Latest Images
Black hole mass (MBH) versus bolometric luminos...
Gaussian fittings to detect BLAGN signatures fo...
The redshift distribution of our sample of BLAG...
Eddington ratio (λedd) versus redshift for our ...
FWHMHα,broad versus Log LHα,broad for our sampl...
Known LRDs from our BLAGN sample. Blue and red ...
Known LRDs from our BLAGN sample. Blue and red ...
Known LRDs from our BLAGN sample. Blue and red ...
BPT diagram of our sample of BLAGNs. ⋆ show poi...
JWST NIRSpec spectra for identified BLAGNs. The...
JWST NIRSpec spectra for identified BLAGNs. The...
JWST NIRSpec spectra for identified BLAGNs. The...
Comparison of [Fe/H] and [α/Fe] estimates betwe...
[α/Fe]–[Fe/H] diagrams for DESI EDR and APOGEE ...
Sketch of the pretraining and fine-tuning workf...
Effect of fine-tuning sample size on the one-to...
Effect of fine-tuning sample size (0, 100, 200,...
Effect of fine-tuning sample size on the predic...
Saliency maps of the output iron abundance with...
Loss landscapes for different fine-tuning strat...
Effect of the number of trainable parameters on...
[α/Fe]–[Fe/H] diagrams for the DESI EDR and the...
Effect of learning rate on models trained from ...
Effect of learning rate on models trained from ...
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