The Slit-Less Spectroscopic Survey of Galaxies (SPICY) with the InfraRed Camera (IRC) Onboard AKARI (ASTRO-F) Satellite

Details The Slit-Less Spectroscopic Survey of Galaxies (SPICY) with the InfraRed Camera (IRC) Onboard AKARI (ASTRO-F) Satellite The Slit-Less Spectroscopic Survey of Galaxies (SPICY) with the InfraRed Camera (IRC) Onboard AKARI (ASTRO-F) Satellite

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..381..517o&link_type=abstract

The Second Annual Spitzer Science Center Conference: Infrared Diagnostics of Galaxy Evolution. ASP Conference Series, Vol. 381,

Astronomy and Astrophysics

Astronomy

1

Scientific paper

AKARI (formerly ASTRO-F) is a new space telescope for NIR-MIR-FIR observations. The InfraRed Camera (IRC) onboard, covering NIR-MIR, has a capability of low-resolution (R=λ/Δλ=20-50) slit-less spectroscopy, and one can simultaneously obtain spectral information of all objects within the camera's large FOV (10× 10 arcmin^2) over wide wavelength range (2-26μm). To exploit this unique capability, we will perform a deep NIR-MIR spectroscopic survey, the `S'pectrosco`PIC' surve`Y' of galaxies (the `SPICY' mission program), down to ≃ 1 mJy around 15-24μm, to study galaxy evolution at z≃ 0.5-1.0.

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