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<ri:Resource created="2021-12-07T16:20:24Z" 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>Bayesian Ages For Field LowEr-mass Stars</title><shortName>J/ApJ/898/27</shortName><identifier>ivo://CDS.VizieR/J/ApJ/898/27</identifier><altIdentifier>doi:10.26093/cds/vizier.18980027</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Stanford-Moore S.A.</name></creator><creator><name>Nielsen E.L.</name></creator><creator><name>De Rosa R.J.</name></creator><creator><name>Macintosh B.</name></creator><creator><name>Czekala I.</name></creator><date role="Updated">2022-10-04T11:53:01Z</date><date role="Created">2021-12-07T16:20:24Z</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>stellar-ages</subject><subject>stellar-spectral-types</subject><subject>visible-astronomy</subject><description>Age is a fundamental parameter of stars, yet in many cases, ages of individual stars are presented without robust estimates of the uncertainty. We have developed a Bayesian framework, BAFFLES, to produce the age posterior for a star from its calcium emission strength (log(R_HK_^'^)) or lithium abundance (Li EW) and B-V color. We empirically determine the likelihood functions for calcium and lithium as functions of age from literature measurements of stars in benchmark clusters with well-determined ages. We use a uniform prior on age, which reflects a uniform star formation rate. The age posteriors we derive for several test cases are consistent with literature ages found from other methods. BAFFLES represents a robust method to determine the age posterior probability distribution for any field star with 0.45&lt;=B-V0.9 and a measurement of R_HK_^'^ and/or 0.35&lt;=B-V&lt;=1.9 and measured Li EW. We compile colors, R_HK_^'^, and Li EW from over 2630 nearby field stars from the literature, and present the derived BAFFLES age posterior for each star.</description><source format="bibcode">2020ApJ...898...27S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/898/27</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/II/122">II/122 : UBV Photoelectric Catalog: data 1953-1985 (Mermilliod 1987)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/150">III/150 : Perkins Revised MK Types for the Cooler Stars (Keenan+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/159">III/159 : Ca II H and K Measurements Made at MWO (Duncan+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/284">I/284 : The USNO-B1.0 Catalog (Monet+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/322">I/322 : UCAC4 Catalogue (Zacharias+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/106/1059">J/AJ/106/1059 : Lithium in the Pleiades (Soderblom+, 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/111/439">J/AJ/111/439 : Chromospheric emission in late-type stars. 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39321 39362 39364 39377 39403 39422 39464 39487 39490 39500 39543 39557 39562 39566 39568 39583 39646 39654 39674 39676 39693 39709 39730 39735 39744 39767 39808 39841 39853 39861 39864 39866 39888 39926 39948 39950 39988 40000 40012 40021 40030 40054 40085 40101 40105 40220 40242 40271 40276 40400 40426 40442 40453 40679 40704 40716 40739 40784 40823 40892 40921 40932 40968 40970 40981 40985 41055 41062 41089 41094 41136 41163 41165 41167 41194 41210 41221 41225 41259 41272 41290 41295 41319 41323 41336 41371 41393 41399 41412 41424 41427 41429 41432 41441 41446 41450 41453 41468 41481 41528 41549 41553 41556-41557 41562 41570 41588 41590 41607 41610 41625 41631 41648 41678 41708 41721 41723-41724 41798 41861 41873 41935 41941 41965 41969 41972 41980 41984 41990-41991 42009 42042-42043 42053 42063 42070 42091 42093 42096 42102 42115 42143 42146 42151 42156-42157 42174 42200 42205 42221 42228 42238 42285 42287 42319 42355 42360 42438 42448 42458 42460-42461 42463 42468 42479 42519 42559 42563 42588 42596 42602 42618 42620 42622 42632 42634 42637 42656 42662 42700 42708 42710 42751 42759-42760 42794 42837 42857 42864 42869 42874 42887 42889-42890 42892 42899 42911 42918 42921 42933-42934 42979 43012 43017 43023 43047 43051 43072 43074 43136 43153 43167 43171 43193 43209 43228 43233 43240 43258 43277 43282 43290 43296 43315 43318 43329 43331-43332 43387 43426 43458 43468 43473 43484 43518 43538 43540 43555-43556 43571 43639 43649-43650 43655 43663 43668 43670 43676-43677 43680 43687 43698-43699 43708 43710 43714 43724 43738 43774 43782 43797 43803-43804 43822 43844 43856 43858 43892 43902 43910-43912 43944 43977 43989 44006 44010 44013 44045 44054 44078 44096 44113 44115 44131 44136 44183 44195 44212 44220 44223 44226 44228 44286 44292 44316 44323 44368 44398 44401 44410-44411 44435 44507 44549 44557 44573 44591 44669 44740 44753 44761 44792 