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<ri:Resource created="2022-10-07T09:24:42Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Sagittarius stream with eDR3</title><shortName>J/A+A/666/A64</shortName><identifier>ivo://CDS.VizieR/J/A+A/666/A64</identifier><altIdentifier>doi:10.26093/cds/vizier.36660064</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ramos P.</name></creator><creator><name>Antoja T.</name></creator><creator><name>Yuan Z.</name></creator><creator><name>Arentsen A.</name></creator><creator><name>Oria P.-A.</name></creator><creator><name>Famaey B.</name></creator><creator><name>Ibata R.,Mateu C.</name></creator><creator><name>Carballo-Bello J.A.</name></creator><date role="Updated">2022-10-10T15:04:50Z</date><date role="Created">2022-10-07T09:24:42Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>galaxies</subject><subject>stellar-populations</subject><subject>visible-astronomy</subject><description>The Sagittarius dwarf spheroidal (Sgr) is a dissolving galaxy being tidally disrupted by the Milky Way (MW). Its stellar stream still poses serious modelling challenges, which hinders our ability to use it effectively as a prospective probe of the MW gravitational potential at large radii. Our goal is to construct the largest and most stringent sample of stars in the stream with which we can advance our understanding of the Sgr-MW interaction, focusing on the characterisation of the bifurcations. We improved on previous methods based on the use of the wavelet transform to systematically search for the kinematic signature of the Sgr stream throughout the whole sky in the Gaia data. We then refined our selection via the use of a clustering algorithm on the statistical properties of the colour-magnitude diagrams. Our final sample contains more than 700000 candidate stars and is three times larger than previous Gaia samples. With it, we have been able to detect the bifurcation of the stream in both the northern and southern hemispheres, which requires four branches (two bright and two faint) to fully describe the system. We present the detailed proper motion distribution of the trailing arm as a function of the angular coordinate along the stream, showing, for the first time, the presence of a sharp edge (on the side of the small proper motions) beyond which there are no Sgr stars. We also characterise the correlation between kinematics and distance. Finally, the chemical analysis of our sample shows that the faint branch of the bifurcation is more metal poor than the bright. We provide analytical descriptions for the proper motion trends as well as for the sky distribution of the four branches of the stream. Based on our analysis, we interpret the bifurcations as a misaligned overlap of the material stripped at the antepenultimate pericentre (faint branches) with the stars ejected at the penultimate pericentre (bright branch), given that Sgr just went through its perigalacticon. The source of this misalignment is still unknown, but we argue that models with some internal rotation in the progenitor - at least during the time of stripping of the stars that are now in the faint branches - are worth exploring</description><source format="bibcode">2022A&amp;A...666A..64R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/666/A64</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 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46679 46682 46691-46692 46695 46700-46702 46722 46726 46728-46730 46735 46737 46740 46742-46743 46754 46758 46761-46763 46765-46769 46771 46777-46779 46789-46791 46849 46851 46853-46855 46857-46859 46865-46866 46868 46870 46888-46890 46893-46895 46944-46945 46947 47080 47082-47083 47183 47187-47190 47192 47195 47197-47198 47203-47204 47217 47224 47228 47230 47286 47289 47291 47293 47298 47302 47305 47307 47312 47316 47321-47322 47328-47329 47341 47345 47360-47361 47366 47368-47369 47371 47374-47376 47379 47382 47387-47388 47390-47391 47393-47394 47399 47401 47408 47410-47412 47414-47416 47418 47420 47426-47427 47436 47439 47442 47444 47446-47447 47450-47451 47453-47455 47458-47459 47461 47463-47464 47467-47469 47471 47491 47510-47512 47514 47518-47519 47523 47536 47539 47541-47542 47545 47547 47553-47555 47585-47587 47618 47631 47638 47640 47666 47681 47742 47744 47747 47783 47809 47819-47820 47829 47831 47835 47841 47848 47858 47865 47867 47874 47877 47885 47887 47889 47891 47909-47913 47915 47936 47938-47939 47980-47981 47983-47984 47986-47987 47992 48052 48054-48055 48060 48080-48081 48093 48096 48103 48128 48131 48137-48139 48232-48233 48235 48308 48310-48311 48316-48317 48319-48320 48322-48323 48328-48329 48331-48334 48344 48346-48347 48353-48358 48360-48362 48364 48366-48367 48369-48373 48376-48377 48383 48429-48433 48435 48444 48446-48447 48456-48457 48459 48476 48478-48479 48493-48494 48497 48500-48501 48503 48508 48512-48514 48520 48524 48527-48530 48532 48536-48537 48539-48540 48544 48546-48547 48549-48551 48555 48557 48572-48573 48576 48578 48583-48584 48588-48589 48594 48597-48598 48604 48607 48616 48620 48622-48623 48639 48648-48650 48653 48655 48660 48662 48668 48672 48676 48681 48705 48707 48713 48725 48728 48731 48746-48747 48753 48756-48757 48763 48808 48910 48912 48918-48919 48921 48924 48926 48942-48943 48951-48952 48955 48958 48962 48967-48968 48977 48980 48985 49013 49024 49035 49037 49041 49074 49081-49082 49086 49088 49091 49097 49106 49115 49124</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/666/A64?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/666/A64/tablec1</name><description>Candidate stars in the Sagittarius stream from the Gaia eDR3 sample</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SNRgLAMOST</name><description>? Signal to noise in g-band (LAMOST) (snrg_LAMOST)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNRSEGUE</name><description>? Signal to noise (SEGUE) (SNR_SEGUE)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ProbBright</name><description>Probability to belong to bright arm (Prob_bright)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ProbFaint</name><description>Probability to belong to faint arm (Prob_faint)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ProbSGR</name><description>Probability to belong to the stream (Prob_sgr)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ProbPlx</name><description>Parallax score (Prob_plx)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) at Epoch=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) at Epoch=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>GaiaEDR3</name><description>Gaia eDR3 Unique source identifier (source_id)</description><ucd>meta.id;meta.main</ucd></column><column><name>Gmag</name><description>G-band mean magnitude (phot_g_mean_mag)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>BP-RP</name><description>G_BP_ minus G_RP_ colour (bp_rp)</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RA_ICRS</name><description>Right ascension (ICRS) at Ep=2015.5 (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Ep=2015.5 (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>pmRA</name><description>Proper motion in right ascension direction (J2015.5) (pmra)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>pmDE</name><description>Proper motion in declination direction (J2015.5) (pmdec)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_pmRA</name><description>Error in pmRA (pmra_error)</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pmDE</name><description>Error in pmDE (pmdec_error)</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DistWGBPRP</name><description>? Photometric distance (only RR Lyrae.) (Dist_WGBPRP)</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_DistWGBPRP</name><description>? Error in distance (only RR Lyrae) (Dist_WGBPRP_err)</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Vlos</name><description>? Line of sight velocity (vlos)</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>r_Vlos</name><description>Source of the radal velocity (vlos_source)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>[Fe/H]APOGEE</name><description>? Metallicity from APOGEE (FEH_APOGEE)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[alpha/M]APOGEE</name><description>? Alpha over iron from APOGEE (ALPHA_M_APOGEE)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Fe/H]LAMOST</name><description>? Metallicity from LAMOST (FEH_LAMOST)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]SEGUE</name><description>? Metallicity from SEGUE (FEH_SEGUE)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNRAPOGEE</name><description>? Signal to noise (APOGEE, SNREV) (SNR_APOGEE)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>