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Table 3.

Selected targets for the surface brightness profile comparison of the HUDF WFC3 IR mosaics.

ID IAU ID MUSE ID α δ z PA b/a Sky background limiting radius
(1) (2) (3) (4) (5) (6) (7) (8) (9)
(degrees) (degrees) (degrees) (kpc)
HUDF-1 J033237.30–274729.3 5 53.16164 −27.78025 0.618 −14.18 0.878 80
HUDF-2 J033241.40–274717.1 870 53.17254 −27.78812 0.619 −30.61 0.599 140
HUDF-5 J033237.30–274729.3 862 53.15545 −27.79150 0.667 75.18 0.900 140
ABYSS-1 J033240.78–274615.6 1 53.16993 −27.77106 0.622 −15.82 0.884 80
ABYSS-2 J033242.25–274625.3 916 53.17606 −27.77371 1.288 −3.31 0.890 80
ABYSS-3 J033237.96–274651.9 7 53.15815 −27.78109 0.620 64.69 0.860 80

Notes.

Columns: (1) ID. (2) IAU ID. (3) MUSE catalogue ID. (4) Right ascension (degrees). (5) Declination (degrees). (6) Spectroscopic z from the MUSE HUDF catalogue (Bacon et al. 2017). (7) Position angle (degrees, anti-clockwise from north). (8) Axis ratio of the minor over the major axis. (9) Minimum galactocentric radius used to calculate the local sky background (kpc).

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