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J/MNRAS/444/757
  HII complexes optical and IR emissions (Khramtsova+, 2014)
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2014MNRAS.444..757K
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Post annotation 		img(gal)
1.J/MNRAS/444/757/table1(c)Summary of galaxies included in the work (9 rows)
2.J/MNRAS/444/757/table2(c)List of studied HII complexes in galaxies IC 1727 and NGC 7741 and results of spectroscopy of HII complexes (21 rows)
3.J/MNRAS/444/757/complexes(c)Results of aperture IR photometry of HII complexes (table4) and edrived parameters (table5) (110 rows)
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Simple ConstraintList Of Constraints
 
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)
   (ALL)Galaxy (char) (i) Galaxy name (meta.id;meta.main)
  (1)N   [6/21] Number of studied HII complexes (meta.number)
  (1)N2  (n) [10/11] Number of HII complexes in table2 (meta.number)
  (1)Dist Mpc [3.4/15.1] Adopted distance (pos.distance;pos.heliocentric)
  (1)r_Dist  Distance reference (Note 1)   (meta.ref;pos.frame)
  (1)MType (char) Morphological type (src.morph.type)
  (1)r_MType (char) Morphological type reference (Note 1)   (meta.note)
  (1)Simbad (char) ask the Simbad data-base about this object (meta.ref.url)
  (1+2)_RA deg (i) Right Ascension (J2000) from SIMBAD (not part of the original data) (pos.eq.ra;meta.main)
  (1+2)_DE deg (i) Declination (J2000) from SIMBAD (not part of the original data) (pos.eq.dec;meta.main)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)Complex (char) Designation of complex (meta.id;meta.main)
  (2)oRA arcsec Offset in right ascension (from the galaxy) (pos.eq.ra;arith.diff)
  (2)oDE arcsec Offset in declination (from the galaxy) (pos.eq.dec;arith.diff)
  (2)I(3728)   [2.2/5.2] Bright line intensity of [OII] λ3727+3729 normalized to Hβ (spect.line.intensity;arith.ratio)
  (2)e_I(3728)   [0.1/1.2] rms uncertainty on I(3728) (stat.error)
  (2)I(4959)   [0.1/1.5] Bright line intensity of [OIII] λ4959 normalized to Hβ (spect.line.intensity;em.line.OIII;arith.ratio)
  (2)e_I(4959)   [0.01/0.12] rms uncertainty on I([OIII])1 (stat.error)
  (2+3)I(5007)   [0.19/4.20] Bright line intensity of [OIII] λ5007 normalized to Hβ (spect.line.intensity;em.line.OIII;arith.ratio)
  (2+3)e_I(5007)   [0.01/0.11] rms uncertainty on I([OIII])2 (stat.error)
  (2)I(Ha)   [2.7/3.1] Bright line intensities of Hα normalized to Hβ (meta.note)
  (2)e_I(Ha)   [0.02/0.15] rms uncertainty on I(Ha) (stat.error)
  (2)I([NII])   [0.17/0.82] Bright line intensity of [NII]λ6548+6584 normalized to Hβ (spect.line.intensity;arith.ratio)
  (2)e_I([NII])   [0.02/0.22] rms uncertainty on I([NII]) (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)I([SII])   [0.42/1.14] Bright line intensity or [SII] λ6717+6731 normalized to Hβ (spect.line.intensity)
  (2)e_I([SII])   [0.03/0.37] rms uncertainty on I([SII]) (stat.error)
  (2)EWHb 0.1nm [4/130] Hβ equivalent width (spect.line.eqWidth;em.line.Hbeta)
  (2)e_EWHb 0.1nm [0.1/2.5] rms uncertainty on EWHb (stat.error)
  (2)E(B-V) mag [0.04/0.39] Redenning (phot.color.excess)
  (2)e_E(B-V) mag [0.01/0.19] rms uncertainty on E(B-V) (stat.error)
  (2+3)Ab(O) [-] [7.9/8.5] Abundance 12+log(O/H), estimated by the ONS method (Note G1)   (phys.abund)
  (2+3)e_Ab(O) [-] [0.03/0.13] rms uncertainty on Ab(O) (stat.error)
  (2)r/R25   [0.1/0.8] Radial distance from the centre of a galaxy normalized to a R25 (pos.distance)
  (3)RAJ2000 "h:m:s" (i) Rigth ascension (J2000) (pos.eq.ra;meta.main)
  (3)DEJ2000 "d:m:s" (i) Declination (J2000) (pos.eq.dec;meta.main)
  (3)Ap arcsec [4/14] Aperture radius (phys.angSize)
  (3)F3.6 mJy Spitzer/IRAC flux at 3.6um (phot.mag;em.IR.3-4um)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)e_F3.6 mJy rms uncertainty on F3.6um (stat.error)
  (3)F4.5 mJy Spitzer/IRAC flux at 4.5um (phot.mag;em.IR.4-8um)
  (3)e_F4.5 mJy rms uncertainty on F4.5um (stat.error)
  (3)F5.8 mJy Spitzer/IRAC flux at 5.8um (phot.flux.density;em.IR.4-8um)
  (3)e_F5.8 mJy rms uncertainty on F5.8um (stat.error)
  (3)F8.0 mJy Spitzer/IRAC flux at 8.0um (phot.flux.density;em.IR.8-15um)
  (3)e_F8.0 mJy rms uncertainty on F8.0um (stat.error)
  (3)F8.0e mJy PAH emission at 8.0um (Note 1)   (phot.flux.density;em.IR.8-15um)
  (3)e_F8.0e mJy rms uncertainty on F24e (stat.error)
  (3)F24 mJy Spitzer/MIPS flux at 24um (phot.flux.density;em.IR.15-30um)
  (3)e_F24 mJy rms uncertainty on F24um (stat.error)
  (3)F24e mJy PAH emission at 24um (phot.flux.density;em.IR.15-30um)
  (3)e_F24e mJy rms uncertainty on F24e (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)Age Myr (n) [0.1/8.6] Age (time.age)
  (3)e_Age Myr (n) [0.01/1.1] rms uncertainty on Age (stat.error;time.age)

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