ogle Webivo://astro.upjs/ogle/q/ts-webUPJŠ DC TeamSoszyński, I.Udalski, A.Szymański, M.K.Pietrukowicz, P.Skowron, D.M.Skowron, J.Poleski, R.Mróz, P.Kozłowski, S.Ulaczyk, K.Iwanek, P.Gromadzki, M.Rybicki, K.Wrona, M.Ratajczak, M.Mróz, M.Borowicz, J.Głowacki, M.Urbanowicz, M.2026-03-22T19:51:39ZUPJŠ Archive

Jesenná 5, 040 01 Košice, Slovakia

olga.vozyakova@student.upjs.sklight-curvesvariable-starssurveys The **Optical Gravitational Lensing Experiment (OGLE)** is a long-term photometric survey operated by the University of Warsaw at Las Campanas Observatory. Most of the observations are carried out in the Cousins *I* filter, with auxiliary measurements in the *V* filter. High-cadence, long-term observations of crowded fields have led to the systematic discovery and classification of variable stars. The OGLE Collection of Variable Stars (OCVS) contains over one million objects. OCVS light curves span three survey phases: OGLE-II (1996-2000), OGLE-III (2001-2009), and OGLE-IV (2010-present). The VO-compliant re-publication of the OCVS light curve collection allows bulk download for objects with a specific variability class and parameters, which can be very handy for ML-based light curve analysis and related applications. The original data of the republished collection can be found at: https://www.astrouw.edu.pl/ogle/ogle4/OCVS/ While republishing, we almost preserve the original data structure. That is, there are tables with variable star parameters split by variability type (Cepheids, Eclipsing and Ellipsoidal Binaries, RR Lyrae stars, etc.) and by sky field: Galactic Bulge (BLG), Magellanic Clouds (LMC, SMC), Galactic Disc (GD). A few tables are related only to a variability class (e.g., Cataclysmic Variables - CV, BLAPs, Anomalous Cepheids in the Milky Way - ACEP/GAL) or a specific field (M54 variables, which comprise diverse classes). All observed objects with their main parameters are aggregated in the object_all table, which facilitates generic queries across all classes. This table is served by Cone Search. The ts_ssa table is the main table for light-curve queries. It is served by TAP and SSA services. The time series themselves, as well as previews of folded and unfolded light curves, can be accessed via DataLink from the ts_ssa and ObsCore tables. Direct links to previews of folded curves are placed in the *preview* column of both the *ts_ssa* and *ObsCore* tables.https://skvo.science.upjs.sk/ogle/q/ts-web/infoSurveyResearchIsServedByPavol Jozef Šafárik University Archive Obscore If you use or refer to the data obtained from this catalog in your scientific work, please cite the appropriate papers: :bibcode: `2014AcA....64..177S` (RR Lyr stars in the Galactic bulge) :bibcode: `2015AcA....65..297S` (Classical Cepheids in the LMC and SMC) :bibcode: `2015AcA....65..233S` (Anomalous Cepheids in the LMC and SMC) :bibcode: `2016AcA....66..131S` (RR Lyr stars in the LMC and SMC) :bibcode: `2016AcA....66..405S` (Eclipsing stars in the Galactic bulge) :bibcode: `2016AcA....66..421P` (Eclipsing stars in the LMC and SMC) :bibcode: `2017AcA....67..103S` (Classical and anomalous Cepheids in the LMC and SMC) :bibcode: `2017AcA....67..297S` (Classical, type II, and anomalous Cepheids toward the Galactic Center) :bibcode: `2018AcA....68...89S` (Type II Cepheids in the LMC and SMC) :bibcode: `2018AcA....68..315U` (Clasical and type II cepheids in Galactic disk and bulge) :bibcode: `2019AcA....69..321S` (RR Lyr stars in the Galactic Disk and Bulge) :bibcode: `2020AcA....70..241P` (delta Scuti stars towards Galactic bulge) :bibcode: `2021AcA....71..189S` (delta Scuti stars in the Milky Way) :bibcode: `2022ApJS..259...16W` (One Thousand Heartbeat Stars) :bibcode: `2022ApJS..928..135W` (Photometric Analysis of the OGLE Heartbeat Stars) :bibcode: `2022ApJS..260...46I` (Miras in the Milky Way) :bibcode: `2022AcA....72..245S` (delta Sct Stars in the Small Magellanic Clouds) :bibcode: `2023AcA....73..105S` (delta Scuti Stars in the Large Magellanic Cloud) :bibcode: `2023AcA....73..127M` (Transiting Planets in Galactic Bulge)https://skvo.science.upjs.sk/ogle/q/sdl/dlgethttps://skvo.science.upjs.sk/ogle/q/sdl/dlmetaGETapplication/x-votable+xml;content=datalinkIDThe publisher DID of the dataset of interestmeta.id;meta.maincharresponseformatFile format requested for output.meta.code.mimecharmaxrecMaximum number of records returned. Pass 0 to