Revisiting dual AGN candidates with spatially resolved LBT spectroscopy - The impact of spillover light contamination

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Volume 639 (July 2020)

A&A, 639 (2020) A117

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Table 1.

Sample and observations.

Name ^(a)	z	Δd^(b)	Instrument	Date	t_exp	Airmass	Seeing ^(c)
SDSS J031722.06+004801.8	0.15722	28	MODS1	2016-02-05	2 × 750 s	1.5	20
SDSS J080523.29+281815.8	0.12844	23	MODS1	2016-02-04	2 × 450 s	1.1	13
SDSS J085837.68+182223.4	0.05894	26	MODS1	2016-02-04	2 × 300 s	1.1	11
SDSS J094741.58+633939.2	0.13973	22	MODS1	2016-02-05	2 × 300 s	1.2	12
SDSS J111519.98+542316.7	0.07043	83	MODS1	2016-02-04	2 × 300 s	1.1	11
SDSS J160933.41+283058.4	0.16960	27	MODS2	2016-05-26	3 × 900 s	1.2	12
SDSS J164658.48+241134.1	0.08728	21	MODS2	2016-05-26	2 × 750 s	1.2	11

^(a)

Notes.Identifier from the Sloan Digital Sky Survey of one of the nuclei.

^(b)

Angular distance between the two nuclei as inferred from the optical continuum light.

^(c)

Inferred FWHM of the seeing during the observations at 6000 Å.

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