, R.G.
Collier, J.
Frank, B.
Taylor, A.R.
Santos, M.G.
Vaccari, M.
Afonso, J.
Ao, Y.
Delhaize, J.
Knowles, K.
Kolwa, S.
Randriamampandry, S.M.
Randriamanakoto, Z.
Smirnov, O.
Smith, D.J.B.
White, S.V.
MIGHTEE: Multi-wavelength counterparts in the COSMOS field
title MIGHTEE: Multi-wavelength counterparts in the COSMOS field
title_full MIGHTEE: Multi-wavelength counterparts in the COSMOS field
title_fullStr MIGHTEE: Multi-wavelength counterparts in the COSMOS field
title_full_unstemmed MIGHTEE: Multi-wavelength counterparts in the COSMOS field
title_short MIGHTEE: Multi-wavelength counterparts in the COSMOS field
title_sort mightee: multi-wavelength counterparts in the cosmos field
url http://purl.org/au-research/grants/arc/DP210102103
http://hdl.handle.net/20.500.11937/94776