TheHerschel-SPIRE submillimetre spectrum of Mars
نویسندگان
چکیده
منابع مشابه
The Herschel-SPIRE submillimetre spectrum of Mars*
We have obtained the first continuous disk averaged spectrum of Mars from 450 to 1550 Ghz using the Herschel-SPIRE Fourier-transform spectrometer. The spectrum was obtained at a constant resolution of 1.4 GHz across the whole band. The flux from the planet is such that the instrument was operated in “bright source” mode to prevent saturation of the detectors. This was the first successful use o...
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Submillimetre maps of NGC 891 have been obtained with the PRONAOS balloonborne telescope and with the ISOPHOT instrument on board the ISO satellite. In this article, we also gather data from IRAS and SCUBA to present the complete submillimetre spectrum of this nearby edge-on spiral galaxy. We derive submillimetre emission profiles along the major axis. The modified blackbody fits, assuming a si...
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We present colour–colour diagrams of detected sources in the Herschel-ATLAS science demonstration field from 100 to 500 μm using both PACS and SPIRE. We fit isothermal modified black bodies to the spectral energy distribution (SED) to extract the dust temperature of sources with counterparts in Galaxy And Mass Assembly (GAMA) or SDSS surveys with either a spectroscopic or a photometric redshift...
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Emission features from ionized carbon dioxide and carbon monoxide were measured in the 1900- to 4300-angstrom spectral region. The Lyman alpha 1216-angstrom line of atomic hydrogen and the 1304-, 1356-, and 2972-angstrom lines of atomic oxygen were observed.
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R. Nartallo, W. K. Gear, A. G. Murray, E. I Robson and J. H. Hough 1 University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, U.K. 2 Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, U.K. 3 Department of Physics, Queen Mary and Westfield College, Mile End Road, London E1 4NS, U.K. 4 Joint Astronomy Centre, 660 North A’ohōkū Place, University Park, Hilo, Hawaii 96720, USA 5 Division of Ph...
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ژورنال
عنوان ژورنال: Astronomy and Astrophysics
سال: 2010
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361/201014717