The SDSS-V Local Volume Mapper (LVM): Data Analysis Pipeline
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arXiv
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| Main Authors: | , , , , , , , , , , , , |
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| Format: | Preprint |
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2024
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| author | Sanchez, Sebastian F. Mejía-Narvaez, Alfredo Egorov, Oleg V. Kreckel, Kathryn Drory, Niv Blanc, Guillermo A. Méndez-Delgado, J. Eduardo Barrera-Ballesteros, Jorge K. Ibarra, Hector Bizyaev, Dmitry García, Pablo Wofford, Aida Lugo-Aranda, Alejandra Z. |
| author_facet | Sanchez, Sebastian F. Mejía-Narvaez, Alfredo Egorov, Oleg V. Kreckel, Kathryn Drory, Niv Blanc, Guillermo A. Méndez-Delgado, J. Eduardo Barrera-Ballesteros, Jorge K. Ibarra, Hector Bizyaev, Dmitry García, Pablo Wofford, Aida Lugo-Aranda, Alejandra Z. |
| contents | We introduce the Data Analysis Pipeline (DAP) for the Sloan Digital Sky Survey V (SDSS-V) Local Volume Mapper (LVM) project, referred to as the LVM-DAP. We outline our methods for recovering both stellar and emission line components from the optical integral field spectroscopy, highlighting the developments and changes implemented to address specific challenges of the data set. The observations from the LVM project are unique because they cover a wide range of physical resolutions, from approximately 0.05 pc to 100 pc, depending on the distance to the targets. This, along with the varying number of stars sampled in each aperture (ranging from zero, just one of a few, to thousands), presents challenges in using previous spectral synthesis methods and interpreting the spectral fits. We provide a detailed explanation of how we model the stellar content and separate it from the ionized gas emission lines. To assess the accuracy of our results, we compare them with both idealized and more realistic simulations, highlighting the limitations of our methods. We find that the DAP robustly correct for stellar continuum features and recover emission line parameters (e.g. flux, equivalent width, systemtic velocity and velocity dispersion) with a precision and accuracy that fulfill the requirements of the primary goal of the analysis. In addition, the recovered stellar parameters are reliable for single stars, the recovery of integrated populations is less precise. We conclude with a description of the data products we provide, instructions for downloading and using our software, and a showcase illustrating the quality of the data and the analysis on a deep exposure taken on the Huygens region at the center of the Orion Nebula. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2411_09729 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The SDSS-V Local Volume Mapper (LVM): Data Analysis Pipeline Sanchez, Sebastian F. Mejía-Narvaez, Alfredo Egorov, Oleg V. Kreckel, Kathryn Drory, Niv Blanc, Guillermo A. Méndez-Delgado, J. Eduardo Barrera-Ballesteros, Jorge K. Ibarra, Hector Bizyaev, Dmitry García, Pablo Wofford, Aida Lugo-Aranda, Alejandra Z. Instrumentation and Methods for Astrophysics Astrophysics of Galaxies We introduce the Data Analysis Pipeline (DAP) for the Sloan Digital Sky Survey V (SDSS-V) Local Volume Mapper (LVM) project, referred to as the LVM-DAP. We outline our methods for recovering both stellar and emission line components from the optical integral field spectroscopy, highlighting the developments and changes implemented to address specific challenges of the data set. The observations from the LVM project are unique because they cover a wide range of physical resolutions, from approximately 0.05 pc to 100 pc, depending on the distance to the targets. This, along with the varying number of stars sampled in each aperture (ranging from zero, just one of a few, to thousands), presents challenges in using previous spectral synthesis methods and interpreting the spectral fits. We provide a detailed explanation of how we model the stellar content and separate it from the ionized gas emission lines. To assess the accuracy of our results, we compare them with both idealized and more realistic simulations, highlighting the limitations of our methods. We find that the DAP robustly correct for stellar continuum features and recover emission line parameters (e.g. flux, equivalent width, systemtic velocity and velocity dispersion) with a precision and accuracy that fulfill the requirements of the primary goal of the analysis. In addition, the recovered stellar parameters are reliable for single stars, the recovery of integrated populations is less precise. We conclude with a description of the data products we provide, instructions for downloading and using our software, and a showcase illustrating the quality of the data and the analysis on a deep exposure taken on the Huygens region at the center of the Orion Nebula. |
| title | The SDSS-V Local Volume Mapper (LVM): Data Analysis Pipeline |
| topic | Instrumentation and Methods for Astrophysics Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2411.09729 |