dc.contributor.author | Telesco, C.M. | |
dc.contributor.author | Ciardi, D. | |
dc.contributor.author | French, J. | |
dc.contributor.author | Ftaclas, C. | |
dc.contributor.author | Hanna, K.T. | |
dc.contributor.author | Hough, J. | |
dc.contributor.author | Julian, J. | |
dc.contributor.author | Kidger, M. | |
dc.contributor.author | Packham, C. | |
dc.contributor.author | Pina, R.K. | |
dc.contributor.author | Varosi, F. | |
dc.contributor.author | Sellar, R.G. | |
dc.date.accessioned | 2009-04-16T09:25:12Z | |
dc.date.available | 2009-04-16T09:25:12Z | |
dc.date.issued | 2003 | |
dc.identifier.citation | Telesco , C M , Ciardi , D , French , J , Ftaclas , C , Hanna , K T , Hough , J , Julian , J , Kidger , M , Packham , C , Pina , R K , Varosi , F & Sellar , R G 2003 , CanariCam: a multimode mid-infrared camera for the Gran Telescopio CANARIAS . in Instrument Design and Performance for Optical/Infrared Ground-based Telescopes 4841 . Proceedings of the SPIE , vol. 4841 , Int Soc for Optical Engineering , pp. 913-922 . https://doi.org/10.1117/12.458979 | |
dc.identifier.other | dspace: 2299/3184 | |
dc.identifier.uri | http://hdl.handle.net/2299/3184 | |
dc.description | Copyright 2003 Society of Photo-Optical Instrumentation Engineers. DOI: 10.1117/12.458979 [Full text of this article is not available in the UHRA] | |
dc.description.abstract | The University of Florida is developing a mid-infrared camera for the 10.4-meter Gran Telescopio CANARIAS. CanariCam has four science modes and two engineering modes, which use the same 320 x 240-pixel, arsenic-doped silicon, blocked-impurity-band detector from Raytheon. Each mode can be remotely selected quickly during an observing sequence. The pixel scale is 0.08 arcsec, resulting in Nyquist sampling of the diffraction-limited point-spread-function at 8 μm, the shortest wavelength for which CanariCam is optimized. The total available field of view for imaging is 26 arcsec x 19 arcsec. The primary science mode will be diffraction-limited imaging using one of several available spectral filters in the 10 μm (8-14 μm) and 20 μm (16-25 μm) atmospheric windows. Any one of four plane gratings can be inserted for low and moderate-resolution (R = 100 - 1300) slit spectroscopy in the 10 and 20-μm regions. Insertion of appropriate field and pupil stops converts the camera into a coronagraph, while insertion of an internal rotating half-wave plate, a field mask, and a Wollaston prism converts the camera into a dual-beam polarimeter. | en |
dc.language.iso | eng | |
dc.publisher | Int Soc for Optical Engineering | |
dc.relation.ispartof | Instrument Design and Performance for Optical/Infrared Ground-based Telescopes 4841 | |
dc.relation.ispartofseries | Proceedings of the SPIE | |
dc.title | CanariCam: a multimode mid-infrared camera for the Gran Telescopio CANARIAS | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Department of Management, Leadership and Organisation | |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
rioxxterms.versionofrecord | 10.1117/12.458979 | |
rioxxterms.type | Other | |
herts.preservation.rarelyaccessed | true | |