EROS light curve data base
arXiv:2512.12745 · doi:10.1051/0004-6361/202557321
Abstract
The EROS project (Expérience de Recherche d'Objets Sombres) carried out photometric surveys of dense stellar fields towards the Magellanic Clouds (LMC and SMC), the Galactic Bulge and Galactic spiral arms, over the period 1990-2003. The main goal of the experiment was to search for the Galactic Dark Matter in the form of massive compact objects (machos), through the gravitational microlensing effect. The historical record of the flux variations of the monitored stars by EROS-2 will be a unique asset for time domain astronomy and to complement current and future searches of transient sources. We describe the set of light curves obtained by EROS-2 program over the years 1996 to 2003, monitoring more than 86 million stars, which is publicly released through the Centre de Données de Strasbourg (CDS). The numbers of light curves in this data set are 28.7 and 4.0 million in LMC, respectively SMC, 42.9 million in the Galactic Bulge and 10.4 million towards the Galactic spiral arms, with several hundred measurements for each object. Data from EROS-1 is also being released. The object catalog and light curves and images are accessible through the CDS portal. This will be useful for checking the past behavior of newly discovered variable objects.
15 pages, 15 figures, accepted in A&A , Lightcurve data at CDS : https://cdsarc.cds.unistra.fr/viz-bin/cat/II/390
References in corpus (23)
- The Gaia mission
- Gaia Data Release 3: Summary of the content and survey properties
- Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
- Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds
- The Magellanic Clouds Photometric Survey: The Large Magellanic Cloud Stellar Catalog and Extinction Map
- OGLE 2003-BLG-235/MOA 2003-BLG-53: A planetary microlensing event
- Microlensing optical depth towards the Galactic bulge from MOA observations during 2000 with Difference Image Analysis
- The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs
- Galactic Bulge Microlensing Optical Depth from EROS-2
- Fink, a new generation of broker for the LSST community
- The EPOCH Project: I. Periodic variable stars in the EROS-2 LMC database
- No massive black holes in the Milky Way halo
- Type Ia supernova rate at a redshift of ~ 0.1
- New Magellanic Cloud R Coronae Borealis and DY Per type stars from the EROS-2 database: the connection between RCBs, DYPers and ordinary carbon stars
- Microlensing optical depth and event rate toward the Large Magellanic Cloud based on 20 years of OGLE observations
- R Coronae Borealis stars in the Galactic Bulge discovered by EROS-2
- The EROS2 search for microlensing events towards the spiral arms: the complete seven season results
- Gravitational Microlensing I: A Unique Astrophysical Tool
- Understanding EROS2 observations toward the spiral arms within a classical Galactic model framework
- Limits on planetary-mass primordial black holes from the OGLE high-cadence survey of the Magellanic Clouds
- Observation of periodic variable stars towards the galactic spiral arms by EROS II
- EROS 2 proper motion survey: Constraints on the halo white dwarfs
- Microlensing optical depth, event rate, and limits on compact objects in dark matter based on 20 yr of OGLE observations of the Small Magellanic Cloud