Name | OT1_jsmith01_1 |
Title | Beyond the Peak: Resolved Far-Infrared Spectral Mapping of Nearby Galaxies with SPIRE/FTS |
URL | http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342224769&instrument_name=SPIRE&product_level=LEVEL0&compress=true |
DOI | https://doi.org/10.5270/esa-cl6gxmp |
Author | smith, j. d. |
Description | We propose a spatially-resolved far-infrared spectroscopic survey of a sample of 23 nuclear and extranuclear regions within 22 nearby galaxies, selected to represent the broadest range of key physical properties, including luminosity, gas and stellar mass, star-formation density, and infrared activity. Combined with our wealth of ancillary imaging and spatially resolved spectroscopy from the heritage of SINGS/KINGFISH and related surveys (ultraviolet, optical, infrared, low-J CO, and radio), the proposed SPIRE/FTS dataset will provide key insights into the processes that shape the interstellar medium and govern star formation. Detection of the continuum emission from large grains over 200-650 microns will place new constraints on the long-wavelength behavior of dust emissivity. The richness of the emission line spectrum in this wavelength regime will allow us to quantify the excitation conditions of CO over a wide range of environments, and to characterize the physical properties of warm and dense gas within galaxies on kiloparsec scales, interpreting these properties using models of photo- and X-ray-dissociated gas, and comparing directly with resolved tracers of star formation, heating, and AGN activity. With capabilities unmatched by existing or planned ground- or space-based facilities, SPIRE/FTS mapping of a well-studied sample of nearby galaxies will serve as a crucial, unique, and lasting foundation for interpreting ALMA observations of galaxies at high redshift. |
Publication |
|
Instrument | SPIRE_SpireSpectrometer_ |
Temporal Coverage | 2011-07-27T03:57:50Z/2012-10-06T21:52:20Z |
Version | SPG v14.1.0 |
Mission Description | Herschel was launched on 14 May 2009! It is the fourth cornerstone mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities. |
Creator Contact | https://support.cosmos.esa.int/h®erschel/ |
Date Published | 2013-04-06T17:35:05Z |
Keywords | Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, smith et al., 2013, 'Beyond the Peak: Resolved Far-Infrared Spectral Mapping of Nearby Galaxies with SPIRE/FTS', SPG v14.1.0, European Space Agency, https://doi.org/10.5270/esa-cl6gxmp |