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The MeerKAT Galaxy Cluster Legacy Survey I. Survey Overview and Highlights

by Gouws, M , Camilo, F , Kotzé, P P A , Retana-Montenegro, E , Kapp, F B , Marais, S J , Deane, R , van Balla, T J , Frank, B S , Sambu, N , Maree, M D J , Brüggen, M , Rudnick, L , Jordaan, J D B , Bennett, T G H , Ngcebetsha, B , Rust, A N , Kriek, N , Ramanujam, N M , Sirothia, S K , Welz, M G , Hoosen, S W , Horn, D M , Venter, A J , Namumba, B , Esterhuyse, S W P , Williams, L P , Tasse, C , Kasper, V A , Krishnan, V K , Schwardt, L C , Abbott, T D , R Van Wyk , Madisa, K , Millenaar, R P , Schwartz, R L , Goedhart, S , Schollar, C T G , Toruvanda, O , Mphego, M C , Mhlahlo, N , Passmoor, S S , Ranchod, S , Horrell, J M G , Gumede, S C , Hlakola, M J , Sofeya, L , Dikgale-Mahlakoana, M A , Murphy, E , Xaia, B , Sikhosana, S P , Venturi, T , Bietenholz, M F , Julie, R P M , Legodi, L S , Ngoasheng, K J , Renil, R , Slabber, M , du Toit, L J , Ockards, M T , van der Byl, A , Moodley, K , Fataar, S , Lunsky, B M , Ramudzuli, Z R , Robyntjies, A , Loubser, S I , Pillay, D S , Siebrits, R , Botha, A G , Main, J P L , Mauch, T , Kesebonye, K C , Peens-Hough, A , Cotton, W D , Magnus, L G , Kolokythas, K , Patel, A A , Foley, A R , Chibueze, J O , Lord, R T , Kusel, T W , Marchegiani, P , Fadana, G , van der Merwe, C , Smirnov, O , Button, C , G

in Cosmic dust / Cubes / Faraday effect / Field of view / Galactic clusters / Image enhancement / Mapping / Polarization / Radio galaxies / Sensitivity / Star formation

2021

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The MeerKAT Galaxy Cluster Legacy Survey I. Survey Overview and Highlights

in Cosmic dust / Cubes / Faraday effect / Field of view / Galactic clusters / Image enhancement / Mapping / Polarization / Radio galaxies / Sensitivity / Star formation

2021

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The MeerKAT Galaxy Cluster Legacy Survey I. Survey Overview and Highlights

in Cosmic dust / Cubes / Faraday effect / Field of view / Galactic clusters / Image enhancement / Mapping / Polarization / Radio galaxies / Sensitivity / Star formation

2021

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Paper

The MeerKAT Galaxy Cluster Legacy Survey I. Survey Overview and Highlights

Gouws, M,

Camilo, F,

Kotzé, P P A,

Retana-Montenegro, E,

Kapp, F B,

Marais, S J,

Deane, R,

van Balla, T J,

Frank, B S,

Sambu, N,

Maree, M D J,

Brüggen, M,

Rudnick, L,

Jordaan, J D B,

Bennett, T G H,

Ngcebetsha, B,

Rust, A N,

Kriek, N,

Ramanujam, N M,

Sirothia, S K,

Welz, M G,

Hoosen, S W,

Horn, D M,

Venter, A J,

Namumba, B,

Esterhuyse, S W P,

Williams, L P,

Tasse, C,

Kasper, V A,

Krishnan, V K,

Schwardt, L C,

Abbott, T D,

R Van Wyk,

Madisa, K,

Millenaar, R P,

Schwartz, R L,

Goedhart, S,

Schollar, C T G,

Toruvanda, O,

Mphego, M C,

Mhlahlo, N,

Passmoor, S S,

Ranchod, S,

Horrell, J M G,

Gumede, S C,

Hlakola, M J,

Sofeya, L,

Dikgale-Mahlakoana, M A,

Murphy, E,

Xaia, B,

Sikhosana, S P,

Venturi, T,

Bietenholz, M F,

Julie, R P M,

Legodi, L S,

Ngoasheng, K J,

Renil, R,

Slabber, M,

du Toit, L J,

Ockards, M T,

van der Byl, A,

Moodley, K,

Fataar, S,

Lunsky, B M,

Ramudzuli, Z R,

Robyntjies, A,

Loubser, S I,

Pillay, D S,

Siebrits, R,

Botha, A G,

Main, J P L,

Mauch, T,

Kesebonye, K C,

Peens-Hough, A,

Cotton, W D,

Magnus, L G,

Kolokythas, K,

Patel, A A,

Foley, A R,

Chibueze, J O,

Lord, R T,

Kusel, T W,

Marchegiani, P,

Fadana, G,

van der Merwe, C,

Smirnov, O,

Button, C,

2021

Overview

MeerKAT's large number of antennas, spanning 8 km with a densely packed 1 km core, create a powerful instrument for wide-area surveys, with high sensitivity over a wide range of angular scales. The MeerKAT Galaxy Cluster Legacy Survey (MGCLS) is a programme of long-track MeerKAT L-band (900-1670 MHz) observations of 115 galaxy clusters, observed for \\(\\sim\\)6-10 hours each in full polarisation. The first legacy product data release (DR1), made available with this paper, includes the MeerKAT visibilities, basic image cubes at \\(\\sim\\)8\" resolution, and enhanced spectral and polarisation image cubes at \\(\\sim\\)8\" and 15\" resolutions. Typical sensitivities for the full-resolution MGCLS image products are \\(\\sim\\)3-5 {\\mu}Jy/beam. The basic cubes are full-field and span 4 deg^2. The enhanced products consist of the inner 1.44 deg^2 field of view, corrected for the primary beam. The survey is fully sensitive to structures up to \\(\\sim\\)10' scales and the wide bandwidth allows spectral and Faraday rotation mapping. HI mapping at 209 kHz resolution can be done at \\(0

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Publisher

Cornell University Library, arXiv.org

Subject

/ Cubes

/ Mapping