J/PASP/136/I4203    Validation of Gaia DR3 Orbital Solutions  (Nagarajan+, 2024)

Validation of Gaia DR3 Orbital and Acceleration Solutions with Hierarchical Triples Nagarajan P., El-Badry K. <Publ. Astron. Soc. Pac. 136, 094203 (2024)> =2024PASP..136i4203N 2024PASP..136i4203N (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Optical Keywords: Astrometric binary stars - Trinary stars - Astrostatistics Abstract: Using data from Gaia DR3, we construct a sample of 14791 gravitationally bound wide pairs in which one of the components is an unresolved binary with an astrometric orbital or acceleration solution. These systems are hierarchical triples, with inner binary separations of order 1au, and outer separations of 100-100000au. Leveraging the fact that the inner binary and outer tertiary should have nearly identical parallaxes, we use the sample to calibrate the parallax uncertainties for orbital and acceleration binary solutions. We find that the parallax uncertainties of orbital solutions are typically underestimated by a factor of 1.3 at G>14, and by a factor of 1.7 at G=8-14. The true parallax uncertainties are nevertheless a factor of ∼10 smaller than those of the single-star astrometric solutions for the same sources. The parallax uncertainties of acceleration solutions are underestimated by larger factors of 2-3 but still represent a significant improvement compared to the sources' single-star solutions. We provide tabulated uncertainty inflation factors for astrometric binary solutions and make the catalog of hierarchical triples publicly available. Description: We present a catalog of 14791 gravitationally bound wide pairs where one of the components is an unresolved binary with an astrometric orbital or acceleration solution in Gaia DR3. The catalog is separated into two tables corresponding to orbital solutions and acceleration solutions, respectively. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file acc.dat 2656 6998 Gravitationally bound wide pairs where one of the components is an unresolved binary with an astrometric orbital or acceleration solution in Gaia DR3, acceleration solutions orb.dat 2656 7820 Gravitationally bound wide pairs where one of the components is an unresolved binary with an astrometric orbital or acceleration solution in Gaia DR3, orbital solutions -------------------------------------------------------------------------------- See also: I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022) I/357 : Gaia DR3 Part 3: Non-single stars I/358 : Gaia DR3 Part 4: Variability Byte-by-byte Description of file: acc.dat orb.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 I19 --- Id1 Gaia DR3 source_id of the astrometric binary (source_id1) 21- 39 I19 --- Id2 Gaia DR3 source_id of the putative tertiary (source_id2) 41- 55 F15.11 deg RAdeg Astrometric binary right ascension (ICRS) at Ep=2016.0 (ra1) 57- 71 F15.11 deg RA2deg Putative tertiary right ascension (ICRS) at Ep=2016.0 (ra2) 73- 87 F15.11 deg DEdeg Astrometric binary declination (ICRS) at Ep=2016.0 (dec1) 89- 103 F15.11 deg DE2deg Putative tertiary declination (ICRS) at Ep=2016.0 (dec2) 105- 112 F8.3 mas/yr pmRA1 Astrometric binary proper motion along RA, pmRA*cosDE (pmra1) 114- 121 F8.3 mas/yr pmRA2 Putative tertiary proper motion along RA, pmRA*cosDE (pmra2) 123- 130 F8.3 mas/yr pmDE1 Astrometric binary proper motion along DE (pmdec1) 132- 139 F8.3 mas/yr pmDE2 Putative tertiary proper motion along DE (pmdec2) 141- 149 F9.6 mas Plx1 Astrometric binary parallax (parallax1) 151- 159 F9.6 mas Plx2 Putative tertiary parallax (parallax2) 161- 168 F8.6 mas e_Plx1 Astrometric binary parallax error (parallax_error1) 170- 177 F8.6 mas e_Plx2 Putative tertiary parallax error (parallax_error2) 179- 186 F8.6 mas/yr e_pmRA1 Astrometric binary proper motion along RA error (pmra_error1) 188- 195 F8.6 mas/yr e_pmRA2 Putative tertiary proper motion along RA error (pmra_error2) 197- 204 F8.6 mas/yr e_pmDE1 Astrometric binary proper motion along DE error (pmdec_error1) 206- 213 F8.6 mas/yr e_pmDE2 Putative tertiary proper motion along DE error (pmdec_error2) 215- 222 F8.5 mag Gmag1 Astrometric binary G magnitude (photgmean_mag1) 224- 231 F8.5 mag Gmag2 Putative tertiary G magnitude (photgmean_mag2) 233- 239 F7.5 um-1 nueff1 ?