Surveys · 3 of 6
OGLEOCVS
Ground-based, bands I, V, 3 series. Detections from 1997-01-07 to 2026-01-15.
Footprint
Brightness is stars per cell with a light curve from OGLE (HEALPix order 6, log scale), over the whole archive in gray. Galactic Mollweide, Galactic center in the middle, east left, 30° graticule. It shows where the archive holds light curves, not the survey's full footprint.
Time system
- native column
- hjd
- time scale
- UTC
- reference frame
- heliocentric
- origin
- JD − 2450000
- reference position
- source
- archive time axis
- BJD_TDB (bjd_tdb)
Converted to BJD_TDB by removing the heliocentric correction and applying the barycentric one. The native hjd is also served.
Bands
| band | λ_eff | saturation | collection | stars with a light curve | epochs | detections | era |
|---|---|---|---|---|---|---|---|
| OGLE-II Iogle:ii:I | 789 nm | 12 mag | curves_static | 60,414 | 17,630,186 | 17,630,186 | 1997-01-07 → 2001-02-20 |
| OGLE-II Vogle:ii:V | 551 nm | 12 mag | curves_static | 58,170 | 543,400 | 542,944 | 1997-01-23 → 2000-06-11 |
| OGLE-III Iogle:iii:I | 789 nm | 12 mag | curves_static | 300,475 | 171,472,082 | 171,472,082 | 2001-06-12 → 2009-05-26 |
| OGLE-III Vogle:iii:V | 551 nm | 12 mag | curves_static | 277,677 | 1,824,225 | 1,824,225 | 2001-07-22 → 2009-05-04 |
| OGLE-IV Iogle:iv:I | 789 nm | 12 mag | curves_static | 669,930 | 1,165,247,844 | 1,165,247,844 | 2010-03-05 → 2026-01-15 |
| OGLE-IV Vogle:iv:V | 551 nm | 12 mag | curves_static | 526,032 | 33,124,048 | 33,124,011 | 2010-03-05 → 2025-09-14 |
Epoch selection
- good epochs
- every epoch (no quality flag is published)
- detections
- every good epoch (no limiting magnitude is published)
- non-detections
- not reported
Alias frequencies
|f ± k·f_sid| (k=1,2), |f ± 1/365.25|, window at 365.25 / 182.63 / 29.53 d
Crossmatch to VSX
Measured radius 1″, 0.27% chance matches.
VSX imported OGLE's positions, so name and position are not independent. The ~1% of counterparts beyond 1.0″ are linked by name.
- ID column
- ogle_id
- catalog epoch
- J2015
OGLE IDs are not permanent: the December 2024 revision removed and reclassified some.
Caveats
- OGLE-II, -III and -IV are separate series and are processed separately.
Bulk access
Light curves are in the nested lc_ogle column of curves_static.
# read the release directly over HTTPS
import json, lsdb
from upath import UPath
root = UPath("https://data.varchive.app")
ptr = json.loads((root / "catalogs/latest.json").read_text())
RA, DEC = 0.0, 0.0 # your field center, degrees
# curves_static: OGLE I, V
static = lsdb.read_hats(root / ptr["collections"]["curves_static"]["path"],
columns=["varchive_id", "ra", "dec", "lc_ogle"])
df = static.cone_search(RA, DEC, 600).compute() # radius in arcsec
lc = df["lc_ogle"].iloc[0] # band, bjd_tdb, mag, mag_err, detected, series, hjd
i = lc[(lc["band"] == "I") & (lc["series"] == "iv")] # one band, one series
# never concatenate across bands or surveys; bjd_tdb is the time axis for scienceMore in the data guide.
Citation
- Udalski et al. 2015, AcA 65, 1 OGLE-IV: Fourth Phase of the Optical Gravitational Lensing Experiment
This work uses data from the Optical Gravitational Lensing Experiment (OGLE) Collection of Variable Stars.
BibTeX · 1 entry from NASA ADS
@ARTICLE{2015AcA....65....1U,
author = {{Udalski}, A. and {Szyma{\'n}ski}, M.~K. and {Szyma{\'n}ski}, G.},
title = "{OGLE-IV: Fourth Phase of the Optical Gravitational Lensing Experiment}",
journal = {\actaa},
keywords = {Surveys, Techniques: Photometric, Galaxy: bulge, Galaxy: disk, Magellanic Clouds, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
year = 2015,
month = mar,
volume = {65},
number = {1},
pages = {1-38},
doi = {10.48550/arXiv.1504.05966},
archivePrefix = {arXiv},
eprint = {1504.05966},
primaryClass = {astro-ph.SR},
adsurl = {https://ui.adsabs.harvard.edu/abs/2015AcA....65....1U},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}Also cite, by subset · 34 subsets, 27 papers; a star's page names its own
- blg/cep, blg/t2cep → Soszyński et al. 2017, AcA 67, 297, Udalski et al. 2018, AcA 68, 315, Soszyński et al. 2020, AcA 70, 101
- gal/acep → Soszyński et al. 2017, AcA 67, 103, Soszyński et al. 2017, AcA 67, 297, Udalski et al. 2018, AcA 68, 315, Soszyński et al. 2020, AcA 70, 101
- gd/cep, gd/t2cep → Udalski et al. 2018, AcA 68, 315, Soszyński et al. 2020, AcA 70, 101
- lmc/cep, smc/cep → Soszyński et al. 2015, AcA 65, 297
- lmc/acep, smc/acep → Soszyński et al. 2015, AcA 65, 233
- lmc/t2cep, smc/t2cep → Soszyński et al. 2018, AcA 68, 89
- blg/rrlyr → Soszyński et al. 2014, AcA 64, 177, Soszyński et al. 2019, AcA 69, 321
- gd/rrlyr → Soszyński et al. 2019, AcA 69, 321
- lmc/rrlyr, smc/rrlyr → Soszyński et al. 2016, AcA 66, 131
- blg/dsct → Pietrukowicz et al. 2020, AcA 70, 241, Soszyński et al. 2021, AcA 71, 189, Pietrukowicz et al. 2022, AcA 72, 161
- gd/dsct → Soszyński et al. 2021, AcA 71, 189
- lmc/dsct → Soszyński et al. 2023, AcA 73, 105
- smc/dsct → Soszyński et al. 2022, AcA 72, 245
- blg/ecl → Soszyński et al. 2016, AcA 66, 405
- blg/short_period_ecl → Soszyński et al. 2015, AcA 65, 39
- blg/dpv → Rojas García et al. 2021, ApJ 922, 30
- lmc/ecl, smc/ecl → Głowacki et al. 2024, AcA 74, 241
- blg/hb, lmc/hb, smc/hb → Wrona et al. 2022, ApJS 259, 16, Wrona et al. 2022, ApJ 928, 135
- blg/lpv, gd/lpv → Iwanek et al. 2022, ApJS 260, 46
- blg/rot → Iwanek et al. 2024, AcA 74, 1
- blg/transits → Mróz et al. 2023, AcA 73, 127
- CBO → Urbanowicz et al. 2026, AcA 76, 83
- CV → Mróz et al. 2015, AcA 65, 313
- M54 → Hamanowicz et al. 2016, AcA 66, 197
Also cite AAVSO VSX and Gaia.
- license
- public, with the per-class discovery paper requested
- data
- https://ogle.astrouw.edu.pl/
- release
- OCVS