| 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 asample 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, andinfrared activity. Combined with our wealth of ancillary imaging andspatially resolved spectroscopy from the heritage of SINGS/KINGFISH andrelated surveys (ultraviolet, optical, infrared, low-J CO, and radio),the proposed SPIRE/FTS dataset will provide key insights into theprocesses that shape the interstellar medium and govern star formation.Detection of the continuum emission from large grains over 200-650microns will place new constraints on the long-wavelength behavior ofdust emissivity. The richness of the emission line spectrum in thiswavelength regime will allow us to quantify the excitation conditions ofCO over a wide range of environments, and to characterize the physicalproperties of warm and dense gas within galaxies on kiloparsec scales,interpreting these properties using models of photo- andX-ray-dissociated gas, and comparing directly with resolved tracers ofstar formation, heating, and AGN activity. With capabilities unmatchedby existing or planned ground- or space-based facilities, SPIRE/FTSmapping of a well-studied sample of nearby galaxies will serve as acrucial, unique, and lasting foundation for interpreting ALMAobservations of galaxies at high redshift. |
| Publication |
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| 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 |
| Last Update | 2026-03-02 |
| Keywords | Herschel Space Observatory data, ESA Herschel mission dataset, far-infrared astronomy observations, submillimeter astronomy data, infrared space telescope observations, PACS photometer data, PACS spectrometer data, SPIRE photometer data, SPIRE Fourier transform spectrometer data, HIFI heterodyne spectroscopy data, far-infrared spectroscopy dataset, submillimeter spectral line observations, cold universe observations dataset, star formation infrared data, molecular cloud far-infrared observations, interstellar medium spectroscopy data, protoplanetary disk infrared observations, galaxy evolution far-infrared data, dust emission submillimeter observations, cosmic infrared background measurements, extragalactic infrared survey data, calibrated level 2 data products, FITS files astronomy, spectral cubes far-infrared, flux-calibrated maps, continuum photometry data, spectral energy distribution measurements, ESA Herschel Science Archive data |
| 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 |