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Статті в журналах з теми "Supernova spectroscopy"
Chevalier, R. A. "The Early Evolution of Supernova Remnants." International Astronomical Union Colloquium 101 (1988): 31–42. http://dx.doi.org/10.1017/s0252921100102076.
Повний текст джерелаArcavi, Iair. "Type II SN Light Curves from the Caltech Core Collapse Project." Proceedings of the International Astronomical Union 7, S285 (September 2011): 431–53. http://dx.doi.org/10.1017/s1743921312001329.
Повний текст джерелаKuncarayakti, Hanindyo. "The explosion sites of nearby supernovae seen with integral field spectroscopy." Proceedings of the International Astronomical Union 11, A29B (August 2015): 276–77. http://dx.doi.org/10.1017/s1743921316005330.
Повний текст джерелаAnderson, 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 (April 2011): 183–86. http://dx.doi.org/10.1017/s1743921312012896.
Повний текст джерелаKuncarayakti, Hanindyo, Mamoru Doi, Greg Aldering, Nobuo Arimoto, Keiichi Maeda, Tomoki Morokuma, Rui Pereira, Tomonori Usuda, and Yasuhito Hashiba. "Mass and metallicity constraints on supernova progenitors derived from integral field spectroscopy of the environment." Proceedings of the International Astronomical Union 7, S279 (April 2011): 343–44. http://dx.doi.org/10.1017/s1743921312013269.
Повний текст джерелаChevalier, R. A. "High-energy Emission from Supernovae and Remnants." Symposium - International Astronomical Union 195 (2000): 135–42. http://dx.doi.org/10.1017/s0074180900162874.
Повний текст джерелаFolatelli, Gastón, Nidia Morrell, Mark M. Phillips, Eric Hsiao, Abdo Campillay, Carlos Contreras, Sergio Castellón, et al. "SPECTROSCOPY OF TYPE Ia SUPERNOVAE BY THE CARNEGIE SUPERNOVA PROJECT." Astrophysical Journal 773, no. 1 (July 25, 2013): 53. http://dx.doi.org/10.1088/0004-637x/773/1/53.
Повний текст джерелаEllis, 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.
Повний текст джерелаHowell, D. A., M. Sullivan, K. Perrett, T. J. Bronder, I. M. Hook, P. Astier, E. Aubourg, et al. "Gemini Spectroscopy of Supernovae from the Supernova Legacy Survey: Improving High‐Redshift Supernova Selection and Classification." Astrophysical Journal 634, no. 2 (December 2005): 1190–201. http://dx.doi.org/10.1086/497119.
Повний текст джерелаP. Kirshner, Robert. "Supernovae and the Cosmic Distance Scale." International Astronomical Union Colloquium 145 (1996): 19–28. http://dx.doi.org/10.1017/s0252921100007879.
Повний текст джерелаДисертації з теми "Supernova spectroscopy"
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.
Повний текст джерелаType Ia supernovae have been successfully used as standardized candles 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 dark energy. 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.
However, there are several points related to supernova measurements which need careful analysis in order to doubtlessly establish the validity of the concordance model. As the amount and quality of data increases, the need of controlling possible systematic effects which may bias the results becomes crucial. Also important is the improvement of our knowledge of the physics of supernovae events to assure and possibly refine their calibration as standardized candle.
This thesis addresses some of those issues through the quantitative analysis of supernova spectra. The stress is put on a careful treatment of the data and on the definition of spectral measurement methods. The comparison of measurements for a large set of spectra from nearby supernovae is used to study the homogeneity and to search for spectral parameters which may further refine the calibration of the standardized candle. One such parameter is found to reduce the dispersion in the distance estimation of a sample of supernovae to below 6%, a precision which is comparable with the current lightcurve-based calibration, and is obtained in an independent manner. Finally, the comparison of spectral measurements from nearby and distant objects is used to test the possibility of evolution with cosmic time of the intrinsic brightness of type Ia supernovae.
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.
Повний текст джерелаRigault, 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.
