Table 1: Protostellar jets with X-ray data and/or NIR spectra.
Jet flow He I 1.0830 $\mu $m X-rays Reference Comment
HH 158 $\times$ $\times$ 1, 2 [Fe II]
HH 154 $\times$ $\times$ 3, 4, 5 [Fe II]
HH 210   $\times$ 6  
HH 1G $-\times$ $-\times$ 7, 8 H2 + [Fe II]
HH 2H   $\times$ 8  
TKH 8   $\times$ 9  
HH 43 $-\times$   10 H2
HH 24A $-\times$   11 H2 + [Fe II]
HH 25 $-\times$   11 H2
HH 26 $-\times$   11 H2
HH 72 $-\times$   11 H2
Vel IRS17 $-\times$   12 H2
HH 320 $-\times$   11 H2
HH 321 $-\times$   11 H2
HH 80   $\times$ 13  
HH 81   $\times$ 13  
Ser SMM1 $-\times$ $-\times$ 14, 15 H2
HH 99-B0 $\times$   16 H2 + [Fe II]
Notes to the table: $\times =$ detected, $-\times$ means observed but not detected. H2 indicates the presence of ro-vibrationally excited H2 lines; [Fe II] the presence of [Fe II] lines; H2 + [Fe II] the presence of both species along the same line of sight/inside spectrograph slit. When possible, HH-nomenclature follows that of Reipurth (1999).
References: (1) Takami et al. (2002); (2) Güdel et al. (2005); (3) Itoh et al. (2000); (4) Liseau et al. (2005); (5) Favata et al. (2002); (6) Grosso et al. (2006); (7) Nisini et al. (2005); (8) Pravdo et al. (2001); (9) Tsujimoto et al. (2004); (10) Giannini et al. (2002); (11) Giannini et al. (2004); (12) Giannini et al. (2005); (13) Pravdo et al. (2004); (14) Liseau (unpublished); (15) Preibisch (2003); (16) McCoey et al. (2004).

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