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  We created a synthetic dataset, RSyntHyperPDID, based on the AVIRIS database.
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  The dataset is sufficiently large to serve as a training set for hyperspectral dehazing models.
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- Official Dataset for HyperHazeOff: Hyperspectral Remote Sensing Image Dehazing Benchmark. [Preprints.org](https://www.preprints.org/manuscript/202510.1565)
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- Official Code: [GitHub](https://github.com/iitpvisionlab/hyperhazeoff).
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  ### RGB/
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  For each split part (train/test) and clear hyperspectral image, two types of RGB visualizations are provided:
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  ### Hyperspectral Images (HSI)
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- Each RSyntHyperPDID hyperspectral image has a size of 256×256 pixels with 182 spectral bands.
 
 
 
 
 
 
 
 
 
 
 
 
 
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  ## Dataset Structure
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  ```
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
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  ```
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  ## Data Source
 
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  We created a synthetic dataset, RSyntHyperPDID, based on the AVIRIS database.
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  The dataset is sufficiently large to serve as a training set for hyperspectral dehazing models.
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+ *Official Dataset for HyperHazeOff: Hyperspectral Remote Sensing Image Dehazing Benchmark.* [Preprints.org](https://www.preprints.org/manuscript/202510.1565)
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+ *Official Code:* [GitHub](https://github.com/iitpvisionlab/hyperhazeoff).
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  ### RGB/
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  For each split part (train/test) and clear hyperspectral image, two types of RGB visualizations are provided:
 
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  ### Hyperspectral Images (HSI)
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+ The RSyntHyperPDID dataset contains hyperspectral images of size 256×256 pixels with 182 spectral bands.
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+
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+ It is divided into three categories: *clear, train, and test*.
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+
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+ Each train and test sample includes hyperspectral images with synthetic haze, created based on a corresponding clear ground truth (GT) image.
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+
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+ The naming convention ensures the link between hazy and clear images:
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+ - for example, **clear/XXXX.npy** serves as the GT for train/test samples named **XXXX_YYYY.npy**,
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+ - where **XXXX** is the GT image identifier and **YYYY** represents haze synthesis parameters.
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+
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+ This naming scheme ensures straightforward pairing of hazy images with their clear counterparts for training and evaluation.
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+ It supports reproducible experiments in haze removal and spectral image restoration.
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+
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+ Additionally, wavelength information for the hyperspectral bands is provided in the file *wavelengths_synthyper.npy*, supporting spectral analysis across the dataset.
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  ## Dataset Structure
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  ```
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+ RSHPDID
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+ |-- rgb
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+ | |-- clear
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+ | | |-- CSNC
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+ | | | |-- 0001.png
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+ | | | |-- ........
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+ | | | `-- 0220.png
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+ | | `-- CSSO
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+ | | |-- 0001.png
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+ | | |-- ........
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+ | | `-- 0220.png
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+ | |-- test
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+ | | |-- CSNC
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+ | | | |-- 0010_0030.png
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+ | | | |-- .............
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+ | | | `-- 0219_4040.png
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+ | | `-- CSSO
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+ | | |-- 0010_0030.png
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+ | | |-- .............
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+ | | `-- 0219_4040.png
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+ | `-- train
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+ | |-- CSNC
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+ | | |-- 0001_0030.png
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+ | | |-- .............
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+ | | `-- 0220_4040.png
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+ | `-- CSSO
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+ | |-- 0001_0030.png
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+ | |-- .............
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+ | `-- 0220_4040.png
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+ |-- clear
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+ | |-- 0001.npy
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+ | |-- ........
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+ | `-- 0220.npy
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+ |-- test
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+ | |-- 0010_0030.npy
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+ | |-- .............
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+ | `-- 0219_4040.npy
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+ |-- train
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+ | |-- 0001_0030.npy
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+ | |-- .............
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+ | `-- 0220_4040.npy
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+ `-- wavelengths_synthyper.npy
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  ```
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  ## Data Source