Table Description:
This table is available for ADQL queries and through the TAP endpoint.
Resource Description:
For a list of all services and tables belonging to this table's resource, see Information on resource 'The Sixth Fundamental Catalogue (FK6)'
Resource Reference URL: ARI FK6 pages
To cite the table as such, we suggest the following BibTeX entry:
@MISC{vo:fk6_part3, year=2008, title={The Sixth Fundamental Catalogue (FK6)}, author={{GAVO} Data Centre}, url={http://dc.zah.uni-heidelberg.de/tableinfo/fk6.part3}, howpublished={{VO} resource provided by the {GAVO} Data Center} }
The FK5 consists of observations coming from the past 200 years. Three parts were published giving the results of that work: First we have the Basic FK5 with 1535 stars, second the FK5 Extension with 3117 objects , and third the FK5 Supplement with 995 objects.
The results from the HIPPARCOS mission were published in 1997 (The Hipparcos and Tycho Catalogues).
The combination of the Hipparcos data and the FK5 was primarily done using only probable single stars. Two parts were published:
In FK6 part I (published 1999) 878 single stars (or objects that could be treated as single) were used from the Basic FK5, in FK6 part III (published 2000) 3272 single stars (or objects that could be treated as single) from the FK5 Extension and the FK5 Supplement were added.
The FK6 catalogue gives three solutions for each star: Besides the standard model for single stars, in which these were treated with a constant space velocitiy (single star mode, "SI"), two further solutions were added. The data of the standard single star mode "SI" are valid for real single stars only. For all other samples of stars it is, however, necessary to include the statistically significant influence of stars with companions in the solutions. The principles of this statistical astrometry were described by 1997A&A...325..367W and are also given in the printed FK6 catalogues.
The uncertain knowledge of the included correlations allows merely to produce two approximate solutions for short-period predictions of the position (short term prediction, "STP") or predictions for longer terms (long term predictions, "LTP"). The data of the STP mode should be used for epochs near to 1991.25, the mean observational epoch of Hipparcos, the data from the LTP mode for epochs differing from this mean epoch by more than 10-20 years.
Note that part II of the catalog (containing binary stars with orbits) was never published. See 2000A&A...360..399W for an orbit of Polaris.
Sorted by DB column index. [Sort alphabetically]
Name | Table Head | Description | Unit | UCD |
---|---|---|---|---|
localid | Identifier | FK6 number of the star (it is identical with its FK5 or FK4sup number) | N/A | meta.id;meta.main |
subsample | Subsamp. | Flag for the subsample of FK6(III) stars; BX and FX denote stars from the bright and faint FK5 extensions, respectively, RS denotes stars from RSup (1993VeARI..34....1S) | N/A | meta.id;meta.dataset |
hipno | HIP# | Number of the star in the HIPPARCOS Catalogue (ESA 1997) | N/A | meta.id |
comname | Name | Common Name | N/A | meta.id |
raj2000 | RA | The right ascension alpha of the star at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6. | deg | pos.eq.ra;meta.main |
dej2000 | Dec | The declination delta of the star at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6. | deg | pos.eq.dec;meta.main |
pmra | PM α | The proper-motion component of the star in alpha at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6, cos(delta) applied. | deg/yr | pos.pm;pos.eq.ra;meta.main |
pmde | PM δ | The proper-motion component mu_delta of the star in delta at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6. | deg/yr | pos.pm;pos.eq.dec;meta.main |
epra | Ep(RA) | Central epoch of raj2000 in the SI mode. | yr | time.epoch;pos.eq.ra |
e_raj2000 | Err(RA) | Mean error of raj2000 in the SI mode, cos(delta) applied. | deg | stat.error;pos.eq.ra;meta.main |
e_pmra | Err(PM RA) | Mean error of pmra in the SI mode. | deg/yr | stat.error;pos.pm;pos.eq.ra;meta.main |
epde | Ep(Dec) | Central epoch of delta in the SI mode. | yr | time.epoch;pos.eq.dec |
