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VizieR

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J/ApJ/725/2232
  Deep NIR survey of the Pipe Nebula. II. (Roman-Zuniga+, 2010)
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img(gal)
1.J/ApJ/725/2232/table2(c)CLUMPFIND-2D identifications in high-resolution extinction maps of the Pipe Nebula (220 rows)
2.J/ApJ/725/2232/tablea1(c)Near-infrared observations of Pipe Nebula fields (197 rows)
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Query by Constraints constraints help applied on Columns (Output Order: + - )
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1)Reg (char) Region name (see Fig.2) (obs.field)
  (1)PID (char) Peak identification from RLA09 ([R/N]NNN) (Note 1)   (meta.id;stat.max)
  (1)m_PID (char) [a-h] close peaks (Note 2)   (meta.code.multip)
  (1)n_PID (char) [*] Note on PID (Note 3)   (meta.note)
  (1)Av mag Maximum extinction (Note 4)   (phys.absorption;stat.max)
  (1)Req pc [0.022/0.146] Equivalent radius of the peak (phys.size.radius;stat.max)
  (1)Mass Msun [0.054/4.812] Mass of the extinction peak region (phys.mass)
  (1)n 10+4cm-3 [0.41/4.687] Average density of the peak (phys.density)
  (1)_RA deg (n)(i) Positions from Rathborne et al. 2009, Cat. J/ApJ/699/742 (the close peaks having different m_PID numbers were assigned the same position) (right ascension part) (pos.eq.ra;meta.main)
  (1)_DE deg (n)(i) Positions from Rathborne et al. 2009, Cat. J/ApJ/699/742 (the close peaks having different m_PID numbers were assigned the same position) (declination part) (pos.eq.dec;meta.main)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)Inst (char) Instrument used for observations (SOFI-NTT, ISAAC-VLT, or OMEGA 2000-CAHA 3.5m) (instr.setup)
  (2)Field (char) Field identification (meta.id;obs.field)
  (2)Date "Y:M:D" (n)Date of observation (time.epoch)
  (2)RAJ2000 deg (i) Center right ascension (J2000) (pos.eq.ra;meta.main)
  (2)DEJ2000 deg (i) Center declination (J2000) (pos.eq.dec;meta.main)
  (2)F (char) Filter (J, H, or Ks) (meta.code;instr.filter)
  (2)See arcsec Estimated seeing based on the average FWHM of the stars detected in each field (instr.obsty.seeing)
  (2)Pmag mag [16.75/24.5] Peak of the observed magnitude distribution (phys.luminosity.fun)
  (2)Map (char) Corresponding figure number in large-scale maps (figures 3-7) and atlas (meta.bib.fig)

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(n) indicates a possible blank or NULL column(i)indexed column
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