retrieve service parameters.integerverbExhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns.integerLas CampanasWarsaw 1.3m Telescope2/112 3/338 369 454-457 472 513 515-517 520 583 589 591-592 594 613 615 621 623 651-653 659 662-663 669 4/896 1301 1303 1309 1344 1346 1376-1377 1379 1382 1385 1387-1388 1390-1391 1484-1485 1487 1496 1810-1811 1814 1833 1836-1837 1840-1842 1844-1845 1847 1866-1867 1892 1894-1895 1900-1901 1903 1912 1914-1915 2001 2004 2051 2057-2059 2072-2074 2084-2086 2088-2090 2112-2114 2118-2119 2314 2325-2327 2336-2338 2344 2346 2372 2374 2400-2402 2408 2410 2432 2451 2457 2459 2481 2496 2498 2504 2536 2538 2590-2591 2597-2599 2601-2603 2616-2617 2633-2635 2643 2645-2647 2656-2657 2660-2661 2688-2690 2692 2696 2986-2987 2990-2991 5/3242 5200-5201 5203 5209 5233 5245 5247 5333 5380 5382 5388 5390-5391 5432 5434 5512-5513 5515 5520 5522 5534 5537 5539 5556 5558-5559 5893 5895 5945 5947 5952 5954 5960 5962-5963 5992-5994 6033 6036-6037 7232 7234-7235 7237-7239 7248 7250-7251 7260 7262-7263 7329 7341 7372-7374 7385 7392-7394 7482 7574 7588-7589 7591 7608-7609 7611 7626 7654-7655 7664 7672 7674-7676 7678-7679 8000-8001 8020-8022 8024-8025 8028-8029 8199 8203 8225 8227 8300-8302 8304-8306 8308-8309 8348-8350 8364-8366 8368-8370 8384-8386 8460-8461 8463-8466 8520 8704-8706 9273-9275 9297 9299 9327 9356-9358 9360-9362 9380 9382 9413 9415 9421 9423 9445 9447 9453 9455 9492 9520 9522 9612 9614 9638 9736-9738 9760 9797 9799 9933 9935 9957 9959 9965 10024-10026 10112 10114 10120 10122 10346-10347 10349-10351 10358-10359 10381-10383 10386-10387 10401-10403 10472-10474 10480-10481 10484 10526-10527 10529-10531 10569-10571 10579 10632-10634 10636-10637 10688-10689 10692-10693 10703 10741 10764-10766 10772 10792 11284-11285 11328-11329 11332-11333 11344-11345 11348-11349 11520-11521 11937-11939 11943 11952 11954-11955 11958 12008-12010 6/12963 12966 12972 12986-12987 12990 14352-14354 14356 14360 14368 14370-14373 14376 20757 20809 20811 20833 20844-20845 20847 20976-20977 20979 20985 21329 21341 21534 21556-21558 21698 21706 21740 21742 22056-22057 22059 22084 22086-22087 22092 22094-22095 22128 22130 22147 22180-22181 22230 22440 22442-22443 23568-23569 23571 23577 23579 23604-23605 23607 23613 23615 23701 23703 23709 23777 23779 23820 23822 23844 23846-23847 23954 23960 23962-23963 23984 23986 24140-24141 24152-24153 24320 24322 28932 28934-28935 28947 28998 29018 29046 29312-29313 29315 29324-29325 29327 29360-29361 29363 29373 29408-29410 29424-29425 29428 29500-29502 29536-29537 29549 29580-29581 29584-29586 29649 29652-29653 29738 29824 29834 29839 29850-29851 29854-29855 29920 29922-29923 29932 29934-29935 30288 30290-30291 30300 30302-30303 30336-30337 30340-30341 30343 30360-30361 30363 30388-30389 30391 30440-30441 30496 30498-30499 30508 30510-30511 30608 30610-30611 30660 30662 30666 30668-30669 30692 30694-30695 30710 31824-31825 31828-31829 31831 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40110 40112 40114 40452 40460 40462 40484 40486-40487 40492 40494-40495 40602 40624 40626 40632-40634 41213-41215 41383 41394-41395 41419 41422-41423 41430-41431 41501-41503 41517 41519 41522-41523 41539 41541-41543 41601-41603 41900 41902 41904-41906 41928-41930 41932 41940-41942 42047 42090-42091 42093-42095 42102-42103 42114-42115 42273-42275 42311 42315 42540-42542 42552-42553 42592-42593 42596-42597 42624 42760-42761 42764-42765 42776-42777 42780-42781 42783 42805-42807 42900-42901 42903 42944-42946 42948 42961 43068-43070 43092-43094 43096 43104-43106 43108 43152-43154 43172 43176 43178 43264 45125-45127 45132-45133 45135 45144-45145 45148-45149 45320-45322 45324-45325 45336-45337 45340-45341 45343 45384-45385 45388-45390 45400-45401 45403-45405 46088-46089 46092-46093 46096-46098 47662-47663 47745 47747 47760 47762 47766-47768 47770-47771 47814 47826-47827 47836 47838-47839 48011 48013-48015 48026 48044-48046 48048 4810649999.5 60624.013461.80585987e-19 4.095764654e-19https://skvo.science.upjs.sk/ogle/q/ts-web/coverageOpticalogle The **Optical Gravitational Lensing Experiment (OGLE)** is a long-term photometric survey operated by the University of Warsaw at Las Campanas Observatory. Most of the observations are carried out in the Cousins *I* filter, with auxiliary measurements in the *V* filter. High-cadence, long-term observations of crowded fields have led to the systematic discovery and classification