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Table 1.

Some examples of low surface brightness (satellite) galaxies surrounding NGC 1042 explored in this work.

Name RA (2000) Dec (2000) mg mr μg(0) μr(0) Re, g Re, r Reference
(mag) (mag) (mag/″2) (mag/″2) (″) (″)
SDSS J024007.01–081344.4 02:40:07.0 −08:13:44.4 17.17 16.70 23.81 23.30 11.1 10.9 (1)
NGC 1052-DF1 02:40:04.6 −08:26:48.3 19.52 18.95 26.69 26.03 15.2 15.1 (2)
T20-12000 02:39:39.3 −08:13:42.3 19.23 18.47 24.40 23.85 6.9 8.9 (3)
LSB21 02:40:28.8 −08:14:36.5 19.98 19.56 26.12 25.72 10.9 11.2 (4)
LBT1 02:40:40.6 −08:23:08.9 22.70 22.06 27.11 26.41 4.2 4.9 (5)

Notes. The structural properties provided correspond to those found in this work. This table includes the name of the galaxies, their spatial location, their apparent magnitudes in the g and r bands, their central surface brightness, and their effective radii in arcsec. To the best of our knowledge the above galaxies were first found/discussed in the following references: (1) Abazajian et al. (2003), (2) Cohen et al. (2018), (3) Tanoglidis et al. (2021); object also known as SDSS J023939.36–081342.0, (4) Román et al. (in prep.); object also known as SDSS J024028.61–081436.7, (5) this work. The apparent magnitudes and surface brightness have been corrected by the following Galactic extinction: Ag = 0.095 and Ar = 0.065 mag. The quantities are given showing only the significant figures up to which the values can be regarded as reliable.

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