PTF10ops – a subluminous, normal‐width light curve Type Ia supernova in the middle of nowhere
Identifieur interne : 006358 ( Main/Exploration ); précédent : 006357; suivant : 006359PTF10ops – a subluminous, normal‐width light curve Type Ia supernova in the middle of nowhere
Auteurs : K. Maguire [Royaume-Uni] ; M. Sullivan [Royaume-Uni] ; R. C. Thomas [États-Unis] ; P. Nugent [États-Unis] ; D. A. Howell [États-Unis] ; A. Gal-Yam [Israël] ; I. Arcavi [Israël] ; S. Ben-Ami [Israël] ; S. Blake [Royaume-Uni] ; J. Botyanszki [États-Unis] ; C. Buton [Allemagne] ; J. Cooke [Australie] ; R. S. Ellis [États-Unis] ; I. M. Hook [Royaume-Uni, Italie] ; M. M. Kasliwal [États-Unis] ; Y. Pan [Royaume-Uni] ; R. Pereira [France] ; P. Podsiadlowski [Royaume-Uni] ; A. Sternberg [Israël] ; N. Suzuki [États-Unis] ; D. Xu [Israël] ; O. Yaron [Israël] ; J. S. Bloom [États-Unis] ; S. B. Cenko [États-Unis] ; S. R. Kulkarni [États-Unis] ; N. Law [Canada] ; E. O. Ofek [États-Unis] ; D. Poznanski [États-Unis] ; R. M. Quimby [États-Unis]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2011-12-01.
Descripteurs français
- Pascal (Inist)
- Wicri :
- topic : Classification.
English descriptors
- KwdEn :
- Absolute magnitude, Absolute magnitude limit, Absorption features, Benetti, Bolometric, Bolometric luminosity, California institute, Centre, Classification, Colour terms, Cool photosphere, Cool spectra, Cumbres observatory, Distance modulus, Equivalent widths, Exotic explosion, Explosion mechanism, Extinction, Faint group, Faint host galaxies, Galactic extinction, Galaxies, Galaxy, Globular, Globular cluster, Globular clusters, Halo, Host galaxies, Host galaxy, Host galaxy extinction, Host velocities, Howell, Hubble space telescope, Input parameters, July, Large distance, Large distances, Lawrence berkeley, Light curve, Light curve width, Light curves, Luminosity, Magnitude space, Massive galaxies, Massive galaxy, Massive spiral galaxy, Massive star, Maximum light, Maximum magnitude, Metallicity, Mnras, Models, Monthly notices, More detail, More details, Nancial support, National aeronautics, Nearby spiral galaxy, Nearby supernova factory, Normal luminosity, Normal template, Normal templates, Optical magnitudes, Optical spectra, Optical spectrum, Palomar observatory, Pasp, Peak bband magnitude, Peak luminosity, Peak magnitude, Photometry, Photospheric, Photospheric phase spectra, Physique nucl, Positions, Progenitor, Progenitor model, Progenitor star, Red shift, Redshift, Rest frame, Rise time, Same redshift, Samuel oschin telescope, Santa barbara, Sdss system, Secondary maxima, Secondary peak, Sifto, Similar properties, Space administration, Space telescope science institute, Spanish observatorio, Spectral, Spectral features, Spectral properties, Spectral template, Spectrum, Spiral galaxy, Stellar, Stellar population, Stellar populations, Stretch value, Stretch values, Strong lines, Subluminous, Subluminous events, Subluminous objects, Subluminous template, Substantial host galaxy extinction, Supernova, Synapps, Taubenberger, Technology facilities council, Telescope, Template, Template spectrum, Tertiary standards, Third epochs, Tting, Tting code synapps, Type I supernova, Velocity gradient group, Weizmann institute.
