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Table 2

Equivalent width (negative for emission, positive for absorption) of the main lines observed in the spectra obtained with Magellan/MIKE and Keck/LRIS in its low- and high-resolution modes (the three different setups are separated by a double line).

Object SpT Hβ [OI] [OI] [OI] [NII] [NII] HeI [SII] [SII]
4861 5577 6300 6364 6548 6581 6678 6717 6731
EW(Å) eEW EW(Å) eEW EW(Å) eEW EW(Å) eEW EW(Å) eEW EW(Å) eEW EW(Å) eEW EW(Å) eEW EW(Å) eEW

LOri050 M4.0 –9.41  ±  1.64 –0.53  ±  0.04 –0.58  ±  0.03 –0.44  ±  0.07
LOri055 M4.0 –5.11  ±  0.30
LOri056 M4.5 –5.16  ±  0.78
LOri060 M4.0 –4.13  ±  0.47 –1.14  ±  0.42 0.91  ±  0.10
LOri063 M4.0 0.73  ±  0.05 –2.51  ±  0.39 –0.93  ±  0.22 –0.78  ±  0.07
LOri068 M4.75 –5.49  ±  0.62
LOri075 M5.25 –5.47  ±  1.53 –1.76  ±  0.50

LOri098 M5.0 –2.24  ±  0.58
LOri107 M6.0 –0.68  ±  0.13
LOri114 M6.0 –2.39  ±  0.86
LOri115 M5.0 –0.95  ±  0.03
LOri139 M5.75 –2.76  ±  0.28 –0.88  ±  0.18 –1.13  ±  0.30
LOri140 M7.0 –11.82  ±  3.64 –4.24  ±  0.17
LOri155 M8.0 –4.28  ±  0.82 –4.42  ±  0.55 –2.81  ±  0.64

LOri068 M4.75 –1.42  ±  0.24 –0.76  ±  0.38 –0.41  ±  0.18
LOri071 M5.0 –0.49  ±  0.11 –1.13  ±  0.59 –0.07  ±  0.01
LOri077 M5.0 –0.72  ±  0.25 –1.14  ±  0.52
LOri089 M5.0 –0.42  ±  0.11 –0.82  ±  0.38
LOri091 M4.75 –0.11  ±  0.01 –0.95  ±  0.31 –0.95  ±  0.69 –0.34  ±  0.10
LOri094 M5.5 –1.87  ±  0.39 –1.21  ±  0.82
LOri099 M5.5 –0.58  ±  0.12
LOri106 M5.5 –0.58  ±  0.19 –1.01  ±  0.25 –0.19  ±  0.02 –0.26  ±  0.04
LOri109 M5.75 –1.14  ±  0.22 –0.15  ±  0.04
LOri113 M5.5 –0.17  ±  0.05 –1.10  ±  0.14 –1.73  ±  0.42
LOri119 M5.5 –4.16  ±  1.03 –0.58  ±  0.19 –0.25  ±  0.08
LOri129 M6.0 –0.68  ±  0.15

Notes. We only show objects where at least one of the forbidden lines, and/or Hβ, and/or HeI have been measured. The measurements of Hα and the Ca II triplet are shown in Table 6 (with the opposite convention: positive for emission). The symbol “–” indicates that the line has not been detected while a white space means that the line falls outside of the wavelength coverage of the spectra. Spectral types (SpT) from Paper I (averaged when more than one spectral type was given).

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