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J/ApJ/705/14/catalog Seyfert galaxies in the mid-IR (Deo+, 2009)
Seyfert galaxies studied: optical and mid-IR properties (tables 1 and 2 of paper) (109 rows)
  recno=49
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ColumnValue  Explain   (UCD)
_RAJ200003 33 36.3100 "h:m:s" Right ascension (FK5, Equinox=J2000.0) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.ra)
_DEJ2000-36 08 27.800 "d:m:s" Declination (FK5, Equinox=J2000.0) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.dec)
_RAB195003 31 41.7268 "h:m:s" Right ascension (FK4, Equinox=B1950.0) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.ra)
_DEB1950-36 18 28.745 "d:m:s" Declination (FK4, Equinox=B1950.0) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.dec)
_Glon237.9572499 deg Galactic longitude (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.galactic.lon)
_Glat-54.5982659 deg Galactic latitude (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.galactic.lat)
49recno 49  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)

NameNGC 1365  (i) Galaxy name (meta.id;meta.main)

SBB   B indicates Starbust-to-AGN flux ratios are computed in table3 (meta.ref.url)

z0.0055  NED redshift (src.redshift)
SyTS1.8  Seyfert type (Note 1)   (src.class)
b/a 0.55  Axial ratio (Note 2)   (phys.angSize;arith.ratio)
AOR12480768  Spitzer archive AOR number (meta.id;obs)
ObsM   [SM] Observing mode for Spitzer/IRS spectrum: (S=staring or M=mapping) (meta.code;obs)
Ap120.354 arcsec First extraction aperture (instr.fov)
Ap230.120 arcsec Second extraction aperture (instr.fov)
scale 112 pc/arcsec Radial extent of the extraction aperture for the galaxy (phys.angSize;src)

VVVV  Display the Quasars and AGN data (Veron et al. 2010, Cat. VII/258) (meta.ref.url)
NEDNED  ask the NED data-base about this object

5.5um 7.29e-01 Jy Spitzer/IRS 5.5um continuum flux density (phot.flux.density;em.IR.4-8um)
e_5.5um 1.26e-01 Jy 1σ error in 5.5um (stat.error)
10um 1.23e+00 Jy Spitzer/IRS 10um continuum flux density (phot.flux.density;em.IR.8-15um)
e_10um 7.41e-02 Jy 1σ error in 10um (stat.error)
14.7um 2.69e+00 Jy Spitzer/IRS 14.7um continuum flux density (phot.flux.density;em.IR.8-15um)
e_14.7um 1.28e-01 Jy 1σ error in 14.7um (stat.error)
20um 4.89e+00 Jy Spitzer/IRS 20um continuum flux density (phot.flux.density;em.IR.15-30um)
e_20um 1.18e-01 Jy 1σ error in 20um (stat.error)
30um 1.23e+01 Jy Spitzer/IRS 30um continuum flux density (phot.flux.density;em.IR.15-30um)
e_30um 3.43e-01 Jy 1σ error in 30um (stat.error)
tau 0.2823   Observed optical depth (apparent) at 9.7um (phys.absorption.opticalDepth)

_RA053.40129 deg (i) Positions from Simbad (many galaxies have no position in the original table) (right ascension part) (pos.eq.ra;meta.main)
_DE-36.14106 deg (i) Positions from Simbad (many galaxies have no position in the original table) (declination part) (pos.eq.dec;meta.main)

RAdeg 53.402894 deg (i) Extraction rectangle for mapping mode: right ascension in decimal degrees (J2000) (Note 3)   (pos.eq.ra;meta.main)
DEdeg-36.143278 deg (i) Extraction rectangle for mapping mode: declination in decimal degrees (J2000) (Note 3)   (pos.eq.dec;meta.main)

SimbadNameNGC 1365  Designation understandable by the Simbad data-base
  
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