=- Astrometric binary effective wavenumber used in astrometric solution (nueffusedinastrometry1) 241- 247 F7.5 um-1 nueff2 ?=- Putative tertiary effective wavenumber used in astrometric solution (nueffusedinastrometry2) 249- 255 F7.5 um-1 pscol1 ?=- Astrometric binary pseudocolour (pseudocolour1) 257- 264 F8.6 um-1 pscol2 ?=- Putative tertiary pseudocolour (pseudocolour2) 266- 280 F15.11 deg ELAT1 Astrometric binary ecliptic latitude (ecl_lat1) 282- 296 F15.11 deg ELAT2 Putative tertiary ecliptic latitude (ecl_lat2) 298- 299 I2 --- Solved1 ?=- Astrometric binary which parameters have been solved for? (astrometricparamssolved1) 301- 302 I2 --- Solved2 ?=- Putative tertiary which parameters have been solved for? (astrometricparamssolved2) 304- 314 F11.9 deg theta Angular separation (pairdistance) 316- 326 F11.4 au sepAU Projected separation (sep_AU) 328- 336 F9.4 --- Sigma18 Sigma 18 Sigma18) 338- 349 E12.6 --- R R chance align (Rchancealign) 351- 369 I19 --- SolID1 Astrometric binary solution identifier (solution_id1) 371- 389 I19 --- SolID2 Putative tertiary solution identifier (solution_id2) 391- 400 I10 --- RandomI1 ?=- Astrometric binary random index (random_index1) 402- 411 I10 --- RandomI2 ?=- Putative tertiary random index (random_index2) 413- 416 I4 yr refEpoch1 [2016] Astrometric binary reference epoch (ref_epoch1) 418- 421 I4 yr refEpoch2 [2016] Putative tertiary reference epoch (ref_epoch2) 423- 430 F8.6 mas e_RAdeg Astrometric binary right ascension error (ra_error1) 432- 439 F8.6 mas e_RA2deg Putative tertiary right ascension error (ra_error2) 441- 448 F8.6 mas e_DEdeg Astrometric binary declination error (dec_error1) 450- 457 F8.6 mas e_DE2deg Putative tertiary declination error (dec_error2) 459- 467 F9.4 --- RPlx1 Astrometric binary parallax divided by its standard error (parallaxovererror1) 469- 478 F10.5 --- RPlx2 Putative tertiary parallax divided by its standard error (parallaxovererror2) 480- 489 F10.6 mas/yr PM1 Astrometric binary total proper motion (pm1) 491- 500 F10.6 mas/yr PM2 Putative tertiary total proper motion (pm2) 502- 510 F9.6 --- RADEcor1 Astrometric binary correlation between RA and DE (radeccorr1) 512- 520 F9.6 --- RADEcor2 Putative tertiary correlation between RA and DE (radeccorr2) 522- 530 F9.6 --- RAPlxcor1 Astrometric binary correlation between RA and plx (raparallaxcorr1) 532- 540 F9.6 --- RAPlxcor2 Putative tertiary correlation between RA and plx (raparallaxcorr2) 542- 550 F9.6 --- RApmRAcor1 Astrometric binary correlation between RA and pmRA (rapmracorr1) 552- 560 F9.6 --- RApmRAcor2 Putative tertiary correlation between RA and pmRA (rapmracorr2) 562- 570 F9.6 --- RApmDEcor1 Astrometric binary correlation between RA and pmDE (rapmdeccorr1) 572- 580 F9.6 --- RApmDEcor2 Putative tertiary correlation between RA and pmDE (rapmdeccorr2) 582- 590 F9.6 --- DEPlxcor1 Astrometric binary correlation between DE and plx (decparallaxcorr1) 592- 600 F9.6 --- DEPlxcor2 Putative tertiary correlation between DE and plx (decparallaxcorr2) 602- 610 F9.6 --- DEpmRAcor1 Astrometric binary correlation between DE and pmRA (decpmracorr1) 612- 620 F9.6 --- DEpmRAcor2 Putative tertiary correlation between DE and pmRA (decpmracorr2) 622- 630 F9.6 --- DEpmDEcor1 Astrometric binary correlation between DE and pmDE (decpmdeccorr1) 632- 640 F9.6 --- DEpmDEcor2 Putative tertiary correlation between DE and pmDE (decpmdeccorr2) 642- 650 F9.6 --- PlxpmRAcor1 Astrometric binary correlation between plx and pmRA (parallaxpmracorr1) 652- 660 F9.6 --- PlxpmRAcor2 Putative tertiary correlation between plx and pmRA (parallaxpmracorr2) 662- 670 F9.6 --- PlxpmDEcor1 Astrometric binary correlation between plx and pmDE (parallaxpmdeccorr1) 672- 680 F9.6 --- PlxpmDEcor2 correlation between plx and pmDE (parallaxpmdeccorr2) 682- 690 F9.6 --- pmRApmDEcor1 Astrometric binary correlation between pmRA and pmDE (pmrapmdeccorr1) 692- 700 F9.6 --- pmRApmDEcor2 Putative tertiary correlation between pmRA and pmDE (pmrapmdeccorr2) 702- 705 I4 --- NAL1 ?=- Astrometric binary total number of observations in along-scan (AC) (astrometricnobs_al1) 707- 710 I4 --- NAL2 ?=- Putative tertiary total number of observations in along-scan (AC) (astrometricnobs_al2) 712- 715 I4 --- NAC1 ?