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@@ -71,10 +71,20 @@ For each galaxy, multi-band (u, g, r, i, z) cutouts of size 300×300 pixels (0.3
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  Regression (predicting continuous redshift value from multi-band images).
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  ### Total Samples
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- 41,650 galaxies.
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  ### Split
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  - Training set: 10,100 samples
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- - Test set: 31,600 samples
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- The split is performed using **redshift-stratified sampling** to ensure consistent redshift distributions between training and test sets.
 
 
 
 
 
 
 
 
 
 
 
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  Regression (predicting continuous redshift value from multi-band images).
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  ### Total Samples
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+ 50,896 galaxies.
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  ### Split
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  - Training set: 10,100 samples
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+ - Test set: 40,796 samples
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+ The split is performed using **redshift-stratified sampling** to ensure consistent redshift distributions between training and test sets.
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+ ## 4. `lens-detection`: Gravitational Lens Detection (Object Detection)
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+ ### Description
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+ This dataset is designed for **strong gravitational lens detection** in wide-field survey images. It likely consists of image cutouts from surveys such as DESI, LSST, or the Kilo-Degree Survey (KiDS), annotated with bounding boxes around candidate lens systems (e.g., Einstein rings, arcs).
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+ The dataset supports the **object detection** downstream task evaluated in the FAMA paper, where the model demonstrated significant gains over supervised baselines.
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+ ### Task Type
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+ Object detection (localization + binary classification: lens vs. non-lens).