Mid‐infrared spectroscopy of infrared‐luminous galaxies at z∼ 0.5–3
Identifieur interne : 000130 ( Main/Exploration ); précédent : 000129; suivant : 000131Mid‐infrared spectroscopy of infrared‐luminous galaxies at z∼ 0.5–3
Auteurs : A. Hernán-Caballero [Espagne] ; I. Pérez-Fournon [Espagne] ; E. Hatziminaoglou [Allemagne] ; A. Afonso-Luis [Espagne] ; M. Rowan-Robinson ; D. Rigopoulou ; D. Farrah [États-Unis] ; C. J. Lonsdale [États-Unis] ; T. Babbedge ; D. Clements ; S. Serjeant ; F. Pozzi [Italie] ; M. Vaccari [Italie] ; F. M. Montenegro-Montes [Espagne, Italie] ; I. Valtchanov [Espagne] ; E. González-Solares ; S. Oliver ; D. Shupe [États-Unis] ; C. Gruppioni [Italie] ; B. Vila-Vilar [États-Unis] ; C. Lari [Italie] ; F. La Franca [Italie]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2009-05-21.
English descriptors
Abstract
We present results on low‐resolution mid‐infrared (MIR) spectra of 70 IR‐luminous galaxies obtained with the infrared spectrograph (IRS) onboard Spitzer. We selected sources from the European Large Area Infrared Survey with S15 > 0.8 mJy and photometric or spectroscopic z > 1. About half of the samples are quasi‐stellar objects (QSOs) in the optical, while the remaining sources are galaxies, comprising both obscured active galactic nuclei (AGN) and starbursts. Redshifts were obtained from optical spectroscopy, photometric redshifts and the IRS spectra. The later turn out to be reliable for obscured and/or star‐forming sources, thus becoming an ideal complement to optical spectroscopy for redshift estimation. We estimate monochromatic luminosities at several rest‐frame wavelengths, equivalent widths and luminosities for the polycyclic aromatic hydrocarbon (PAH) features, and strength of the silicate feature in individual spectra. We also estimate integrated 8–1000 μm IR luminosities via spectral energy distribution fitting to MIR and far‐IR (FIR) photometry from the Spitzer Wide‐Area Infrared Extragalactic survey and the MIR spectrum. Based on these measurements, we classify the spectra using well‐known IR diagnostics, as well as a new one that we propose, into three types of source: those dominated by an unobscured AGN, mostly corresponding to optical quasars (QSOs), those dominated by an obscured AGN and starburst‐dominated sources. Starbursts concentrate at z∼ 0.6–1.0 favoured by the shift of the 7.7‐μm PAH band into the selection 15‐μm band, while AGN spread over the 0.5 < z < 3.1 range. Star formation rates (SFR) are estimated for individual sources from the luminosity of the PAH features. An estimate of the average PAH luminosity in QSOs and obscured AGN is obtained from the composite spectrum of all sources with reliable redshifts. The estimated mean SFR in the QSOs is 50–100 M⊙ yr−1, but the implied FIR luminosity is 3–10 times lower than that obtained from stacking analysis of the FIR photometry, suggesting destruction of the PAH carriers by energetic photons from the AGN. The SFR estimated in obscured AGN is two to three times higher than in QSOs of similar MIR luminosity. This discrepancy might not be due to luminosity effects or selection bias alone, but could instead indicate a connection between obscuration and star formation. However, the observed correlation between silicate absorption and the slope of the NIR to MIR spectrum is compatible with the obscuration of the AGN emission in these sources being produced in a dust torus.
Url:
DOI: 10.1111/j.1365-2966.2009.14660.x
Affiliations:
- Allemagne, Espagne, Italie, États-Unis
- Bavière, Canaries, Communauté de Madrid, District de Haute-Bavière, Latium, Vénétie, Émilie-Romagne, État de New York
- Bologne, Garching bei München, Ithaca (New York), Madrid, Padoue, Rome
- Université Cornell, Université de Bologne, Université de Padoue
Links toward previous steps (curation, corpus...)
