[[["https://export.arxiv.org/api/query?id_list=astro-ph/9812133"], {}, "\n\n \n ArXiv Query: search_query=&id_list=astro-ph/9812133&start=0&max_results=10\n http://arxiv.org/api/SfKekabpSjI/htnxCLpK3q9AsUs\n 2018-08-09T00:00:00-04:00\n 1\n 0\n 10\n \n http://arxiv.org/abs/astro-ph/9812133v1\n 1998-12-08T03:27:34Z\n 1998-12-08T03:27:34Z\n Measurements of Omega and Lambda from 42 High-Redshift Supernovae\n We report measurements of the mass density, Omega_M, and\ncosmological-constant energy density, Omega_Lambda, of the universe based on\nthe analysis of 42 Type Ia supernovae discovered by the Supernova Cosmology\nProject. The magnitude-redshift data for these SNe, at redshifts between 0.18\nand 0.83, are fit jointly with a set of SNe from the Calan/Tololo Supernova\nSurvey, at redshifts below 0.1, to yield values for the cosmological\nparameters. All SN peak magnitudes are standardized using a SN Ia lightcurve\nwidth-luminosity relation. The measurement yields a joint probability\ndistribution of the cosmological parameters that is approximated by the\nrelation 0.8 Omega_M - 0.6 Omega_Lambda ~= -0.2 +/- 0.1 in the region of\ninterest (Omega_M <~ 1.5). For a flat (Omega_M + Omega_Lambda = 1) cosmology we\nfind Omega_M = 0.28{+0.09,-0.08} (1 sigma statistical) {+0.05,-0.04}\n(identified systematics). The data are strongly inconsistent with a Lambda = 0\nflat cosmology, the simplest inflationary universe model. An open, Lambda = 0\ncosmology also does not fit the data well: the data indicate that the\ncosmological constant is non-zero and positive, with a confidence of P(Lambda >\n0) = 99%, including the identified systematic uncertainties. The best-fit age\nof the universe relative to the Hubble time is t_0 = 14.9{+1.4,-1.1} (0.63/h)\nGyr for a flat cosmology. The size of our sample allows us to perform a variety\nof statistical tests to check for possible systematic errors and biases. We\nfind no significant differences in either the host reddening distribution or\nMalmquist bias between the low-redshift Calan/Tololo sample and our\nhigh-redshift sample. The conclusions are robust whether or not a\nwidth-luminosity relation is used to standardize the SN peak magnitudes.\n\n \n S. Perlmutter\n The Supernova Cosmology Project\n \n \n G. Aldering\n The Supernova Cosmology Project\n \n \n G. Goldhaber\n The Supernova Cosmology Project\n \n \n R. A. Knop\n The Supernova Cosmology Project\n \n \n P. Nugent\n The Supernova Cosmology Project\n \n \n P. G. Castro\n The Supernova Cosmology Project\n \n \n S. Deustua\n The Supernova Cosmology Project\n \n \n S. Fabbro\n The Supernova Cosmology Project\n \n \n A. Goobar\n The Supernova Cosmology Project\n \n \n D. E. Groom\n The Supernova Cosmology Project\n \n \n I. M. Hook\n The Supernova Cosmology Project\n \n \n A. G. Kim\n The Supernova Cosmology Project\n \n \n M. Y. Kim\n The Supernova Cosmology Project\n \n \n J. C. Lee\n The Supernova Cosmology Project\n \n \n N. J. Nunes\n The Supernova Cosmology Project\n \n \n R. Pain\n The Supernova Cosmology Project\n \n \n C. R. Pennypacker\n The Supernova Cosmology Project\n \n \n R. Quimby\n The Supernova Cosmology Project\n \n \n C. Lidman\n The Supernova