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The goal of the "Evolution of interstellar dust" guaranteed time key project (PI: A. Abergel & A. Zavagno) is to
explore with Herschel the far-infrared (FIR) to submillimeter (submm) emission properties of dust particles in a wide
range of regions within our Galaxy, from very diffuse clouds to sites of star formation and proto-stars.
Photometric data taken with SPIRE and PACS are complemented with spectroscopy using the FTS of SPIRE and PACS to derive
the physical conditions of the gas from the lines of [CI], the high-level rotational lines of CO, and the major cooling lines of [CII] and [OI].
If you use SAG-4 data, please cite Abergel et al. (2010).
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SAG-4 Overview
SAG-4 Primary Data Access
