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Table 10

HRS galaxies with data in the literature: equivalent widths (in Å).

K92 This
work
HRS [Oii] Hβ [Oiii] [Oiii] [Nii] Hα [Nii] [Sii] [Sii] run [Oii] Hβ [Oiii] [Oiii] [Nii] Hα [Nii] [Sii] [Sii]
λ3727 λ4861 λ4959 λ5007 λ6548 λ6563 λ6584 λ6717 λ6731 λ3727 λ4861 λ4959 λ5007 λ6548 λ6563 λ6584 λ6717 λ6731
4 10 5 2.3 7 0 34.8 0 – 5 – – – – – – – – – –
20 44 16 7.7 23 4.5 77.0 13.3 – 32 – – – – – – – – – –
275 35 11 4.7 14 3.2 46.1 9.6 – 17 – – – – – – – – – –
295 9 6 0.3 1 2.8 22.7 8.3 – 6 – – – – – – – – – –
J00 This
work
HRS [Oii] Hβ [Oiii] [Oiii] [Nii] Hα [Nii] [Sii] [Sii] run [Oii] Hβ [Oiii] [Oiii] [Nii] Hα [Nii] [Sii] [Sii]
λ3727 λ4861 λ4959 λ5007 λ6548 λ6563 λ6584 λ6717 λ6731 λ3727 λ4861 λ4959 λ5007 λ6548 λ6563 λ6584 λ6717 λ6731
29 23.2 5.9 2.4 4.6 1.7 26.3 5.4 5.7 4.2 1 16.7 6.2 1.6 4.8 1.8 27.6 6.3 5.7 4.7
35 3.1 – – – –1 1.8 0.6 0.3 0.3 – – – – – – – – – –
64 14.2 2.5 1.2 1.8 0.7 14.2 2.6 3.7 2.6 – – – – – – – – – –
67 44.9 9.9 5.8 13.8 1.4 40.9 5.2 9 5.8 1 53.1 9.7 5 16.9 2.0 47.4 6.8 9.2 6.5
271 18.7 3.5 2.4 2.9 0.8 18.1 2.8 5.1 3.7 – – – – – – – – – –
MK06 This
work
HRS [Oii] Hβ [Oiii] [Oiii] [Nii] Hα [Nii] [Sii] [Sii] run [Oii] Hβ [Oiii] [Oiii] [Nii] Hα [Nii] [Sii] [Sii]
λ3727 λ4861 λ4959 λ5007 λ6548 λ6563 λ6584 λ6717 λ6731 λ3727 λ4861 λ4959 λ5007 λ6548 λ6563 λ6584 λ6717 λ6731
20 39.5 12.65 6.24 18.71 4.82 66.70 14.47 13.72 9.22 – – – – – – – – – –
27 24.4 10.12 2.14 6.42 5.33 50.40 15.99 10.08 7.00 – – – – – – – – – –
36 13.5 5.68 0.93 2.79 5.92 30.30 17.76 5.82 4.72 – – – – – – – – – –
60 7.5 2.56 0.55 1.648 1.56 10.45 4.68 2.26 1.72 1 7.93 1.20 – 1.65 1.58 11.92 5.77 2.28 1.92
73 6.3 2.72 0.05 0.14 1.17 9.16 3.52 1.61 0.90 – – – – – – – – – –
74 13.42 6.40 1.41 4.24 3.84 30.60 11.53 5.90 4.20 1 13.43 6.17 2.62 4.46 4.09 37.27 13.34 6.01 4.55
76 26.4 7.31 4.94 14.81 0.96 30.70 2.87 5.85 3.23 1 35.41 7.86 6.17 19.91 1.02 39.99 4.50 6.43 4.84
85 10.2 3.28 0.55 1.66 2.13 15.18 6.39 3.26 2.18 – – – – – – – – – –
102 10.21 6.06 0.63 1.88 3.81 33.50 11.44 4.8 3.14 2 – 4.86 – 1.18 3.09 31.49 10.20 4.22 3.03
114 9.46 6.26 0.81 2.43 4.33 31.30 13 4.76 3.66 2 7.81 5.36 3.31 1.69 3.76 31.40 12.56 4.83 3.36
122 3 3.09 0.47 1.42 2.34 19.76 7.01 1.84 0.98 1 – 3.05 – – 2.42 20.00 7.21 1.79 1.25
217 3.1 0.30 0.37 1.12 0.95 3.71 2.86 1.42 0.81 2 – – – – 0.41 4.81 2.75 0.74 0.84
246 13.6 3.65 0.96 2.88 1.92 15.28 5.75 3.69 2.78 2 – 2.43 0.62 1.03 1.69 15.19 5.74 2.79 1.85
250 17.4 5.36 1.13 3.38 3.27 25.80 9.82 5.38 4.34 – – – – – – – – – –
262 39.5 11.20 4.34 13.03 3.94 54.10 11.82 11.58 7.74 1 42.77 11.17 4.51 12.65 3.65 59.40 11.77 12.19 7.93
290 13.4 4.17 0.99 2.97 2.19 18.45 6.57 4.94 3.26 1 11.96 3.05 2.07 2.62 1.79 22.27 6.70 4.47 3.26
M10 This
work
HRS [Oii] Hβ [Oiii] [Oiii] [Nii] Hα [Nii] [Sii] [Sii] run [Oii] Hβ [Oiii] [Oiii] [Nii] Hα [Nii] [Sii] [Sii]
λ3727 λ4861 λ4959 λ5007 λ6548 λ6563 λ6584 λ6717 λ6731 λ3727 λ4861 λ4959 λ5007 λ6548 λ6563 λ6584 λ6717 λ6731
102 5.00 5.14 0.39 1.16 2.97 30.39 8.92 3.56 2.57 2 – 4.86 – 1.18 3.09 31.49 10.2 4.22 3.03
122 4.98 3.22 0.27 0.81 2.24 17.09 6.73 2.36 1.73 1 – 3.05 – – 2.42 20.00 7.21 1.79 1.25
170 7.10 0.46 0.37 1.12 0.54 2.09 1.63 0.94 0.66 2 – – – – 0.70 3.65 1.70 0.76 0.77
205 13.60 3.30 0.42 1.27 3.04 20.61 9.12 5.07 3.81 1 – 3.08 – 2.65 3.06 26.22 9.78 5.31 4.19
211 – 0.62 – – – – – – – 2 – – – – – – – – –
217 3.45 0.43 0.31 0.94 1.36 4.18 4.07 1.28 0.94 2 – – – – 0.41 4.81 2.75 0.74 0.84
220 9.57 0.78 0.53 1.60 1.33 2.96 3.99 2.01 1.14 2 – – – – 1.01 4.88 3.52 1.90 1.14
263 – 1.00 – – 0.50 – 1.50 – – – – – – – – – – – –

