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<ri:Resource created="2024-10-21T15:51:19Z" status="active" updated="2025-06-13T15:25:00Z" 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>CFHT monitoring of M67 &amp; members from Gaia EDR3</title><shortName>J/ApJ/938/118</shortName><identifier>ivo://CDS.VizieR/J/ApJ/938/118</identifier><altIdentifier>doi:10.26093/cds/vizier.19380118</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dungee R.</name></creator><creator><name>van Saders J.</name></creator><creator><name>Gaidos E.</name></creator><creator><name>Chun M.</name></creator><creator><name>Garcia R.A.</name></creator><creator><name>Magnier E.A.,Mathur S.</name></creator><creator><name>Santos A.R.G.</name></creator><date role="Updated">2025-02-12T20:09:18Z</date><date role="Created">2024-10-21T15:51:19Z</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>open-star-clusters</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>proper-motions</subject><subject>trigonometric-parallax</subject><subject>k-stars</subject><description>We present stellar rotation periods for late K- and early M-dwarf members of the 4Gyr old open cluster M67 as calibrators for gyrochronology and tests of stellar spin-down models. Using Gaia EDR3 astrometry for cluster membership and Pan-STARRS (PS1) photometry for binary identification, we build this set of rotation periods from a campaign of monitoring M67 with the Canada-France-Hawaii Telescope's MegaPrime wide-field imager. We identify 1807 members of M67, of which 294 are candidate single members with significant rotation period detections. Moreover, we fit a polynomial to the period versus color- derived effective temperature sequence observed in our data. We find that the rotation of very cool dwarfs can be explained by simple solid-body spin-down between 2.7 and 4Gyr. We compare this rotational sequence to the predictions of gyrochronological models and find that the best match is Skumanich-like spin-down, P_rot_{propto}t^0.62^, applied to the sequence of Ruprecht 147. This suggests that, for spectral types K7-M0 with near-solar metallicity, once a star resumes spinning down, a simple Skumanich-like relation is sufficient to describe their rotation evolution, at least through the age of M67. Additionally, for stars in the range M1-M3, our data show that spin-down must have resumed prior to the age of M67, in conflict with the predictions of the latest spin-down models.</description><source format="bibcode">2022ApJ...938..118D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/938/118</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, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/39">IV/39 : TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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Effective temperature computed from PS1 r-i</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Prot</name></column></table><table><name>J/ApJ/938/118/table3</name><description>*Detected Lomb-Scargle failure modes (see Section 5.1)</description><column><name>Fap</name><description>False Alarm probability of rotation period</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>HalfPer</name><description>[2.9/413]? If present in periodogram, lomb-scargle failure mode with m=2 &amp; n=0</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>3dPer</name><description>[2.79/275]? If present in periodogram, lomb-scargle failure mode with m=3 &amp; n=0</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Month1n-2</name><description>[3.69/47]? If present in periodogram, lomb-scargle failure mode with m=1 &amp; n=-2, for ~month peak in window function, {delta}P~29.5days</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Month2n-1</name><description>[3.3/806]? If present in periodogram, lomb-scargle failure mode with m=1 &amp; n=-1, for ~month peak in window function, {delta}P~29.5days</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Month3n+1</name><description>[2.89/28.7]? If present in periodogram, lomb-scargle failure mode with m=1 &amp; n=+1, for ~month peak in window function, {delta}P~29.5days</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</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>Gaia</name><description>The Gaia EDR3 source_id number of star</description><ucd>meta.id;meta.main</ucd></column><column><name>Prot</name></column></table></schema></tableset></ri:Resource>