VizieR

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

VizieR

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J/MNRAS/482/154
  GHASP. spiral galaxies dark matter distribution (Korsaga+, 2019)
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2019MNRAS.482..154K
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Post annotation 		img(gal)
1.J/MNRAS/482/154/tablea1(c)Global properties (124 rows)
2.J/MNRAS/482/154/tablea2Parameters of mass models using the BFM and fixed M/L techniques with the pseudo-isothermal (ISO) model (100 rows)
3.J/MNRAS/482/154/tablea3Parameters of mass models using the MDM technique with the pseudo-isothermal (ISO) model (100 rows)
4.J/MNRAS/482/154/tablea4Parameters of mass models using the BFM and fixed M/L techniques with the NFW model (100 rows)

Simple ConstraintList Of Constraints
 
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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)param (char) indicates parameters of mass models in tables A2-A4 (meta.ref.url)
   (ALL)ID (char) (i) Name of the galaxy in the UGC catalogue (UGC NNNNN) (meta.id;meta.main)
  (1)f_B-V (char) [*] * for galaxies with no B-V colour available in the RC3 catalogue, the value has been computed (Note 1)   (meta.code)
  (1)Type (char) Morphological type taken from the RC3 catalogue (Third Reference Cat. of Bright Galaxies (RC3) de Vaucouleurs et al. 1991rc3..book.....D, Cat. VII/155) (Note 2)   (src.morph.type)
  (1)BMAG mag Absolute B magnitude from Epinat et al. (2008MNRAS.388..500E, Cat. J/MNRAS/388/500) (phys.magAbs)
  (1)B-V mag (B-V) colours corrected for galactic and internal extinction from RC3 catalogue when available (phot.color;em.opt.B;em.opt.V)
  (1)mu0obs mag/arcsec2Central surface brightness from the observed data (phot.mag.sb)
  (1)R25/h  Isophotal radius at the limiting surface brightness of 25mag/arcsec2 normalized by the disc scale length (phys.angSize;src)
  (1)Rlast/h  The last radius of the RC normalized by the disc scale length (src.morph.scLength;arith.ratio)
  (1)mu0 mag/arcsec2Central surface brightness of the disc (phot.mag.sb)

