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J/A+A/600/A20
  Lupus YSOs X-shooter spectroscopy (Alcala+, 2017)
img(gal)
    J/A+A/600/A20/table1(c)Observing log for the new sample (57 rows)
    J/A+A/600/A20/tablea23Confirmed YSOs of the total sample with spectral types, extinction, and physical parameters (table A2) and accretion properties (table A3) (81 rows)
    J/A+A/600/A20/tablee1Extinction-corrected fluxes and equivalent widths of Balmer lines for the new sample: Hα to Hε (46 rows)
    J/A+A/600/A20/tablee2Extinction-corrected fluxes and equivalent widths of Balmer lines: H8 to H11 (46 rows)
    J/A+A/600/A20/tablee3Extinction-corrected fluxes and equivalent widths of Balmer lines: H12 to H15 (46 rows)
    J/A+A/600/A20/tablee4Extinction-corrected fluxes and equivalent widths of Paschen lines: Paβ to Pa8 (46 rows)
    J/A+A/600/A20/tablee5Extinction-corrected fluxes and equivalent widths of Pa9, Pa10, and Brγ (46 rows)
    J/A+A/600/A20/tablee6Extinction-corrected fluxes and equivalent widths of helium lines (46 rows)
    J/A+A/600/A20/tablee7Extinction-corrected fluxes and equivalent widths of helium lines (46 rows)
    J/A+A/600/A20/tablee8Extinction-corrected fluxes and equivalent widths of CaII H and K and IRT lines (46 rows)
    J/A+A/600/A20/tablee9Extinction-corrected fluxes and equivalent widths of the NaI D lines (46 rows)

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       (c)  indicates tables which contain celestial coordinates 
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