- Teeft :
- Absolute magnitude, Absolute magnitude limit, Absorption features, Benetti, Bolometric, Bolometric luminosity, California institute, Centre, Colour terms, Cool photosphere, Cool spectra, Cumbres observatory, Distance modulus, Equivalent widths, Exotic explosion, Explosion mechanism, Extinction, Faint group, Faint host galaxies, Galactic extinction, Galaxy, Globular, Globular cluster, Globular clusters, Halo, Host galaxies, Host galaxy, Host galaxy extinction, Host velocities, Howell, Hubble space telescope, Input parameters, July, Large distance, Large distances, Lawrence berkeley, Light curve, Light curve width, Light curves, Luminosity, Magnitude space, Massive galaxies, Massive galaxy, Massive spiral galaxy, Massive star, Maximum light, Maximum magnitude, Metallicity, Mnras, Monthly notices, More detail, More details, Nancial support, National aeronautics, Nearby spiral galaxy, Nearby supernova factory, Normal luminosity, Normal template, Normal templates, Optical magnitudes, Optical spectra, Palomar observatory, Pasp, Peak bband magnitude, Peak luminosity, Peak magnitude, Photometry, Photospheric, Photospheric phase spectra, Physique nucl, Progenitor, Progenitor model, Progenitor star, Redshift, Rest frame, Rise time, Same redshift, Samuel oschin telescope, Santa barbara, Sdss system, Secondary maxima, Secondary peak, Sifto, Similar properties, Space administration, Space telescope science institute, Spanish observatorio, Spectral, Spectral features, Spectral properties, Spectral template, Spectrum, Spiral galaxy, Stellar, Stellar population, Stellar populations, Stretch value, Stretch values, Strong lines, Subluminous, Subluminous events, Subluminous objects, Subluminous template, Substantial host galaxy extinction, Supernova, Synapps, Taubenberger, Technology facilities council, Telescope, Template, Template spectrum, Tertiary standards, Third epochs, Tting, Tting code synapps, Velocity gradient group, Weizmann institute.
Abstract
PTF10ops is a Type Ia supernova (SN Ia), whose light curve and spectral properties place it outside the current SN Ia subtype classifications. Its spectra display the characteristic lines of subluminous SNe Ia, but it has a normal‐width light curve with a long rise time, typical of normal‐luminosity SNe Ia. The early‐time optical spectra of PTF10ops were modelled using a spectral fitting code and found to have all the lines typically seen in subluminous SNe Ia, without the need to invoke more uncommon elements. The host galaxy environment of PTF10ops is also unusual with no galaxy detected at the position of the SN down to an absolute limiting magnitude of r≥−12.0 mag, but a very massive galaxy is present at a separation of ∼148 kpc and at the same redshift as suggested by the SN spectral features. The progenitor of PTF10ops is most likely a very old star, possibly in a low‐metallicity environment, which affects its explosion mechanism and observational characteristics. PTF10ops does not easily fit into any of the current models of either subluminous or normal SN Ia progenitor channels.
Url:
DOI: 10.1111/j.1365-2966.2011.19526.x
Affiliations:
- Allemagne, Australie, Canada, France, Israël, Italie, Royaume-Uni, États-Unis
- Angleterre, Californie, District de Cologne, Ontario, Oxfordshire, Rhénanie-du-Nord-Westphalie
- Bonn, Oxford, Toronto
- Université d'Oxford, Université de Toronto
Links toward previous steps (curation, corpus...)
