astronomy object detection parquet survey
The Zwicky Transient Facility (ZTF) is a time-domain astronomy survey that uses the Palomar 48 inch Schmidt telescope and a custom-built wide-field camera to image the night sky in three photometric filters (g, r, and i). It is a fully-automated survey aimed at a systematic exploration of optical transient phenomena. It completes a scan of the observable northern sky approximately every three nights.
ZTF datasets may be updated approximately twice per year. The data may also be presented in new ways as the products become available.
https://irsa.ipac.caltech.edu/data_use_terms.html
https://irsa.ipac.caltech.edu/Missions/ztf.html
See all datasets managed by IRSA.
https://irsa.ipac.caltech.edu/docs/help_desk.html
Zwicky Transient Facility (ZTF) was accessed on DATE
from https://registry.opendata.aws/ztf. If you use the Objects Table, please cite the Digital Object Identifier (DOI): 10.26131/IRSA597. If you use the Lightcurves, please cite the Digital Object Identifier (DOI): 10.26131/IRSA598. In addition, please follow the ZTF acknowledgement guidelines and the IRSA acknowledgement guidelines.
arn:aws:s3:::ipac-irsa-ztf/contributed/dr23/objects/hats
us-east-1
aws s3 ls --no-sign-request s3://ipac-irsa-ztf/contributed/dr23/objects/hats/
arn:aws:s3:::ipac-irsa-ztf/contributed/dr23/lc/hats
us-east-1
aws s3 ls --no-sign-request s3://ipac-irsa-ztf/contributed/dr23/lc/hats/