=- Astrometric binary total number of observations in across-scan (AL) (astrometricnobs_ac1) 717- 720 I4 --- NAC2 ?=- Putative tertiary total number of observations in across-scan (AL) (astrometricnobs_ac2) 722- 725 I4 --- NgAL1 ?=- Astrometric binary number of good observations in along-scan (AL) (astrometricngoodobsal1) 727- 730 I4 --- NgAL2 ?=- Putative tertiary number of good observations in along-scan (AL) (astrometricngoodobsal2) 732- 733 I2 --- NbAL1 ?=- Astrometric binary number of bad observations in along-scan (AL) (astrometricnbadobsal1) 735- 737 I3 --- NbAL2 ?=- Putative tertiary number of bad observations in along-scan (AL) (astrometricnbadobsal2) 739- 747 F9.5 --- gofAL1 Astrometric binary goodness of fit statistic of model (astrometricgofal1) 749- 759 F11.6 --- gofAL2 Putative tertiary goodness of fit statistic of model (astrometricgofal2) 761- 772 E12.6 --- chi2AL1 Astrometric binary AL chi-square value (astrometricchi2al1) 774- 785 E12.6 --- chi2AL2 Putative tertiary AL chi-square value (astrometricchi2al2) 787- 794 F8.6 mas epsi1 Astrometric binary excess noise (astrometricexcessnoise1) 796- 803 F8.6 mas epsi2 Putative tertiary excess noise (astrometricexcessnoise2) 805- 816 E12.6 --- sepsi1 Astrometric binary significance of excess noise (astrometricexcessnoise_sig1) 818- 829 E12.6 --- sepsi2 Putative tertiary significance of excess noise (astrometricexcessnoise_sig2) 831 I1 --- APF1 [0/1] Astrometric binary primary or secondary (astrometricprimaryflag1) 833 I1 --- APF2 [0/1] Putative tertiary primary or secondary (astrometricprimaryflag2) 835- 842 F8.6 um-1 e_pscol1 ?=- Astrometric binary pseudocolour error (pseudocolour_error1) 844- 851 F8.6 um-1 e_pscol2 ?=- Putative tertiary pseudocolour error (pseudocolour_error2) 853- 861 F9.6 --- RApscolCorr1 ?=- Astrometric binary correlation between RA and pscol (rapseudocolourcorr1) 863- 871 F9.6 --- RApscolCorr2 ?=- Putative tertiary correlation between RA and pscol (rapseudocolourcorr2) 873- 881 F9.6 --- DEpscolCorr1 ?=- Astrometric binary correlation between DE and pscol (decpseudocolourcorr1) 883- 891 F9.6 --- DEpscolCorr2 ?=- Putative tertiary correlation between DE and pscol (decpseudocolourcorr2) 893- 901 F9.6 --- PlxpscolCorr1 ?=- Astrometric binary correlation between plx and pscol (parallaxpseudocolourcorr1) 903- 911 F9.6 --- PlxpscolCorr2 ?=- Putative tertiary correlation between plx and pscol (parallaxpseudocolourcorr2) 913- 921 F9.6 --- pmRApscolCorr1 ?=- Astrometric binary correlation between pmRA and pscol (pmrapseudocolourcorr1) 923- 931 F9.6 --- pmRApscolCorr2 ?=- Putative tertiary correlation between pmRA and pscol (pmrapseudocolourcorr2) 933- 941 F9.6 --- pmDEpscolCorr1 ?=- Astrometric binary correlation between pmDE and pscol (pmdecpseudocolourcorr1) 943- 951 F9.6 --- pmDEpscolCorr2 ?=- Putative tertiary correlation between pmDE and pscol (pmdecpseudocolourcorr2) 953- 955 I3 --- MatchObsA1 ?=- Astrometric binary matched FOV transits (astrometricmatchedtransits1) 957- 959 I3 --- MatchObsA2 ?=- Putative tertiary matched FOV transits (astrometricmatchedtransits2) 961- 962 I2 --- Nper1 ?=- Astrometric binary number of visibility periods (visibilityperiodsused1) 964- 965 I2 --- Nper2 ?=- Putative tertiary number of visibility periods (visibilityperiodsused2) 967- 974 F8.6 mas amax1 Astrometric binary longest semi-major axis (astrometricsigma5dmax1) 976- 983 F8.6 mas amax2 Putative tertiary longest semi-major axis (astrometricsigma5dmax2) 985- 987 I3 --- MatchObs1 ?=- Astrometric binary number of transits matched to this source (matched_transits1) 989- 991 I3 --- MatchObs2 ?=- Putative tertiary number of transits matched to this source (matched_transits2) 993- 995 I3 --- NewMatchObs1 ?=- Astrometric binary number of transits newly incorporated (newmatchedtransits1) 997- 999 I3 --- NewMatchObs2 ?=- Putative tertiary number of transits newly incorporated (newmatchedtransits2) 1001-1002 I2 --- MatchObsrm1 ?=- Astrometric binary number of transits removed (matchedtransitsremoved1) 1004-1005 I2 --- MatchObsrm2 ?