Le document en format XML
<record><TEI wicri:istexFullTextTei="biblStruct"><teiHeader><fileDesc><titleStmt><title xml:lang="en">Mid‐infrared spectroscopy of infrared‐luminous galaxies at z∼ 0.5–3</title><author><name sortKey="Hernan Aballero, A" sort="Hernan Aballero, A" uniqKey="Hernan Aballero A" first="A." last="Hernán-Caballero">A. Hernán-Caballero</name></author><author><name sortKey="Perez Ournon, I" sort="Perez Ournon, I" uniqKey="Perez Ournon I" first="I." last="Pérez-Fournon">I. Pérez-Fournon</name></author><author><name sortKey="Hatziminaoglou, E" sort="Hatziminaoglou, E" uniqKey="Hatziminaoglou E" first="E." last="Hatziminaoglou">E. Hatziminaoglou</name></author><author><name sortKey="Afonso Uis, A" sort="Afonso Uis, A" uniqKey="Afonso Uis A" first="A." last="Afonso-Luis">A. Afonso-Luis</name></author><author><name sortKey="Rowan Obinson, M" sort="Rowan Obinson, M" uniqKey="Rowan Obinson M" first="M." last="Rowan-Robinson">M. Rowan-Robinson</name></author><author><name sortKey="Rigopoulou, D" sort="Rigopoulou, D" uniqKey="Rigopoulou D" first="D." last="Rigopoulou">D. Rigopoulou</name></author><author><name sortKey="Farrah, D" sort="Farrah, D" uniqKey="Farrah D" first="D." last="Farrah">D. Farrah</name></author><author><name sortKey="Lonsdale, C J" sort="Lonsdale, C J" uniqKey="Lonsdale C" first="C. J." last="Lonsdale">C. J. Lonsdale</name></author><author><name sortKey="Babbedge, T" sort="Babbedge, T" uniqKey="Babbedge T" first="T." last="Babbedge">T. Babbedge</name></author><author><name sortKey="Clements, D" sort="Clements, D" uniqKey="Clements D" first="D." last="Clements">D. Clements</name></author><author><name sortKey="Serjeant, S" sort="Serjeant, S" uniqKey="Serjeant S" first="S." last="Serjeant">S. Serjeant</name></author><author><name sortKey="Pozzi, F" sort="Pozzi, F" uniqKey="Pozzi F" first="F." last="Pozzi">F. Pozzi</name></author><author><name sortKey="Vaccari, M" sort="Vaccari, M" uniqKey="Vaccari M" first="M." last="Vaccari">M. Vaccari</name></author><author><name sortKey="Montenegro Ontes, F M" sort="Montenegro Ontes, F M" uniqKey="Montenegro Ontes F" first="F. M." last="Montenegro-Montes">F. M. Montenegro-Montes</name></author><author><name sortKey="Valtchanov, I" sort="Valtchanov, I" uniqKey="Valtchanov I" first="I." last="Valtchanov">I. Valtchanov</name></author><author><name sortKey="Gonzalez Olares, E" sort="Gonzalez Olares, E" uniqKey="Gonzalez Olares E" first="E." last="González-Solares">E. González-Solares</name></author><author><name sortKey="Oliver, S" sort="Oliver, S" uniqKey="Oliver S" first="S." last="Oliver">S. Oliver</name></author><author><name sortKey="Shupe, D" sort="Shupe, D" uniqKey="Shupe D" first="D." last="Shupe">D. Shupe</name></author><author><name sortKey="Gruppioni, C" sort="Gruppioni, C" uniqKey="Gruppioni C" first="C." last="Gruppioni">C. Gruppioni</name></author><author><name sortKey="Vila Ilar, B" sort="Vila Ilar, B" uniqKey="Vila Ilar B" first="B." last="Vila-Vilar">B. Vila-Vilar</name></author><author><name sortKey="Lari, C" sort="Lari, C" uniqKey="Lari C" first="C." last="Lari">C. Lari</name></author><author><name sortKey="Franca, F La" sort="Franca, F La" uniqKey="Franca F" first="F. La" last="Franca">F. La Franca</name></author></titleStmt><publicationStmt><idno type="wicri:source">ISTEX</idno><idno type="RBID">ISTEX:037B92F95BE3FC2E745738718BAAA8B939A1A6F5</idno><date when="2009" year="2009">2009</date><idno type="doi">10.1111/j.1365-2966.2009.14660.x</idno><idno type="url">https://api.istex.fr/document/037B92F95BE3FC2E745738718BAAA8B939A1A6F5/fulltext/pdf</idno><idno type="wicri:Area/Main/Corpus">000961</idno><idno type="wicri:Area/Main/Curation">000961</idno><idno type="wicri:Area/Main/Exploration">000130</idno><idno type="wicri:explorRef" wicri:stream="Main" wicri:step="Exploration">000130</idno></publicationStmt><sourceDesc><biblStruct><analytic><title level="a" type="main" xml:lang="en">Mid‐infrared spectroscopy of infrared‐luminous galaxies at z∼ 0.5–3</title><author><name