Relevant bibliographies by topics / Supernova spectroscopy

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  2. Dissertations / Theses
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Academic literature on the topic 'Supernova spectroscopy'

Author: Grafiati
Published: 10 December 2022
Last updated: 31 July 2025

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Journal articles on the topic "Supernova spectroscopy"

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Chevalier, R. A. "The Early Evolution of Supernova Remnants." International Astronomical Union Colloquium 101 (1988): 31–42. http://dx.doi.org/10.1017/s0252921100102076.

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AbstractThe density distribution of the supernova ejecta and that of the surrounding medium are the most important parameters for the early evolution of supernova remnants. The distribution of the ejecta depends on the detailed hydrodynamics of the explosion, but the outer parts of a supernova can probably be represented by a steep power law density distribution with radius. Self-similar solutions are especially useful for modeling the interaction of a supernova with its surrounding. The supernova first interacts with mass loss from the progenitor star. Evidence for circumstellar interaction i
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Arcavi, Iair. "Type II SN Light Curves from the Caltech Core Collapse Project." Proceedings of the International Astronomical Union 7, S285 (2011): 431–53. http://dx.doi.org/10.1017/s1743921312001329.

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We presented our analysis of a sample of type II supernova (SN) light curves measured by the Caltech Core Collapse Project (CCCP). CCCP is a large observational program which made use of the robotic 60-in and the Hale 200-in telescopes to obtain optical photometry, spectroscopy and IR photometry of 49 nearby core-collapse supernovae (SNe). It provides a fair sample of core-collapse events, with well-defined selection criteria, and uniform, high-quality optical/IR observations. Our goal is to characterize the little-studied properties of core-collapse supernovae as a population. Preliminary dat
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Anderson, Joseph P., Stacey M. Habergham, Phil A. James, and M. Hamuy. "The Local Environments of Core-Collapse SNe within Host Galaxies." Proceedings of the International Astronomical Union 7, S279 (2011): 183–86. http://dx.doi.org/10.1017/s1743921312012896.

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AbstractWe present constraints on core-collapse supernova progenitors through observations of their environments within host galaxies. This is achieved through 2 routes. Firstly, we investigate the spatial correlation of supernovae with host galaxy star formation using pixel statistics. We find that the main supernova types form a sequence of increasing association to star formation. The most logical interpretation is that this implies an increasing progenitor mass sequence going from the supernova type Ia arising from the lowest mass, through the type II, type Ib, and the supernova type Ic ar
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Kuncarayakti, Hanindyo. "The explosion sites of nearby supernovae seen with integral field spectroscopy." Proceedings of the International Astronomical Union 11, A29B (2015): 276–77. http://dx.doi.org/10.1017/s1743921316005330.

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AbstractIntegral field spectroscopy of nearby supernova sites within ~30 Mpc have been obtained using multiple IFU spectrographs in Hawaii and Chile. This technique enables both spatial and spectral information of the explosion sites to be acquired simultaneously, thus providing the identification of the parent stellar population of the supernova progenitor and the estimates for its physical parameters including age and metallicity via the spectrum. While this work has mainly been done in the optical wavelengths using instruments such as VIMOS, GMOS, and MUSE, a near-infrared approach has also
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Kuncarayakti, Hanindyo, Mamoru Doi, Greg Aldering, et al. "Mass and metallicity constraints on supernova progenitors derived from integral field spectroscopy of the environment." Proceedings of the International Astronomical Union 7, S279 (2011): 343–44. http://dx.doi.org/10.1017/s1743921312013269.

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AbstractWe have obtained optical integral field spectroscopy of the explosion sites of more than 25 nearby type-IIP/IIL/Ib/Ic supernovae using UH88/SNIFS, and additionally Gemini/GMOS IFU. This technique enables us to obtain both spatial and spectral information of the immediate environment of the supernovae. Using strong line method we measured the metallicity of the star cluster present at the explosion site, presumably the coeval parent stellar population of the supernova progenitor, and comparison with simple stellar population models gives age estimate of the cluster. With this method we
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Chevalier, R. A. "High-energy Emission from Supernovae and Remnants." Symposium - International Astronomical Union 195 (2000): 135–42. http://dx.doi.org/10.1017/s0074180900162874.

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An early burst of energetic radiation is expected from a supernova at the time of shock breakout. This emission has not been directly observed but has been inferred from the photoionization around SN 1987A. X-ray emission has been detected from core-collapse supernovae in the days to years after the explosion as they interact with their circumstellar winds. Young Galactic supernova remnants provide the possibility of determining the composition structure of the ejecta through X-ray spectroscopy. An exciting finding for older remnants is that a number of remnants that appear to be interacting w
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Ellis, Richard, and Mark Sullivan. "Verifying the Use of Supernovae as Probes of the Cosmic Expansion." Symposium - International Astronomical Union 201 (2005): 231–40. http://dx.doi.org/10.1017/s007418090021629x.

