Show | Sort | Join tables | Column | Constraint | Explain (UCD) |
| | (ALL) | recno | | Record number assigned by the VizieR team. Should Not be used for identification. (meta.record) (RECORD) |
| | (1+2+3+4+5) | Name | (char) | Planetary nebula name (meta.id;meta.main) (ID_MAIN) |
| | (ALL) | Ref | (char) | Reference (meta.ref;pos.frame) (REFER_CODE) |
| | (1+2+3+4+5) | f_Ref | (char) | Flag on Ref (Note G1)
(meta.code) (CODE_MISC) |
| | (1) | ne[SII] | cm-3 | (n) Electron density derived from the [SII]λ6716/λ6731 diagnosis (phys.density;phys.electron) (PHYS_DENSITY_ELECT) |
| | (1) | ne[OII] | cm-3 | (n) Electron density derived from the [OII]λ3726/λ3729 diagnosis (phys.density;phys.electron) (PHYS_DENSITY_ELECT) |
| | (1) | ne[ClIII] | cm-3 | (n) Electron density derived from the [ClIII]λ5518/λ5538 diagnosis (phys.density;phys.electron) (PHYS_DENSITY_ELECT) |
| | (1) | ne[ArIV] | cm-3 | (n) Electron density derived from the [ArIV]λ4711/λ4740 diagnosis (phys.density;phys.electron) (PHYS_DENSITY_ELECT) |
| | (1) | ne | cm-3 | Geometric mean of the electron density (Note 1)
(phys.density;stat.mean) (PHYS_DENSITY_ELECT) |
| | (1) | Te[NII] | K | Electron temperature obtained from the diagnostics [NII]λ5755/ (λ6548+λ6583) (phys.temperature.electron;phys.electron) (PHYS_TEMP_ELECT) |
| | (1) | Te[OIII] | K | Electron temperature obtained from the diagnostics [OIII]λ4363/ (λ4959+λ5007) (phys.temperature.electron;phys.electron) (PHYS_TEMP_ELECT) |
ALL cols | | | |
| | (1+2+3+4+5) | ptot | | Final score of the spectrum (see Section 6.9) (meta.code.qual) (CODE_QUALITY) |
| | (1) | SimbadName | (char) | (n)Designation understandable by the Simbad data-base (meta.id) (ID_ALTERNATIVE) |
| | (1) | _RA | deg | (i) Right Ascension (J2000) from SIMBAD (not part of the original data) (pos.eq.ra;meta.main) (POS_EQ_RA_MAIN) |
| | (1) | _DE | deg | (i) Declination (J2000) from SIMBAD (not part of the original data) (pos.eq.dec;meta.main) (POS_EQ_DEC_MAIN) |
| | (2) | O+(b) | | 12+log(O+/H+) abundance calculated using the blue [OII] lines (phys.abund) (PHYS_ABUND_MISC) |
| | (2) | O+(r) | | (n) 12+log(O+/H+) abundance calculated using the red [OII] lines (phys.abund) (PHYS_ABUND_MISC) |
| | (2) | O++ | | 12+log(O++/H+) abundance (phys.abund) (PHYS_ABUND_MISC) |
| | (2) | N+ | | 12+log(N+/H+) abundance (phys.abund) (PHYS_ABUND_MISC) |
| | (2) | Ne++ | | (n) 12+log(Ne++/H+) abundance (phys.abund) (PHYS_ABUND_MISC) |
| | (2) | S+ | | 12+log(S+/H+) abundance (phys.abund) (PHYS_ABUND_MISC) |
| | (2) | S++ | | (n) 12+log(S++/H+) abundance (phys.abund) (PHYS_ABUND_MISC) |
| | (2) | Ar++ | | (n) 12+log(Ar++/H+) abundance (phys.abund) (PHYS_ABUND_MISC) |
| | (2) | Cl++ | | (n) 12+log(Cl++/H+) abundance (phys.abund) (PHYS_ABUND_MISC) |
ALL cols | | | |
| | (3) | He+4026 | | (n) 12+log(He+/H) abundance derived from the λ4026 line (phys.abund.Y) (PHYS_ABUND_Y) |
| | (3) | He+4388 | | (n) 12+log(He+/H) abundance derived from the λ4388 line (phys.abund.Y) (PHYS_ABUND_Y) |
| | (3) | He+4922 | | (n) 12+log(He+/H) abundance derived from the λ4922 line (phys.abund.Y) (PHYS_ABUND_Y) |
| | (3) | He+4471 | | (n) 12+log(He+/H) abundance derived from the λ4471 line (phys.abund.Y) (PHYS_ABUND_Y) |
| | (3) | He+5876 | | 12+log(He+/H) abundance derived from the λ5876 line (phys.abund.Y) (PHYS_ABUND_Y) |
| | (3) | He+6678 | | (n) 12+log(He+/H) abundance derived from the λ6678 line (phys.abund.Y) (PHYS_ABUND_Y) |