sortKey="Hernan Aballero, A" sort="Hernan Aballero, A" uniqKey="Hernan Aballero A" first="A." last="Hernán-Caballero">A. Hernán-Caballero</name><affiliation wicri:level="2"><country xml:lang="fr">Espagne</country><wicri:regionArea>Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, E‐38200 La Laguna</wicri:regionArea><placeName><region nuts="2" type="communauté">Canaries</region></placeName></affiliation></author><author><name sortKey="Perez Ournon, I" sort="Perez Ournon, I" uniqKey="Perez Ournon I" first="I." last="Pérez-Fournon">I. Pérez-Fournon</name><affiliation wicri:level="2"><country xml:lang="fr">Espagne</country><wicri:regionArea>Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, E‐38200 La Laguna</wicri:regionArea><placeName><region nuts="2" type="communauté">Canaries</region></placeName></affiliation></author><author><name sortKey="Hatziminaoglou, E" sort="Hatziminaoglou, E" uniqKey="Hatziminaoglou E" first="E." last="Hatziminaoglou">E. Hatziminaoglou</name><affiliation wicri:level="3"><country xml:lang="fr">Allemagne</country><wicri:regionArea>European Southern Observatory, Karl‐Schwarzschild‐Str. 2, 85748 Garching bei München</wicri:regionArea><placeName><region type="land" nuts="1">Bavière</region><region type="district" nuts="2">District de Haute-Bavière</region><settlement type="city">Garching bei München</settlement></placeName></affiliation></author><author><name sortKey="Afonso Uis, A" sort="Afonso Uis, A" uniqKey="Afonso Uis A" first="A." last="Afonso-Luis">A. Afonso-Luis</name><affiliation wicri:level="2"><country xml:lang="fr">Espagne</country><wicri:regionArea>Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, E‐38200 La Laguna</wicri:regionArea><placeName><region nuts="2" type="communauté">Canaries</region></placeName></affiliation></author><author><name sortKey="Rowan Obinson, M" sort="Rowan Obinson, M" uniqKey="Rowan Obinson M" first="M." last="Rowan-Robinson">M. Rowan-Robinson</name><affiliation><wicri:noCountry code="subField">2BW</wicri:noCountry></affiliation></author><author><name sortKey="Rigopoulou, D" sort="Rigopoulou, D" uniqKey="Rigopoulou D" first="D." last="Rigopoulou">D. Rigopoulou</name><affiliation><wicri:noCountry code="subField">3RH</wicri:noCountry></affiliation></author><author><name sortKey="Farrah, D" sort="Farrah, D" uniqKey="Farrah D" first="D." last="Farrah">D. Farrah</name><affiliation wicri:level="4"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Astronomy, Cornell University, Space Sciences Building, Ithaca, NY 14853</wicri:regionArea><orgName type="university">Université Cornell</orgName><placeName><settlement type="city">Ithaca (New York)</settlement><region type="state">État de New York</region></placeName></affiliation><affiliation></affiliation></author><author><name sortKey="Lonsdale, C J" sort="Lonsdale, C J" uniqKey="Lonsdale C" first="C. J." last="Lonsdale">C. J. Lonsdale</name><affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125</wicri:regionArea><wicri:noRegion>CA 91125</wicri:noRegion></affiliation></author><author><name sortKey="Babbedge, T" sort="Babbedge, T" uniqKey="Babbedge T" first="T." last="Babbedge">T. Babbedge</name><affiliation><wicri:noCountry code="subField">2BW</wicri:noCountry></affiliation></author><author><name sortKey="Clements, D" sort="Clements, D" uniqKey="Clements D" first="D." last="Clements">D. Clements</name><affiliation><wicri:noCountry code="subField">2BW</wicri:noCountry></affiliation></author><author><name sortKey="Serjeant, S" sort="Serjeant, S" uniqKey="Serjeant S" first="S." last="Serjeant">S. Serjeant</name><affiliation><wicri:noCountry code="subField">7NR</wicri:noCountry></affiliation></author><author><name sortKey="Pozzi, F" sort="Pozzi, F" uniqKey="Pozzi F" first="F." last="Pozzi">F. Pozzi</name><affiliation wicri:level="4"><country xml:lang="fr">Italie</country><wicri:regionArea>Dipartimento di Astronomia, Università di Bologna, via Ranzani 1, I‐40127 Bologna</wicri:regionArea><orgName type="university">Université