- to stream Istex, to step Corpus: 002D17
- to stream Istex, to step Curation: 002D17
- to stream Istex, to step Checkpoint: 000777
- to stream Main, to step Merge: 006734
- to stream PascalFrancis, to step Corpus: 001759
- to stream PascalFrancis, to step Curation: 004750
- to stream PascalFrancis, to step Checkpoint: 001812
- to stream Main, to step Merge: 006C63
- to stream Main, to step Curation: 006358
Le document en format XML
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Pereira</name><affiliation wicri:level="1"><country xml:lang="fr">France</country><wicri:regionArea>Université de Lyon, F‐69622 France; Université de Lyon 1, Villeurbanne; CNRS/IN2P3, Institut de Physique Nucléaire de Lyon</wicri:regionArea><wicri:noRegion>Institut de Physique Nucléaire de Lyon</wicri:noRegion><wicri:noRegion>Institut de Physique Nucléaire de Lyon</wicri:noRegion></affiliation></author><author><name sortKey="Podsiadlowski, P" sort="Podsiadlowski, P" uniqKey="Podsiadlowski P" first="P." last="Podsiadlowski">P. Podsiadlowski</name><affiliation wicri:level="4"><orgName type="university">Université d'Oxford</orgName><country>Royaume-Uni</country><placeName><settlement type="city">Oxford</settlement><region type="nation">Angleterre</region><region type="région" nuts="1">Oxfordshire</region></placeName></affiliation></author><author><name sortKey="Sternberg, A" sort="Sternberg, A" uniqKey="Sternberg A" first="A." last="Sternberg">A. Sternberg</name><affiliation wicri:level="1"><country xml:lang="fr">Israël</country><wicri:regionArea>Department of Particle Physics and Astrophysics, Faculty of Physics, The Weizmann Institute of Science, Rehovot 76100</wicri:regionArea><wicri:noRegion>Rehovot 76100</wicri:noRegion></affiliation></author><author><name sortKey="Suzuki, N" sort="Suzuki, N" uniqKey="Suzuki N" first="N." last="Suzuki">N. Suzuki</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Computational Cosmology Center, Lawrence Berkeley National Laboratory, 1 Cyclotron Rd., Berkeley, CA 94720</wicri:regionArea><placeName><region type="state">Californie</region></placeName></affiliation></author><author><name sortKey="Xu, D" sort="Xu, D" uniqKey="Xu D" first="D." last="Xu">D. Xu</name><affiliation wicri:level="1"><country xml:lang="fr">Israël</country><wicri:regionArea>Department of Particle Physics and Astrophysics, Faculty of Physics, The Weizmann Institute of Science, Rehovot 76100</wicri:regionArea><wicri:noRegion>Rehovot 76100</wicri:noRegion></affiliation></author><author><name sortKey="Yaron, O" sort="Yaron, O" uniqKey="Yaron O" first="O." last="Yaron">O. Yaron</name><affiliation wicri:level="1"><country xml:lang="fr">Israël</country><wicri:regionArea>Department of Particle Physics and Astrophysics, Faculty of Physics, The Weizmann Institute of Science, Rehovot 76100</wicri:regionArea><wicri:noRegion>Rehovot 76100</wicri:noRegion></affiliation></author><author><name sortKey="Bloom, J S" sort="Bloom, J S" uniqKey="Bloom J" first="J. S." last="Bloom">J. S. Bloom</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Astronomy, University of California, Berkeley, CA 94720‐3411</wicri:regionArea><placeName><region type="state">Californie</region></placeName></affiliation></author><author><name sortKey="Cenko, S B" sort="Cenko, S B" uniqKey="Cenko S" first="S. B." last="Cenko">S. B. Cenko</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Astronomy, University of California, Berkeley, CA 94720‐3411</wicri:regionArea><placeName><region type="state">Californie</region></placeName></affiliation></author><author><name sortKey="Kulkarni, S R" sort="Kulkarni, S R" uniqKey="Kulkarni S" first="S. R." last="Kulkarni">S. R. Kulkarni</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125</wicri:regionArea><placeName><region type="state">Californie</region></placeName></affiliation></author><author><name sortKey="Law, N" sort="Law, N" uniqKey="Law