=- Putative tertiary number of transits removed (matchedtransitsremoved2) 1007-1014 F8.6 --- IPDgofha1 Astrometric binary Amplitude of the IPD GoF versus position angle of scan (ipdgofharmonic_amplitude1) 1016-1023 F8.6 --- IPDgofha2 Putative tertiary Amplitude of the IPD GoF versus position angle of scan (ipdgofharmonic_amplitude2) 1025-1034 F10.6 deg IPDgofhp1 Astrometric binary Phase of the IPD GoF versus position angle of scan (ipdgofharmonic_phase1) 1036-1045 F10.6 deg IPDgofhp2 Putative tertiary Phase of the IPD GoF versus position angle of scan (ipdgofharmonic_phase2) 1047 I1 --- IPDfmp1 ?=- Astrometric binary Percent of successful-IPD windows with more than one peak (ipdfracmulti_peak1) 1049-1050 I2 --- IPDfmp2 ?=- Putative tertiary Percent of successful-IPD windows with more than one peak (ipdfracmulti_peak2) 1052-1053 I2 --- IPDfow1 ?=- Astrometric binary Percent of transits with truncated windows or multiple gate (ipdfracodd_win1) 1055-1056 I2 --- IPDfow2 ?=- Putative tertiary Percent of transits with truncated windows or multiple gate (ipdfracodd_win2) 1058-1065 F8.5 --- RUWE1 Astrometric binary Renormalised unit weight error (ruwe1) 1067-1075 F9.6 --- RUWE2 Putative tertiary Renormalised unit weight error (ruwe2) 1077-1084 F8.6 --- SDSk11 ?=- Astrometric binary degree of concentration of scan directions across the source (scandirectionstrength_k11) 1086-1093 F8.6 --- SDSk12 ?=- Putative tertiary degree of concentration of scan directions across the source (scandirectionstrength_k12) 1095-1102 F8.6 --- SDSk21 ?=- Astrometric binary degree of concentration of scan directions across the source (scandirectionstrength_k21) 1104-1111 F8.6 --- SDSk22 ?=- Putative tertiary degree of concentration of scan directions across the source (scandirectionstrength_k22) 1113-1120 F8.6 --- SDSk31 ?=- Astrometric binary degree of concentration of scan directions across the source (scandirectionstrength_k31) 1122-1129 F8.6 --- SDSk32 ?=- Putative tertiary degree of concentration of scan directions across the source (scandirectionstrength_k32) 1131-1138 F8.6 --- SDSk41 ?=- Astrometric binary degree of concentration of scan directions across the source (scandirectionstrength_k41) 1140-1147 F8.6 --- SDSk42 ?=- Putative tertiary degree of concentration of scan directions across the source (scandirectionstrength_k42) 1149-1159 F11.6 deg SDMk11 ?=- Astrometric binary mean position angle of scan directions across the source (scandirectionmean_k11) 1161-1171 F11.6 deg SDMk12 ?=- Putative tertiary mean position angle of scan directions across the source (scandirectionmean_k12) 1173-1182 F10.6 deg SDMk21 ?=- Astrometric binary mean position angle of scan directions across the source (scandirectionmean_k21) 1184-1193 F10.6 deg SDMk22 ?=- Putative tertiary mean position angle of scan directions across the source (scandirectionmean_k22) 1195-1204 F10.6 deg SDMk31 ?=- Astrometric binary mean position angle of scan directions across the source (scandirectionmean_k31) 1206-1215 F10.6 deg SDMk32 ?=- Putative tertiary mean position angle of scan directions across the source (scandirectionmean_k32) 1217-1226 F10.6 deg SDMk41 ?=- Astrometric binary mean position angle of scan directions across the source (scandirectionmean_k41) 1228-1237 F10.6 deg SDMk42 ?=- Putative tertiary mean position angle of scan directions across the source (scandirectionmean_k42) 1239 I1 --- Dup1 [0,1] Astrometric binary multiple source identifiers (duplicated_source1) 1241 I1 --- Dup2 [0,1] Putative tertiary multiple source identifiers (duplicated_source2) 1243-1246 I4 --- o_Gmag1 ?=- Astrometric binary number of observations contributing to G photometry (photgn_obs1) 1248-1251 I4 --- o_Gmag2 ?=- Putative tertiary number of observations contributing to G photometry (photgn_obs2) 1253-1264 E12.6 e-/s FG1 Astrometric binary G-band mean flux (photgmean_flux1) 1266-1277 E12.6 e-/s FG2 Putative tertiary G-band mean flux (photgmean_flux2) 1279-1290 E12.6 e-/s e_FG1 Astrometric binary FG error (photgmeanfluxerror1) 1292-1303 E12.6 e-/s e_FG2 Putative tertiary FG error (photgmeanfluxerror2) 1305-1316 E12.6 --- RFG1 Astrometric binary G-band mean flux divided by its error (photgmeanfluxover_error1) 1318-1329 E12.6 --- RFG2 Putative tertiary G-band mean flux divided by its error (photgmeanfluxover_error2) 1331-1333 I3 --- o_BPmag1 ?=- Astrometric binary BPmag error (photbpn_obs1) 1335-1337 I3 --- o_BPmag2 ?=- BPmag error (photbpn_obs2) 1339-1350 E12.6 e-/s FBP1 ?