supernova.lbl.gov

Supernova Cosmology Project

HST Cluster Supernova Survey. Lensed Type Ia supernovae as probes of cluster mass models. J Nordin, et al., MNRAS (2014). Available at http:/ adsabs.harvard.edu/abs/2014MNRAS.440.2742N. Precision Measurement of The Most Distant Spectroscopically Confirmed Supernova Ia with the Hubble Space Telescope. D Rubin, et al., ApJ (2013). Available at http:/ adsabs.harvard.edu/abs/2013ApJ.763.35R. J Meyers, et al., ApJ (2012). Available at http:/ adsabs.harvard.edu/abs/2012ApJ.750.1M. Data and Additional Info.

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Supernova Cosmology Project | supernova.lbl.gov Reviews

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HST Cluster Supernova Survey. Lensed Type Ia supernovae as probes of cluster mass models. J Nordin, et al., MNRAS (2014). Available at http:/ adsabs.harvard.edu/abs/2014MNRAS.440.2742N. Precision Measurement of The Most Distant Spectroscopically Confirmed Supernova Ia with the Hubble Space Telescope. D Rubin, et al., ApJ (2013). Available at http:/ adsabs.harvard.edu/abs/2013ApJ.763.35R. J Meyers, et al., ApJ (2012). Available at http:/ adsabs.harvard.edu/abs/2012ApJ.750.1M. Data and Additional Info.

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Supernova Cosmology Project | supernova.lbl.gov Reviews

https://supernova.lbl.gov

HST Cluster Supernova Survey. Lensed Type Ia supernovae as probes of cluster mass models. J Nordin, et al., MNRAS (2014). Available at http:/ adsabs.harvard.edu/abs/2014MNRAS.440.2742N. Precision Measurement of The Most Distant Spectroscopically Confirmed Supernova Ia with the Hubble Space Telescope. D Rubin, et al., ApJ (2013). Available at http:/ adsabs.harvard.edu/abs/2013ApJ.763.35R. J Meyers, et al., ApJ (2012). Available at http:/ adsabs.harvard.edu/abs/2012ApJ.750.1M. Data and Additional Info.

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supernova.lbl.gov

1

Supernova Cosmology Project

http://supernova.lbl.gov/video.html

What We Can See in a Supernova. The Supernova Cosmology Project. The image above and the movie clips ( QuickTime. This clip was prepared by the Supernova Cosmology Project (P. Nugent: spectral sequence; A. Conley: image sequence) with the help of Lawrence Berkeley National Laboratory's Computer Visualization Laboratory (N. Johnston: animation) at the National Energy Research Scientific Computing Center.

2

Untitled Document

http://supernova.lbl.gov/slides.html

Color Figures for Slides from Perlmutter et al, LBNL-41801, 1998,ApJ. Figure 1: Hubble Diagram with 42 High-Redshift. Supernovae (Log Redshift scale). Postscript. Figure 7: Confidence Region on. Omega Mass vs. Omega Lambda Plane. Postscript. Figure 10: Confidence Region on. Omega Mass vs. w Plane, for an additional. Energy density characterized by an equation. Of state w = p/rho. Postscript. Figure 2: Hubble Diagram with 42 High-. Redshift Supernovae (Linear Redshift scale),.

3

Supernova Cosmology Project

http://supernova.lbl.gov/2009ClusterSurvey

The Hubble Space Telescope. Survey for z 1 Type Ia Supernovae by Targeting Galaxy Clusters. Survey Paper: Dawson et al. (The Supernova Cosmology Project) 2009, AJ, 138, 1271 [ ADS. We present a new survey strategy to discover and study high redshift Type Ia supernovae (SNe Ia) using the Hubble Space Telescope (HST). By targeting massive galaxy clusters at 0.9. Control Time Simulations for Rates Calculation:. Barbary et al. 2011b [ FITS Table. From Suzuki et al. 2011. Lightcurves and Spectra of SN SCP06F6.

4

Supernova Cosmology Project

http://supernova.lbl.gov/people.html

Saul Perlmutter / PI. Saul Perlmutter - Lead Scientist. Lawrence Berkeley National Laboratory. Space Telescope Science Institute. Paris Supernova Cosmology Group. Collaboration Meeting at LBNL:.

5

Supernova Cosmology Project

http://supernova.lbl.gov/news.html

February 18, 2016. The Wide-Field Infrared Survey Telescope project begins! More information can be found here. November 10, 2014. The Supernova Cosmology Project and High-Z Team share the 2015 Breakthrough Prize in Fundamental Physics! More information can be found here. May 1, 2014. Hubble Astronomers Check the Prescription of a Cosmic Lens. January 9, 2013. The Farthest Supernova Yet for Measuring Cosmic History. More information can be found here. October 4, 2011. More information can be found here.

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ダークエネルギー - Wikipedia

https://ja.wikipedia.org/wiki/ダークエネルギー

出典: フリー百科事典ウィキペディア Wikipedia. 全体に広がって負の圧力を持ち、実質的に反発する重力としての効果を及ぼしている仮想的なエネルギー. ダークエネルギーと言う用語は、フリッツツビッキー. ダークマターになぞらえて、マイケルターナー. BAO)の観測を合わせると、宇宙は減速膨張から加速膨張へ 66.2億年前に移行し、現在では宇宙のエネルギーの72.9% 観測誤差1.4%)を暗黒エネルギーが占めていることが測定されている。また、宇宙の状態方程式は7 の精度で求められ、曲率は0.6%の精度で Λ-CDMモデル. 大規模な銀河探索であるスローンデジタルスカイサーベイ. が大きなスケールで 0 になるような臨界密度. 全天Ｘ線監視装置搭載 X 線 CCD カメラ. 29-33 (2011) . http:/ www.jasma.info/journal/wp-content/uploads/past/assets/images/jornal/28-1/28-1/2011 p029.pdf. Phys Rev. Lett. 565 86. arXiv.