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We present preliminary results of a follow-up survey which aims to characterise in detail those galaxies which hosted Type Ia supernovae found by the Supernova Cosmology Project. Our survey has two components: Hubble Space Telescope imaging with STIS and Keck spectroscopy with ESI, the goal being to classify each host galaxy into one of three broad morphological/spectral classes and hence to investigate the dependence of supernovae properties on host galaxy type over a large range in redshift. Of particular interest is the supernova Hubble diagram characterised by host galaxy class which sugge
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Folatelli, Gastón, Nidia Morrell, Mark M. Phillips, et al. "SPECTROSCOPY OF TYPE Ia SUPERNOVAE BY THE CARNEGIE SUPERNOVA PROJECT." Astrophysical Journal 773, no. 1 (2013): 53. http://dx.doi.org/10.1088/0004-637x/773/1/53.

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P. Kirshner, Robert. "Supernovae and the Cosmic Distance Scale." International Astronomical Union Colloquium 145 (1996): 19–28. http://dx.doi.org/10.1017/s0252921100007879.

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Knowledge of the size and age of the Universe depends on understanding supernovae. The direct geometric measurement of the circumstellar ring of SN 1987A using IUE spectra and HST images provides an independent test of the Cepheid distance scale to the Large Magellanic Cloud. Understanding the details of the mass distribution in the circumstellar matter is important to improving the precision of this distance. Type la supernovae have a narrow distribution in absolute magnitude, and new Cepheid distances to IC 4182 (the site of SN 1937C) and to NGC 5253 (the site of SN 1972E) obtained with HST
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Howell, D. A., M. Sullivan, K. Perrett, et al. "Gemini Spectroscopy of Supernovae from the Supernova Legacy Survey: Improving High‐Redshift Supernova Selection and Classification." Astrophysical Journal 634, no. 2 (2005): 1190–201. http://dx.doi.org/10.1086/497119.

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Dissertations / Theses on the topic "Supernova spectroscopy"

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Folatelli, Gastón. "Type Ia Supernova Cosmology : Quantitative Spectral Analysis." Doctoral thesis, Stockholm University, Department of Physics, 2004. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-80.

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<p>Type Ia supernovae have been successfully used as <i>standardized candles</i> to study the expansion history of the Universe. In the past few years, these studies led to the exciting result of an accelerated expansion caused by the repelling action of some sort of <i>dark energy</i>. This result has been confirmed by measurements of cosmic microwave background radiation, the large-scale structure, and the dynamics of galaxy clusters. The combination of all these experiments points to a “concordance model” of the Universe with flat large-scale geometry and a dominant component of dark energy
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Kasai, Eli Kunwiji. "SALT spectroscopy and classification of supernova spectra using Bayesian techniques." Doctoral thesis, University of Cape Town, 2017. http://hdl.handle.net/11427/27283.

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In this thesis, we present the Southern African Large Telescope spectroscopic follow-up programme for supernova candidates discovered by the international Dark Energy Survey, the goals of which are to measure the expansion history of the Universe and shed light on the mysterious nature of dark energy. In total, we took spectra for 36 supernova candidates. These were classified using a new Bayesian Supernova spectra classifier, SuperNovaMC, that we developed to address limitations with existing algorithms. SuperNovaMC simultaneously finds the best fitting supernova and host galaxy using Bayesia
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Rigault, Mickaël. "Analyses des propriétés locales des galaxies hôtes des Supernovae de type Ia dans la collaboration The Nearby Supernova Factory." Thesis, Lyon 1, 2013. http://www.theses.fr/2013LYO10145/document.

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Les supernovae de type Ia (SNe Ia) sont de puissants indicateurs de distance cosmologique. Elles sont à l'origine de la découverte de l'énergie noire dans l'univers et restent aujourd'hui la meilleure méthode pour contraindre son équation d'état. Cependant, nous ignorons toujours le phénomène exact donnant naissance à ces supernovae. Notamment, nous ne connaissons pas l'influence de l'évolution des paramètres stellaires avec le redshift sur la luminosité de ces objets et donc sur les ajustements cosmologiques. De récentes études ont mis en évidence évidence des biais environnementaux ayant un
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Hayashi, Ichizou. "Systematic X-ray Spectroscopy of Supernova Remnants in the Magellanic Clouds." 京都大学 (Kyoto University), 1997. http://hdl.handle.net/2433/202434.