N" first="N." last="Law">N. Law</name><affiliation wicri:level="4"><country xml:lang="fr">Canada</country><wicri:regionArea>Dunlap Institute for Astronomy and Astrophysics, University of Toronto, 50 St George Street, Toronto M5S 3H4, Ontario</wicri:regionArea><orgName type="university">Université de Toronto</orgName><placeName><settlement type="city">Toronto</settlement><region type="state">Ontario</region></placeName></affiliation></author><author><name sortKey="Ofek, E O" sort="Ofek, E O" uniqKey="Ofek E" first="E. O." last="Ofek">E. O. Ofek</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125</wicri:regionArea><placeName><region type="state">Californie</region></placeName></affiliation></author><author><name sortKey="Poznanski, D" sort="Poznanski, D" uniqKey="Poznanski D" first="D." last="Poznanski">D. Poznanski</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Computational Cosmology Center, Lawrence Berkeley National Laboratory, 1 Cyclotron Rd., Berkeley, CA 94720</wicri:regionArea><placeName><region type="state">Californie</region></placeName></affiliation><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Astronomy, University of California, Berkeley, CA 94720‐3411</wicri:regionArea><placeName><region type="state">Californie</region></placeName></affiliation></author><author><name sortKey="Quimby, R M" sort="Quimby, R M" uniqKey="Quimby R" first="R. M." last="Quimby">R. M. Quimby</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125</wicri:regionArea><placeName><region type="state">Californie</region></placeName></affiliation></author></analytic><monogr></monogr><series><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="alt">MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY</title><idno type="ISSN">0035-8711</idno><idno type="eISSN">1365-2966</idno><imprint><biblScope unit="vol">418</biblScope><biblScope unit="issue">2</biblScope><biblScope unit="page" from="747">747</biblScope><biblScope unit="page" to="758">758</biblScope><biblScope unit="page-count">12</biblScope><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2011-12-01">2011-12-01</date></imprint><idno type="ISSN">0035-8711</idno></series></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Absolute magnitude</term><term>Absolute magnitude limit</term><term>Absorption features</term><term>Benetti</term><term>Bolometric</term><term>Bolometric luminosity</term><term>California institute</term><term>Centre</term><term>Classification</term><term>Colour terms</term><term>Cool photosphere</term><term>Cool spectra</term><term>Cumbres observatory</term><term>Distance modulus</term><term>Equivalent widths</term><term>Exotic explosion</term><term>Explosion mechanism</term><term>Extinction</term><term>Faint group</term><term>Faint host galaxies</term><term>Galactic extinction</term><term>Galaxies</term><term>Galaxy</term><term>Globular</term><term>Globular cluster</term><term>Globular clusters</term><term>Halo</term><term>Host galaxies</term><term>Host galaxy</term><term>Host galaxy extinction</term><term>Host velocities</term><term>Howell</term><term>Hubble space telescope</term><term>Input parameters</term><term>July</term><term>Large distance</term><term>Large distances</term><term>Lawrence berkeley</term><term>Light curve</term><term>Light curve width</term><term>Light curves</term><term>Luminosity</term><term>Magnitude space</term><term>Massive galaxies</term><term>Massive galaxy</term><term>Massive spiral galaxy</term><term>Massive star</term><term>Maximum light</term><term>Maximum magnitude</term><term>Metallicity</term><term>Mnras</term><term>Models</term><term>Monthly notices</term><term>More detail</term><term>More details</term><term>Nancial support</term><term>National aeronautics</term><term>Nearby spiral galaxy</term><term>Nearby supernova factory</term><term>Normal luminosity</term><term>Normal template</term><term>Normal templates</term><term>Optical magnitudes</term><term>Optical