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Table 5.

Log of observatories and instrumentations used to obtain our spectroscopic observations.

Observatory Telescope (†) Spectrograph Camera Res. (‡) Observer Reference Label (*)
CrAO (a) 260 slit SPEM SPEC-10 1000 Tarasova 1 (iv)
Asiago (b) 182 echelle EEV CCD47-10 21000 Munari 2 (iii)
SPO (c) 130 echelle Andor iKon-L 936 34000 Komžík, Sekeráš 3,4,5 (i)
Asiago 122 Boller&Chivens Andor iDus DU440A 1000 Munari 6,7 (iii)
SLO,G1 60 echelle ATIK 460EX 11000 Shugarov, Kundra 4 (ii)
Durtal 51 echelle KAF-3200ME 11000 Charbonnel 8,9 (x)
la Tourbière 40 echelle ATIK 460EX 11000 Garde 1,9 (viii)
DCO (d) 35 LISA ATIK 460EX 1000 Sims 1,9 (xiii)
Mill Ridge 31 echelle ASI 1600 mm CMOS 12000 Lester 1,9 (ix)
AOKS 28 LISA ATIK 460EX 680 Dubovský 10 (v)
CTO (e) 25 UVEX SWO CMOS 1200 Buil 9,11 (vi)
OCT-FR (f) 20 slit Alpy 600 ATIK 314L+ 500 Boussin 9 (vii)
L’Aquila (g) 20 slit Alpy 600 SBIG ST-8300M 1600 Sollecchia 9 (xi)
Balzaretto (h) 20 slit Alpy 600 SXVF-M7 530 Franco 9 (xii)

Notes.

(a)

Crimean Astrophysical Observatory,

(b)

Asiago Astrophysical Observatory,

(c)

Skalnaté Pleso Observatory,

(d)

private Desert Celestial Observatory in Gilbert Arizona,

(e)

Castanet Tolosan Observatory,

(f)

Observatory de l’Eridan,

(g)

private station in L’Aquila,

(h)

A81 Balzaretto Observatory.

(†)Diameter of the primary mirror in cm,

(‡)average resolution,

(*)label of the observatory in Tables 6 and 7.

References. 1 – Skopal et al. (2017), 2 – Munari & Lattanzi (1992), 3 – Baudrand & Bohm (1992), 4 – Pribulla et al. (2015), 5 – Döhring et al. (2019), 6 – Ciroi et al. (2014), 7 – Siviero (2014), 8 – Skopal et al. (2014), 9 – Teyssier (2019), 10 – Kudzej & Dubovský (2014), 11 – http://www.astrosurf.com/buil/UVEX_project_us/.

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