=- Astrometric binary integrated BP mean flux (photbpmean_flux1) 1352-1363 E12.6 e-/s FBP2 ?=- Putative tertiary integrated BP mean flux (photbpmean_flux2) 1365-1376 E12.6 e-/s e_FBP1 ?=- Astrometric binary FBP error (photbpmeanfluxerror1) 1378-1389 E12.6 e-/s e_FBP2 ?=- Putative tertiary FBP error (photbpmeanfluxerror2) 1391-1402 E12.6 --- RFBP1 ?=- Astrometric binary integrated BP mean flux divided by its error (photbpmeanfluxover_error1) 1404-1415 E12.6 --- RFBP2 ?=- Putative tertiary integrated BP mean flux divided by its error (photbpmeanfluxover_error2) 1417-1424 F8.5 mag BPmag1 ?=- Astrometric binary integrated BP mean magnitude (photbpmean_mag1) 1426-1433 F8.5 mag BPmag2 ?=- Putative tertiary integrated BP mean magnitude (photbpmean_mag2) 1435-1437 I3 --- o_RPmag1 ?=- Astrometric binary RPmag error (photrpn_obs1) 1439-1441 I3 --- o_RPmag2 ?=- Putative tertiary RPmag error (photrpn_obs2) 1443-1454 E12.6 e-/s FRP1 ?=- Astrometric binary integrated RP mean flux (photrpmean_flux1) 1456-1467 E12.6 e-/s FRP2 ?=- Putative tertiary integrated RP mean flux (photrpmean_flux2) 1469-1480 E12.6 e-/s e_FRP1 ?=- Astrometric binary FRP error (photrpmeanfluxerror1) 1482-1493 E12.6 e-/s e_FRP2 ?=- Putative tertiary FRP error (photrpmeanfluxerror2) 1495-1506 E12.6 --- RFRP1 ?=- Astrometric binary integrated RP mean flux divided by its error (photrpmeanfluxover_error1) 1508-1519 E12.6 --- RFRP2 ?=- Putative tertiary integrated RP mean flux divided by its error (photrpmeanfluxover_error2) 1521-1528 F8.5 mag RPmag1 ?=- Astrometric binary RPmag error (photrpmean_mag1) 1530-1537 F8.5 mag RPmag2 ?=- Putative tertiary RPmag error (photrpmean_mag2) 1539-1545 F7.5 --- E(BP/RP)1 ?=- Astrometric binary BP/RP excess factor (photbprpexcessfactor1) 1547-1555 F9.5 --- E(BP/RP)2 ?=- Putative tertiary BP/RP excess factor (photbprpexcessfactor2) 1557-1558 I2 --- NBPcont1 ?=- Astrometric binary number of BP contaminated transits (photbpncontaminatedtransits1) 1560-1561 I2 --- NBPcont2 ?=- Putative tertiary number of BP contaminated transits (photbpncontaminatedtransits2) 1563-1565 I3 --- NBPblend1 ?=- Astrometric binary number of RP contaminated transits (photbpnblendedtransits1) 1567-1569 I3 --- NBPblend2 ?=- Putative tertiary number of RP contaminated transits (photbpnblendedtransits2) 1571-1572 I2 --- NRPcont1 ?=- Astrometric binary number of BP contaminated transits (photrpncontaminatedtransits1) 1574-1575 I2 --- NRPcont2 ?=- Putative tertiary number of BP contaminated transits (photrpncontaminatedtransits2) 1577-1579 I3 --- NRPblend1 ?=- Astrometric binary number of BP blended transits (photrpnblendedtransits1) 1581-1583 I3 --- NRPblend2 ?=- Putative tertiary number of BP blended transits (photrpnblendedtransits2) 1585 I1 --- Mode1 [0]? Astrometric binary photometry processing mode (photprocmode1) 1587 I1 --- Mode2 ?=- Putative tertiary photometry processing mode (photprocmode2) 1589-1597 F9.6 mag BP-RP1 ?=- Astrometric binary GP-RP colour (bp_rp1) 1599-1607 F9.6 mag BP-RP2 ?=- Putative tertiary GP-RP colour (bp_rp2) 1609-1617 F9.6 mag BP-G1 ?=- Astrometric binary BP-G colour (bp_g1) 1619-1627 F9.6 mag BP-G2 ?=- Putative tertiary BP-G colour (bp_g2) 1629-1637 F9.6 mag G-RP1 ?=- Astrometric binary G-RP colour (g_rp1) 1639-1647 F9.6 mag G-RP2 ?=- Putative tertiary G-RP colour (g_rp2) 1649-1659 F11.6 km/s RV1 ?=- Astrometric binary radial velocity (radial_velocity1) 1661-1671 F11.6 km/s RV2 ?=- Putative tertiary radial velocity (radial_velocity2) 1673-1681 F9.6 km/s e_RV1 ?=- Astrometric binary RV error (radialvelocityerror1) 1683-1691 F9.6 km/s e_RV2 ?=- Putative tertiary RV error (radialvelocityerror2) 1693 I1 --- n_RV1 ?=- Astrometric binary method used to obtain the radial velocity (rvmethodused1) 1695 I1 --- n_RV2 ?=- Putative tertiary method used to obtain the radial velocity (rvmethodused2) 1697-1699 I3 --- o_RV1 ?=- Astrometric binary number of transits used to compute the radial velocity (rvnbtransits1) 1701-1702 I2 --- o_RV2 ?=- Putative tertiary number of transits used to compute the radial velocity (rvnbtransits2) 1704-1705 I2 --- o_RVd1 ?=- Astrometric binary number of valid transits that have undergone deblending (rvnbdeblended_transits1) 1707-1708 I2 --- o_RVd2 ?