spectra</term><term>Optical spectrum</term><term>Palomar observatory</term><term>Pasp</term><term>Peak bband magnitude</term><term>Peak luminosity</term><term>Peak magnitude</term><term>Photometry</term><term>Photospheric</term><term>Photospheric phase spectra</term><term>Physique nucl</term><term>Positions</term><term>Progenitor</term><term>Progenitor model</term><term>Progenitor star</term><term>Red shift</term><term>Redshift</term><term>Rest frame</term><term>Rise time</term><term>Same redshift</term><term>Samuel oschin telescope</term><term>Santa barbara</term><term>Sdss system</term><term>Secondary maxima</term><term>Secondary peak</term><term>Sifto</term><term>Similar properties</term><term>Space administration</term><term>Space telescope science institute</term><term>Spanish observatorio</term><term>Spectral</term><term>Spectral features</term><term>Spectral properties</term><term>Spectral template</term><term>Spectrum</term><term>Spiral galaxy</term><term>Stellar</term><term>Stellar population</term><term>Stellar populations</term><term>Stretch value</term><term>Stretch values</term><term>Strong lines</term><term>Subluminous</term><term>Subluminous events</term><term>Subluminous objects</term><term>Subluminous template</term><term>Substantial host galaxy extinction</term><term>Supernova</term><term>Synapps</term><term>Taubenberger</term><term>Technology facilities council</term><term>Telescope</term><term>Template</term><term>Template spectrum</term><term>Tertiary standards</term><term>Third epochs</term><term>Tting</term><term>Tting code synapps</term><term>Type I supernova</term><term>Velocity gradient group</term><term>Weizmann institute</term></keywords><keywords scheme="Pascal" xml:lang="fr"><term>Classification</term><term>Courbe lumière</term><term>Déplacement vers le rouge</term><term>Galaxies</term><term>Luminosité</term><term>Magnitude absolue</term><term>Modèle</term><term>Métallicité</term><term>Position</term><term>Propriété spectrale</term><term>Spectre optique</term><term>Supernova type I</term></keywords><keywords scheme="Teeft" xml:lang="en"><term>Absolute magnitude</term><term>Absolute magnitude limit</term><term>Absorption features</term><term>Benetti</term><term>Bolometric</term><term>Bolometric luminosity</term><term>California institute</term><term>Centre</term><term>Colour terms</term><term>Cool photosphere</term><term>Cool spectra</term><term>Cumbres observatory</term><term>Distance modulus</term><term>Equivalent widths</term><term>Exotic explosion</term><term>Explosion mechanism</term><term>Extinction</term><term>Faint group</term><term>Faint host galaxies</term><term>Galactic extinction</term><term>Galaxy</term><term>Globular</term><term>Globular cluster</term><term>Globular clusters</term><term>Halo</term><term>Host galaxies</term><term>Host galaxy</term><term>Host galaxy extinction</term><term>Host velocities</term><term>Howell</term><term>Hubble space telescope</term><term>Input parameters</term><term>July</term><term>Large distance</term><term>Large distances</term><term>Lawrence berkeley</term><term>Light curve</term><term>Light curve width</term><term>Light curves</term><term>Luminosity</term><term>Magnitude space</term><term>Massive galaxies</term><term>Massive galaxy</term><term>Massive spiral galaxy</term><term>Massive star</term><term>Maximum light</term><term>Maximum magnitude</term><term>Metallicity</term><term>Mnras</term><term>Monthly notices</term><term>More detail</term><term>More details</term><term>Nancial support</term><term>National aeronautics</term><term>Nearby spiral galaxy</term><term>Nearby supernova factory</term><term>Normal luminosity</term><term>Normal template</term><term>Normal templates</term><term>Optical magnitudes</term><term>Optical spectra</term><term>Palomar observatory</term><term>Pasp</term><term>Peak bband magnitude</term><term>Peak luminosity</term><term>Peak