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Table 1

Details of the observations of GRB hosts in the sample.

GRB host Date Instrument Exp. time Slit width* Dispersion Wavelength range Seeing Airmass Reference
(mag) (s) () (Å/pixel) (Å) ()

050416A 0.026 2011-01-19 VLT/X-Shooter 4 × 900/4 × 900/12 × 300 1.0/0.9/0.9 0.4/0.4/1.0 3000–25 000 0.7 1.5 (1)
050525A 0.083 2012-09-18 VLT/X-Shooter 4 × 630/4 × 664/4 × 695 1.0/0.9/0.9JH 0.4/0.4/1.0 3000–20000 1.5 1.6 (1)
060614 0.019 2006-07-23 VLT/FORS2 1 × 1500 1.0 3.3 3000–9600 1.2 1.2 (2)
2007-04-26 VLT/FORS1 2 × 1200 1.3 1.5 3600–6000 0.8 1.5 (3)
060912A 0.046 2012-09-21 VLT/X-Shooter 2 × 900/2 × 934/2 × 965 1.3/1.2/1.2 0.4/0.4/1.0 3000–25 000 0.7 1.5 (1)
061021 0.051 2013-03-21 VLT/X-Shooter 12 × 940/12 × 900/36 × 320 1.0/0.9/0.9JH 0.4/0.4/1.0 3000–20000 0.9 1.1 (1)
071112C 0.105 2007-11-13 VLT/FORS2 2 × 1800 1.0 3.3 3000–9500 1.0 1.7 (4)
080319B 0.010 2014-02-26 GTC/OSIRIS 4 × 825 1.23 2.6 5100–10 000 0.8 1.1 (3)
2014-02-28 GTC/OSIRIS 4 × 825 1.23 2.6 5100–10 000 1.2 1.1 (3)
080430 0.011 2014-01-07 GTC/OSIRIS 8 × 825 1.23 2.6 5100–10 000 1.1 1.1 (3)
080916A 0.017 2008-09-17 VLT/FORS1 6 × 600 1.0 3.3 3000–9500 0.8 1.2 (4)
081007 0.014 2015-05-16 VLT/X-Shooter 4 × 700/4 × 700/12 × 250 1.3/1.2/1.2 0.4/0.4/1.0 3000–25000 1.0-2.1 1.2 (3)
2015-06-20 VLT/X-Shooter 8 × 700/8 × 700/24 × 250 1.3/1.2/1.2 0.4/0.4/1.0 3000–25000 0.8-1.0 1.1 (3)
2008-11-03 VLT/FORS2 3 × 2700 1.0 3.2 5700–10 000 0.5 1.1 (5)
090424 0.022 2009-05-22 VLT/FORS2 3 × 3600 1.0 3.2 6000–10 200 0.7 1.4 (5)
2013-04-08 GTC/OSIRIS 3 × 800 1.23 2.1 3630–7500 0.9 1.1 (5)
091018 0.026 2009-10-18 VLT/X-Shooter 4 × 600/4 × 600/4 × 600 1.0/0.9/0.9 0.4/0.4/1.0 3000–25 000 0.9 2.0 (6)
091127 0.035 2010-02-12 VLT/X-Shooter 4 × 1500/4 × 1500/4 × 750 1.0/0.9/0.9 0.4/0.4/1.0 3000–25 000 1.0 1.1 (7)
100621A 0.027 2012-10-16 VLT/X-Shooter 2 × 1200/2 × 1200/8 × 300 1.0/0.9/0.9JH 0.4/0.4/1.0 3000–20000 0.9 1.3 (1)

Notes. For each GRB we report Galactic reddening in its line of sight and the information regarding the spectroscopic observation of its host galaxy: date of observation, telescope and instrument, instrumental setup (exposure time, slit widths, dispersion, wavelength range of the obtained spectrum), observing conditions (seeing and airmass), and the reference of the first published work presenting the spectrum.

(*)

0.9JH stands for the X-Shooter near-infrared slits with a special K-blocking filter (Vernet et al. 2011).

(†)

Spectra are dominated by afterglow emission.

Reference. (1) Krühler et al. (2015); (2) Della Valle et al. (2006); (3) This study; (4) Fynbo et al. (2009); (5) Jin et al. (2013); (6) Wiersema et al. (2012); (7) Vergani et al. (2011).

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