Spectrum of hot water in the 4750–13 000 cm−1 wavenumber range (0.769–2.1 μm)
The high resolution laboratory spectrum of hot water vapour has been recorded in the 500–13 000 cm−1 wavenumber range and we report on the analysis of the 4750–13 000 cm−1 (0.769–2.1 μm) portion. The emission spectrum was recorded using an oxy-acetylene welding torch and a Fourier transform spectrom...
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2008-07, Vol.387 (3), p.1093-1098 |
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| container_title | Monthly notices of the Royal Astronomical Society |
| container_volume | 387 |
| creator | Zobov, Nikolai F. Shirin, Sergei V. Ovsyannikov, Roman I. Polyansky, Oleg L. Barber, Robert J. Tennyson, Jonathan Bernath, Peter F. Carleer, Michel Colin, Reginald Coheur, Pierre-François |
| description | The high resolution laboratory spectrum of hot water vapour has been recorded in the 500–13 000 cm−1 wavenumber range and we report on the analysis of the 4750–13 000 cm−1 (0.769–2.1 μm) portion. The emission spectrum was recorded using an oxy-acetylene welding torch and a Fourier transform spectrometer. Line assignments in the laboratory spectrum as well as in an absorption spectrum of a sunspot umbra were made with the help of the BT2 line-list. Our torch spectrum is the first laboratory observation of the 9300 Å ‘steam bands’ seen in M-stars and brown dwarfs. |
| doi_str_mv | 10.1111/j.1365-2966.2008.13234.x |
| format | Article |
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The emission spectrum was recorded using an oxy-acetylene welding torch and a Fourier transform spectrometer. Line assignments in the laboratory spectrum as well as in an absorption spectrum of a sunspot umbra were made with the help of the BT2 line-list. Our torch spectrum is the first laboratory observation of the 9300 Å ‘steam bands’ seen in M-stars and brown dwarfs.</description><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Fourier transforms</subject><subject>infrared: stars</subject><subject>line: identification</subject><subject>molecular data</subject><subject>Spectrum analysis</subject><subject>sunspots</subject><subject>Water</subject><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2008</creationdate><recordtype>article</recordtype><recordid>eNqNkElOwzAUhi0EEmW4g8UKFgkeEg8bJIQYVaYCEmJjJcaGBNIUJ6HtjiVruA5n4BA9CW6DWIGEN_aT_-9_7_0AQIxC7M9mHmLK4oBIxkKCkPAloVE4mgOdn4950EGIxoHgGC-CparKEUIRJawDLi8GRteuKWBp4X1Zw2FSGwezPqzvDYx4jCYv75hCD0BdTF7fsFc8m35TpF7mkv6dgeso5Ex6HQkx_PwoNlbAgk0eK7P6fS-Dq73dy52DoHu6f7iz3Q00YSIKNLPcIIM0I9yaWyHjyPqpkESp0FKkMopjbTilRNxaLW1KklRILSllaWqNoctgrfUduPKpMVWt8rJxfd9SEcQpJ1wQLxKtSLuyqpyxauCyInFjhZGaRqhyNU1KTZNS0wjVLEI18uhWiw6zRzP-N6eOT3qzpzegrUHZDP7Ag9_aBi2VVbUZ_XCJe1DMbxWrg-sb1TsSvXN8xlWXfgGXbJUG</recordid><startdate>200807</startdate><enddate>200807</enddate><creator>Zobov, Nikolai F.</creator><creator>Shirin, Sergei V.</creator><creator>Ovsyannikov, Roman I.</creator><creator>Polyansky, Oleg L.</creator><creator>Barber, Robert J.</creator><creator>Tennyson, Jonathan</creator><creator>Bernath, Peter F.</creator><creator>Carleer, Michel</creator><creator>Colin, Reginald</creator><creator>Coheur, Pierre-François</creator><general>Blackwell Publishing Ltd</general><general>Oxford University Press</general><scope>BSCLL</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>200807</creationdate><title>Spectrum of hot water in the 4750–13 000 cm−1 wavenumber range (0.769–2.1 μm)</title><author>Zobov, Nikolai F. ; Shirin, Sergei V. ; Ovsyannikov, Roman I. ; Polyansky, Oleg L. ; Barber, Robert J. ; Tennyson, Jonathan ; Bernath, Peter F. ; Carleer, Michel ; Colin, Reginald ; Coheur, Pierre-François</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c2684-c6f7e0e0c627fed8954f432090b8c98b9455ce73328dfc9fb2ab89c9336bbfee3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2008</creationdate><topic>Astronomy</topic><topic>Astrophysics</topic><topic>Fourier transforms</topic><topic>infrared: stars</topic><topic>line: identification</topic><topic>molecular data</topic><topic>Spectrum analysis</topic><topic>sunspots</topic><topic>Water</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Zobov, Nikolai F.</creatorcontrib><creatorcontrib>Shirin, Sergei V.</creatorcontrib><creatorcontrib>Ovsyannikov, Roman I.</creatorcontrib><creatorcontrib>Polyansky, Oleg L.</creatorcontrib><creatorcontrib>Barber, Robert J.</creatorcontrib><creatorcontrib>Tennyson, Jonathan</creatorcontrib><creatorcontrib>Bernath, Peter F.</creatorcontrib><creatorcontrib>Carleer, Michel</creatorcontrib><creatorcontrib>Colin, Reginald</creatorcontrib><creatorcontrib>Coheur, Pierre-François</creatorcontrib><collection>Istex</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Zobov, Nikolai F.</au><au>Shirin, Sergei V.</au><au>Ovsyannikov, Roman I.</au><au>Polyansky, Oleg L.</au><au>Barber, Robert J.</au><au>Tennyson, Jonathan</au><au>Bernath, Peter F.</au><au>Carleer, Michel</au><au>Colin, Reginald</au><au>Coheur, Pierre-François</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Spectrum of hot water in the 4750–13 000 cm−1 wavenumber range (0.769–2.1 μm)</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><stitle>Monthly Notices of the Royal Astronomical Society</stitle><addtitle>Monthly Notices of the Royal Astronomical Society</addtitle><date>2008-07</date><risdate>2008</risdate><volume>387</volume><issue>3</issue><spage>1093</spage><epage>1098</epage><pages>1093-1098</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>The high resolution laboratory spectrum of hot water vapour has been recorded in the 500–13 000 cm−1 wavenumber range and we report on the analysis of the 4750–13 000 cm−1 (0.769–2.1 μm) portion. The emission spectrum was recorded using an oxy-acetylene welding torch and a Fourier transform spectrometer. Line assignments in the laboratory spectrum as well as in an absorption spectrum of a sunspot umbra were made with the help of the BT2 line-list. Our torch spectrum is the first laboratory observation of the 9300 Å ‘steam bands’ seen in M-stars and brown dwarfs.</abstract><cop>Oxford, UK</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1111/j.1365-2966.2008.13234.x</doi><tpages>6</tpages></addata></record> |
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| subjects | Astronomy Astrophysics Fourier transforms infrared: stars line: identification molecular data Spectrum analysis sunspots Water |
| title | Spectrum of hot water in the 4750–13 000 cm−1 wavenumber range (0.769–2.1 μm) |
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