Повний текст джерелаType Ia supernovae (SNe Ia) are powerful cosmological distance indicators. They were key tools for the discovery of the accelerating expansion of the Universe and today they remain the strongest demonstrated technique for measuring the dark-energy equation of state. However, a major issue remains: despite decades of study, their progenitors are as yet undetermined. Notably, we still ignore the influence of the redshift-evolution of stellar properties on the absolute luminosity of the SNe Ia and therefore on the fitted cosmological parameters. Recent studies have highlighted potential biases correlated with the global properties of their host galaxies, large enough to induce systematic errors into cosmological measurements if not properly treated. However, those studies analyse hosts of Type Ia supernovae globally thus neglecting the known stellar and gas property variations across galaxies. ! In this thesis, I show how integral field spectroscopy data from the Nearby Supernova Factory allow the study of the local environment of the SNe Ia (~kpc). In the first part of this document, I introduce the physical principals and the scientific context of this work. In a second part, I start by detailing the technical extraction tools developed in order to extract the local host properties. Then, I show how one could measure the star formation activity in the SN vicinity from those data. I focus the analysis on this star formation activity and notably I show how the SNe Ia properties -- particularly their standardised Hubble residuals -- depend on the local host environment, which corresponds to a significant cosmological bias. I finish this second part by introducing a simple model based on the known evolution of the galactic star formation activity. This model enables me to estimate the potential influence of the aforementioned environmental bias on cosmology. I also show that this model can be tested using public data and a first analyses tend to confirm our hypotheses. Those results have been published in Astronomy & Astrophysics (Rigault et al. 2013). The third and last part of the document introduces new approaches and future work perspectives. ! In this thesis, I have highlighted significant environmental biases in SNe Ia properties, thanks to the local approach. However, those biases are less an issue for the cosmological analyses using Type Ia supernovae than a new opportunity to improve them as cosmological probes. ! This Document is written in French. The figures are in English
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.
Повний текст джерелаGalbany, 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.
Повний текст джерелаEsta tesis engloba el trabajo realizado durante los últimos cuatro años como estudiante de doctorado en el Institut de Física d’Altes Energies (IFAE), enmarcardo en la colabaración Sloan Digital Sky Survey II Supernova (SDSS-II/SNe) Survey. En el primer capítulo (§1) se introducen los principales conceptos del Modelo Estándar de Cosmología, presentando sus orígenes, las propiedades de sus contenidos, y las medidas de distancia y brillo. También se reconstruyen la historia del universo desde el Big Bang y se resumen algunos de los descubrimientos más excitantes que han confirmado las predicciones del Modelo Estándar. Seguidamente (§2), se da una explicación detallada de las supernovas (SNe), incluyendo el mecanismo físico que da lugar a las explosiones, las diferencias entre los diferentes tipos, y su clasificación espectral. También se describen las propiedades fotomètricas y espectroscópicas de las supernovas de tipo Ia. A continuación, se resumen las medidas del ritmo de explosión, las propiedades de las galaxias donde residen las supernovas, y su uso en Cosmología a través del diagrama de Hubble. En el siguiente capítulo, (§3) se describe SDSS-II/SNe Survey, una extensión de tres años (2005-2007) del proyecto Sloan (SDSS) que ha detectado y medido curvas de luz para centenares de supernovas a través de escanear el cielo en repetidas ocasiones. Como parte del seguimiento espectroscópico de las supernova de SDSS-II/SNe, contribuímos obteniendo 23 espectros de supernovas durante 4 noches de Octubre y Noviembre (5-6 Oct. y 4-5 Nov.) del 2007, utilizando el Telescopio Nazionale Galileo (TNG) situado en el Observatorio del Roque de Los Muchachos (ORM) en La Palma. En el capítulo §4 se describe toda la reducción de datos, desde la adquisición de las imágenes hasta los espectros calibrados en flujo y longitud de onda. Siguiendo la reducción de los espectros, en el capítulo §5, se describe una de las supernovas de tipo Ia menos luminosa jamàs conocida, la peculiar 2007qd, para la cual medimos el primer espectro. Las propiedades observadas de la 2007qd la sitúan en la subclase llamada 2002cx, como miembro intermedio entre las supernovas 2002cx y 2008ha, enlazándolas. Se presentan las observaciones espectroscópicas y fotométricas de la supernova 2007qd y se comparan su propiedades con un conjunto de otras supernovas. Éste análisis fue publicado en McClelland et al. (2010). En el capítulo §6, se utilizan las supernovas Ia descubiertas por SDSS-II/SNe Survey durante los tres años de actividad, para buscar dependencias entre las propiedades fotométricas de las supernovas Ia y la proyección de la distancia hasta el centro de la galaxia donde residen, utilizando la distancia como aproximación a las propiedades locales de las galaxias (ritmo de creación de estrellas, metalicidad local, etc.). Encontramos que el exceso de color de las supernovas, parametrizado por AV en MLCS2k2 y por c en SALT2 decrece con la distancia, en particular para las galaxias espirales. Además, y con menos significancia, también se encuentra que la amplitud de la curva de luz, obtenida con MLCS2k2, está correlacionada con la separación entre la supernova y el centro de la galaxia para las galaxias elípticas, así las supernovas con curvas de luz más estrechas, y menos luminosas, se observan a más distancia del centro galactico. Este análisis fue presentado en la conferencia Supernovae and their Host Galaxies que tuvo lugar en Junio del 2011 en Sydney, y serà publicado en Galbany et al. (2011). Finalmente, en §7, se resume y se presentan las conclusiones de esta tesis.
