Unveiling the environment and faint features of the isolated galaxy CIG 96 with deep optical and HI observations

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Volume 619 (November 2018)

A&A, 619 (2018) A163

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Table 3.

Data of the optical observations.

Telescope (Instrument)	Filter	Binning	Spatial scale^a (″ pixel⁻¹)	Total exp. time^b (# × time)	Field of view^c (′×′/kpc × kpc)	SB limit (mag arcsec⁻²)	Seeing (″)
CAHA2.2m	Cousins R	2 × 2	1.04	3h 56m	12 × 12	27.5	1.59
(CAFOS)				(71 × 200 s)	71 × 71

CAHA1.23m	B, G, R	1 × 1	1.04	3h 38m	15 × 16	−	1.56
(DLR-MKIII)	Photographic^d			(30_B, 37_G, 42_R × 120 s)^e	88 × 94

VST	SDSS r	2 × 2	0.21	5h 10m	60 × 60	28.7	1.10
(OmegaCAM)				(122 × 154 s)	350 × 350

Notes.

^(a)

Spatial scale according to the binning used.

^(b)

Total number of exposures × exposure time of each exposure.

^(c)

The top value of each telescope is the field of view in square arcminutes; the bottom value is the field of view according to the distance to the galaxy (see Table 1).

^(d)

CAHA1.23m images in photographic B and R filters were converted to SDSS g and r, respectively (see Sect. 2.4.2).

^(e)

The subindex indicates the filter of each corresponding number of exposures. Regardless of the filter, each one has an exposure time of 120 s.

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