A dataset provided by the European Space Agency

Name OT1_bzuckerm_1
Title Do stars with rocky terrestrial planets also have Edgeworth-Kuiper Belts?
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342224222&instrument_name=PACS&product_level=LEVEL0&compress=true
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http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342238833&instrument_name=PACS&product_level=LEVEL0&compress=true
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http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342248726&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342248727&instrument_name=PACS&product_level=LEVEL0&compress=true
DOI https://doi.org/10.5270/esa-rh7vktf
Author zuckerman, b.
Description We propose to measure with PACS the broadband far-infraredspectrum of some young A- and F-type main sequence stars with known,exceptionally luminous, mid-infrared emission. Such stars are uncommonbut are of special interest because they point to and delineate the era ofrocky terrestrial planet formation. Herschel observations will establishwhether cool dusty regions analogous to the Suns Kuiper Belt regionaccompany inner regions where terrestrial planet formation is occurring.
Publication
  • The Absence of Cold Dust around Warm Debris Disk Star HD 15407A | Fujiwara Hideaki et al. | The Astrophysical Journal Letters Volume 759 Issue 1 article id. L18 5 pp. (2012). | 759 | 10.1088/2041-8205/759/1/L18 | 2012ApJ...759L..18F | http://adsabs.harvard.edu/abs/2012ApJ...759L..18F
  • Herschel Observations of Dusty Debris Disks | Vican Laura et al. | The Astrophysical Journal Volume 833 Issue 2 article id. 263 19 pp. (2016). | 833 | 10.3847/1538-4357/833/2/263 | 2016ApJ...833..263V | http://adsabs.harvard.edu/abs/2016ApJ...833..263V
Instrument PACS_PacsPhoto_largeScan
Temporal Coverage 2011-07-15T02:39:32Z/2012-07-27T04:06:26Z
Version SPG v14.2.0
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 2013-01-27T04:03:42Z
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, zuckerman et al., 2013, 'Do stars with rocky terrestrial planets also have Edgeworth-Kuiper Belts?', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-rh7vktf