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Table 2.

Spectroscopic observations in the 2009−2019 period.

Date Instrumentation (a) Wavelength range (Å) Res. power Main emission lines Ref
2012-Mar-16 SDSS-BOSS 3600−10 400 2000 Lyα, C IV, C III], Mg II 1
2012-Mar-29 SDSS-BOSS 3600−10 400 2000 Lyα, C IV, C III], Mg II 1
2013-Apr-13 GTC-OSIRIS-R500R 4850−9250 400 C IV, C III], Mg II 2
2014-Mar-27 GTC-OSIRIS-R500R 4850−9250 400 C IV, C III], Mg II 3
2014-May-20 GTC-OSIRIS-R500B 3600−7200 320 Lyα, C IV, C III] 3
2016-Feb-18 HST-WFC3-UVIS 2000−6000 70 Lyα, C IV 4
2017-Apr-06 VLT-X-shooter 3050−20 700 6700, 8900, 5600 Lyα, C IV, C III], Mg II, Hβ, [O III] 5
2018-Feb-23 VLT-X-shooter 3050−20 700 6700, 8900, 5600 Lyα, C IV, C III], Mg II, Hβ, [O III] 5
2019-Mar-15 TNG-NICS-HK 13 500−24 700 500 Hα 6
2019-Jun-10 NOT-ALFOSC-G18 3450−5350 1000 Lyα, C IV 6

Notes.

(a)

SDSS-BOSS ≡ Baryon Oscillation Spectroscopic Survey (BOSS) spectrograph for the SDSS, GTC-OSIRIS-R500x ≡ OSIRIS instrument (R500x grism) on the 10.4 m Gran Telescopio Canarias (GTC), HST-WFC3-UVIS ≡ UVIS channel of the WFC3 instrument on the Hubble Space Telescope (HST), VLT-X-shooter ≡ X-shooter spectrograph (UVB, VIS, and NIR arms) on the 8.2 m Very Large Telescope (VLT), TNG-NICS-HK ≡ NICS instrument (HK grism) on the 3.6 m Telescopio Nazionale Galileo (TNG), and NOT-ALFOSC-G18 ≡ ALFOSC instrument (grism #18) on the 2.5 m Nordic Optical Telescope (NOT).

References. (1) Dawson et al. (2013); (2) Paper I; (3) Paper II; (4) Lusso et al. (2018); (5) VLT-X-shooter programme 099.A-0018 (PI: M. Fumagalli); (6) This paper.

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