pyHIIExplorerV2: a tool for detecting and extracting physical properties from HII regions.
Beyond 1D
Alejandra Zaavik
Lugo Aranda
Date Submitted
2021-04-30 00:00:00
Universidad Nacional Autónoma de México
A. Z. Lugo Aranda & S. F. Sánchez Sánchez
MUSE is the most modern instrument to obtain data with the integral-field spectroscopy technique in the optical range, its high spectral and spatial resolution allows to recover more information than any other IFS instruments. To explore and exploit the information that MUSE provides, we present the code pyHIIExplorerV2 to detect clumpy regions of Halpha maps (candidates to HII regions) and extract as much spectroscopic information as possible (for both the underlying stellar populations and emission lines). Simultaneously during the detection and extraction of the clumpy regions, pyHIIExplorerV2 builds a diffuse ionized gas model (DIG). The construction of DIG will allow us to decontaminate the information of the HII regions candidates.
All attendees are expected to show respect and courtesy to other attendees and staff, and to adhere to the NAM Code of Conduct.