of variable stars. The OGLE Collection of Variable Stars (OCVS) contains over one million objects. OCVS light curves span three survey phases: OGLE-II (1996-2000), OGLE-III (2001-2009), and OGLE-IV (2010-present). The VO-compliant re-publication of the OCVS light curve collection allows bulk download for objects with a specific variability class and parameters, which can be very handy for ML-based light curve analysis and related applications. The original data of the republished collection can be found at: https://www.astrouw.edu.pl/ogle/ogle4/OCVS/ While republishing, we almost preserve the original data structure. That is, there are tables with variable star parameters split by variability type (Cepheids, Eclipsing and Ellipsoidal Binaries, RR Lyrae stars, etc.) and by sky field: Galactic Bulge (BLG), Magellanic Clouds (LMC, SMC), Galactic Disc (GD). A few tables are related only to a variability class (e.g., Cataclysmic Variables - CV, BLAPs, Anomalous Cepheids in the Milky Way - ACEP/GAL) or a specific field (M54 variables, which comprise diverse classes). All observed objects with their main parameters are aggregated in the object_all table, which facilitates generic queries across all classes. This table is served by Cone Search. The ts_ssa table is the main table for light-curve queries. It is served by TAP and SSA services. The time series themselves, as well as previews of folded and unfolded light curves, can be accessed via DataLink from the ts_ssa and ObsCore tables. Direct links to previews of folded curves are placed in the *preview* column of both the *ts_ssa* and *ObsCore* tables.output The **Optical Gravitational Lensing Experiment (OGLE)** is a long-term photometric survey operated by the University of Warsaw at Las Campanas Observatory. Most of the observations are carried out in the Cousins *I* filter, with auxiliary measurements in the *V* filter. High-cadence, long-term observations of crowded fields have led to the systematic discovery and classification of variable stars. The OGLE Collection of Variable Stars (OCVS) contains over one million objects. OCVS light curves span three survey phases: OGLE-II (1996-2000), OGLE-III (2001-2009), and OGLE-IV (2010-present). The VO-compliant re-publication of the OCVS light curve collection allows bulk download for objects with a specific variability class and parameters, which can be very handy for ML-based light curve analysis and related applications. The original data of the republished collection can be found at: https://www.astrouw.edu.pl/ogle/ogle4/OCVS/ While republishing, we almost preserve the original data structure. That is, there are tables with variable star parameters split by variability type (Cepheids, Eclipsing and Ellipsoidal Binaries, RR Lyrae stars, etc.) and by sky field: Galactic Bulge (BLG), Magellanic Clouds (LMC, SMC), Galactic Disc (GD). A few tables are related only to a variability class (e.g., Cataclysmic Variables - CV, BLAPs, Anomalous Cepheids in the Milky Way - ACEP/GAL) or a specific field (M54 variables, which comprise diverse classes). All observed objects with their main parameters are aggregated in the object_all table, which facilitates generic queries across all classes. This table is served by Cone Search. The ts_ssa table is the main table for light-curve queries. It is served by TAP and SSA services. The time series themselves, as well as previews of folded and unfolded light curves, can be accessed via DataLink from the ts_ssa and ObsCore tables. Direct links to previews of folded curves are placed in the *preview* column of both the *ts_ssa* and *ObsCore* tables.location_radegpos.eq.ra;meta.mainssa:Char.SpatialAxis.Coverage.Location.Value.C1floatnullablelocation_decdegpos.eq.dec;meta.mainssa:Char.SpatialAxis.Coverage.Location.Value.C2floatnullableaccrefAccess key for the datameta.ref.url;meta.datasetssa:Access.Referencecharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namechart_minLower bound of times represented in the data setdtime.start;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.starttimedoublenullablet_maxUpper bound of times represented in the data setdtime.end;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.stoptimedoublenullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.BandpasscharnullabledatalinkA link to a datalink document for this timeseriesmeta.ref.urlcharnullable