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J/MNRAS/485/586
  Star formation in galaxy cluster cores (Rodriguez-Munoz+, 2019)
img(gal)
    J/MNRAS/485/586/table1(c)Description of the galaxy cluster sample (24 rows)
    J/MNRAS/485/586/table2Overview of the photometric bands used in this work (26 rows)
    J/MNRAS/485/586/table3Limiting fluxes (5σ) of the Spitzer and Herschel photometric catalogues used in this work (24 rows)
    J/MNRAS/485/586/table4Summary of some of the quantities used for the identification of cluster members and an evaluation of the technique (10 rows)
    J/MNRAS/485/586/table5Number of galaxies selected with the different criteria used to build the final samples of star-forming cluster members (R/R200<0.1), and average SF activity indicators (24 rows)
    J/MNRAS/485/586/table6Number of galaxies selected with the different criteria used to build the final samples of star-forming cluster members (0.1<R/R200<0.2), and average SF activity indicators (24 rows)
    J/MNRAS/485/586/table7Number of galaxies selected with the different criteria used to build the final samples of star-forming cluster members (0.2<R/R200<0.3), and average SF activity indicators (24 rows)
    J/MNRAS/485/586/table8Number counts and average properties of field galaxy samples (24 rows)

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       (c)  indicates tables which contain celestial coordinates 
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