Cosmology Project\n \n \n R. S. Ellis\n The Supernova Cosmology Project\n \n \n M. Irwin\n The Supernova Cosmology Project\n \n \n R. G. McMahon\n The Supernova Cosmology Project\n \n \n P. Ruiz-Lapuente\n The Supernova Cosmology Project\n \n \n N. Walton\n The Supernova Cosmology Project\n \n \n B. Schaefer\n The Supernova Cosmology Project\n \n \n B. J. Boyle\n The Supernova Cosmology Project\n \n \n A. V. Filippenko\n The Supernova Cosmology Project\n \n \n T. Matheson\n The Supernova Cosmology Project\n \n \n A. S. Fruchter\n The Supernova Cosmology Project\n \n \n N. Panagia\n The Supernova Cosmology Project\n \n \n H. J. M. Newberg\n The Supernova Cosmology Project\n \n \n W. J. Couch\n The Supernova Cosmology Project\n \n 10.1086/307221\n \n 21 pages and 10 figures. Accepted for publication in the\n Astrophysical Journal. Individual color figures, supplementary tables, and\n preprint also available at http://www-supernova.lbl.gov/\n Astrophys.J.517:565-586,1999\n \n \n \n \n \n \n \n\n", 200, null], [["http://dx.doi.org/10.1086/307221"], {"headers": {"accept": "application/x-bibtex"}}, "@article{Perlmutter_1999,\n\tdoi = {10.1086/307221},\n\turl = {https://doi.org/10.1086%2F307221},\n\tyear = 1999,\n\tmonth = {jun},\n\tpublisher = {{IOP} Publishing},\n\tvolume = {517},\n\tnumber = {2},\n\tpages = {565--586},\n\tauthor = {S. Perlmutter and G. Aldering and G. Goldhaber and R. A. Knop and P. Nugent and P. G. Castro and S. Deustua and S. Fabbro and A. Goobar and D. E. Groom and I. M. Hook and A. G. Kim and M. Y. Kim and J. C. Lee and N. J. Nunes and R. Pain and C. R. Pennypacker and R. Quimby and C. Lidman and R. S. Ellis and M. Irwin and R. G. McMahon and P. Ruiz-Lapuente and N. Walton and B. Schaefer and B. J. Boyle and A. V. Filippenko and T. Matheson and A. S. Fruchter and N. Panagia and H. J. M. Newberg and W. J. Couch and The Supernova Cosmology Project},\n\ttitle = {Measurements of $\\{upOmega}$ and $\\{upLambda}$ from 42 High-Redshift Supernovae},\n\tjournal = {The Astrophysical Journal}\n}", 200, null], [["https://export.arxiv.org/api/query?id_list=astro-ph/9812133"], {}, "\n\n \n ArXiv Query: search_query=&id_list=astro-ph/9812133&start=0&max_results=10\n http://arxiv.org/api/SfKekabpSjI/htnxCLpK3q9AsUs\n 2018-08-09T00:00:00-04:00\n 1\n 0\n 10\n \n http://arxiv.org/abs/astro-ph/9812133v1\n 1998-12-08T03:27:34Z\n 1998-12-08T03:27:34Z\n Measurements of Omega and Lambda from 42 High-Redshift Supernovae\n We report measurements of the mass density, Omega_M, and\ncosmological-constant energy density, Omega_Lambda, of the universe based on\nthe analysis of 42 Type Ia supernovae discovered by the Supernova Cosmology\nProject. The magnitude-redshift data for these SNe, at redshifts between 0.18\nand 0.83, are fit jointly with a set of SNe from the Calan/Tololo Supernova\nSurvey, at redshifts below 0.1, to yield values for the cosmological\nparameters. All SN peak magnitudes are standardized using a SN Ia lightcurve\nwidth-luminosity relation. The measurement yields a joint probability\ndistribution of the cosmological parameters that is approximated by the\nrelation 0.8 Omega_M - 0.6 Omega_Lambda ~= -0.2 +/- 0.1 in the region