de Bologne</orgName><placeName><settlement type="city">Bologne</settlement><region nuts="2" type="region">Émilie-Romagne</region></placeName></affiliation></author><author><name sortKey="Vaccari, M" sort="Vaccari, M" uniqKey="Vaccari M" first="M." last="Vaccari">M. Vaccari</name><affiliation></affiliation><affiliation wicri:level="4"><country xml:lang="fr">Italie</country><wicri:regionArea>Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 5, 35122 Padua</wicri:regionArea><orgName type="university">Université de Padoue</orgName><placeName><settlement type="city">Padoue</settlement><region type="region" nuts="2">Vénétie</region></placeName></affiliation></author><author><name sortKey="Montenegro Ontes, F M" sort="Montenegro Ontes, F M" uniqKey="Montenegro Ontes F" first="F. M." last="Montenegro-Montes">F. M. Montenegro-Montes</name><affiliation wicri:level="2"><country xml:lang="fr">Espagne</country><wicri:regionArea>Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, E‐38200 La Laguna</wicri:regionArea><placeName><region nuts="2" type="communauté">Canaries</region></placeName></affiliation><affiliation wicri:level="1"><country xml:lang="fr">Italie</country><wicri:regionArea>Istituto di Radioastronomia, INAF, Via Gobetti 101, I‐40129 Bologna</wicri:regionArea><wicri:noRegion>I‐40129 Bologna</wicri:noRegion></affiliation></author><author><name sortKey="Valtchanov, I" sort="Valtchanov, I" uniqKey="Valtchanov I" first="I." last="Valtchanov">I. Valtchanov</name><affiliation></affiliation><affiliation wicri:level="3"><country xml:lang="fr">Espagne</country><wicri:regionArea>ESA European Space Astronomy Centre, PO Box 78, 28691 Villanueva de la Cañada, Madrid</wicri:regionArea><placeName><settlement type="city">Madrid</settlement><region nuts="2" type="region">Communauté de Madrid</region></placeName></affiliation></author><author><name sortKey="Gonzalez Olares, E" sort="Gonzalez Olares, E" uniqKey="Gonzalez Olares E" first="E." last="González-Solares">E. González-Solares</name><affiliation><wicri:noCountry code="subField">0HA</wicri:noCountry></affiliation></author><author><name sortKey="Oliver, S" sort="Oliver, S" uniqKey="Oliver S" first="S." last="Oliver">S. Oliver</name><affiliation><wicri:noCountry code="subField">9QJ</wicri:noCountry></affiliation></author><author><name sortKey="Shupe, D" sort="Shupe, D" uniqKey="Shupe D" first="D." last="Shupe">D. Shupe</name><affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Spitzer Science Center, MS 220‐6, Caltech, Jet Propulsion Lab, Pasadena, CA 91125</wicri:regionArea><wicri:noRegion>CA 91125</wicri:noRegion></affiliation></author><author><name sortKey="Gruppioni, C" sort="Gruppioni, C" uniqKey="Gruppioni C" first="C." last="Gruppioni">C. Gruppioni</name><affiliation wicri:level="1"><country xml:lang="fr">Italie</country><wicri:regionArea>INAF ‐ Osservatorio Astronomico di Bologna, via Ranzani 1, I‐40127 Bologna</wicri:regionArea><wicri:noRegion>I‐40127 Bologna</wicri:noRegion></affiliation></author><author><name sortKey="Vila Ilar, B" sort="Vila Ilar, B" uniqKey="Vila Ilar B" first="B." last="Vila-Vilar">B. Vila-Vilar</name><affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country><wicri:regionArea>University of Arizona, Steward Observatory, 933 N. Cherry Ave., Tucson, AZ 85721</wicri:regionArea><wicri:noRegion>AZ 85721</wicri:noRegion></affiliation></author><author><name sortKey="Lari, C" sort="Lari, C" uniqKey="Lari C" first="C." last="Lari">C. Lari</name><affiliation wicri:level="1"><country xml:lang="fr">Italie</country><wicri:regionArea>Istituto di Radioastronomia, INAF, Via Gobetti 101, I‐40129 Bologna</wicri:regionArea><wicri:noRegion>I‐40129 Bologna</wicri:noRegion></affiliation></author><author><name sortKey="Franca, F La" sort="Franca, F La" uniqKey="Franca F" first="F. La" last="Franca">F. La Franca</name><affiliation wicri:level="1"><country xml:lang="fr">Italie</country><wicri:regionArea>Dipartimento di Fisica, Università degli Studi Roma Tre, via