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GRECO, Emanuele. "X-Ray Spectroscopy of Ejecta and Compact Objects in Supernova Remnants." Doctoral thesis, Università degli Studi di Palermo, 2021. http://hdl.handle.net/10447/520391.

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Galbany, i. Gonzàlez Lluís. "Supernova studies in the SDSS-II/SNe Survey: Spectroscopy of the peculiar SN 2007qd, and photometric properties of Type-Ia supernovae as a function of the distance to the host galaxy." Doctoral thesis, Universitat Autònoma de Barcelona, 2011. http://hdl.handle.net/10803/83974.

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Aquesta tesi engloba el treball fet durant els ultims quatre anys com a estudiant de doctorat a l’Institut de Física d’Altes Energies (IFAE), emmarcat dins de la col·labaració Sloan Digital Sky Survey II Supernova (SDSS-II/SNe) Survey. Al primer capítol (§1) s’introdueixen els principals conceptes del Model Estàndar de Cosmologia, presentant els seus orígens, les propietats dels seus continguts, i les mesures de distància i brillantor. També es reconstrueix l’història de l’univers des del Big Bang i es resumeixen alguns dels descobriments més excitants que han confirmat les prediccions
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Cellier-Holzem, Flora. "Spectroscopie des supernovae de type Ia des expériences SuperNova Legacy Survey et Nearby SuperNova Factory pour la cosmologie." Paris 6, 2013. http://www.theses.fr/2013PA066568.

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Les supernovae de type Ia (SNe Ia) sont aujourd'hui un outil puissant en cosmologie pour étudier l'accélération de l'expansion de l'univers. Utilisées comme chandelles standard, elles permettent de contraindre l'équation d'état de l'énergie noire à travers un diagramme de Hubble. La spectroscopie est une étape essentielle à la construction de ce diagramme à la fois pour s'assurer que les objets sont bien des SNe Ia et déterminer leur décalage vers le rouge, mais également pour mieux comprendre leurs propriétés physiques et ainsi réduire les incertitudes systématiques qui limitent l'utilisation
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Spyromilio, Jason. "Infrared spectroscopy of supernovae." Thesis, Imperial College London, 1989. http://hdl.handle.net/10044/1/47669.

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Fasia, Alexandra. "Spectroscopic study of core-collapse supernovae." Thesis, Imperial College London, 1999. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.313777.

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Rigault, Mickaël. "Analyses des propriétés locales des galaxies hôtes des Supernovae de type Ia dans la collaboration The Nearby Supernova Factory." Phd thesis, Université Claude Bernard - Lyon I, 2013. http://tel.archives-ouvertes.fr/tel-00905574.

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Les supernovae de type Ia (SNe Ia) sont de puissants indicateurs de distance cosmologique. Elles sont à l'origine de la découverte de l'énergie noire dans l'univers et restent aujourd'hui la meilleure méthode pour contraindre son équation d'état. Cependant, nous ignorons toujours le phénomène exact donnant naissance à ces supernovae. Notamment, nous ne connaissons pas l'influence de l'évolution des paramètres stellaires avec le redshift sur la luminosité de ces objets et donc sur les ajustements cosmologiques. De récentes études ont mis en évidence évidence des biais environnementaux ayant un
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Books on the topic "Supernova spectroscopy"

1

United States. National Aeronautics and Space Administration., ed. The abundances of major elements in Cas A and tycho supernova remnants: Final report. National Aeronautics and Space Administration, 1995.

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Book chapters on the topic "Supernova spectroscopy"

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Gómez, G., and R. López. "Ten Years of Supernova Spectroscopy." In Highlights of Spanish Astrophysics III. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-1778-6_70.

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Katsuda, Satoru. "High-Resolution X-Ray Spectroscopy of Supernova Remnants." In High-Resolution X-ray Spectroscopy. Springer Nature Singapore, 2023. http://dx.doi.org/10.1007/978-981-99-4409-5_13.

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Dewey, Daniel. "Kinematics of Supernova Remnants: Status of X-Ray Observations." In High-Resolution X-Ray Spectroscopy. Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-9884-2_15.

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Katsuda, Satoru. "Correction to: High-Resolution X-Ray Spectroscopy of Supernova Remnants." In High-Resolution X-ray Spectroscopy. Springer Nature Singapore, 2023. http://dx.doi.org/10.1007/978-981-99-4409-5_14.

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Hughes, John P. "X-Ray Spectroscopy of Young Supernova Remnants: Mixing in the Ejecta of Type I and II Supernovae." In Supernovae. Springer New York, 1991. http://dx.doi.org/10.1007/978-1-4612-2988-9_98.