Notes. 

(a)

References are K92 – Kennicutt (1992b); J00 – Jansen et al. (2000); MK06 - Moustakas & Kennicutt (2006); M10 – Moustakas et al. (2010).

(b)

for consistency with our work, the original data of Kennicutt (1992b) are corrected for the underlying Balmer absorption in Hβ (5 Å) and Hα (2.8 Å). The [Oiii]λ4959 and the [Nii]λ6548 equivalent widths are inferred from the [Oiii]λ5007 and the [Nii]λ6584 measurements assuming a standard ratio [Oiii]λ5007/[Oiii]λ4959 = 3 and [Nii]λ6584/[Nii]λ6548 = 3 (Osterbrock & Ferland 2005). The [Sii]λ6731 equivalent width includes the emission of both [Sii]λ6717 and [Sii]λ6731 lines.

(c)

the original data of Jansen et al. (2000) are corrected only for the underlying Balmer absorption in Hα (2.8 Å), but not for that in Hβ given that the spectral resolution of these data, comparable to our, allows the direct measurement of the underlying absorption.

(d)

the [Oiii]λ4959 and the [Nii]λ6548 equivalent widths of Moustakas et al. (2010) and Moustakas & Kennicutt (2006) are inferred from the [Oiii]λ5007 and the [Nii]λ6584 measurements assuming a standard ratio [Oiii]λ5007/[Oiii]λ4959 = 3 and [Nii]λ6584/[Nii]λ6548 = 3 (Osterbrock & Ferland 2005).

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