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<ri:Resource created="2024-04-10T08:10:26Z" 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>SRG/eROSITA all-sky survey coronal content</title><shortName>J/A+A/684/A121</shortName><identifier>ivo://CDS.VizieR/J/A+A/684/A121</identifier><altIdentifier>doi:10.26093/cds/vizier.36840121</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Freund S.</name></creator><creator><name>Czesla S.</name></creator><creator><name>Predehl P.</name></creator><creator><name>Robrade J.</name></creator><creator><name>Salvato M.</name></creator><creator><name>Schneider P.C.,Starck H.</name></creator><creator><name>Wolf J.</name></creator><creator><name>Schmitt J.H.M.M.</name></creator><date role="Updated">2024-11-29T20:01:32Z</date><date role="Created">2024-04-10T08:10:26Z</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>x-ray-sources</subject><subject>late-type-stars</subject><subject>astronomical-object-identification</subject><description>The first eROSITA all-sky survey (eRASS1) performed onboard of the Spectrum-Roentgen-Gamma mission (SRG) provides more than 900000 X-ray sources in the 0.2-2.3keV band located in the western hemisphere. We present identifications of the eRASS1 sources obtained using our HamStar method, which was designed for the identification of coronal X-ray sources. HamStar is a Bayesian framework that estimates coronal probabilities for each eRASS1 source based on a cross-match with optical counterparts from Gaia DR3. It considers geometric properties, such as the angular separation and positional uncertainty, as well as additional properties namely the fractional X-ray flux, color, and distance. We identify 138800 coronal eRASS1 sources and estimate a completeness and reliability of about 91.5% for this sample, which we confirmed with Chandra detections. This is the largest available sample of coronal X-ray emitters and we find nearly five times as many coronal sources as in the ROSAT all-sky survey. The coronal eRASS1 sources are made up sources of all spectral types and the onset of convection and the saturation limit are clearly visible. As opposed to previous samples, rare source types are also well populated. About 10% of the coronal eRASS1 sources have a correlated secondary counterpart, which is a wide binary companion or belongs to the same stellar cluster. We also identify 6700 known unresolved binaries, and an excess of fast binary periods below 10d. Furthermore, the binary sequence is clearly visible in a color-magnitude diagram. When combining the coronal eRASS1 sources with rotation modulations from Gaia DR3, we find 3700 X-ray sources with known rotation periods, which is the largest sample of this kind. We fitted the rotation-activity relation and convection turnover times for our flux limited sample. We do not detect the low-amplitude fast rotators discovered in the Gaia DR3 sample in X-rays.</description><source format="bibcode">2024A&amp;A...684A.121F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/684/A121</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/355">I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/482/A34">J/A+A/482/A34 : SRG/eROSITA all-sky survey catalogs (eRASS1) (Merloni+, 2024)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/684/A121</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/684/A121</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/684/A121</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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28301-28304 28307-28309 28313-28315 28320-28322 28324-28326 28328-28329 28331 28344-28346 28364 28366-28367 28372 28374-28376 28378-28379 28384 28386-28387 28393-28398 28409-28411 28413 28437 28439 28441-28442 28445 28447 28456-28457 28459 28464-28465 28467-28469 28471 28477-28479 28489-28492 28494-28495 28504 28506 28513 28515 28520-28521 28523 28525-28526 28528 28545-28548 28550-28553 28555 28568 28570-28571 28573-28575 28577-28582 28585-28587 28589-28593 28595 28597-28602 28614 28620 28641-28643 28648 28732-28734 28744-28746 28768 28820 28822 28828 28830 28856 28858 29200 29202 29208 29228-29230 29324 29326 29348 29350 29356 29358 30720-30722 30728-30730 30753-30755 31232 31234-31235 31398 32769-32771 32808 32810-32811 33344-33346 33532-33534 33724-33725 33727 33776-33777 33779 34444-34446 34504-34506 34753-34755 34772-34774 34789-34791 34840-34841 34843-34844 34846-34847 34853-34855 34861-34863 34888-34890 34896-34897 34899-34902 34924-34925 34927 34964-34966 34996-34998 35000 35002-35003 35025-35027 35080-35081 35083 35100 35102-35103 35132 35134-35135 35165-35166 35184-35186 35204-35206 35212-35214 35264-35265 35267 35277-35279 35293-35295 35305-35307 35340-35341 35345-35347 35364-35365 35373-35378 35408-35409 35411 35413-35415 35441-35443 35460-35462 35473-35475 35477-35478 35484 35486-35487 35492-35493 35495 35500-35502 35504 35506-35507 35520 35522-35523 35528-35530 35536 35538-35540 35542-35543 35554-35557 35559-35562 