A medium resolution ground based submillimeter spectrometer
Identifieur interne : 000767 ( Main/Exploration ); précédent : 000766; suivant : 000768A medium resolution ground based submillimeter spectrometer
Auteurs : B. Maffei [France] ; F. Pajot [France] ; T. G. Phillips [États-Unis] ; D. Benford [États-Unis] ; E. Caux [France] ; R. Gispert [France] ; N. Halverson [États-Unis] ; T. Hunter [États-Unis] ; G. Jegoudez [France] ; M. Josse [France] ; J. M. Lamarre [France] ; J. P. Lepeltier [France] ; H. Moseley [États-Unis] ; A. Origné [France] ; S. Petuchowsky [États-Unis] ; M. Rabottin [France] ; J. C. Renault [France] ; C. Rioux [France] ; G. Serabyn [États-Unis] ; N. Wang [États-Unis]Source :
- Infrared Physics and Technology [ 1350-4495 ] ; 1994.
Abstract
We present a Submillimeter spectrometer based on a cooled scanning Fabry-Pérot working at 1.4 K temperature and using gold inductive grids deposited on quartz substrates as reflective faces. The detection is achieved by an array of 24 silicon bolometers cooled at 0. l K by an adiabatic demagnetization refrigerator. This spectrometer will be operated at the focus of the 10 m ground based antenna of the Caltech Submillimeter Observatory and is the precursor of balloon borne or space instruments. It is mainly dedicated to high redshift galaxy observations, and especially to the CII line (158 μm) studies in these objects. The observations will be carried out in two atmospheric windows centered on 350 and 450 μm, and the spectrometer will be able to detect galaxies at a redshift of about 1–2 with a FIR luminosity of a few l012L⊙.
Url:
DOI: 10.1016/1350-4495(94)90090-6
Affiliations:
- France, États-Unis
- Aquitaine, Midi-Pyrénées, Nouvelle-Aquitaine, Occitanie (région administrative), Provence-Alpes-Côte d'Azur, Île-de-France
- Le Barp, Marseille, Orsay, Paris, Toulouse
- Université Paris-Sud
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Halverson</name></author><author><name sortKey="Hunter, T" sort="Hunter, T" uniqKey="Hunter T" first="T." last="Hunter">T. Hunter</name></author><author><name sortKey="Jegoudez, G" sort="Jegoudez, G" uniqKey="Jegoudez G" first="G." last="Jegoudez">G. Jegoudez</name></author><author><name sortKey="Josse, M" sort="Josse, M" uniqKey="Josse M" first="M." last="Josse">M. Josse</name></author><author><name sortKey="Lamarre, J M" sort="Lamarre, J M" uniqKey="Lamarre J" first="J. M." last="Lamarre">J. M. Lamarre</name></author><author><name sortKey="Lepeltier, J P" sort="Lepeltier, J P" uniqKey="Lepeltier J" first="J. P." last="Lepeltier">J. P. Lepeltier</name></author><author><name sortKey="Moseley, H" sort="Moseley, H" uniqKey="Moseley H" first="H." last="Moseley">H. Moseley</name></author><author><name sortKey="Origne, A" sort="Origne, A" uniqKey="Origne A" first="A." last="Origné">A. 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Downs Laboratory of Physics, Mail Stop 320-47, Pasadena, CA 91125</wicri:regionArea><wicri:noRegion>CA 91125</wicri:noRegion></affiliation></author><author><name sortKey="Wang, N" sort="Wang, N" uniqKey="Wang N" first="N." last="Wang">N. Wang</name><affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country><wicri:regionArea>CALTECH, G.W. Downs Laboratory of Physics, Mail Stop 320-47, Pasadena, CA 91125</wicri:regionArea><wicri:noRegion>CA 91125</wicri:noRegion></affiliation></author></analytic><monogr></monogr><series><title level="j">Infrared Physics and Technology</title><title level="j" type="abbrev">INFPHY</title><idno type="ISSN">1350-4495</idno><imprint><publisher>ELSEVIER</publisher><date type="published" when="1994">1994</date><biblScope unit="volume">35</biblScope><biblScope unit="issue">2–3</biblScope><biblScope unit="page" from="321">321</biblScope><biblScope unit="page" to="329">329</biblScope></imprint><idno type="ISSN">1350-4495</idno></series><idno type="istex">EF4158A86384D8B49D70A2F7B4EF2F932D175545</idno><idno