VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

  
J/A+A/706/A136
  Rest-frame NIR substructures detections (Mercier+, 2026)
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img(gal)
1.J/A+A/706/A136/sample*Catalogue containing the selected sample of galaxies with M*>109M{sun} at 1<z<4 (Note) (48486 rows)

 
Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Detec (char) indicates substructures in detec.dat file (meta.ref.url)
  IDSE++  (i) Unique identifier used to match the galaxies to the COSMOS2025 catalogue of Shuntov et al. (2025A&A...704A.339S, Cat. J/A+A/704/A339, arXiv:2506.03243) (meta.id;meta.main)
  pSint=1  Probability that galaxies host exactly one substructure of any size detected with the intrinsic approach (stat.fit.goodness)
  pCint=1  Probability that galaxies host exactly one clump detected with the intrinsic approach (stat.fit.goodness)
  pMint=1  Probability that galaxies host exactly one moderately large substructure detected with the intrinsic approach (stat.fit.goodness)
  pLint=1  Probability that galaxies host exactly one extended substructure detected with the intrinsic approach (stat.fit.goodness)
  pSopt=1  Probability that galaxies host exactly one substructure of any size detected with the optimal approach (stat.fit.goodness)
  pCopt=1  Probability that galaxies host exactly one clump detected with the optimal approach (stat.fit.goodness)
  pMopt=1  Probability that galaxies host exactly one moderately large substructure detected with the optimal approach (stat.fit.goodness)
  pLopt=1  Probability that galaxies host exactly one extended substructure detected with the optimal approach (stat.fit.goodness)

ALL cols
    
 (i)indexed column
  pSint>=1  Probability that galaxies host one or more substructures of any size detected with the intrinsic approach (stat.fit.goodness)
  pCint>=1  Probability that galaxies host one or more clumps detected with the intrinsic approach (stat.fit.goodness)
  pMint>=1  Probability that galaxies host one or more moderately large substructures detected with the intrinsic approach (stat.fit.goodness)
  pLint>=1  Probability that galaxies host one or more extended substructures detected with the intrinsic approach (stat.fit.goodness)
  pSopt>=1  Probability that galaxies host one or more substructures of any size detected with the optimal approach (stat.fit.goodness)
  pCopt>=1  Probability that galaxies host one or more clumps detected with the optimal approach (stat.fit.goodness)
  pMopt>=1  Probability that galaxies host one or more moderately large substructures detected with the optimal approach (stat.fit.goodness)
  pLopt>=1  Probability that galaxies host one or more extended substructures detected with the optimal approach (stat.fit.goodness)
  pSint>=2  Probability that galaxies host two or more substructures of any size detected with the intrinsic approach (stat.fit.goodness)
  pCint>=2  Probability that galaxies host two or more clumps detected with the intrinsic approach (stat.fit.goodness)
  pMint>=2  Probability that galaxies host two or more moderately large substructures detected with the intrinsic approach (stat.fit.goodness)
  pLint>=2  Probability that galaxies host two or more extended substructures detected with the intrinsic approach (stat.fit.goodness)
  pSopt>=2  Probability that galaxies host two or more substructures of any size detected with the optimal approach (stat.fit.goodness)
  pCopt>=2  Probability that galaxies host two or more clumps detected with the optimal approach (stat.fit.goodness)
  pMopt>=2  Probability that galaxies host two or more moderately large substructures detected with the optimal approach (stat.fit.goodness)
  pLopt>=2  Probability that galaxies host two or more extended substructures detected with the optimal approach (stat.fit.goodness)

ALL cols
    
 (i)indexed column
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