e_dej2000 | Err(Dec) | Mean error of dej2000 at the central epoch epde | deg | stat.error;pos.eq.ra;meta.main |
e_pmde | Err(PM Dec) | Mean error of pmde in the SI mode. | deg/yr | stat.error;pos.pm;pos.eq.dec;meta.main |
pres | Parallax | 'Resulting' parallax p_res of the star. This is either the HIPPARCOS parallax or a photometric/spectroscopic parallax. | deg | pos.parallax |
e_pres | Err.(Par.) | Mean error of parallax | deg | stat.error;pos.parallax |
src_par | Src(Par.) | Source of parallax (H=HIPPARCOS, P=Newly determined photometric or spectroscopic parallax) | N/A | meta.code;pos.parallax |
v_rad | v_rad | Radial velocity | km/s | spect.dopplerVeloc;pos.heliocentric |
vmag | m_V | Apparent visual magnitude m_V of the star, taken from the HIPPARCOS Catalogue | mag | phot.mag;em.opt.V |
varFlag | Var? | Flag for the variability of the brightness of the star, taken from the HIPPARCOS Catalogue (see note) [Note V] | N/A | meta.code;src.var |
K_bin | Binarity | Flag for the double-star nature of the object (see note) [Note M] | N/A | meta.code.multip |
K_Delta_mu | Dmu | Flag for the double-star nature of the object based on differences between various proper motions (see note) [Note D] | N/A | meta.code.multip |
K_ae | Excellent? | Flag for astrometrically excellent stars, larger numbers are better (3 is best) | N/A | meta.code.qual |
sect | FK6 part | FK6 part of this record | N/A | meta.id.part;meta.main |
pmraLTP | PM RA (LTP) | Proper motion in RA, cos(delta) applied, in LTP mode | deg/yr | pos.pm;pos.eq.ra |
pmdeLTP | PM Dec (LTP) | Proper motion in Dec in LTP mode | deg/yr | pos.pm;pos.eq.dec |
e_pmraLTP | Err. PM RA (LTP) | Mean error in PM(RA)*cos(delta) in LTP mode | deg/yr | stat.error;pos.pm;pos.eq.ra |
e_pmdeLTP | Err. PM Dec (LTP) | Mean error in PM(Dec) in LTP mode | deg/yr | stat.error;pos.pm;pos.eq.dec |
pmraSTP | PM RA (STP) | Proper motion in RA, cos(delta) applied, in STP mode | deg/yr | pos.pm;pos.eq.ra |
pmdeSTP | PM Dec (STP) | Proper motion in Dec in STP mode | deg/yr | pos.pm;pos.eq.dec |
e_pmraSTP | Err. PM RA (STP) | Mean error in PM(RA)*cos(delta) in STP mode | deg/yr | stat.error;pos.pm;pos.eq.ra |
e_pmdeSTP | Err. PM Dec (STP) | Mean error in PM(Dec) in STP mode | deg/yr | stat.error;pos.pm;pos.eq.dec |
pmraHIP | PM RA (HIP) | Proper motion in RA, cos(delta) applied, in HIP mode | deg/yr | pos.pm;pos.eq.ra |
pmdeHIP | PM Dec (HIP) | Proper motion in Dec in HIP mode | deg/yr | pos.pm;pos.eq.dec |
e_pmraHIP | Err. PM RA (HIP) | Mean error in PM(RA)*cos(delta) in HIP mode | deg/yr | stat.error;pos.pm;pos.eq.ra |
e_pmdeHIP | Err. PM Dec (HIP) | Mean error in PM(Dec) in HIP mode | deg/yr | stat.error;pos.pm;pos.eq.dec |
hipdup | HIP dup. | HIPPARCOS indicators for a suspected visual binary; d=duplicity induced variability (H52), s=Hipparcos suspected non-single (H61), t=both | N/A | meta.code.multip |
hipfitqual | HIP fit | HIPPARCOS goodness-of-fit parameter (HIP Field H30, F2); A large value of F2 (e.g. larger than 3) may be caused by a duplicity of the object, but other reasons cannot be excluded. NULL means a negative goodness-of-fit in HIP. | N/A | meta.code.qual |
speckleflag | Speckle dup? | Indications on binarity provided by the catalogue of speckle observations (1999AJ....117.1890M); b=binarity resolved, u=possibly resolved, n=object observed but not resolved | N/A | meta.code.multip |
viscomp | Vis. comp. | Indicator for a star which has one (or more) visual component(s) with a separation rho of at least 60 arcsec. [Note VC] | N/A | meta.code.multip |
binindsrv | RV Indicators | Indications for binarity provided by radial velocities from various sources (see Note) [Note RV] | N/A | meta.code.multip |
binindecl | Eclipsing? | Indicators for binarity from photometric variability (a=Algol-type, b=β Lyr-type, e=uncertain type, w=W UMa type) | N/A | meta.code;src.var |
pulsating | Pulsating? | Indicator for a variability of the radial velocity V_rad due to stellar pulsation (which may be confused with a variability of V_rad due to spectroscopic binarity; c=Cepheid, s=δ Sct, b=β Cep) | N/A | meta.code;src.var |
note | Note | Note for this object | N/A | meta.note |
Columns that are parts of indices are marked like this.
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