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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/A+A/688/A49
  M dwarfs observed with eROSITA and TESS (Joseph+, 2024)
ReadMe+ftp
2024A&A...688A..49J
Similar Catalogs
Post annotation 		img(gal)
1.J/A+A/688/A49/tableb1Stellar parameters from eRASS (25 rows)

Simple ConstraintList Of Constraints
 
Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  GaiaDR2  Gaia ID from data release 2 (GaiaDR2) (meta.id;meta.main)
  RA2 deg (i) Proper motion corrected X-ray right ascension during eRASS 2 (J2000) (RACORReRASS2) (pos.eq.ra;meta.main)
  RA3deg deg Proper motion corrected X-ray right ascension during eRASS 3 (J2000) (RACORReRASS3) (pos.eq.ra)
  DE2 deg (i) Proper motion corrected X-ray declination during eRASS 2 (J2000) (DECCORReRASS2) (pos.eq.dec;meta.main)
  DE3deg deg Proper motion corrected X-ray declination during eRASS 3 (J2000) (DECCORReRASS3) (pos.eq.dec)
  Sep2 arcsec Separation along a great circle between the proper motion corrected Gaia-DR2 coordinates and the matched eRASS coordinates RA CORR eRASS2 and DEC CORR eRASS2 (Separation_eRASS2) (pos.angDistance)
  Sep3 arcsec Separation along a great circle between the proper motion corrected Gaia-DR2 coordinates and the matched eRASS coordinates RA CORR eRASS3 and DEC CORR eRASS3 (separation_eRASS3) (pos.angDistance)
  DetLike2  Detection likelihood in energy band 0.2-5 KeV during eRASS2 (DETLIKEeRASS2) (stat.likelihood)
  DetLike3  Detection likelihood in energy band 0.2-5 KeV during eRASS2 (DETLIKEeRASS3) (stat.likelihood)
  MLrate02 ct/s Count rate in energy band 0.2-5 KeV during eRASS2 (MLRATE0_eRASS2) (phot.count;em.X-ray)
  MLrate03  Count rate in energy band 0.2-5 KeV during eRASS2 (MLRATE0_eRASS3) (phot.count;em.X-ray)
  Lx 10-7W X-ray luminosity from the average MLRATE0 from eRASS 2 and eRASS 3 and Gaia distances (L_x) (phys.luminosity;em.X-ray)
  Fxsurf mW/m2 X-ray surface flux from the average MLRATE0 from eRASS 2 and eRASS3 (Fxsurf) (phot.flux;em.X-ray)

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