della Vasca Navale 84, 00146 Roma</wicri:regionArea><placeName><settlement type="city">Rome</settlement><region nuts="2">Latium</region></placeName></affiliation></author></analytic><monogr></monogr><series><title level="j">Monthly Notices of the Royal Astronomical Society</title><idno type="ISSN">0035-8711</idno><idno type="eISSN">1365-2966</idno><imprint><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2009-05-21">2009-05-21</date><biblScope unit="volume">395</biblScope><biblScope unit="issue">3</biblScope><biblScope unit="page" from="1695">1695</biblScope><biblScope unit="page" to="1722">1722</biblScope></imprint><idno type="ISSN">0035-8711</idno></series><idno type="istex">037B92F95BE3FC2E745738718BAAA8B939A1A6F5</idno><idno type="DOI">10.1111/j.1365-2966.2009.14660.x</idno><idno type="ArticleID">MNR14660</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>galaxies: active</term><term>galaxies: high‐redshift</term><term>galaxies: starburst</term><term>quasars: general</term></keywords></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">We present results on low‐resolution mid‐infrared (MIR) spectra of 70 IR‐luminous galaxies obtained with the infrared spectrograph (IRS) onboard Spitzer. We selected sources from the European Large Area Infrared Survey with S15 > 0.8 mJy and photometric or spectroscopic z > 1. About half of the samples are quasi‐stellar objects (QSOs) in the optical, while the remaining sources are galaxies, comprising both obscured active galactic nuclei (AGN) and starbursts. Redshifts were obtained from optical spectroscopy, photometric redshifts and the IRS spectra. The later turn out to be reliable for obscured and/or star‐forming sources, thus becoming an ideal complement to optical spectroscopy for redshift estimation. We estimate monochromatic luminosities at several rest‐frame wavelengths, equivalent widths and luminosities for the polycyclic aromatic hydrocarbon (PAH) features, and strength of the silicate feature in individual spectra. We also estimate integrated 8–1000 μm IR luminosities via spectral energy distribution fitting to MIR and far‐IR (FIR) photometry from the Spitzer Wide‐Area Infrared Extragalactic survey and the MIR spectrum. Based on these measurements, we classify the spectra using well‐known IR diagnostics, as well as a new one that we propose, into three types of source: those dominated by an unobscured AGN, mostly corresponding to optical quasars (QSOs), those dominated by an obscured AGN and starburst‐dominated sources. Starbursts concentrate at z∼ 0.6–1.0 favoured by the shift of the 7.7‐μm PAH band into the selection 15‐μm band, while AGN spread over the 0.5 < z < 3.1 range. Star formation rates (SFR) are estimated for individual sources from the luminosity of the PAH features. An estimate of the average PAH luminosity in QSOs and obscured AGN is obtained from the composite spectrum of all sources with reliable redshifts. The estimated mean SFR in the QSOs is 50–100 M⊙ yr−1, but the implied FIR luminosity is 3–10 times lower than that obtained from stacking analysis of the FIR photometry, suggesting destruction of the PAH carriers by energetic photons from the AGN. The SFR estimated in obscured AGN is two to three times higher than in QSOs of similar MIR luminosity. This discrepancy might not be due to luminosity effects or selection bias alone, but could instead indicate a connection between obscuration and star formation. However, the observed correlation between silicate absorption and the slope of the NIR to MIR spectrum is compatible with the obscuration of the AGN emission in these sources being produced in a dust torus.