Radio-optical analysis of extended radio sources in the first look survey field
| dc.contributor.advisor | Cress, Catherine Marion | |
| dc.contributor.author | Hons, Claudio Moises Paulo | |
| dc.date.accessioned | 2014-07-07T11:06:05Z | |
| dc.date.accessioned | 2024-10-30T10:23:08Z | |
| dc.date.available | 2014-07-07T11:06:05Z | |
| dc.date.available | 2024-10-30T10:23:08Z | |
| dc.date.issued | 2010 | |
| dc.description | >Magister Scientiae - MSc | en_US |
| dc.description.abstract | I combine 610 MHz Giant Metrewave Radio Telescope (GMRT) data, 1.4 GHz Very Large Array (VLA) data and 1.4 GHz Westerbork Synthesis Radio Telescope (WSRT) observations, encompassing a ∼ 4 square degree field (sq. deg. field) centred on the verification strip of the Spitzer First Look Survey (FLS) field (RA = 17h18m00s, Dec = 59◦30′30′′), to study radio sources down to fluxes of about 0.1 mJy. The results of an analysis of a sample of 107 multi-component radio sources obtained by cross-correlating the VLA and GMRT catalogues are shown. The spectral index analysis shows that the majority of multi-component sources are steep-spectrum sources. Nevertheless the spread in the spectral distribution is wide, with a significant number of ultrasteep,flat or inverted sources. By cross-correlating 107 multi-component radio sources with the optical catalogues of Marleau et al. (2007) and Papovich et al. (2006), 23 objects were identified and spectroscopically classified as galaxies. Some of them are classified as star-forming or star-burst galaxies, perhaps indicating that AGN and starformation activity are ongoing in the same galaxy. The measured redshifts span the range 0 < z < 1.8 and peak at z ∼ 0.2. According to their radio power (P), 6 of the identified objects are in the range of FR II sources (P1.4GHz > 1024.5W/Hz) while 17 are in the range of FR I sources (P1.4GHz < 1024.5W/Hz). Most of the sources having P1.4GHz < 1024.5W/Hz are compact and few are extended and peculiar, while all sources in the range of P1.4GHz > 1024.5W/Hz are extended. Further optical followup is recommended to allow a more complete census of the sub-mJy population and more information on AGN feedback from such sources. | en_US |
| dc.identifier.uri | https://hdl.handle.net/10566/16582 | |
| dc.language.iso | en | en_US |
| dc.subject | Radio astronomy | en_US |
| dc.subject | Sub-mJy population | en_US |
| dc.subject | Telescopes: WSRT, VLA, GMRT | en_US |
| dc.subject | Spitzer FLS field | en_US |
| dc.subject | Optical identification | en_US |
| dc.subject | Galaxies: active | en_US |
| dc.subject | Galaxies: distances and redshifts | en_US |
| dc.subject | Galaxies: evolution | en_US |
| dc.subject | Galaxies: high-redshift | en_US |
| dc.subject | Galaxies: jets | en_US |
| dc.title | Radio-optical analysis of extended radio sources in the first look survey field | en_US |
| dc.type | Thesis | en_US |