35577-35579 35581-35583 35600 35602-35603 35608-35609 35611 35617-35619 35636-35637 35639 35648-35649 35651 35672-35673 35675 35712 35714-35716 35718-35719 35729-35731 35744 35746-35747 35752-35753 35755 35765-35766 35781-35783 35788-35789 35791-35794 35804 35806-35807 35816 35818 35829-35834 35836-35837 35869-35871 35972-35974 35976-35978 36012-36014 36041-36043 36065-36067 36080-36082 36140-36141 36143 36165-36167 36204 36206-36207 36273-36275 36384 36386-36387 36389-36391 36453-36455 36468-36470 36472 36474-36475 36505-36507 36517-36521 36524 36536 36545-36547 36552-36554 36564-36565 36567 36580 36688-36690 36744 36746-36747 36784-36786 36788-36789 36791 38604-38606 38644 38646-38647 38860 38862-38863 38880-38881 38883 40264 40266-40267 40273-40275 40352-40354 40372-40373 40375 40404-40406 40440-40442 40444-40446 40808-40809 40811 40840-40841 40843 40929-40931 40946-40947 40949-40951 42008-42010 42052-42054 43516 43518-43519 43972 43974 44113-44115 44189-44191 44256 44258-44259 44337-44339 44380-44382 44412 44414-44415 44424-44426 44444-44446 44464-44465 44467-44470 44472-44474 44488 44490-44491 44500-44502 44561-44563 44704 44706-44707 44732-44734 44756-44757 44759 44828-44830 44848 44850-44851 44853-44855 44864-44866 44896-44897 44899 44904 44906-44907 44932-44933 44935-44936 44938-44939 44980-44982 44984-44986 45032 45034-45035 45120-45122 45152 45154-45155 45180 45182-45183 45356-45357 45359-45361 45363 45369-45374 45420-45421 45423 45432 45434-45435 45453-45455 45504-45505 45507 45528 45530-45531 45548-45549 45551 45560-45561 45584-45585 45587 45605-45607 45612-45613 45615 45640-45641 45643 45784-45786 45825-45827 45836 45838-45840 45842-45843 45873-45876 45878-45879 45904-45905 45907 45925-45927 45929-45931 45944-45946 45948-45949 45951 45960 45962-45963 45996-45997 45999 46012 46014-46015 46017-46021 46023 46061-46063 46096 46098-46099 46105-46107 46116-46117 46119-46121 46123 46133 46135 46137-46139 46164 46166-46170 46172 46174-46177 46179 46220-46221 46223 46225 46227 46236 46238-46239 46241-46243 46272-46273 46275 46281-46283 46292 46294-46295 46308 46310-46311 46320-46321 46323-46325 46327 46334 46377-46379 46384 46386-46387 46404 46406-46407 46409-46411 46417 46419-46422 46428-46430 46440-46441 46443-46446 46448 46450-46451 46460 46462-46463 46484-46485 46487 46500-46501 46503 46505-46507 46513 46515-46516 46520 46529-46531 46540 46548 46560 46600-46601 46603 46632-46634 46640-46641 46643 46668 46670-46671 46680-46682 46684-46685 46688 46690-46694 46696-46698 46736-46738 46740-46741 46743-46744 46746 46756-46758 46760 46762 46849-46850 47108-47110 47225-47227 47368 47370-47371 47384-47385 47387 47398-47399 47440 47442-47444 47446-47447 47457-47459 47461-47462 47464-47466 47472 47516-47518 47536-47538 47544 47552 47648 47650-47651 47688-47690 47692-47694 47716 47718-47719 47740 47742 47756-47758 47828 47832-47834 47852-47854 47876 47878 47880-47882 47904</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/684/A121?format=ascii</footprint><waveband>X-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/684/A121/like_ctp</name><description>Likely coronal identifications of the eRASS1 main sources</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>ERO</name><description>IAU name of the eRASS1 source (ERO_IAUNAME)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>MJD</name><description>[58828.93/59011.42] Epoch of the observation of the eRASS1 source (ERO_MJD)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag></column><column><name>ePos</name><description>Positional uncertainty of the eRASS1 source (ERO_POS_ERR)</description><unit>arcsec</unit><ucd>stat.error;pos</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CtpRank</name><description>[1/4] Rank of the counterpart that increase for less likely alternative counterparts (CTP_RANK)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CtpId</name><description>Identifier of the counterpart (CTP_ID) (1)</description><ucd>meta.id</ucd></column><column><name>CtpSep</name><description>Proper motion corrected angular separation between eRASS1 source and counterpart (CTP_SEP) (2)</description><unit>arcsec</unit><ucd>pos.pm;pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p-coronal</name><description>[0/1] Probability of the eRASS1 source to be coronal (p_coronal)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p-ij</name><description>[0/1] Probability of the counterpart to be associated to the eRASS1 source (p_ij)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RAJ2000</name><description>Proper motion corrected right ascension of the counterpart adopting the observation time of the eRASS1 source as provided by ERO_MJD, J2000 (RAdeg)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Proper motion corrected declination of the counterpart adopting the observation time of the eRASS1 source as provided by ERO_MJD, J2000 (DEdeg)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>FX</name><description>X-ray flux in the 