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@arXiv_astrophGA_bot@mastoxiv.page
2025-06-24 09:36:39

The JWST/AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. I. A Diversity of Nebular Attenuation Curves and Evidence for Non-Unity Dust Covering Fractions
Naveen A. Reddy, Alice E. Shapley, Ryan L. Sanders, Michael W. Topping, Richard S. Ellis, Max Pettini, Gabriel Brammer, Fergus Cullen, Natascha M. Forster Schreiber, Ali A. Khostovan, Derek J. McLeod, Ross J. McLure, Desika Narayanan, Pascal A. Oesch, Anthony J. Pahl, Charles…

@arXiv_csIR_bot@mastoxiv.page
2025-06-03 07:21:20

Query Drift Compensation: Enabling Compatibility in Continual Learning of Retrieval Embedding Models
Dipam Goswami, Liying Wang, Bart{\l}omiej Twardowski, Joost van de Weijer
arxiv.org/abs/2506.00037

@arXiv_econEM_bot@mastoxiv.page
2025-06-10 08:00:12

Does Residuals-on-Residuals Regression Produce Representative Estimates of Causal Effects?
Apoorva Lal, Winston Chou
arxiv.org/abs/2506.07462

@arXiv_astrophGA_bot@mastoxiv.page
2025-06-18 09:59:31

Sulphur abundances in star-forming regions from optical emission lines: A new approach based on photoionization models consistent with the direct method
Enrique P\'erez-Montero, Borja P\'erez-D\'iaz, Jos\'e M. V\'ilchez, Igor A. Zinchenko, Asier Castrillo, Marta Gavil\'an, Sandra Zamora, \'Angeles I. D\'iaz

@arXiv_nuclth_bot@mastoxiv.page
2025-06-06 09:50:20

This arxiv.org/abs/2504.01814 has been replaced.
initial toot: mastoxiv.page/@arXiv_nuc…