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Grant: Discovery Grants Program - Individual

University of Lethbridge

$69,000.00

Astronomical imaging spectroscopy at far infrared and submillimetre wavelenghts

EF 2012-13

Résumé
My research program is centred on a laboratory for experimental astrophysics. The primary goal of this well-found laboratory is the development of sensitive far-infrared and submillimetre spectrometers and radiometers for use in a range of ground and space-based astronomical projects. Building on a long-standing research program in Fourier transform spectroscopy at the James Clerk Maxwell Telescope and the development of an Infrared Radiometer for Millimetre Astronomy (IRMA), my group leads Canada in two major imaging spectroscopy projects: Herschel/SPIRE and SCUBA-2/FTS-2. Building on this success I am leading Canadian participation on the imaging spectrometer being developed for the Space Infrared Telescope for Cosmology and Astrophysics (SPICA), an exciting new space mission under development by the Japanese and European Space agencies. These projects combine recent advances in array detector technology with Fourier spectrometers to provide a unique spectral imaging capability at far infrared and submillimetre wavelengths. The imaging spectrometers have a wide range of application from the study of star and planet formation to galactic evolution and the early universe. My primary astronomical interests lie in applying this technology to the study of the physics of the interstellar medium as it pertains to star formation.
Programme
Discovery Grants Program - Individual
Emplacement
Alberta, Canada
Type de bénéficiaire
Academia
Type
Grant
Source
NSERC's Awards Data

Tel que publié

Application id
5437-2011
Name nom
Naylor, David
Department département
Physics & Astronomy
Organization id
12
Institution établissement
University of Lethbridge
Province en
Alberta
Province fr
Alberta
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2012
Competition year année de concours
2011
Award amount
69000
Program id
RGPIN
Program name en
Discovery Grants Program - Individual
Program name fr
Programme de subventions à la découverte - individuelles
Group en
Discovery grants programs
Group fr
Programmes de subventions à la découverte
Committee code
1505
Committee name en
Physics
Committee name fr
Physique
Area of application code
1204
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Space and astronomy
Area of application fr
Sciences spatiales et astronomie
Research subject code
3205
Research subject group en
Astronomy and astrophysics
Research subject group fr
Astronomie et astrophysique
Research subject en
Instrumentation
Research subject fr
Instrumentation
Partie
2
Nb partie
5
Application title
Astronomical imaging spectroscopy at far infrared and submillimetre wavelenghts
Keyword
NSERC
Application summary
My research program is centred on a laboratory for experimental astrophysics. The primary goal of this well-found laboratory is the development of sensitive far-infrared and submillimetre spectrometers and radiometers for use in a range of ground and space-based astronomical projects. Building on a long-standing research program in Fourier transform spectroscopy at the James Clerk Maxwell Telescope and the development of an Infrared Radiometer for Millimetre Astronomy (IRMA), my group leads Canada in two major imaging spectroscopy projects: Herschel/SPIRE and SCUBA-2/FTS-2. Building on this success I am leading Canadian participation on the imaging spectrometer being developed for the Space Infrared Telescope for Cosmology and Astrophysics (SPICA), an exciting new space mission under development by the Japanese and European Space agencies. These projects combine recent advances in array detector technology with Fourier spectrometers to provide a unique spectral imaging capability at far infrared and submillimetre wavelengths. The imaging spectrometers have a wide range of application from the study of star and planet formation to galactic evolution and the early universe. My primary astronomical interests lie in applying this technology to the study of the physics of the interstellar medium as it pertains to star formation.