=- Putative tertiary number of valid transits that have undergone deblending (rvnbdeblended_transits2) 1710-1711 I2 --- RVNper1 ?=- Astrometric binary number of visibility periods used to estimate the radial velocity (rvvisibilityperiods_used1) 1713-1714 I2 --- RVNper2 ?=- Putative tertiary number of visibility periods used to estimate the radial velocity (rvvisibilityperiods_used2) 1716-1725 F10.5 --- RVS/N1 ?=- Astrometric binary expected signal to noise ratio in the combination of the spectra used to obtain the radial velocity (rvexpectedsigtonoise1) 1727-1736 F10.5 --- RVS/N2 ?=- Putative tertiary expected signal to noise ratio in the combination of the spectra used to obtain the radial velocity (rvexpectedsigtonoise2) 1738-1748 F11.6 --- RVgof1 ?=- Astrometric binary radial velocity renormalised goodness of fit (rvrenormalisedgof1) 1750-1760 F11.6 --- RVgof2 ?=- Putative tertiary radial velocity renormalised goodness of fit (rvrenormalisedgof2) 1762-1769 F8.6 --- RVchi21 ?=- Astrometric binary P-value for constancy based on a chi-squared criterion (rvchisqpvalue1) 1771-1778 F8.6 --- RVchi22 ?=- Putative tertiary P-value for constancy based on a chi-squared criterion (rvchisqpvalue2) 1780-1790 F11.6 d RVTdur1 ?=- Astrometric binary Time coverage of the radial velocity time series (rvtimeduration1) 1792-1800 F9.4 d RVTdur2 ?=- Putative tertiary Time coverage of the radial velocity time series (rvtimeduration2) 1802-1811 F10.6 km/s RVamp1 ?=- Astrometric binary total amplitude in the radial velocity time series after outlier removal (rvamplituderobust1) 1813-1822 F10.6 km/s RVamp2 ?=- Putative tertiary total amplitude in the radial velocity time series after outlier removal (rvamplituderobust2) 1824-1828 I5 K RVtempTeff1 ?=- Astrometric binary Teff of the template used to compute the radial velocity (rvtemplateteff1) 1830-1834 I5 K RVtempTeff2 ?=- Putative tertiary Teff of the template used to compute the radial velocity (rvtemplateteff2) 1836-1843 F8.6 [cm/s2] RVtemplogg1 ?=- Astrometric binary logg of the template used to compute the radial velocity (rvtemplatelogg1) 1845-1847 F3.1 [cm/s2] RVtemplogg2 ?=- Putative tertiary logg of the template used to compute the radial velocity (rvtemplatelogg2) 1849-1857 F9.6 --- RVtemp[Fe/H]1 ?=- Astrometric binary [Fe/H] of the template used to compute the radial velocity (rvtemplatefe_h1) 1859-1867 F9.6 --- RVtemp[Fe/H]2 ?=- Putative tertiary [Fe/H] of the template used to compute the radial velocity (rvtemplatefe_h2) 1869-1871 I3 --- Vatmparam1 ?=- Astrometric binary origin of the atmospheric parameters associated to the template (rvatmparam_origin1) 1873-1875 I3 --- Vatmparam2 ?=- Putative tertiary origin of the atmospheric parameters associated to the template (rvatmparam_origin2) 1877-1885 F9.5 km/s Vbroad1 ?=- Astrometric binary spectral line broadening parameter (vbroad1) 1887-1895 F9.5 km/s Vbroad2 ?=- Putative tertiary spectral line broadening parameter (vbroad2) 1897-1906 F10.6 km/s e_Vbroad1 ?=- Astrometric binary Vbroad error (vbroad_error1) 1908-1917 F10.6 km/s e_Vbroad2 ?=- Putative tertiary Vbroad error (vbroad_error2) 1919-1920 I2 --- o_Vbroad1 ?=- Astrometric binary number of transits used to compute vbroad (vbroadnbtransits1) 1922-1923 I2 --- o_Vbroad2 ?=- Putative tertiary number of transits used to compute vbroad (vbroadnbtransits2) 1925-1932 F8.5 mag GRVSmag1 ?=- Astrometric binary integrated Grvs magnitude (grvs_mag1) 1934-1941 F8.5 mag GRVSmag2 ?=- Putative tertiary integrated Grvs magnitude (grvs_mag2) 1943-1950 F8.6 mag e_GRVSmag1 ?=- Astrometric binary Grvs magnitude uncertainty (grvsmagerror1) 1952-1959 F8.6 mag e_GRVSmag2 ?=- Putative tertiary Grvs magnitude uncertainty (grvsmagerror2) 1961-1963 I3 --- o_GRVSmag1 ?=- Astrometric binary number of transits used to compute Grvs (grvsmagnb_transits1) 1965-1966 I2 --- o_GRVSmag2 ?=- Putative tertiary number of transits used to compute Grvs (grvsmagnb_transits2) 1968-1975 F8.4 --- RVSS/N1 ?=- Astrometric binary signal to noise ratio in the mean RVS spectrum (rvsspecsigtonoise1) 1977-1984 F8.4 --- RVSS/N2 ?