of\ninterest (Omega_M <~ 1.5). For a flat (Omega_M + Omega_Lambda = 1) cosmology we\nfind Omega_M = 0.28{+0.09,-0.08} (1 sigma statistical) {+0.05,-0.04}\n(identified systematics). The data are strongly inconsistent with a Lambda = 0\nflat cosmology, the simplest inflationary universe model. An open, Lambda = 0\ncosmology also does not fit the data well: the data indicate that the\ncosmological constant is non-zero and positive, with a confidence of P(Lambda >\n0) = 99%, including the identified systematic uncertainties. The best-fit age\nof the universe relative to the Hubble time is t_0 = 14.9{+1.4,-1.1} (0.63/h)\nGyr for a flat cosmology. The size of our sample allows us to perform a variety\nof statistical tests to check for possible systematic errors and biases. We\nfind no significant differences in either the host reddening distribution or\nMalmquist bias between the low-redshift Calan/Tololo sample and our\nhigh-redshift sample. The conclusions are robust whether or not a\nwidth-luminosity relation is used to standardize the SN peak magnitudes.\n\n \n S. Perlmutter\n The Supernova Cosmology Project\n \n \n G. Aldering\n The Supernova Cosmology Project\n \n \n G. Goldhaber\n The Supernova Cosmology Project\n \n \n R. A. Knop\n The Supernova Cosmology Project\n \n \n P. Nugent\n The Supernova Cosmology Project\n \n \n P. G. Castro\n The Supernova Cosmology Project\n \n \n S. Deustua\n The Supernova Cosmology Project\n \n \n S. Fabbro\n The Supernova Cosmology Project\n \n \n A. Goobar\n The Supernova Cosmology Project\n \n \n D. E. Groom\n The Supernova Cosmology Project\n \n \n I. M. Hook\n The Supernova Cosmology Project\n \n \n A. G. Kim\n The Supernova Cosmology Project\n \n \n M. Y. Kim\n The Supernova Cosmology Project\n \n \n J. C. Lee\n The Supernova Cosmology Project\n \n \n N. J. Nunes\n The Supernova Cosmology Project\n \n \n R. Pain\n The Supernova Cosmology Project\n \n \n C. R. Pennypacker\n The Supernova Cosmology Project\n \n \n R. Quimby\n The Supernova Cosmology Project\n \n \n C. Lidman\n The Supernova Cosmology Project\n \n \n R. S. Ellis\n The Supernova Cosmology Project\n \n \n M. Irwin\n The Supernova Cosmology Project\n \n \n R. G. McMahon\n The Supernova Cosmology Project\n \n \n P. Ruiz-Lapuente\n The Supernova Cosmology Project\n \n \n N. Walton\n The Supernova Cosmology Project\n \n \n B. Schaefer\n The Supernova Cosmology Project\n \n \n B. J. Boyle\n The Supernova Cosmology Project\n \n \n A. V. Filippenko\n The Supernova Cosmology Project\n \n \n T. Matheson\n The Supernova Cosmology Project\n \n \n A. S. Fruchter\n The Supernova Cosmology Project\n \n \n N. Panagia\n The Supernova Cosmology Project\n \n \n H. J. M. Newberg\n The Supernova Cosmology Project\n \n \n W. J. Couch\n The Supernova Cosmology Project\n \n 10.1086/307221\n \n 21 pages and 10 figures. Accepted for publication in the\n Astrophysical Journal. Individual color figures, supplementary tables, and\n preprint also available at http://www-supernova.lbl.gov/\n Astrophys.J.517:565-586,1999\n \n \n \n \n \n \n \n\n", 200, null], [["http://dx.doi.org/10.1086/307221"], {"headers": {"accept": "application/x-bibtex"}}, "@article{Perlmutter_1999,\n\tdoi = {10.1086/307221},\n\turl = {https://doi.org/10.1086%2F307221},\n\tyear = 1999,\n\tmonth = {jun},\n\tpublisher = {{IOP} Publishing},\n\tvolume = {517},\n\tnumber = {2},\n\tpages = {565--586},\n\tauthor = {S. Perlmutter and G. Aldering and G. Goldhaber and R. A. Knop and P. Nugent and P. G. Castro and S. Deustua and S. Fabbro and A. Goobar and D. E. Groom and I. M. Hook and A. G. Kim and M. Y. Kim and J. C. Lee and N. J. Nunes and R. Pain and C. R. Pennypacker and R. Quimby and C. Lidman and R. S. Ellis and M. Irwin and R. G. McMahon and P. Ruiz-Lapuente and N. Walton and B. Schaefer and B. J. Boyle and A. V. Filippenko and T. Matheson and A. S. Fruchter and N. Panagia and H. J. M. Newberg and W. J. Couch and The Supernova Cosmology Project},\n\ttitle = {Measurements of $\\{upOmega}$ and $\\{upLambda}$ from 42 High-Redshift Supernovae},\n\tjournal = {The Astrophysical Journal}\n}", 200, null], [["https://export.arxiv.org/api/query?id_list=math/0211159"], {}, "\n\n \n ArXiv Query: search_query=&id_list=math/0211159&start=0&max_results=10\n http://arxiv.org/api/4nVRTcAL5Np4oaGFQnqVPG0+c5k\n 2018-08-09T00:00:00-04:00\n 1\n 0\n 10\n \n http://arxiv.org/abs/math/0211159v1\n 2002-11-11T16:11:49Z\n 2002-11-11T16:11:49Z\n The entropy formula for the Ricci flow and its geometric applications\n We present a monotonic expression for the Ricci flow, valid in all dimensions\nand without curvature assumptions. It is interpreted as an entropy for a\ncertain canonical ensemble. Several geometric applications are given. In\nparticular, (1) Ricci flow, considered on the space of riemannian metrics\nmodulo diffeomorphism and scaling, has no nontrivial periodic orbits (that is,\nother than fixed points); (2) In a region, where singularity is forming in\nfinite time, the injectivity radius is controlled by the curvature; (3) Ricci\nflow can not quickly turn an almost euclidean region into a very curved one, no\nmatter what happens far away. We also verify several assertions related to\nRichard Hamilton's program for the proof of Thurston geometrization conjecture\nfor closed three-manifolds, and give a sketch of an eclectic proof of this\nconjecture, making use of earlier results on collapsing with local lower\ncurvature bound.\n\n \n Grisha Perelman\n \n 39 pages\n \n \n \n \n \n \n\n", 200, null], [["http://dx.doi.org/10.1007/BF01700692"], {"headers": {"accept": "application/x-bibtex"}}, "@article{G_del_1931,\n\tdoi = {10.1007/bf01700692},\n\turl = {https://doi.org/10.1007%2Fbf01700692},\n\tyear = 1931,\n\tmonth = {dec},\n\tpublisher = {Springer Nature},\n\tvolume = {38-38},\n\tnumber = {1},\n\tpages = {173--198},\n\tauthor = {Kurt G\u00f6del},\n\ttitle = {\u00dcber formal unentscheidbare S\u00e4tze der Principia Mathematica und verwandter Systeme I},\n\tjournal = {Monatshefte f\u00fcr Mathematik und Physik}\n}", 200, null], [["http://dx.doi.org/999999"], {"headers": {"accept": "application/x-bibtex"}}, "\n\n\nError: DOI Not Found\n\n\n\n\n \n\n\n\n\n\n\n
\n\"Logo\"\n
\n\n
\n
\n
\n\n\n\n\n\n \n \n \n \n
\"\"\n HOME  | HANDBOOK  | FACTSHEETS  | FAQs  |  RESOURCES  | USERS  | NEWS  | MEMBERS AREA\n
\n\n\n
\n
\n\n\n\n \n\n\n\n\n\n\n\n\n\n\n
\n\"\"\n
\n\n