| | (3) | He+ | | 12+log(He+/H) abundance (phys.abund.Y) (PHYS_ABUND_Y) |
| | (3) | He++ | | (n) 12+log(He++/H) abundance (phys.abund.Y) (PHYS_ABUND_Y) |
| | (3) | He | | 12+log(He/H) abundance (phys.abund.Y) (PHYS_ABUND_Y) |
| | (4) | O(b) | | 12+log(O/H) abundance calculated using the blue [OII] lines (phys.abund) (PHYS_ABUND_MISC) |
| | (4) | N(b) | | 12+log(N/H) abundance calculated using the blue [OII] lines (phys.abund) (PHYS_ABUND_MISC) |
| | (4) | Ne(b) | | (n) 12+log(Ne/H) abundance calculated using the blue [OII] lines (phys.abund) (PHYS_ABUND_MISC) |
| | (4) | S(b) | | (n) 12+log(S/H) abundance calculated using the blue [OII] lines (phys.abund) (PHYS_ABUND_MISC) |
ALL cols | | | |
| | (4) | Ar(b) | | (n) 12+log(Ar/H) abundance calculated using the blue [OII] lines (phys.abund) (PHYS_ABUND_MISC) |
| | (4) | Cl(b) | | (n) 12+log(Cl/H) abundance calculated using the blue [OII] lines (phys.abund) (PHYS_ABUND_MISC) |
| | (4) | O(r) | | (n) 12+log(O/H) abundance calculated using the red [OII] lines (phys.abund) (PHYS_ABUND_MISC) |
| | (4) | N(r) | | (n) 12+log(N/H) abundance calculated using the red [OII] lines (phys.abund) (PHYS_ABUND_MISC) |
| | (4) | Ne(r) | | (n) 12+log(Ne/H) abundance calculated using the red [OII] lines (phys.abund) (PHYS_ABUND_MISC) |
| | (4) | S(r) | | (n) 12+log(S/H) abundance calculated using the red [OII] lines (phys.abund) (PHYS_ABUND_MISC) |
| | (4) | Ar(r) | | (n) 12+log(Ar/H) abundance calculated using the red [OII] lines (phys.abund) (PHYS_ABUND_MISC) |
| | (4) | Cl(r) | | (n) 12+log(Cl/H) abundance calculated using the red [OII] lines (phys.abund) (PHYS_ABUND_MISC) |
| | (5) | p0 | | [0/10] Score indicating whether the spectra was obtained with a CCD (p0=10) or not (p0=0) (meta.code.qual) (CODE_QUALITY) |
| | (5) | p1 | | [20] Score related to the available temperature diagnostics (meta.code.qual) (CODE_QUALITY) |
| | (5) | N | | Number of density diagnostics (meta.number) (NUMBER) |
| | (5) | p2 | | Score related to the density diagnosis (p2=9-15 for 1-4 working density diagnostics) (meta.code.qual) (CODE_QUALITY) |
| | (5) | [NII] | | (n) [NII] λ6584/λ6548 line ratio (spect.line.intensity;arith.ratio) (SPECT_LINE_RATIO) |
ALL cols | | | |
| | (5) | p3 | | [0/10] Score associated to [NII] (meta.code.qual) (CODE_QUALITY) |
| | (5) | [OIII] | | (n) [OIII] λ5007/λ4959 line ratio (spect.line.intensity;arith.ratio) (SPECT_LINE_RATIO) |
| | (5) | p4 | | [0/10] Score associated to [OIII] (meta.code.qual) (CODE_QUALITY) |
| | (5) | NHeI | | Number of HeI lines unaffected by optical depth effects available in the spectra (meta.number) (NUMBER) |
| | (5) | p5 | | [2/20] Score assigned to NHeI (Note 1)
(meta.code.qual) (CODE_QUALITY) |
| | (5) | NBL | | Number of balmer lines (out of Hα, Hγ and Hδ) whose intensities are listed in the spectra (meta.number) (NUMBER) |
| | (5) | P-B | | (n) Difference between the median deviations of the Paschen and Balmer lines from their expected values (see Section 6.7) (stat.fit.param) (FIT_PARAM_VALUE) |
| | (5) | p6 | | [0/15] Score assigned using the behaviour of all these lines (meta.code.qual) (CODE_QUALITY) |
| | (6) | BibCode | (char) | BibCode (meta.bib.bibcode) (REFER_BIBCODE) |
| | (6) | Aut | (char) | Author's name (meta.bib.author) (ID_AUTHOR) |
| | (6) | Com | (char) | Comments (meta.note) (REMARKS) |
ALL cols | | | |