Pan-STARRS1 Photometry Correction
Kai Xiao
We provide two-dimensional maps and a Python package specifically designed to correct position-dependent systematic errors in PS1 photometry. The corrections can effectively achieve a precision of 1--2 mmag when averaged over 14’ regions. The corrected PS1 photometry not only facilitates high-precision investigations but also serves as a reliable reference for calibrating other surveys.
Files
PS1_Correction.fits
150.02 MB
ps1_correction.py
2.06 kB
README.txt
2.43 kB
Paper Information
Paper Title:
Improvement of the Pan-STARRS Photometric Calibration with LAMOST and Gaia
Publication:
ApJS
Identifier
cstr:
11379.11.101283
DOI:
10.12149/101283
VO Identifier:
ivo://China-VO/data/APJS/xiaokai101283/
Publication date:
2023-08-08
Citation Guidelines
Kai Xiao et al. 2023. Pan-STARRS1 Photometry Correction. Version 1.0. https://doi.org/10.12149/101283
@misc{10.12149/101283,
doi = {10.12149/101283},
url = {https://doi.org/10.12149/101283},
author = {Kai Xiao},
title = {Pan-STARRS1 Photometry Correction},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2023}
}
doi = {10.12149/101283},
url = {https://doi.org/10.12149/101283},
author = {Kai Xiao},
title = {Pan-STARRS1 Photometry Correction},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2023}
}
Versions
Main
This DOI represents all versions, and will always resolve to the latest one.
2023-08-08