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20242026
most citedABC-SN: Attention Based Classifier for Supernova Spectra

1 citations · 1 across the 2 of their papers we have counts for

collaborators

11 papers

astro-ph.IM20261 cited

ABC-SN: Attention Based Classifier for Supernova Spectra

Willow Fox Fortino, Federica B. Bianco, Pavlos Protopapas +2

While significant advances have been made in photometric classification ahead of the millions of transient events and hundreds of supernovae (SNe) each night that the Vera C. Rubin…

astro-ph.IM2026

Deep Learning for Astrophysics: An Open Textbook from the NASA Cosmic Origins AI/ML Science and Technology Interest Group

Yuan-Sen Ting, Digvijay Wadekar, Phill Cargile +21

Recent community assessments identify education as a principal barrier to adopting modern machine learning in astronomy. We present Deep Learning for Astrophysics, a freely availab…

astro-ph.IM2026

Learning What's Real: Disentangling Signal and Measurement Artifacts in Multi-Sensor Data, with Applications to Astrophysics

Pablo Mercader-Perez, Carolina Cuesta-Lazaro, Daniel Muthukrishna +5

Data collected from the physical world is always a combination of multiple sources: an underlying signal from the physical process of interest and a signal from measurement-depende…

astro-ph.EP2026

The GAPS Programme at TNG. LXXIII. Confirmation of the hot sub-Neptune TOI-4602 b (HD 25295 b), a key target for future atmospheric characterization

C. Di Maio, S. Benatti, D. Locci +25

Precise mass and radius measurements of small, transitional exoplanets, such as super-Earths and sub-Neptunes, are essential to constrain their bulk density and formation history,…

astro-ph.IM2026

ASTRAFier: A Novel and Scalable Transformer-based Stellar Variability Classifier

Paul F. X. Gregory, Jeroen Audenaert, Mykyta Kliapets +5

Photometric missions such as Kepler and TESS have generated millions of light curves covering almost the entire sky, offering unprecedented opportunities to study stellar variabili…

astro-ph.EP2026

QLP Data Release Notes 004: TESS-Gaia Light Curve Photometry Implementation

Glen Petitpas, Jack Haviland, Te Han +7

The Quick-Look Pipeline (QLP; Huang et al. 2020, Kunimoto et al. 2021 and references therein) generates light curves for up to 2 million stars every 27.4 days observed by TESS as p…