44871 44887 44891 44909 44920 44924 44931 44935 44956 44981 45029 45034 45062 45107 45112 45121 45135 45137 45175 45196 45237-45238 45241 45253 45258 45272 45299 45309 45337 45351 45382 45388 45396 45420 45430 45444 45458 45472 45485 45511 45527 45541 45544 45551 45621 45627 45646 45653-45654 45668 45673 45687 45770 45799 45811 45834 45843 45865 45874 45892 45917 45927 45929 45941 45944 45948 45956 45986 45992 46022 46040 46056 46065 46076 46080 46083 46100-46101 46113 46129 46135 46145 46160 46170 46172 46234 46247-46248 46263 46277 46297 46306 46320 46325 46333 46342 46363 46467 46472-46473 46481-46482 46484 46488 46501 46523 46526 46551 46581 46593 46603 46626-46627 46640 46654-46655 46682 46685 46728 46734 46750 46765 46767-46768 46777 46790 46800 46820 46843 46874 46916 46922-46923 46944 46967 46977 46982 46987 46991-46992 46998 47001 47020 47027 47045 47073 47107 47114 47120 47127 47133 47137 47176 47183 47198 47205 47232 47234-47235 47274 47279 47287 47292 47311 47377 47385 47429-47430 47461 47463 47502 47543 47550 47576 47584 47598 47606 47638 47663 47702 47706 47730 47742 47754 47780 47791 47824 47842 47858 47863 47873 47894 47904 47910 47918-47919 47930 47935 47943 47945 47949 47953 47959 47975 47985 47991 48004 48007 48014-48015 48019 48022 48065 48082 48104-48105 48119-48120 48172 48176 48182 48199 48202 48212 48223 48230 48249 48254 48259 48274 48283 48291 48305 48334-48335 48373 48394 48402 48414 48545 48583 48607 48658 48672 48705 48736 48757 48773 48785 48807 48821 48862 48883 48905 48915 48943 48955 48967 48980 49026 49064 49084 49089 49097 49118 49128</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/898/27?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/898/27/table2</name><description>BAFFLES ages for nearby stars</description><column><name>SpType</name><description>Spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Ref</name><description>Reference code(s) (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType><flag>nullable</flag></column><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>ID</name><description>Source identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>B-V</name><description>[0.45/1.74] The (B-V) color index</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logRHK</name><description>[-5/-3.7]? log calcium emission strength index; logR'_HK_</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EW</name><description>[-3.3/570]? Lithum equivalent width; in milli-Angstrom units</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>2.5Age1</name><description>[1.8/2850]? R'_HK_ age 2.5% posterior CDF value</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>16Age1</name><description>[8.8/5730]? R'_HK_ age 16% posterior CDF value</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>50Age1</name><description>[69.2/8980]? R'_HK_ age 50% posterior CDF value</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>84Age1</name><description>[443/11700]? R'_HK_ age 84% posterior CDF value</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>97.5Age1</name><description>[1660/12800]? R'_HK_ age 97.5% posterior CDF value</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>2.5Age2</name><description>[1.2/1510]? Li EW age 2.5% posterior CDF value</description><unit>Myr</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>16Age2</name><description>[2.47/4300]? Li EW age 16% posterior CDF value</description><unit>Myr</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>50Age2</name><description>[5.6/8380]? Li EW age 50% posterior CDF value</description><unit>Myr</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>84Age2</name><description>[10/11600]? Li EW age 84% posterior CDF value</description><unit>Myr</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>97.5Age2</name><description>[29/12800]? Li EW age 97.5% posterior CDF value</description><unit>Myr</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>2.5AgeF</name><description>[1.2/2850] Final age 2.5% posterior CDF value</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>16AgeF</name><description>[2.47/5730] Final age 16% posterior CDF value</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>50AgeF</name><description>[5.6/8980] Final age 50% posterior CDF value</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>84AgeF</name><description>[10/11700] Final age 84% posterior CDF value</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>97.5AgeF</name><description>[29/12800] Final age 97.5% posterior CDF value</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BVCat</name><description>Display data from Boro Saikia+, 2018, J/A+A/616/A108 and Guillout+, 2009, J/A+A/504/829 within 2"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>