| dc.contributor.author | Richards, S. | |
| dc.contributor.author | Martin, Bill | |
| dc.contributor.author | Campbell, D. | |
| dc.contributor.author | Jones, H.R.A. | |
| dc.contributor.author | Bland-Hawthorn, J. | |
| dc.contributor.author | Lawrence, J. | |
| dc.contributor.author | Brinks, E. | |
| dc.contributor.author | Bryant, J.J. | |
| dc.contributor.author | Fogarty, L. | |
| dc.contributor.author | Gallaway, M. | |
| dc.contributor.author | Goodwin, M. | |
| dc.contributor.author | Leon-Saval, S. | |
| dc.contributor.author | Sarzi, M. | |
| dc.contributor.author | Smith, Daniel | |
| dc.contributor.editor | Mclean, Ian S. | |
| dc.contributor.editor | Ramsay, Suzanne K. | |
| dc.contributor.editor | Takami, Hideki | |
| dc.date.accessioned | 2014-03-10T09:29:05Z | |
| dc.date.available | 2014-03-10T09:29:05Z | |
| dc.date.issued | 2012-09 | |
| dc.identifier.citation | Richards , S , Martin , B , Campbell , D , Jones , H R A , Bland-Hawthorn , J , Lawrence , J , Brinks , E , Bryant , J J , Fogarty , L , Gallaway , M , Goodwin , M , Leon-Saval , S , Sarzi , M & Smith , D 2012 , BASIS: Bayfordbury single-object integral field spectrograph . in I S Mclean , S K Ramsay & H Takami (eds) , Ground-based and Airborne Instrumentation for Astronomy IV . Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , vol. 8446 , SPIE (International Society for Optics and Phonotics) . https://doi.org/10.1117/12.925378 | |
| dc.identifier.other | Bibtex: urn:40cb5d1df1c4a0ef45427dd9528e479d | |
| dc.identifier.other | ORCID: /0000-0002-7758-9699/work/30407810 | |
| dc.identifier.other | ORCID: /0000-0003-0757-6689/work/41936777 | |
| dc.identifier.other | ORCID: /0000-0001-9708-253X/work/69424326 | |
| dc.identifier.uri | http://hdl.handle.net/2299/13046 | |
| dc.description.abstract | We present an inexpensive (<US$500) and easily replicable integral field unit for use on small aperture telescopes. Based on a commercial small spectrograph (SBIG Self-Guiding Spectrograph) and a 37 optical fibre bundle integral field unit with each fibre having 50μm cores and a pitch of 125μm. It has an overall field-of-view of 40 arc seconds (2.6arcsec/core), a resolution of 9Å from 3995Å to 7170Å and an average system efficiency of 9%, yielding a signal-tonoise ratio of 10 for a 20min exposure of a 13mag/arcsec2 source. Still in commissioning, we present first light observations of Vega and M57. © (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). [Downloading of the abstract is permitted for personal use only] | en |
| dc.language.iso | eng | |
| dc.publisher | SPIE (International Society for Optics and Phonotics) | |
| dc.relation.ispartof | Ground-based and Airborne Instrumentation for Astronomy IV | |
| dc.relation.ispartofseries | Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series | |
| dc.title | BASIS: Bayfordbury single-object integral field spectrograph | en |
| dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | Science & Technology Research Institute | |
| dc.contributor.institution | Centre for Atmospheric and Climate Physics Research | |
| dc.contributor.institution | School of Physics, Engineering & Computer Science | |
| dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | Registry | |
| rioxxterms.versionofrecord | 10.1117/12.925378 | |
| rioxxterms.type | Other | |
| herts.preservation.rarelyaccessed | true | |