magnitude</term><term>Photometry</term><term>Photospheric</term><term>Photospheric phase spectra</term><term>Physique nucl</term><term>Progenitor</term><term>Progenitor model</term><term>Progenitor star</term><term>Redshift</term><term>Rest frame</term><term>Rise time</term><term>Same redshift</term><term>Samuel oschin telescope</term><term>Santa barbara</term><term>Sdss system</term><term>Secondary maxima</term><term>Secondary peak</term><term>Sifto</term><term>Similar properties</term><term>Space administration</term><term>Space telescope science institute</term><term>Spanish observatorio</term><term>Spectral</term><term>Spectral features</term><term>Spectral properties</term><term>Spectral template</term><term>Spectrum</term><term>Spiral galaxy</term><term>Stellar</term><term>Stellar population</term><term>Stellar populations</term><term>Stretch value</term><term>Stretch values</term><term>Strong lines</term><term>Subluminous</term><term>Subluminous events</term><term>Subluminous objects</term><term>Subluminous template</term><term>Substantial host galaxy extinction</term><term>Supernova</term><term>Synapps</term><term>Taubenberger</term><term>Technology facilities council</term><term>Telescope</term><term>Template</term><term>Template spectrum</term><term>Tertiary standards</term><term>Third epochs</term><term>Tting</term><term>Tting code synapps</term><term>Velocity gradient group</term><term>Weizmann institute</term></keywords><keywords scheme="Wicri" type="topic" xml:lang="fr"><term>Classification</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">PTF10ops is a Type Ia supernova (SN Ia), whose light curve and spectral properties place it outside the current SN Ia subtype classifications. Its spectra display the characteristic lines of subluminous SNe Ia, but it has a normal‐width light curve with a long rise time, typical of normal‐luminosity SNe Ia. The early‐time optical spectra of PTF10ops were modelled using a spectral fitting code and found to have all the lines typically seen in subluminous SNe Ia, without the need to invoke more uncommon elements. The host galaxy environment of PTF10ops is also unusual with no galaxy detected at the position of the SN down to an absolute limiting magnitude of r≥−12.0 mag, but a very massive galaxy is present at a separation of ∼148 kpc and at the same redshift as suggested by the SN spectral features. The progenitor of PTF10ops is most likely a very old star, possibly in a low‐metallicity environment, which affects its explosion mechanism and observational characteristics. PTF10ops does not easily fit into any of the current models of either subluminous or normal SN Ia progenitor channels.</div></front></TEI><affiliations><list><country><li>Allemagne</li><li>Australie</li><li>Canada</li><li>France</li><li>Israël</li><li>Italie</li><li>Royaume-Uni</li><li>États-Unis</li></country><region><li>Angleterre</li><li>Californie</li><li>District de Cologne</li><li>Ontario</li><li>Oxfordshire</li><li>Rhénanie-du-Nord-Westphalie</li></region><settlement><li>Bonn</li><li>Oxford</li><li>Toronto</li></settlement><orgName><li>Université d'Oxford</li><li>Université de Toronto</li></orgName></list><tree><country name="Royaume-Uni"><region name="Angleterre"><name sortKey="Maguire, K" sort="Maguire, K" uniqKey="Maguire K" first="K." last="Maguire">K. Maguire</name></region><name sortKey="Blake, S" sort="Blake, S" uniqKey="Blake S" first="S." last="Blake">S. Blake</name><name sortKey="Hook, I M" sort="Hook, I M" uniqKey="Hook I" first="I. M." last="Hook">I. M. Hook</name><name sortKey="Maguire, K" sort="Maguire, K" uniqKey="Maguire K" first="K." last="Maguire">K. Maguire</name><name sortKey="Pan, Y" sort="Pan, Y" uniqKey="Pan Y" first="Y." last="Pan">Y. Pan</name><name sortKey="Podsiadlowski, P" sort="Podsiadlowski, P" uniqKey="Podsiadlowski P" first="P." last="Podsiadlowski">P. Podsiadlowski</name><name