Unified Spectrospatial Forward Models: Spatially Continuous Maps of Weak Emission Lines in the Rosette Nebula with SDSS-V LVM

Analyses of integral field unit data are typically performed on a per-spaxel basis, with each spectrum modelled independently. For low signal-to-noise ratio (S/N) features such as weak emission lines, estimating properties is difficult and imprecise. Arbitrary binning schemes boost S/N at the cost o...

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Autors principals:	Thomas Hilder, Andrew R. Casey, Julianne J. Dalcanton, Kathryn Kreckel, Amelia M. Stutz, Amrita Singh, Guillermo A. Blanc, Sebastián F. Sánchez, J. E. Méndez-Delgado, Andrew K. Saydjari, Luciano Vargas-Herrera, Niv Drory, Dmitry Bizyaev, José G. Fernández-Trincado, Carlos G. Román-Zúñiga, Juna A. Kollmeier, Ivan Yu. Katkov, Evelyn J. Johnston
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2026-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Spectroscopy Astronomy data modeling Interstellar medium H II regions Astrostatistics
Accés en línia:	https://doi.org/10.3847/1538-4357/ae274b
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