FIR/submm spectroscopy with Herschel: first results from the VNGS and H-ATLAS surveys
Maarten Baes, Jacopo Fritz, Naseem Rangwala, Pasquale Panuzzo,, Christine D. Wilson, Steve Eales, Ivan Valtchanov, and the VNGS Consortium, and the H-ATLAS Consortium
TL;DR
This paper reports initial results from Herschel's FIR/submm spectroscopic surveys of nearby and distant galaxies, revealing new insights into the interstellar medium's properties in these galaxies.
Contribution
First FIR/submm spectroscopic results from Herschel's VNGS and H-ATLAS surveys, expanding understanding of galaxy ISM in this under-studied wavelength range.
Findings
Initial spectroscopic data on nearby galaxies
Spectroscopic results on distant galaxies
Insights into ISM properties in different galaxy types
Abstract
The FIR/submm window is one of the least-studied regions of the electromagnetic spectrum, yet this wavelength range is absolutely crucial for understanding the physical processes and properties of the ISM in galaxies. The advent of the Herschel Space Observatory has opened up the entire FIR/submm window for spectroscopic studies. We present the first FIR/submm spectroscopic results on both nearby and distant galaxies obtained in the frame of two Herschel key programs: the Very Nearby Galaxies Survey and the Herschel ATLAS.
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