sortKey="Sullivan, M" sort="Sullivan, M" uniqKey="Sullivan M" first="M." last="Sullivan">M. Sullivan</name></country><country name="États-Unis"><region name="Californie"><name sortKey="Thomas, R C" sort="Thomas, R C" uniqKey="Thomas R" first="R. C." last="Thomas">R. C. Thomas</name></region><name sortKey="Bloom, J S" sort="Bloom, J S" uniqKey="Bloom J" first="J. S." last="Bloom">J. S. Bloom</name><name sortKey="Botyanszki, J" sort="Botyanszki, J" uniqKey="Botyanszki J" first="J." last="Botyanszki">J. Botyanszki</name><name sortKey="Botyanszki, J" sort="Botyanszki, J" uniqKey="Botyanszki J" first="J." last="Botyanszki">J. Botyanszki</name><name sortKey="Cenko, S B" sort="Cenko, S B" uniqKey="Cenko S" first="S. B." last="Cenko">S. B. Cenko</name><name sortKey="Ellis, R S" sort="Ellis, R S" uniqKey="Ellis R" first="R. S." last="Ellis">R. S. Ellis</name><name sortKey="Howell, D A" sort="Howell, D A" uniqKey="Howell D" first="D. A." last="Howell">D. A. Howell</name><name sortKey="Howell, D A" sort="Howell, D A" uniqKey="Howell D" first="D. A." last="Howell">D. A. Howell</name><name sortKey="Kasliwal, M M" sort="Kasliwal, M M" uniqKey="Kasliwal M" first="M. M." last="Kasliwal">M. M. Kasliwal</name><name sortKey="Kulkarni, S R" sort="Kulkarni, S R" uniqKey="Kulkarni S" first="S. R." last="Kulkarni">S. R. Kulkarni</name><name sortKey="Nugent, P" sort="Nugent, P" uniqKey="Nugent P" first="P." last="Nugent">P. Nugent</name><name sortKey="Nugent, P" sort="Nugent, P" uniqKey="Nugent P" first="P." last="Nugent">P. Nugent</name><name sortKey="Ofek, E O" sort="Ofek, E O" uniqKey="Ofek E" first="E. O." last="Ofek">E. O. Ofek</name><name sortKey="Poznanski, D" sort="Poznanski, D" uniqKey="Poznanski D" first="D." last="Poznanski">D. Poznanski</name><name sortKey="Poznanski, D" sort="Poznanski, D" uniqKey="Poznanski D" first="D." last="Poznanski">D. Poznanski</name><name sortKey="Quimby, R M" sort="Quimby, R M" uniqKey="Quimby R" first="R. M." last="Quimby">R. M. Quimby</name><name sortKey="Suzuki, N" sort="Suzuki, N" uniqKey="Suzuki N" first="N." last="Suzuki">N. Suzuki</name><name sortKey="Thomas, R C" sort="Thomas, R C" uniqKey="Thomas R" first="R. C." last="Thomas">R. C. Thomas</name></country><country name="Israël"><noRegion><name sortKey="Gal Am, A" sort="Gal Am, A" uniqKey="Gal Am A" first="A." last="Gal-Yam">A. Gal-Yam</name></noRegion><name sortKey="Arcavi, I" sort="Arcavi, I" uniqKey="Arcavi I" first="I." last="Arcavi">I. Arcavi</name><name sortKey="Ben Mi, S" sort="Ben Mi, S" uniqKey="Ben Mi S" first="S." last="Ben-Ami">S. Ben-Ami</name><name sortKey="Sternberg, A" sort="Sternberg, A" uniqKey="Sternberg A" first="A." last="Sternberg">A. Sternberg</name><name sortKey="Xu, D" sort="Xu, D" uniqKey="Xu D" first="D." last="Xu">D. Xu</name><name sortKey="Yaron, O" sort="Yaron, O" uniqKey="Yaron O" first="O." last="Yaron">O. Yaron</name></country><country name="Allemagne"><region name="Rhénanie-du-Nord-Westphalie"><name sortKey="Buton, C" sort="Buton, C" uniqKey="Buton C" first="C." last="Buton">C. Buton</name></region></country><country name="Australie"><noRegion><name sortKey="Cooke, J" sort="Cooke, J" uniqKey="Cooke J" first="J." last="Cooke">J. Cooke</name></noRegion></country><country name="Italie"><noRegion><name sortKey="Hook, I M" sort="Hook, I M" uniqKey="Hook I" first="I. M." last="Hook">I. M. Hook</name></noRegion></country><country name="France"><noRegion><name sortKey="Pereira, R" sort="Pereira, R" uniqKey="Pereira R" first="R." last="Pereira">R. Pereira</name></noRegion></country><country name="Canada"><region name="Ontario"><name sortKey="Law, N" sort="Law, N" uniqKey="Law N" first="N." last="Law">N. Law</name></region></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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|texte= PTF10ops – a subluminous, normal‐width light curve Type Ia supernova in the middle of nowhere
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