This thesis comprises the work I have been doing during the last four years at Institut de Física d’Altes Energies (IFAE) as a PhD student, and has to be understood within the context of the Sloan Digital Sky Survey II Supernova (SDSS-II/SNe) survey. The content of this thesis is ordered as follows. In the next Chapter (§1) I introduce the main concepts of the Standard Model of Cosmology, presenting the origins, the properties of its contents, and the distance and the brightness measurements. I also reconstruct the history of universe since the Big Bang and summarize some of the most exciting discoveries that have confirmed the Standard Model predictions. In §2, a detailed explanation of supernovae (SNe) is given, including the physical mechanism that accounts for their explosions, the differences among the several types of SNe, and their spectral classification. We also describe the spectroscopic and photometric properties of Type-Ia SNe. After that, we review the SNe rate of the explosion measurements, the properties of their host galaxies, and their use in Cosmology through the Hubble diagram. After that, in §3, I describe the SDSS-II/SNe survey, a three-year (2005-2007) extension of SDSS of which I am an external collaborator, which has detected and measured light-curves for several hundred supernovae through repeat scans of the sky. As a part of the spectroscopic follow-up of the SDSS-II/SNe candidates, we contributed to the project taking spectra of 23 SNe during four nights in October and November (5-6 Oct. and 4-5 Nov.) of 2007 using the Telescopio Nazionale Galileo (TNG) located at the Observatorio del Roque de Los Muchachos (ORM) in La Palma. In §4, the whole reduction procedure, from the acquisition of the raw data by the telescope camera to the final flux-calibrated spectra, is described. Following the spectra reduction, in §5, I describe one of the most subluminous type-Ia events known, the peculiar 2007qd supernova, for which we took the first spectrum. The observed properties of 2007qd place it in the 2002cx subclass of supernovae, specifically as a member intermediate to 2002cx and 2008ha, linking these objects. We present the photometric and spectroscopic observations of 2007qd and compare its unique properties with a range of other SNe. This work was compiled and published in McClelland et al. (2010). Then, in §6, the three-year sample of Type Ia supernovae (SNe Ia) discovered by the SDSS-II/SNe Survey is used to look for dependencies between photometric SN Ia properties and the projected distance to the host galaxy center, using the distance as a proxy for local galaxy properties (local star-formation rate, local metallicity, etc.). We find that the excess color of the SN, parametrized by AV in MLCS2k2 and by c in SALT2 decreases with the projected distance, in particular for spiral galaxies. At a lower significance we find that the light-curve width, as obtained from MLCS2k2 , is correlated with the SN-galaxy separation for elliptical hosts, so that SNe Ia with narrower light-curves, hence dimmer, are more commonly observed at large distances from the host galaxy core. This analysis was presented in the Supernovae and their Host Galaxies conference which was held at Sydney, Australia in June 2011, and will be published in Galbany et al. (2011). Finally, in §7 we give a summary and the conclusions of this thesis.
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.
Повний текст джерелаType Ia supernovae (SNe Ia) are a powerful tool in cosmology today to study the acceleration of the universal expansion. Using as standardisable candles, they allow us to constrain the dark energy equation of state via a Hubble diagram. The spectroscopy is essential to build this diagram, on the one hand to secure the type of SNe Ia and estimate the redhsift, and on the other hand for a better knowledge of their physical properties to reduce the systematic uncertainties which limit the use of SNe Ia for cosmological works. In this context, I build a new sample of SN Ia spectra measured by the Very Large Telescope (VLT) for the SuperNova Legacy Survey (SNLS) experiment. These SN Ia data complete the existing sample to constitute the final VLT spectroscopic dataset of the SNLS. In addition to the inclusion in the Hubble diagram for cosmological analysis, this spectroscopic sample can be used to test if SNe Ia properties evolve with the redshift. I investigate this fundamental question for cosmology using the new VLT spectra sample of distant SNe Ia and the nearby object of the Nearby SuperNova Factory (SNF) experiment. These two samples are also a rich source of physical information for a better knowledge of SNe Ia and a better standardisation. For this purpose, I compare these data with various SNe Ia formation models to identify discriminant spectral area or parameters in order to constrain and improve the models to reproduce the observations and the SNe Ia variability
Spyromilio, Jason. "Infrared spectroscopy of supernovae." Thesis, Imperial College London, 1989. http://hdl.handle.net/10044/1/47669.
Повний текст джерелаFasia, Alexandra. "Spectroscopic study of core-collapse supernovae." Thesis, Imperial College London, 1999. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.313777.
Повний текст джерелаRigault, 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.