=- Putative tertiary signal to noise ratio in the mean RVS spectrum (rvsspecsigtonoise2) 1986-2000 F15.11 deg GLON1 Astrometric binary galactic longitude (l1) 2002-2016 F15.11 deg GLON2 Putative tertiary galactic longitude (l2) 2018-2032 F15.11 deg GLAT1 Astrometric binary galactic latitude (b1) 2034-2048 F15.11 deg GLAT2 Putative tertiary galactic latitude (b2) 2050-2064 F15.11 deg ELON1 Astrometric binary ecliptic longitude (ecl_lon1) 2066-2080 F15.11 deg ELON2 Putative tertiary galactic longitude (ecl_lon2) 2082 I1 --- QSO1 [0,1] Astrometric binary flag indicating the availability of additional information in the QSO candidates table (inqsocandidates1) 2084 I1 --- QSO2 [0,1] Putative tertiary flag indicating the availability of additional information in the QSO candidates table (inqsocandidates2) 2086 I1 --- Gal1 [0,1] Astrometric binary flag indicating the availability of additional information in the galaxy candidates table (ingalaxycandidates1) 2088 I1 --- Gal2 [0,1] Putative tertiary flag indicating the availability of additional information in the galaxy candidates table (ingalaxycandidates2) 2090 I1 --- NSS1 ?=- Astrometric binary flag indicating the availability of additional information in the various Non-Single Star tables (nonsinglestar1) 2092 I1 --- NSS2 ?=- Putative tertiary flag indicating the availability of additional information in the various Non-Single Star tables (nonsinglestar2) 2094 I1 --- XPcont1 [0,1] Astrometric binary flag indicating the availability of mean BP/RP spectrum (hasxpcontinuous1) 2096 I1 --- XPcont2 [0,1] Putative tertiary flag indicating the availability of mean BP/RP spectrum (hasxpcontinuous2) 2098 I1 --- XPsamp1 [0,1] Astrometric binary flag indicating the availability of mean BP/RP spectrum (hasxpsampled1) 2100 I1 --- XPsamp2 [0,1] Putative tertiary flag indicating the availability of mean BP/RP spectrum (hasxpsampled2) 2102 I1 --- RVS1 [0,1] Astrometric binary flag indicating the availability of mean RVS spectrum (has_rvs1) 2104 I1 --- RVS2 [0,1] Putative tertiary flag indicating the availability of mean RVS spectrum (has_rvs2) 2106 I1 --- EpochPh1 [0,1] Astrometric binary flag indicating the availability of epoch photometry (hasepochphotometry1) 2108 I1 --- EpochPh2 [0,1] Putative tertiary flag indicating the availability of epoch photometry (hasepochphotometry2) 2110 I1 --- EpochRV1 [0,1] Astrometric binary flag indicating the availability of epoch radial velocity (hasepochrv1) 2112 I1 --- EpochRV2 [0,1] Putative tertiary flag indicating the availability of epoch radial velocity (hasepochrv2) 2114 I1 --- MCMCGSP1 [0,1] Astrometric binary flag indicating the availability of GSP-Phot MCMC samples (hasmcmcgspphot1) 2116 I1 --- MCMCGSP2 [0,1] Putative tertiary flag indicating the availability of GSP-Phot MCMC samples (hasmcmcgspphot2) 2118 I1 --- MCMCMSC1 [0,1] Astrometric binary flag indicating the availability of MSC MCMC samples for this source (hasmcmcmsc1) 2120 I1 --- MCMCMSC2 [0,1] Putative tertiary flag indicating the availability of MSC MCMC samples for this source (hasmcmcmsc2) 2122 I1 --- And1 [0,1] Astrometric binary flag indicating that the source is present in the Gaia Andromeda Photometric Survey (GAPS) (inandromedasurvey1) 2124 I1 --- And2 [0,1] Putative tertiary flag indicating that the source is present in the Gaia Andromeda Photometric Survey (GAPS) (inandromedasurvey2) 2126-2137 E12.6 --- PQSO1 Astrometric binary probability of being a galaxy (classprobdsccombmod_quasar1) 2139-2150 E12.6 --- PQSO2 ?=- Putative tertiary probability of being a QSO (classprobdsccombmod_quasar2) 2152-2163 E12.6 --- PGal1 Astrometric binary probability of being a QSO (classprobdsccombmod_galaxy1) 2165-2176 E12.6 --- PGal2 ?=- Putative tertiary probability of being a galaxy (classprobdsccombmod_galaxy2) 2178-2189 E12.6 --- PSS1 Astrometric binary probability of being a single star (classprobdsccombmod_star1) 2191-2202 E12.6 --- PSS2 ?=- Putative tertiary probability of being a single star (classprobdsccombmod_star2) 2204-2211 F8.2 K Teff1 ?=- Astrometric binary effective temperature (teff_gspphot1) 2213-2220 F8.2 K Teff2 ?=- Putative tertiary effective temperature (teff_gspphot2) 2222-2229 F8.2 K b_Teff1 ?=- Astrometric binary lower error in Teff (teffgspphotlower1) 2231-2238 F8.2 K b_Teff2 ?=- Putative tertiary lower error in Teff (teffgspphotlower2) 2240-2247 F8.2 K B_Teff1 ?