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Hubbleův vesmírný dalekohled – Wikipedie

https://cs.wikipedia.org/wiki/Hubbleův_vesmírný_dalekohled

Z Wikipedie, otevřené encyklopedie. Hubbleův vesmírný dalekohled z raketoplánu. Během páté servisní mise ( STS-125. Hubble Space Telescope, HST. 500 600 km (pohyblivá). Zhruba 4,3 m. Rozložené schéma Hubbleova vesmírného dalekohledu. Zkratka HST z Hubble Space Telescope. Někdy také jen krátce Hubble) je dalekohled. Který na oběžnou dráhu. Do výše 600 kilometrů vynesl v roce 1990. Současná výška je asi 569 km. Dalekohled předává na Zemi obrazy vesmíru. 160;neovlivněné zemskou atmosférou. Další budoucnost...

snfactory.lbl.gov

Useful Links

http://snfactory.lbl.gov/snf/snf-links.html

Groups (U.S.). Quick Links to SNfactory pages:. Main Components of SNfactory. SNfactory in the News. Computer Schedule Spring 2006.

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FÍSICA EM FOCO: Outubro 2011

http://fisicaemfoco-ierb.blogspot.com/2011_10_01_archive.html

Quarta-feira, 5 de outubro de 2011. ALMA abre seus olhos! O observatório astronômico terrestre mais complexo do mundo, o Atacama Large Millimeter/submillimeter Array (ALMA), abriu oficialmente aos astrônomos e publicou a primeira imagem revelada pelo telescópio. A imagem, das galáxias Antenas, mostra “uma vista sobre o Universo impossível de obter com os telescópios que observam a luz visível e infravermelha”, divulga o ALMA em comunicado. A Ciência em Si ). Compartilhar com o Pinterest. The Supernova Co...

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"Latigasos": Nobel de física

http://ibnfayum.blogspot.com/2011/10/nobel-de-fisica.html

Martes, 4 de octubre de 2011. Ací vos deixe l'article d'El País sobre el premi Nobel de física:. Nobel de Física para la aceleración del universo. Tres científicos que descubrieron el efecto, que puede ser debido a la denominada energía oscura, reciben el galardón. Los descubrimientos premiados se remontan a 1998, y fueron una sorpresa general en la comunidad científica. Además, para mayor solidez del hallazgo, fue logrado por dos grupos competidores trabajando independientemente, uno liderado por Pe...

en.fphysics.com

Law

http://en.fphysics.com/law

The forces of inertia and gravitation. The Law of Gravity. Comparison of generally accepted and proposed approaches to the development of science. The theory of electrical conductivity. Inductance of the electron. History of the electromagnetic mass. On the virial theorem and its physical meaning. Explanation of the phenomena based on the Lorentz force in the mass-specrtometer experimentz. Disadvantages of modern physics textbooks. The Law of Gravity. Starting in the second half of the 20. In our Galaxy,...

panisse.lbl.gov

Supernova Cosmology Project

http://panisse.lbl.gov/pubs.html

Posters and Presentations at AAS Meetings. Lensed Type Ia supernovae as probes of cluster mass models. J Nordin, et al., MNRAS (2014). Available at http:/ adsabs.harvard.edu/abs/2014MNRAS.440.2742N. Precision Measurement of The Most Distant Spectroscopically Confirmed Supernova Ia with the Hubble Space Telescope. D Rubin, et al., ApJ (2013). Available at http:/ adsabs.harvard.edu/abs/2013ApJ.763.35R. The Hubble Space Telescope Cluster Supernova Survey:. VI The Volumetric Type Ia Supernova Rate. Hubble Sp...

panisse.lbl.gov

Supernova Cosmology Project

http://panisse.lbl.gov/slides_new.html

Color Figures for Slides. Hubble Diagram for SCP low-extinction subsample;. Residuals relative to an empty universe. PDF. Top panel only of previous Hubble diagram Figure 6. Confidence regions for Omega Mass vs Omega Lambda. With results from CMB and galaxy cluster data added. PDF. Joint measurements of Omega Mass and w assuming a flat universe and w constant in time. These slides in PowerPoint format.

panisse.lbl.gov

Supernova Cosmology Project

http://panisse.lbl.gov/people.html

Saul Perlmutter / PI. Saul Perlmutter - Lead Scientist. Lawrence Berkeley National Laboratory. Space Telescope Science Institute. Paris Supernova Cosmology Group. Collaboration Meeting at LBNL:.

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Supernova Cosmology Project

HST Cluster Supernova Survey. Lensed Type Ia supernovae as probes of cluster mass models. J Nordin, et al., MNRAS (2014). Available at http:/ adsabs.harvard.edu/abs/2014MNRAS.440.2742N. Precision Measurement of The Most Distant Spectroscopically Confirmed Supernova Ia with the Hubble Space Telescope. D Rubin, et al., ApJ (2013). Available at http:/ adsabs.harvard.edu/abs/2013ApJ.763.35R. J Meyers, et al., ApJ (2012). Available at http:/ adsabs.harvard.edu/abs/2012ApJ.750.1M. Data and Additional Info.

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