The EDGE-CALIFA Survey: An Extragalactic Database for Galaxy Evolution Studies
Fuente:
arXiv
Enregistré dans:
| Auteurs principaux: | , , , , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Format: | Preprint |
| Publié: |
2024
|
| Sujets: | |
| Accès en ligne: | |
| Tags: |
Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
|
| _version_ | 1866911763477299200 |
|---|---|
| author | Wong, Tony Cao, Yixian Luo, Yufeng Bolatto, Alberto D. Sánchez, Sebastián F. Barrera-Ballesteros, Jorge K. Blitz, Leo Colombo, Dario Dannerbauer, Helmut Green, Alex Kalinova, Veselina Khan, Ferzem Kim, Andrew Lacerda, Eduardo A. D. Leroy, Adam K. Levy, Rebecca C. Lin, Xincheng Luo, Yuanze Rosolowsky, Erik W. Rubio, Mónica Teuben, Peter Utomo, Dyas Villanueva, Vicente Vogel, Stuart N. Wang, Xinyu |
| author_facet | Wong, Tony Cao, Yixian Luo, Yufeng Bolatto, Alberto D. Sánchez, Sebastián F. Barrera-Ballesteros, Jorge K. Blitz, Leo Colombo, Dario Dannerbauer, Helmut Green, Alex Kalinova, Veselina Khan, Ferzem Kim, Andrew Lacerda, Eduardo A. D. Leroy, Adam K. Levy, Rebecca C. Lin, Xincheng Luo, Yuanze Rosolowsky, Erik W. Rubio, Mónica Teuben, Peter Utomo, Dyas Villanueva, Vicente Vogel, Stuart N. Wang, Xinyu |
| contents | The EDGE-CALIFA survey provides spatially resolved optical integral field unit (IFU) and CO spectroscopy for 125 galaxies selected from the CALIFA Data Release 3 sample. The Extragalactic Database for Galaxy Evolution (EDGE) presents the spatially resolved products of the survey as pixel tables that reduce the oversampling in the original images and facilitate comparison of pixels from different images. By joining these pixel tables to lower dimensional tables that provide radial profiles, integrated spectra, or global properties, it is possible to investigate the dependence of local conditions on large-scale properties. The database is freely accessible and has been utilized in several publications. We illustrate the use of this database and highlight the effects of CO upper limits on the inferred slopes of the local scaling relations between stellar mass, star formation rate (SFR), and H$_2$ surface densities. We find that the correlation between H$_2$ and SFR surface density is the tightest among the three relations. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2401_13181 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The EDGE-CALIFA Survey: An Extragalactic Database for Galaxy Evolution Studies Wong, Tony Cao, Yixian Luo, Yufeng Bolatto, Alberto D. Sánchez, Sebastián F. Barrera-Ballesteros, Jorge K. Blitz, Leo Colombo, Dario Dannerbauer, Helmut Green, Alex Kalinova, Veselina Khan, Ferzem Kim, Andrew Lacerda, Eduardo A. D. Leroy, Adam K. Levy, Rebecca C. Lin, Xincheng Luo, Yuanze Rosolowsky, Erik W. Rubio, Mónica Teuben, Peter Utomo, Dyas Villanueva, Vicente Vogel, Stuart N. Wang, Xinyu Astrophysics of Galaxies The EDGE-CALIFA survey provides spatially resolved optical integral field unit (IFU) and CO spectroscopy for 125 galaxies selected from the CALIFA Data Release 3 sample. The Extragalactic Database for Galaxy Evolution (EDGE) presents the spatially resolved products of the survey as pixel tables that reduce the oversampling in the original images and facilitate comparison of pixels from different images. By joining these pixel tables to lower dimensional tables that provide radial profiles, integrated spectra, or global properties, it is possible to investigate the dependence of local conditions on large-scale properties. The database is freely accessible and has been utilized in several publications. We illustrate the use of this database and highlight the effects of CO upper limits on the inferred slopes of the local scaling relations between stellar mass, star formation rate (SFR), and H$_2$ surface densities. We find that the correlation between H$_2$ and SFR surface density is the tightest among the three relations. |
| title | The EDGE-CALIFA Survey: An Extragalactic Database for Galaxy Evolution Studies |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2401.13181 |