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Miekle, W. Peter S., David A. Allen, Jason Spyromilio, and Gian Varani. "Spectroscopy of SN 1987A at 1–4 Microns." In Supernovae. Springer New York, 1991. http://dx.doi.org/10.1007/978-1-4612-2988-9_10.

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Spyromilio, Jason, David A. Allen, W. Peter S. Meikle, James R. Graham, Philip A. Pinto, and Ronald G. Eastman. "Infrared Spectroscopy of Supernovae." In Infrared Astronomy with Arrays. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1070-9_14.

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Schlegel, Eric M. "A Spectroscopic Glance at the CfA Supernovae Atlas." In Supernovae. Springer New York, 1991. http://dx.doi.org/10.1007/978-1-4612-2988-9_68.

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Meikle, W. Peter S., Emma J. C. Bowers, Tom R. Geballe, Nic A. Walton, James R. Lewis, and Robert J. Cumming. "Infrared and Optical Spectroscopy of Type Ia Supernovae." In Thermonuclear Supernovae. Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5710-0_3.

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Spyromilio, J. "Infrared Spectroscopy of SN 1987A." In Supernovae and Supernova Remnants. Cambridge University Press, 1996. http://dx.doi.org/10.1017/cbo9780511564734.023.

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Conference papers on the topic "Supernova spectroscopy"

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Kjær, K., B. Leibundgut, C. Fransson, J. Spyromilio, Stefan Immler, and Kurt Weiler. "Integral Field Spectroscopy of SN 1987A." In SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters. AIP, 2007. http://dx.doi.org/10.1063/1.2803625.

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Kjær, K., B. Leibundgut, C. Fransson, J. Spyromilio, Stefan Immler, and Kurt Weiler. "Integral Field Spectroscopy of SN 1987A." In SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters. AIP, 2007. http://dx.doi.org/10.1063/1.3682885.

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Polomski, Elisha, C. E. Woodward, R. D. Gehrz, et al. "Multi-Epoch Spitzer Spectroscopy of SN 1987A." In SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters. AIP, 2007. http://dx.doi.org/10.1063/1.2803559.

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Polomski, Elisha, C. E. Woodward, R. D. Gehrz, et al. "Multi-Epoch Spitzer Spectroscopy of SN 1987A." In SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters. AIP, 2007. http://dx.doi.org/10.1063/1.3682899.

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Crotts, Arlin P. S., Stefan Immler, and Kurt Weiler. "Circumstellar Structure of SNR 1987A Traced by Light Echoes and High-Resolution Spectroscopy." In SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters. AIP, 2007. http://dx.doi.org/10.1063/1.2803550.

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Crotts, Arlin P. S., Stefan Immler, and Kurt Weiler. "Circumstellar Structure of SNR 1987A Traced by Light Echoes and High-Resolution Spectroscopy." In SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters. AIP, 2007. http://dx.doi.org/10.1063/1.3682891.

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Smith, Nathan, Richard McCray, Stefan Immler та Kurt Weiler. "High Resolution Spectroscopy of SN1987A's Rings: He I λ 10830 and Hα from the Hotspots". У SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters. AIP, 2007. http://dx.doi.org/10.1063/1.2803560.

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Smith, Nathan, Richard McCray, Stefan Immler та Kurt Weiler. "High Resolution Spectroscopy of SN1987A's Rings: He I λ 10830 and Hα from the Hotspots". У SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters. AIP, 2007. http://dx.doi.org/10.1063/1.3682900.

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Knežević, Sladjana, Rino Bandiera, Steve Schulze, and Giovanni Morlino. "SPECTROSCOPY OF YOUNG SUPERNOVA REMNANTS WITH VLT/MUSE INSTRUMENT." In XIV Serbian-Bulgarian Astronomical Conference. Astronomical Observatory, 2024. http://dx.doi.org/10.69646/14sbac35a.

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The Multi Unit Spectroscopic Explorer (MUSE) instrument at the ESO Very Large Telescope has shown exceptional capability in observing and studying sources in the visible wavelength range. As a panoramic integral-field spectrograph, it covers a wide simultaneous spectral range. Its extensive field of view and high spatial resolution make it particularly well- suited for studying extended objects. The instrument's very high efficiency offers an unprecedented opportunity to study faint sources. In this report, we will present and compare MUSE observations of the supernova remnant 0509-67.5, spann
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Canizares, C. R. "High resolution spectroscopy of two oxygen-rich SNRs with the Chandra HETG." In The eleventh astrophysics conference on young supernova remnants. AIP, 2001. http://dx.doi.org/10.1063/1.1377096.

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