ALL cols		    
 (i)indexed column
  (1)h kpc Disc scale length of the disc component (src.morph.scLength;phys.size)
  (1)LD 10+8Lsun Luminosity of the disc calculated at the isophotal radius (phys.luminosity)
  (1)mue mag/arcsec2(n) Surface brightness of the bulge at the effective radius (phot.mag.sb)
  (1)re kpc (n) Effective radius of the bulge (phys.size.radius)
  (1)n  (n) Sersic index of the bulge (stat.fit.param)
  (1)LB 10+8Lsun (n) Luminosity of the bulge derived at the isophotal radius (phys.luminosity;em.opt.B)
  (1)f_ID   [1/3] Classification flag of the inner galaxy rotation curves (RCs) (Note 3)   (meta.code)
  (1)Simbad (char) ask the Simbad data-base about this object (meta.ref.url)
  (1)_RA deg (i) Right Ascension (J2000) from SIMBAD (not part of the original data) (pos.eq.ra;meta.main)
  (1)_DE deg (i) Declination (J2000) from SIMBAD (not part of the original data) (pos.eq.dec;meta.main)
  (2)f_ID (char) [*] Flag on ID * : galaxies for which the presence of dark matter is not necessary (meta.code)
  (2)M/LdBFM Msun/LsunM/L of the disc from the best-fitting model (BFM) for pseudo-isothermal (ISO) core model (Note 1)   (phys.composition.massLightRatio)
  (2)E_M/LdBFM Msun/LsunUpper error on M/LDBFM (Note 1)   (stat.error;stat.max)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)e_M/LdBFM Msun/LsunLower error on M/LDBFM (Note 1)   (stat.error)
  (2)M/LbBFM Msun/Lsun(n) M/L of the bulge from the best-fitting model (BFM) for pseudo-isothermal (ISO) core model (Note 1)   (phys.composition.massLightRatio)
  (2)E_M/LbBFM Msun/Lsun(n) Upper error on M/LBBFM (Note 1)   (stat.error;stat.max)
  (2)e_M/LbBFM Msun/Lsun(n) Lower error on M/LBBFM (Note 1)   (stat.error)
  (2)l_r0BFM (char) Lower limit flag on r0BFM (Note 1)   (meta.code.error)
  (2)r0BFM kpc Core radius of the dark matter halo from the best-fitting model (BFM) for pseudo-isothermal (ISO) core model (Note 1)   (phys.size.radius)
  (2)E_r0BFM kpc (n) Upper error on r0BFM (Note 1)   (stat.error;stat.max)
  (2)e_r0BFM kpc (n) Lower error on r0BFM (Note 1)   (stat.error)
  (2)rho0BFM 10-3Msun/pc3Central density of the dark matter halo from the best-fitting model (BFM) for pseudo-isothermal (ISO) core model (Note 1)   (phys.density)
  (2)E_rho0BFM 10-3Msun/pc3Upper error on rho0BFM (Note 1)   (stat.error;stat.max)
  (2)e_rho0BFM 10-3Msun/pc3Lower error on rho0BFM (Note 1)   (stat.error)
  (2)Chi2BFM  Reduced chi-squared from the best-fitting model (BFM) for pseudo-isothermal (ISO) core model (Note 1)   (stat.fit.chi2)
  (2)M/LfML Msun/LsunM/L derived using the B-V colour (Note 2)   (phys.composition.massLightRatio)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)r0fML kpc Core radius of the dark matter halo from pseudo-isothermal (ISO) core model with fixed M/L (Note 3)   (phys.size.radius)
  (2)E_r0fML kpc Upper error on r0fML (Note 3)   (stat.error;stat.max)
  (2)e_r0fML kpc Lower error on r0fML (Note 3)   (stat.error)
  (2)rho0fML 10-3Msun/pc3Central density of the dark matter halo from pseudo-isothermal (ISO) core model with fixed M/L (Note 3)   (phys.density)
  (2)E_rho0fML 10-3Msun/pc3Upper error on rho0fML (Note 3)   (stat.error;stat.max)
  (2)e_rho0fML 10-3Msun/pc3Lower error on rho0fML (Note 3)   (stat.error)
  (2)Chi2fML  Reduced chi-squared from pseudo-isothermal (ISO) core model with fixed M/L (Note 3)   (stat.fit.chi2)
  (3)M/LdMDM Msun/LsunM/L of the disc from the pseudo-isothermal maximum disc model (MDM) (Note 1)   (phys.composition.massLightRatio)
  (3)E_M/LdMDM Msun/LsunUpper error on M/LdMDM (Note 1)   (stat.error;stat.max)
  (3)e_M/LdMDM Msun/LsunLower error on M/LdMDM (Note 1)   (stat.error)
  (3)M/LbMDM Msun/Lsun(n) M/L of the disc from the pseudo-isothermal maximum disc model (MDM) (Note 1)   (phys.composition.massLightRatio)
  (3)E_M/LbMDM Msun/Lsun(n) Upper error on M/LbMDM (Note 1)   (stat.error;stat.max)
  (3)e_M/LbMDM Msun/Lsun(n) Lower error on M/LbMDM (Note 1)   (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)r0MDM kpc Core radius of the dark matter halo from the pseudo-isothermal maximum disc model (MDM) (Note 1)   (phys.size.radius)
  (3)E_r0MDM kpc Upper error on r0MDM (Note 1)   (stat.error;stat.max)
  (3)e_r0MDM kpc Lower error on r0MDM (Note 1)   (stat.error)
  (3)rho0MDM 10-3Msun/pc3Central density of the dark matter halo from the pseudo-isothermal maximum disc model (MDM) (Note 1)   (phys.density)
  (3)E_rho0MDM 10-3Msun/pc3Upper error on rho0MDM (Note 1)   (stat.error;stat.max)
  (3)e_rho0MDM 10-3Msun/pc3Lower error on rho0MDM (Note 1)   (stat.error)
  (3)Chi2MDM  Reduced chi-squared from the pseudo-isothermal maximum disc model (MDM) (Note 1)   (stat.fit.chi2)
  (4)M/LdNFWBFM Msun/LsunM/L of the disc from the best-fitting model (BFM) for lambda-CDM cuspy density profile (Note 1)   (phys.composition.massLightRatio)
  (4)E_M/LdNFWBFM Msun/LsunUpper error on M/LdNFWBFM (Note 1)   (stat.error;stat.max)
  (4)e_M/LdNFWBFM Msun/LsunLower error on M/LdNFWBFM (Note 1)   (stat.error)
  (4)M/LbNFWBFM Msun/Lsun(n) M/L of the bulge from the best-fitting model (BFM) for lambda-CDM cuspy density profile (Note 1)   (phys.composition.massLightRatio)
  (4)E_M/LbNFWBFM Msun/Lsun(n) Upper error on M/LbNFWBFM (Note 1)   (stat.error;stat.max)
  (4)e_M/LbNFWBFM Msun/Lsun(n) Lower error on M/LbNFWBFM (Note 1)   (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)cNFWBFM  Central halo concentration index from the best-fitting model (BFM) for lambda-CDM cuspy density profile (Note 1)   (meta.code;spect.index)
  (4)E_cNFWBFM  Upper error on cNFWBFM (Note 1)   (stat.error;stat.max)
  (4)e_cNFWBFM  Lower error on cNFWBFM (Note 1)   (stat.error)
  (4)VNFWBFM km/s Halo velocity from the best-fitting model (BFM) for lambda-CDM cuspy density profile (Note 1)   (phys.veloc)
  (4)E_VNFWBFM km/s Upper error on VNFWBFM (Note 1)   (stat.error;stat.max)
  (4)e_VNFWBFM km/s Lower error on VNFWBFM (Note 1)   (stat.error)
  (4)Chi2VNFWBFM  Reduced chi-squared from the best-fitting model (BFM) for lambda-CDM cuspy density profile (Note 1)   (stat.fit.chi2)
  (4)M/LNFWfML Msun/LsunM/L derived using the B-V colour (Note 2)   (phys.composition.massLightRatio)
  (4)cNFWfML  Central halo concentration index from lambda-CDM cuspy density profile fitting with fixed M/L (Note 3)   (meta.code;spect.index)
  (4)E_cNFWfML  Upper error on cNFWfML (Note 3)   (stat.error;stat.max)
  (4)e_cNFWfML  Lower error on cNFWfML (Note 3)   (stat.error)
  (4)VNFWfML km/s Halo velocity from lambda-CDM cuspy density profile fitting with fixed M/L (Note 3)   (phys.veloc)
  (4)E_VNFWfML km/s Upper error on VNFWfML (Note 3)   (stat.error;stat.max)
  (4)e_VNFWfML km/s Lower error on VNFWfML (Note 3)   (stat.error)
  (4)Chi2NFWfML  Reduced chi-squared from lambda-CDM cuspy density profile fitting with fixed M/L (Note 3)   (stat.fit.chi2)

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