DOI Not Found

\n\n
 
\n\n\n\n

10/999999

\n\n
 
\n\n\n\n\n

This DOI cannot be found in the DOI System. Possible reasons are:

\n\n\n
    \n\n
  • The DOI is incorrect in your source. Search for the item by name, title, or other metadata using a search engine.
  • \n\n
  • The DOI was copied incorrectly. Check to see that the string includes all the characters before and after the slash and no sentence punctuation marks.
  • \n\n
  • The DOI has not been activated yet. Please try again later, and report the problem if the error continues.
  • \n\n
\n\n\n\n
 
\n\n

You may report this error to the responsible DOI Registration Agency using the form below. Include your email address to receive confirmation and feedback.

\n\n
\n\n
\n\n\n\n\n\n\n\n\n\n\n\n\n
\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
Your Email Address:
Additional Information About the Error:
\n\n

\n\n
\n
\n\n\n\n\n
\"\"
\n\n
 
\n\n\n\n\n\n\n\n\n\n\n\n\n \n\n
\nDOI System Proxy Server Documentation\n
\n\"DOI_disc_logo\"\n\n®, DOI®, DOI.ORG®, and shortDOI® are trademarks of the International DOI Foundation.\n
\n\n\n", 404, "404 Client Error: for url: http://dx.doi.org/999999"], [["http://dx.doi.org/10.1007/BF01700692"], {"headers": {"accept": "application/x-bibtex"}}, "@article{G_del_1931,\n\tdoi = {10.1007/bf01700692},\n\turl = {https://doi.org/10.1007%2Fbf01700692},\n\tyear = 1931,\n\tmonth = {dec},\n\tpublisher = {Springer Nature},\n\tvolume = {38-38},\n\tnumber = {1},\n\tpages = {173--198},\n\tauthor = {Kurt G\u00f6del},\n\ttitle = {\u00dcber formal unentscheidbare S\u00e4tze der Principia Mathematica und verwandter Systeme I},\n\tjournal = {Monatshefte f\u00fcr Mathematik und Physik}\n}", 200, null], [["http://www.ottobib.com/isbn/9782081336742/bibtex"], {"headers": null}, "\n\n\n\n \n \n \n \n \n \n \n \n\n \n\n Bibliography and Works Cited Generator for MLA, APA, Wikipedia and Bibtex - OttoBib.com \n \n \n\n \n \n \n \n \n \n \n \n \n \n \n
\n \n
\n
\n

OttoBib

\n

bibtex Format

\n
\n
\n\n
\n
\n \n
\n
\n
\n\n
\n

\n NOTE!\n
\n

    \n
  1. Verify accuracy of the data (particularly authors)
  2. \n
  3. Remember to do a HANGING INDENT (something I cannot do with HTML here)
  4. \n
  5. I strive for accuracy of the citations but you should treat this tool as a starting point in your works cited, because you still need to look it over.
  6. \n
\n

\n
\n
\n\n
\n \n\n \n", 200, null], [["http://www.ottobib.com/isbn/9999999999999/bibtex"], {"headers": null}, "\n\n\n\n \n \n \n \n \n \n \n \n\n \n\n Bibliography and Works Cited Generator for MLA, APA, Wikipedia and Bibtex - OttoBib.com \n \n \n\n \n \n \n \n \n \n \n \n \n \n \n
\n \n
\n\t

OttoBib

\n\t

Make a bibliography or works cited with just an ISBN. It's free, easy and FAST

\n\t

\n\t about ottobib and history\n\t \n\t

\n\t \n

\n\t
\n
\n\n
\n
\n\n
No Results for 9999999999999
\n
\n

\n Enter ISBN of book(s) - separate with commas (,)\n

\n \n read more about ISBN on Wikipedia\n \n
\n \n \n \n \n \n\n
\n \n
\n
\n\n
\n
\n\n

Did OttoBib help you? Then help us and Like us on Facebook!

\n
\n
\n\n\n
\n\n\n\n\n
\n \n\n \n", 200, null], [["http://www.ottobib.com/isbn/9782081336742/bibtex"], {"headers": null}, "\n\n\n\n \n \n \n \n \n \n \n \n\n \n\n Bibliography and Works Cited Generator for MLA, APA, Wikipedia and Bibtex - OttoBib.com \n \n \n\n \n \n \n \n \n \n \n \n \n \n \n
\n \n
\n
\n

OttoBib

\n

bibtex Format

\n
\n
\n\n
\n
\n \n
\n
\n
\n\n
\n

\n NOTE!\n
\n

    \n
  1. Verify accuracy of the data (particularly authors)
  2. \n
  3. Remember to do a HANGING INDENT (something I cannot do with HTML here)
  4. \n
  5. I strive for accuracy of the citations but you should treat this tool as a starting point in your works cited, because you still need to look it over.
  6. \n
\n

\n
\n
\n\n
\n \n\n \n", 200, null]]