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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