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<ri:Resource created="2026-03-25T14:27:13Z" status="active" updated="2026-07-02T11:52:32Z" 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>Rotation periods of 272 stars from TESS &amp; ZTF</title><shortName>J/AJ/170/15</shortName><identifier>ivo://CDS.VizieR/J/AJ/170/15</identifier><altIdentifier>doi:10.26093/cds/vizier/be-5a-f</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hattori S.</name></creator><creator><name>Angus R.</name></creator><creator><name>Foreman-Mackey D.</name></creator><creator><name>Lu Y.(.</name></creator><creator><name>Colman I.</name></creator><date role="Updated">2026-07-02T11:52:32Z</date><date role="Created">2026-03-25T14:27:13Z</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>photometry</subject><subject>visible-astronomy</subject><subject>dwarf-stars</subject><subject>k-stars</subject><description>The rotation period of a star is an important quantity that provides insight into its structure and state. For stars with surface features like starspots, their periods can be inferred from brightness variations as these features move across the stellar surface. TESS, with its all-sky coverage, is providing the largest sample of stars for obtaining rotation periods. However, most of the periods have been limited to shorter than the 13.7days TESS orbital period due to strong background signals (e.g., scattered light) on those timescales. In this study, we investigated the viability of measuring longer periods (&gt;10days) from TESS light curves for stars in the Northern Continuous Viewing Zone (NCVZ). We first created a reference set of 272 period measurements longer than 10 days for K and M dwarfs in the NCVZ using data from the Zwicky Transient Facility (ZTF) that we consider as the "ground truth" given ZTF's long temporal baseline of 6+years. We then used the unpopular pipeline to detrend TESS light curves and implemented a modified Lomb-Scargle (LS) periodogram that accounts for flux offsets between observing sectors. For 179 out of the 272 sources (66%), the TESS-derived periods match the ZTF-derived periods to within 10%. The match rate increases to 81% (137 out of 170) when restricting to sources with a TESS LS power that exceeds a threshold. Our results confirm the capability of measuring periods longer than 10days from TESS data, highlighting the data set's potential for studying slow rotators.</description><source format="bibcode">2025AJ....170...15H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/170/15</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/IV/34">IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/38">IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)</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/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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(Edvardsson+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/530/A138">J/A+A/530/A138 : Geneva-Copenhagen survey re-analysis (Casagrande+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/48">J/ApJ/743/48 : Stars with rotation periods &amp; X-ray luminosities (Wright+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/24">J/ApJS/211/24 : Rotation periods of Kepler MS stars (McQuillan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/472/1618">J/MNRAS/472/1618 : Kepler study of starspot lifetimes (Giles+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/180">J/AJ/155/180 : A catalog of cool dwarf targets for the TESS (Muirhead+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/102">J/AJ/156/102 : The TESS Input Catalog &amp; Candidate Target List (Stassun+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/244/21">J/ApJS/244/21 : Surface rotation &amp; activity of Kepler stars. I. (Santos+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/250/20">J/ApJS/250/20 : Rot. periods in TESS objects of interest (TOIs) (Canto+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/249/18">J/ApJS/249/18 : The ZTF catalog of periodic variable stars (Chen+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/903/99">J/ApJ/903/99 : Stellar spins in the open cluster NGC 2516 (Healy+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/255/17">J/ApJS/255/17 : Surface rot. &amp; activity for Kepler stars. II. (Santos+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/164/137">J/AJ/164/137 : Untangling the Gal. IV. ~100000 stars with TESS (Kounkel+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/164/251">J/AJ/164/251 : ZTF measured rot. period of 40553 M- or G-dwarfs (Lu+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/268/4">J/ApJS/268/4 : Stellar variab. with TESS 2min cadence phot. 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