Galactic cirrus optical image fits
Yunning Zhao ; Wei Zhang
In this work, we used DESI optical images in the g and r bands, combined with IRAS 100 μm images, to detect the Galactic cirrus clouds. The optical images were downloaded from the Legacy Surveys Imagine sky viewer. In order to better separate cirrus clouds, we used the residual images which were generated by subtracting the model image from the actual imaging data. This dataset contains the optical residual images.
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Paper Information
Paper Title:
Galactic Cirri at High Galactic Latitudes. I. Investigating Scatter in Slopes between Optical and Far-infrared Intensities
Publication:
AJ
Identifiers
CSTR:
11379.11.101579
DOI:
10.12149/101579
VO Identifier:
ivo://China-VO/paperdata/101579
Publication Date:
2025-04-15
Citation Guidelines
Yunning Zhao et al. 2025. Galactic cirrus optical image fits. Version 1.0. https://doi.org/10.12149/101579
@misc{10.12149/101579,
doi = {10.12149/101579},
url = {https://doi.org/10.12149/101579},
author = {Yunning Zhao },
title = {Galactic cirrus optical image fits},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2025}
}
doi = {10.12149/101579},
url = {https://doi.org/10.12149/101579},
author = {Yunning Zhao },
title = {Galactic cirrus optical image fits},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2025}
}
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This DOI represents all versions, and will always resolve to the latest one.
2025-04-15