VizieR

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

VizieR

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
Target Name (resolved by Sesame) or Position:
 Target dimension:
NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/MNRAS/495/1943
  Planet-hosting stars and debris disc (Yelverton+, 2020)
ReadMe+ftp
2020MNRAS.495.1943Y
Similar Catalogs
Post annotation 		img(gal)
1.J/MNRAS/495/1943/table1List of stars in our planet host sample (201 rows)
2.J/MNRAS/495/1943/table2List of stars in our control sample (294 rows)
3.J/MNRAS/495/1943/table3(c)Photometry in the MIPS 70µm, PACS 70µm, and PACS 100µm bands for all systems studied in this paper (495 rows)
4.J/MNRAS/495/1943/table4List of all systems we find to have a significant infrared excess (51 rows)
5.J/MNRAS/495/1943/table5Upper limits on the fractional luminosities of discs in systems without a significant infrared excess (444 rows)
6.J/MNRAS/495/1943/table7Systems with a significant proper motion anomaly (152 rows)

Simple ConstraintList Of Constraints
 
Query by Constraints constraints help applied on Columns (Output Order: + - )
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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)
   (ALL)Name (char) Star name (meta.id;meta.main)
  (1+2)Dist pc Distance from the NASA Exoplanet Archive (Note G1)   (pos.distance)
  (1+2)Teff K Effective temperature from SED modelling (Note G2)   (phys.temperature.effective)
  (1+2)Lum Lsun Luminosity from SED modelling (Note G3)   (phys.luminosity)
  (1+2)abin AU (n) Closest relevant binary separation (Note 1)   (pos.distance;src.orbital)
  (1)Msini Mjup Projected mass from the NASA Exoplanet Archive (phys.mass)
  (1)apl AU (n) Semimajor axis of the most massive planet in the system from the NASA Exoplanet Archive (pos.distance;src.orbital)
  (3)More (char) Link to Tables 1,2,4,5 and 7 (meta.ref.url)
  (3+4+5+6)Sample (char) [CP] Sample (C: control sample ; P: planet host) (src.sample)
  (3)FM70obs mJy (n) Observed flux density in the MIPS 70µm band (phot.flux.density;em.IR.30-60um)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)e_FM70obs mJy (n) Error on FM70obs (stat.error)
  (3)FM70pre mJy Predicted photospheric flux density in the MIPS 70µm band (phot.flux.density;em.IR.30-60um)
  (3)chiM70  (n) Significance on the MIPS 70µm band (Note 1)   (stat.fit.param)
  (3)FP70obs mJy (n) Observed flux density in the PACS 70µm band (phot.flux.density;em.IR.30-60um)
  (3)e_FP70obs mJy (n) Error on FP70obs (stat.error)
  (3)FP70pre mJy Predicted photospheric flux density in the PACS 70µm band (phot.flux.density;em.IR.30-60um)
  (3)chiP70  (n) Significance on the PACS 70µm band (Note 1)   (stat.fit.param)
  (3)FP100obs mJy (n) Observed flux density in the PACS 100µm band (phot.flux.density;em.IR.60-100um)
  (3)e_FP100obs mJy (n) Error on FP100obs (stat.error)
  (3)FP100pre mJy Predicted photospheric flux density in the PACS 100µm band (phot.flux.density;em.IR.60-100um)
  (3)chiP100  (n) Significance on the PACS 100µm band (Note 1)   (stat.fit.param)
  (3)Simbad (char) ask the Simbad data-base about this object (meta.ref.url)
  (3)_RA deg (i) Right Ascension (J2000) from SIMBAD (not part of the original data) (pos.eq.ra;meta.main)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)_DE deg (i) Declination (J2000) from SIMBAD (not part of the original data) (pos.eq.dec;meta.main)
  (4)T K Best-fitting blackbody temperature derived from the SED modelling (phys.temperature)
  (4)e_T K Error on T (stat.error)
  (4)f  Best-fitting fractional luminosity of the disc derived from the SED modelling (phys.luminosity;arith.ratio)
  (4)e_f  Error on f (stat.error)
  (5)flim  Upper limit on the fractional luminosity of the disc (phys.luminosity;arith.ratio)
  (6)Vt m/s Tangential velocity anomaly (src.orbital.meanAnomaly)
  (6)Manom Mjup Minimum companion mass required to explain the proper motion anomaly (Note 1)   (phys.mass)
  (6)known (char) [YN] Indicates if the star has a known binary which could therefore be responsible for the anomaly (meta.code)

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