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Table 4

Data for elements not included in the Kurucz line-list (gfall08oct17.dat).

Ion NUV NVIS References
    
Ga III 3 2 15, 2(28)
Ga IV 69 3
Ga V 37 3
Ge III 1 1(25,18)
Ge IV 7 6 23, 2(28)
Ge V 24 3
As III 1(26,19,17)
As IV 6 2(27), 1(25)
As V 2 1(19)
Se IV* 3 1(22)
Se V* 4 3
Kr IV* 42 6 3
Kr V* 3
Sr IV* 109 1 3

Ion NUV NVIS References
       

Sr V* 23 3
Y III* 1 2 10, 16
Zr IV 11 8 3
Zr V 3
Mo IV* 92 29,3
Mo V* 69 3
Mo VI* 5 3
In III* 5 4
Sn III 13
Sn IV 7 4, 12
Sb III* 1(17)
Sb IV* 1 1(20)
Sb V* 2 4
Te III* 14

Ion NUV NVIS References
       

Te V* 1 1(30)
Te VI* 2 3
Xe IV* 5 3
Xe V* 4 3
Ba V* 2 3
Tl III* 5
Pb III 2 7, 1(24)
Pb IV 17 9 11, 5, 8, 1(24)
Pb V 36 9
Bi III* 1(23)
Bi IV* 1(21)
Bi V* 1 5
Th IV* 2 6

Notes. The number of lines with predicted equivalent width greater than 5 mÅ in the final model of HZ 44 (upper limits marked with *) and in spectral ranges where observations are available for HZ 44 are listed (UV: 916–1980 Å, VIS: 3022–7580 Å). For references from compilations, the compilation is listed first and the individual references in parenthesis.

References. (1) Morton (2000), (2) ALL, van Hoof (2017), (3) TOSS, Rauch et al. (2015), (4) Safronova et al. (2003), (5) Safronova & Johnson (2004), (6) Safronova & Safronova (2013), (7) Alonso-Medina et al. (2009), (8) Alonso-Medina et al. (2011), (9) Colón et al. (2014), (10) Naslim et al. (2011), (11) Naslim et al. (2013), (12) Biswas et al. (2018), (13) Haris & Tauheed (2012), (14) Zhang et al. (2013), (15) Nielsen et al. (2005), (16) Redfors (1991), (17) Andersen & Lindgard (1977), (18) Andersen et al. (1979), (19) Pinnington et al. (1981), (20) Pinnington et al. (1985a), (21) Pinnington et al. (1988), (22) Bahr et al. (1982), (23) Migdałek (1983), (24) Ansbacher et al. (1988), (25) Curtis (1992), (26) Marcinek & Migdalek (1993), (27) Churilov &Joshi (1996), (28) O’Reilly & Dunne (1998), (29) Kurucz (2018), (30) Pinnington et al. (1985b).

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