Cluster Difference Imaging Photometric Survey ("CDIPS")
收藏DataCite Commons2020-07-30 更新2025-04-09 收录
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http://archive.stsci.edu/doi/resolve/resolve.html?doi=10.17909/t9-ayd0-k727
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The TESS mission has been releasing full-frame images recorded at 30 minute cadence. Using the TESS images, the team has begun a Cluster Difference Imaging Photometric Survey (CDIPS), in which they are making light curves for stars that are candidate members of open clusters and moving groups. They have also included stars that show photometric indications of youth. Each light curve represents between 20 and 25 days of observations of a star brighter than Gaia Rp magnitude of 16. The precision of the detrended light curves is generally in line with theoretical expectations. The pipeline is called `cdips-pipeline`, and it is available for inspection as a GitHub repository, and should be cited as an independent software reference (Bhatti et al., 2019, http://doi.org/10.5281/zenodo.3370324).
提供机构:
STScI/MAST
创建时间:
2019-09-30