0.2-2.3keV band assuming a coronal spectrum (Fx)</description><unit>mW.m**-2</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Gmag</name><description>G band magnitude of the counterpart (Gmag)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FlagOpt</name><description>[0/1] 1 if the source is affected by optical loading (FLAG_OPT)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NWAYDCtp</name><description>[0/1] 1 if NWAY provides a different best counterpart (NWAY_DIFFCTP)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BP-RP</name><description>BP-RP color of the counterpart (BP-RP)</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>plx</name><description>Parallax of the counterpart (plx)</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SName</name><description>Name of the Simbad identification if available (SIMBAD_NAME)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="40*">char</dataType></column><column><name>SOType</name><description>Classification in the Simbad database if available (SIMBAD_OTYPE)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>TrainSet</name><description>[0/1] 1 if counterpart to an eRASS:4 training set source (TRAIN_SET)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Coronal</name><description>[0/1] 0 if the properties are untypical for coronal X-ray emitters (CORONAL)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>OB-Star</name><description>[0/1] 1 for likely reddened OB stars (OB_STAR)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/A+A/684/A121/pos_ctp</name><description>Possible but less likely coronal identifications of the eRASS1 main sources</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>ERO</name><description>IAU name of the eRASS1 source (ERO_IAUNAME)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>MJD</name><description>[58828.93/59011.42] Epoch of the observation of the eRASS1 source (ERO_MJD)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag></column><column><name>ePos</name><description>Positional uncertainty of the eRASS1 source (ERO_POS_ERR)</description><unit>arcsec</unit><ucd>stat.error;pos</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CtpRank</name><description>[1/4] Rank of the counterpart that increase for less likely alternative counterparts (CTP_RANK)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CtpId</name><description>Identifier of the counterpart (CTP_ID) (1)</description><ucd>meta.id</ucd></column><column><name>CtpSep</name><description>Proper motion corrected angular separation between eRASS1 source and counterpart (CTP_SEP) (2)</description><unit>arcsec</unit><ucd>pos.pm;pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p-coronal</name><description>[0/1] Probability of the eRASS1 source to be coronal (p_coronal)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p-ij</name><description>[0/1] Probability of the counterpart to be associated to the eRASS1 source (p_ij)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RAJ2000</name><description>Proper motion corrected right ascension of the counterpart adopting the observation time of the eRASS1 source as provided by ERO_MJD, J2000 (RAdeg)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Proper motion corrected declination of the counterpart adopting the observation time of the eRASS1 source as provided by ERO_MJD, J2000 (DEdeg)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>FX</name><description>X-ray flux in the 0.2-2.3keV band assuming a coronal spectrum (Fx)</description><unit>mW.m**-2</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Gmag</name><description>G band magnitude of the counterpart (Gmag)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BP-RP</name><description>BP-RP color of the counterpart (BP-RP)</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>plx</name><description>Parallax of the counterpart (plx)</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SName</name><description>Name of the Simbad identification if available (SIMBAD_NAME)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="40*">char</dataType></column><column><name>SOType</name><description>Classification in the Simbad database if available (SIMBAD_OTYPE)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>TrainSet</name><description>[0/1] 1 if counterpart to an eRASS:4 training set source (TRAIN_SET)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Coronal</name><description>[0/1] 0 if the properties are untypical for coronal X-ray emitters (CORONAL)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>OB-Star</name><description>[0/1] 1 for likely reddened OB stars (OB_STAR)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FlagOpt</name><description>[0/1] 1 if the source is affected by optical loading (FLAG_OPT)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NWAYDCtp</name><description>[0/1] 1 if NWAY provides a different best counterpart (NWAY_DIFFCTP)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>