type="DOI">10.1016/1350-4495(94)90090-6</idno><idno type="PII">1350-4495(94)90090-6</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">1350-4495</idno></seriesStmt></fileDesc><profileDesc><textClass></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">We present a Submillimeter spectrometer based on a cooled scanning Fabry-Pérot working at 1.4 K temperature and using gold inductive grids deposited on quartz substrates as reflective faces. The detection is achieved by an array of 24 silicon bolometers cooled at 0. l K by an adiabatic demagnetization refrigerator. This spectrometer will be operated at the focus of the 10 m ground based antenna of the Caltech Submillimeter Observatory and is the precursor of balloon borne or space instruments. It is mainly dedicated to high redshift galaxy observations, and especially to the CII line (158 μm) studies in these objects. The observations will be carried out in two atmospheric windows centered on 350 and 450 μm, and the spectrometer will be able to detect galaxies at a redshift of about 1–2 with a FIR luminosity of a few l012L⊙.</div></front></TEI><affiliations><list><country><li>France</li><li>États-Unis</li></country><region><li>Aquitaine</li><li>Midi-Pyrénées</li><li>Nouvelle-Aquitaine</li><li>Occitanie (région administrative)</li><li>Provence-Alpes-Côte d'Azur</li><li>Île-de-France</li></region><settlement><li>Le Barp</li><li>Marseille</li><li>Orsay</li><li>Paris</li><li>Toulouse</li></settlement><orgName><li>Université Paris-Sud</li></orgName></list><tree><country name="France"><region name="Île-de-France"><name sortKey="Maffei, B" sort="Maffei, B" uniqKey="Maffei B" first="B." last="Maffei">B. Maffei</name></region><name sortKey="Caux, E" sort="Caux, E" uniqKey="Caux E" first="E." last="Caux">E. Caux</name><name sortKey="Gispert, R" sort="Gispert, R" uniqKey="Gispert R" first="R." last="Gispert">R. Gispert</name><name sortKey="Jegoudez, G" sort="Jegoudez, G" uniqKey="Jegoudez G" first="G." last="Jegoudez">G. Jegoudez</name><name sortKey="Josse, M" sort="Josse, M" uniqKey="Josse M" first="M." last="Josse">M. Josse</name><name sortKey="Lamarre, J M" sort="Lamarre, J M" uniqKey="Lamarre J" first="J. M." last="Lamarre">J. M. Lamarre</name><name sortKey="Lepeltier, J P" sort="Lepeltier, J P" uniqKey="Lepeltier J" first="J. P." last="Lepeltier">J. P. Lepeltier</name><name sortKey="Origne, A" sort="Origne, A" uniqKey="Origne A" first="A." last="Origné">A. Origné</name><name sortKey="Pajot, F" sort="Pajot, F" uniqKey="Pajot F" first="F." last="Pajot">F. Pajot</name><name sortKey="Rabottin, M" sort="Rabottin, M" uniqKey="Rabottin M" first="M." last="Rabottin">M. Rabottin</name><name sortKey="Renault, J C" sort="Renault, J C" uniqKey="Renault J" first="J. C." last="Renault">J. C. Renault</name><name sortKey="Rioux, C" sort="Rioux, C" uniqKey="Rioux C" first="C." last="Rioux">C. Rioux</name></country><country name="États-Unis"><noRegion><name sortKey="Phillips, T G" sort="Phillips, T G" uniqKey="Phillips T" first="T. G." last="Phillips">T. G. Phillips</name></noRegion><name sortKey="Benford, D" sort="Benford, D" uniqKey="Benford D" first="D." last="Benford">D. Benford</name><name sortKey="Halverson, N" sort="Halverson, N" uniqKey="Halverson N" first="N." last="Halverson">N. Halverson</name><name sortKey="Hunter, T" sort="Hunter, T" uniqKey="Hunter T" first="T." last="Hunter">T. Hunter</name><name sortKey="Moseley, H" sort="Moseley, H" uniqKey="Moseley H" first="H." last="Moseley">H. Moseley</name><name sortKey="Petuchowsky, S" sort="Petuchowsky, S" uniqKey="Petuchowsky S" first="S." last="Petuchowsky">S. Petuchowsky</name><name sortKey="Serabyn, G" sort="Serabyn, G" uniqKey="Serabyn G" first="G." last="Serabyn">G. Serabyn</name><name sortKey="Wang, N" sort="Wang, N" uniqKey="Wang N" first="N." last="Wang">N. Wang</name></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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