Full Text Available
Note: Clicking the button above will open the full text document at the original institutional repository in a new window.
The Southern African Large Telescope Fabry-Pérot interferometer has been used in its medium resolution mode to observe three of 30 galaxies of the MHONGOOSE galaxy sample for which very deep HI observation (typically 200 hours/galaxy) will be obtained with MeerKAT. So optical high spatial resolution...
| Main Author: | |
|---|---|
| Other Authors: | |
| Format: | Thesis |
| Language: | English |
| Published: |
Department of Astronomy
2016
|
| Subjects: | |
| Tags: |
No Tags, Be the first to tag this record!
|
| _version_ | 1867613203331022848 |
|---|---|
| access_status_str | Open Access |
| author | Tapsoba, Wendyam Blaise |
| author2 | Williams, Theodore |
| author_browse | Tapsoba, Wendyam Blaise Williams, Theodore |
| author_facet | Williams, Theodore Tapsoba, Wendyam Blaise |
| author_sort | Tapsoba, Wendyam Blaise |
| collection | Thesis |
| description | The Southern African Large Telescope Fabry-Pérot interferometer has been used in its medium resolution mode to observe three of 30 galaxies of the MHONGOOSE galaxy sample for which very deep HI observation (typically 200 hours/galaxy) will be obtained with MeerKAT. So optical high spatial resolution of 2 arcsec data of NGC 7361, NGC 7424 and NGC 7793 have been obtained. The major object of this thesis was to test SALT Fabry-Pérot medium resolution data in order to pursue the survey of all the MHONGOOSE sample, and to be able to compare the accuracy of the kinematic results. Through this work, some FORTRAN based routines have been improved and they allow us to compute kinematic maps with good accuracy. Indeed, the velocities measured from the profiles of the Hα emission in the data cube are accurate with the range of 1 km s⁻¹ to 10 km s⁻¹. So, we computed the kinematic maps and the rotation curves of the three galaxies using DiskFit and ROTCUR. For NGC 7361 and NGC 7424 we compared the rotation curves derived by both methods. For NGC 7793 we were also able to compare our results with previous studies. |
| format | Thesis |
| id | oai:open.uct.ac.za:11427/16494 |
| institution | University of Cape Town (South Africa) |
| language | eng |
| last_indexed | 2026-06-10T12:32:24.523Z |
| license_str | Not specified — see source repository |
| provenance_str_mv | Harvested via OAI-PMH from UCTD — University of Cape Town Open Access Repository |
| publishDate | 2016 |
| publishDateRange | 2016 |
| publishDateSort | 2016 |
| publisher | Department of Astronomy |
| publisherStr | Department of Astronomy |
| record_format | dspace |
| source_str | UCTD — University of Cape Town Open Access Repository |
| spelling | oai:open.uct.ac.za:11427/16494 Analysis of SALT Fabry-Pérot medium resolution data Tapsoba, Wendyam Blaise Williams, Theodore Carignan, Claude Lucero, Danielle M Astrophysics and Space Science The Southern African Large Telescope Fabry-Pérot interferometer has been used in its medium resolution mode to observe three of 30 galaxies of the MHONGOOSE galaxy sample for which very deep HI observation (typically 200 hours/galaxy) will be obtained with MeerKAT. So optical high spatial resolution of 2 arcsec data of NGC 7361, NGC 7424 and NGC 7793 have been obtained. The major object of this thesis was to test SALT Fabry-Pérot medium resolution data in order to pursue the survey of all the MHONGOOSE sample, and to be able to compare the accuracy of the kinematic results. Through this work, some FORTRAN based routines have been improved and they allow us to compute kinematic maps with good accuracy. Indeed, the velocities measured from the profiles of the Hα emission in the data cube are accurate with the range of 1 km s⁻¹ to 10 km s⁻¹. So, we computed the kinematic maps and the rotation curves of the three galaxies using DiskFit and ROTCUR. For NGC 7361 and NGC 7424 we compared the rotation curves derived by both methods. For NGC 7793 we were also able to compare our results with previous studies. 2016-01-21T13:00:56Z 2016-01-21T13:00:56Z 2015 Master Thesis Masters MSc http://hdl.handle.net/11427/16494 eng application/pdf Department of Astronomy Faculty of Science University of Cape Town |
| spellingShingle | Astrophysics and Space Science Tapsoba, Wendyam Blaise Analysis of SALT Fabry-Pérot medium resolution data |
| thesis_degree_str | Master's |
| title | Analysis of SALT Fabry-Pérot medium resolution data |
| title_full | Analysis of SALT Fabry-Pérot medium resolution data |
| title_fullStr | Analysis of SALT Fabry-Pérot medium resolution data |
| title_full_unstemmed | Analysis of SALT Fabry-Pérot medium resolution data |
| title_short | Analysis of SALT Fabry-Pérot medium resolution data |
| title_sort | analysis of salt fabry perot medium resolution data |
| topic | Astrophysics and Space Science |
| url | http://hdl.handle.net/11427/16494 |
| work_keys_str_mv | AT tapsobawendyamblaise analysisofsaltfabryperotmediumresolutiondata |