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A dynamic database of molecular model spectra. ISO-SWS data… A model spectrum T=650K, N=2.75 10 16 cm -2 What spectrafactory is…

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Presentation on theme: "A dynamic database of molecular model spectra. ISO-SWS data… A model spectrum T=650K, N=2.75 10 16 cm -2 What spectrafactory is…"— Presentation transcript:

1 A dynamic database of molecular model spectra

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3 ISO-SWS data… A model spectrum T=650K, N=2.75 10 16 cm -2 What spectrafactory is…

4 observations according to ajmk & jc Science Proposals Observations > Science

5 > Data reduction – makes data useable … helped by various packages Data analysis – makes data useful … helped by …. ?? >

6 Find line list Understand (!) and implement line list Radiative Transfer Convolve with instrumental profile Fit spectrum What spectrafactory is…

7 ISO-SWS data… A model spectrum T=650K, N=2.75 10 16 cm -2 What spectrafactory is…

8 in an ideal world… Observed Spectrum Black box Perfect FitPhysical/chemical parameters

9 in the spectrafactory world Observed Spectrum Grey box Best FitEstimate of Physical/chemical parameters given limitations

10 Black boxGrey box All possible molecular speciesWhat’s available All possible transitionsWhat’s available Full non-LTE radiative transfer Isotherm, LTE Various geometriesSlab All possible instruments On request

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15 search…

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17 plot…

18 compare

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20 zoom…

21 search by line position

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24 compare linelists

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33 download…

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35 request…

36 Currently… moleculesisotopologues temperatures (100 – 2500 K) column densities (10 12 – 10 24 cm -2 ) instrument profiles spectra, 0.3 – 3000 micron Spitzer-IRS LowRes1, LowRes2, HiRes ISO-SWS AOT1, speed1; IRTF SpeX, +LowRes VLT-ISAAC LW MedRes content is community-driven

37 Molecular species molecules detected in space most in sub-mm including isotopologues molecules studied in earth atmosphere line lists available at 296 K (HITRAN) often infrared molecules with good line lists (that we have) H 2 O, TiO, SiO, CO, CO 2 Large frequency range Many levels (electronic, vibrational, rotational) High temperatures

38 Needs & future prospects More / better line lists Need line lists for more species Availability is the only limit! Funding This project is 0% funded Observatories Spitzer (now), soon SOFIA, Herschel, ALMA, … Features Solid state, sub-mm, manipulation, fits, emission, obs. upload, line profiles, wdsr

39 We acknowledge Of course, the line lists HITRAN 04 multiple HITEMP CO CO 2 H 2 O CDSD CO 2 Partridge & Schwenke H 2 O Schwenke TiO Goldman OH Goorvitch CO Langhoff & Bauschlicher SiO


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