=- Astrometric binary upper error in Teff (teffgspphotupper1) 2249-2256 F8.2 K B_Teff2 ?=- Putative tertiary upper error in Teff (teffgspphotupper2) 2258-2263 F6.4 [cm/s2] logg1 ?=- Astrometric binary surface gravity (logg_gspphot1) 2265-2270 F6.4 [cm/s2] logg2 ?=- Putative tertiary surface gravity (logg_gspphot2) 2272-2277 F6.4 [cm/s2] b_logg1 ?=- Astrometric binary lower error in logg (logggspphotlower1) 2279-2284 F6.4 [cm/s2] b_logg2 ?=- Putative tertiary lower error in logg (logggspphotlower2) 2286-2291 F6.4 [cm/s2] B_logg1 ?=- Astrometric binary upper error in logg (logggspphotupper1) 2293-2298 F6.4 [cm/s2] B_logg2 ?=- Putative tertiary upper error in logg (logggspphotupper2) 2300-2308 F9.6 --- [Fe/H]1 ?=- Astrometric binary iron abundance (mh_gspphot1) 2310-2318 F9.6 --- [Fe/H]2 ?=- Putative tertiary iron abundance (mh_gspphot2) 2320-2328 F9.6 --- b_[Fe/H]1 ?=- Astrometric binary lower error in [Fe/H] (mhgspphotlower1) 2330-2338 F9.6 --- b_[Fe/H]2 ?=- Putative tertiary lower error in [Fe/H] (mhgspphotlower2) 2340-2348 F9.6 --- B_[Fe/H]1 ?=- Astrometric binary upper error in [Fe/H] (mhgspphotupper1) 2350-2358 F9.6 --- B_[Fe/H]2 ?=- Putative tertiary upper error in [Fe/H] (mhgspphotupper2) 2360-2368 F9.4 pc Dist1 ?=- Astrometric binary distance (distance_gspphot1) 2370-2379 F10.4 pc Dist2 ?=- Putative tertiary distance (distance_gspphot2) 2381-2389 F9.4 pc b_Dist1 ?=- Astrometric binary lower error in Dist (distancegspphotlower1) 2391-2400 F10.4 pc b_Dist2 ?=- Putative tertiary lower error in Dist (distancegspphotlower2) 2402-2410 F9.4 pc B_Dist1 ?=- Astrometric binary upper error in Dist (distancegspphotupper1) 2412-2421 F10.4 pc B_Dist2 ?=- Putative tertiary upper error in Dist (distancegspphotupper2) 2423-2430 F8.6 mag A01 ?=- Astrometric binary monochromatic extinction A_0 at 547.7nm (azero_gspphot1) 2432-2439 F8.6 mag A02 ?=- Putative tertiary monochromatic extinction A_0 at 547.7nm (azero_gspphot2) 2441-2448 F8.6 mag b_A01 ?=- Astrometric binary lower error in A01 (azerogspphotlower1) 2450-2457 F8.6 mag b_A02 ?=- Putative tertiary lower error in A0 (azerogspphotlower2) 2459-2464 F6.4 mag B_A01 ?=- Astrometric binary upper error in A0 (azerogspphotupper1) 2466-2471 F6.4 mag B_A02 ?=- Putative tertiary upper error in A0 (azerogspphotupper2) 2473-2480 F8.6 mag AG1 ?=- Astrometric binary extinction in G band (ag_gspphot1) 2482-2489 F8.6 mag AG2 ?=- Putative tertiary extinction in G band (ag_gspphot2) 2491-2498 F8.6 mag b_AG1 ?=- Astrometric binary lower error in AG (aggspphotlower1) 2500-2507 F8.6 mag b_AG2 ?=- Putative tertiary lower error in AG (aggspphotlower2) 2509-2514 F6.4 mag B_AG1 ?=- Astrometric binary upper error in AG (aggspphotupper1) 2516-2521 F6.4 mag B_AG2 ?=- Putative tertiary upper error in AG (aggspphotupper2) 2523-2530 F8.6 mag E(BP-RP)1 ?=- Astrometric binary reddening E(GBP-GRP) (ebpminrp_gspphot1) 2532-2539 F8.6 mag E(BP-RP)2 ?=- Putative tertiary reddening E(GBP-GRP) (ebpminrp_gspphot2) 2541-2548 F8.6 mag b_E(BP-RP)1 ?=- Astrometric binary lower error in E(BP-RP) (ebpminrpgspphotlower1) 2550-2557 F8.6 mag b_E(BP-RP)2 ?=- Putative tertiary lower error in E(BP-RP) (ebpminrpgspphotlower2) 2559-2564 F6.4 mag B_E(BP-RP)1 ?=- Astrometric binary upper error in E(BP-RP) (ebpminrpgspphotupper1) 2566-2571 F6.4 mag B_E(BP-RP)2 ?=- Putative tertiary upper error in E(BP-RP) (ebpminrpgspphotupper2) 2573-2576 A4 --- BinType Binary type (binary_type) 2578-2585 F8.5 --- Plx1.5par1 Astrometric binary parallax*1.5 (parallax1_5par) 2587-2594 F8.6 --- e_Plx1.5par1 Astrometric binary parallax*1.5 error (parallaxerror15par) 2596-2603 F8.5 --- Plx1.5par2 Putative tertiary parallax*1.5 (parallax2_5par) 2605-2612 F8.6 --- e_Plx1.5par2 Putative tertiary Parallax*1.5 error (parallaxerror25par) 2614-2624 A11 --- SolType2 Astrometric binary solution type (sol_type2) 2626-2635 A10 --- SolType1 Putative tertiary solution type (sol_type1) 2637-2646 F10.6 --- GoF1 Astrometric binary Goodness of fit (goodnessoffit1) 2648-2656 F9.6 --- GoF2 ?=- Putative tertiary Goodness of fit (goodnessoffit2) -------------------------------------------------------------------------------- History: Copied at https://zenodo.org/records/12791391
(End) Patricia Vannier [CDS] 25-Jul-2025
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line