Повний текст джерелаBazin, Gurvan. "Analyse différée des données du SuperNova Legacy Survey." Paris 7, 2008. http://www.theses.fr/2008PA077135.
Повний текст джерелаThe SuperNova Legacy Survey (SNLS) experiment observed type la supemovae (SNeHa) during 5 years. Its aim is the contraint cosmological parameters. The online reduction pipeline is based on spectroscopic identification for each supernova. Systematically using spectroscopy requires a sufficient signal to noise level. Thus, it could lead to selection biases and would not be possible for future surveys The PhD thesis report a complementary method for data reduction based on a completely photometric selection. This analysis, more efficient to select faint events, approximately double the SNeHa sample of the SNLS. This method show a clear bias in the spectroscopic selection. Brighter SNeHa are systematically selected beyond a redshift of 0. 7. On the other hand, no important impact on cosmology was found. So, corrections on intrinsic variability of SNeHa luminosity are robust. In addition, this work is a first step to study the feasibility of such a purely photometric analysis for cosmology. This is a promising method for future projects
Книги з теми "Supernova spectroscopy"
United States. National Aeronautics and Space Administration., ed. The abundances of major elements in Cas A and tycho supernova remnants: Final report. [Washington, DC: National Aeronautics and Space Administration, 1995.
Знайти повний текст джерелаЧастини книг з теми "Supernova spectroscopy"
Gómez, G., and R. López. "Ten Years of Supernova Spectroscopy." In Highlights of Spanish Astrophysics III, 317–20. Dordrecht: Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-1778-6_70.
Повний текст джерелаDewey, Daniel. "Kinematics of Supernova Remnants: Status of X-Ray Observations." In High-Resolution X-Ray Spectroscopy, 229–48. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-9884-2_15.
Повний текст джерелаHughes, John P. "X-Ray Spectroscopy of Young Supernova Remnants: Mixing in the Ejecta of Type I and II Supernovae." In Supernovae, 661–70. New York, NY: Springer New York, 1991. http://dx.doi.org/10.1007/978-1-4612-2988-9_98.
Повний текст джерелаMiekle, W. Peter S., David A. Allen, Jason Spyromilio, and Gian Varani. "Spectroscopy of SN 1987A at 1–4 Microns." In Supernovae, 102–11. New York, NY: Springer New York, 1991. http://dx.doi.org/10.1007/978-1-4612-2988-9_10.
Повний текст джерелаSpyromilio, 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, 65–68. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1070-9_14.
Повний текст джерелаSchlegel, Eric M. "A Spectroscopic Glance at the CfA Supernovae Atlas." In Supernovae, 480–88. New York, NY: Springer New York, 1991. http://dx.doi.org/10.1007/978-1-4612-2988-9_68.
Повний текст джерелаMeikle, 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, 53–64. Dordrecht: Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5710-0_3.
Повний текст джерелаSpyromilio, J. "Infrared Spectroscopy of SN 1987A." In Supernovae and Supernova Remnants, 193–200. Cambridge University Press, 1996. http://dx.doi.org/10.1017/cbo9780511564734.023.
Повний текст джерелаPetre, R. "X-Ray Spectroscopy of Supernova Remnants." In Supernovae and Supernova Remnants, 357–68. Cambridge University Press, 1996. http://dx.doi.org/10.1017/cbo9780511564734.038.
Повний текст джерелаMcCray, R. A. "Coronal interstellar gas and supernova remnants." In Spectroscopy of Astrophysical Plasmas, 255–78. Cambridge University Press, 1987. http://dx.doi.org/10.1017/cbo9780511564659.011.
Повний текст джерелаТези доповідей конференцій з теми "Supernova spectroscopy"
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.
Повний текст джерелаKjær, 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.
Повний текст джерелаPolomski, Elisha, C. E. Woodward, R. D. Gehrz, D. H. Wooden, B. E. K. Sugerman, Stefan Immler, and Kurt Weiler. "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.
Повний текст джерелаPolomski, Elisha, C. E. Woodward, R. D. Gehrz, D. H. Wooden, B. E. K. Sugerman, Stefan Immler, and Kurt Weiler. "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.
Повний текст джерелаCrotts, 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.
Повний текст джерелаCrotts, 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.
Повний текст джерелаSmith, 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.
Повний текст джерелаSmith, 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.
Повний текст джерелаCanizares, 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.
Повний текст джерелаMizumura, Yoshitaka, Toru Tanimori, and Atsushi Takada. "Possibility of Systematic Study of Supernova Explosions by Nuclear Imaging Spectroscopy." In Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016). Journal of the Physical Society of Japan, 2017. http://dx.doi.org/10.7566/jpscp.14.020607.
Повний текст джерела