</div></front></TEI><affiliations><list><country><li>Allemagne</li><li>Espagne</li><li>Italie</li><li>États-Unis</li></country><region><li>Bavière</li><li>Canaries</li><li>Communauté de Madrid</li><li>District de Haute-Bavière</li><li>Latium</li><li>Vénétie</li><li>Émilie-Romagne</li><li>État de New York</li></region><settlement><li>Bologne</li><li>Garching bei München</li><li>Ithaca (New York)</li><li>Madrid</li><li>Padoue</li><li>Rome</li></settlement><orgName><li>Université Cornell</li><li>Université de Bologne</li><li>Université de Padoue</li></orgName></list><tree><noCountry><name sortKey="Babbedge, T" sort="Babbedge, T" uniqKey="Babbedge T" first="T." last="Babbedge">T. Babbedge</name><name sortKey="Clements, D" sort="Clements, D" uniqKey="Clements D" first="D." last="Clements">D. Clements</name><name sortKey="Gonzalez Olares, E" sort="Gonzalez Olares, E" uniqKey="Gonzalez Olares E" first="E." last="González-Solares">E. González-Solares</name><name sortKey="Oliver, S" sort="Oliver, S" uniqKey="Oliver S" first="S." last="Oliver">S. Oliver</name><name sortKey="Rigopoulou, D" sort="Rigopoulou, D" uniqKey="Rigopoulou D" first="D." last="Rigopoulou">D. Rigopoulou</name><name sortKey="Rowan Obinson, M" sort="Rowan Obinson, M" uniqKey="Rowan Obinson M" first="M." last="Rowan-Robinson">M. Rowan-Robinson</name><name sortKey="Serjeant, S" sort="Serjeant, S" uniqKey="Serjeant S" first="S." last="Serjeant">S. Serjeant</name></noCountry><country name="Espagne"><region name="Canaries"><name sortKey="Hernan Aballero, A" sort="Hernan Aballero, A" uniqKey="Hernan Aballero A" first="A." last="Hernán-Caballero">A. Hernán-Caballero</name></region><name sortKey="Afonso Uis, A" sort="Afonso Uis, A" uniqKey="Afonso Uis A" first="A." last="Afonso-Luis">A. Afonso-Luis</name><name sortKey="Montenegro Ontes, F M" sort="Montenegro Ontes, F M" uniqKey="Montenegro Ontes F" first="F. M." last="Montenegro-Montes">F. M. Montenegro-Montes</name><name sortKey="Perez Ournon, I" sort="Perez Ournon, I" uniqKey="Perez Ournon I" first="I." last="Pérez-Fournon">I. Pérez-Fournon</name><name sortKey="Valtchanov, I" sort="Valtchanov, I" uniqKey="Valtchanov I" first="I." last="Valtchanov">I. Valtchanov</name></country><country name="Allemagne"><region name="Bavière"><name sortKey="Hatziminaoglou, E" sort="Hatziminaoglou, E" uniqKey="Hatziminaoglou E" first="E." last="Hatziminaoglou">E. Hatziminaoglou</name></region></country><country name="États-Unis"><region name="État de New York"><name sortKey="Farrah, D" sort="Farrah, D" uniqKey="Farrah D" first="D." last="Farrah">D. Farrah</name></region><name sortKey="Lonsdale, C J" sort="Lonsdale, C J" uniqKey="Lonsdale C" first="C. J." last="Lonsdale">C. J. Lonsdale</name><name sortKey="Shupe, D" sort="Shupe, D" uniqKey="Shupe D" first="D." last="Shupe">D. Shupe</name><name sortKey="Vila Ilar, B" sort="Vila Ilar, B" uniqKey="Vila Ilar B" first="B." last="Vila-Vilar">B. Vila-Vilar</name></country><country name="Italie"><region name="Émilie-Romagne"><name sortKey="Pozzi, F" sort="Pozzi, F" uniqKey="Pozzi F" first="F." last="Pozzi">F. Pozzi</name></region><name sortKey="Franca, F La" sort="Franca, F La" uniqKey="Franca F" first="F. La" last="Franca">F. La Franca</name><name sortKey="Gruppioni, C" sort="Gruppioni, C" uniqKey="Gruppioni C" first="C." last="Gruppioni">C. Gruppioni</name><name sortKey="Lari, C" sort="Lari, C" uniqKey="Lari C" first="C." last="Lari">C. Lari</name><name sortKey="Montenegro Ontes, F M" sort="Montenegro Ontes, F M" uniqKey="Montenegro Ontes F" first="F. M." last="Montenegro-Montes">F. M. Montenegro-Montes</name><name sortKey="Vaccari, M" sort="Vaccari, M" uniqKey="Vaccari M" first="M." last="Vaccari">M. Vaccari</name></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
EXPLOR_STEP=$WICRI_ROOT/Wicri/Amerique/explor/CaltechV1/Data/Main/Exploration
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 000130 | SxmlIndent | more
Ou
HfdSelect -h $EXPLOR_AREA/Data/Main/Exploration/biblio.hfd -nk 000130 | SxmlIndent | more
Pour mettre un lien sur cette page dans le réseau Wicri
{{Explor lien
|wiki= Wicri/Amerique
|area= CaltechV1
|flux= Main
|étape= Exploration
|type= RBID
|clé= ISTEX:037B92F95BE3FC2E745738718BAAA8B939A1A6F5
|texte= Mid‐infrared spectroscopy of infrared‐luminous galaxies at z∼ 0.5–3
}}
| This area was generated with Dilib version V0.6.32. |  |