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  2. Luminosity function (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Luminosity_function...

    Luminosity functions are used to study the properties of large groups or classes of objects, such as the stars in clusters or the galaxies in the Local Group. Note that the term "function" is slightly misleading, and the luminosity function might better be described as a luminosity distribution. Given a luminosity as input, the luminosity ...

  3. Press–Schechter formalism - Wikipedia

    en.wikipedia.org/wiki/Press–Schechter_formalism

    The Press–Schechter formalism predicts that the number of objects with mass between and + is: = (+) ¯ (+) / ⁡ (() (+) /). where is the index of the power spectrum of the fluctuations in the early universe (), ¯ is the mean (baryonic and dark) matter density of the universe at the time the fluctuation from which the object was formed had gravitationally collapsed, and is a cut-off mass ...

  4. Paul L. Schechter - Wikipedia

    en.wikipedia.org/wiki/Paul_L._Schechter

    Paul L. Schechter (born May 30, 1948) is an American astronomer and observational cosmologist. He is the William A. M. Burden Professor of Astrophysics, Emeritus, at MIT . Schechter received his bachelor's degree from Cornell in 1968, and his Ph.D. degree from Caltech in 1975.

  5. Template:Schechter Handbook of Analysis and Its Foundations ...

    en.wikipedia.org/wiki/Template:Schechter...

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  6. Eric Schechter - Wikipedia

    en.wikipedia.org/wiki/Eric_Schechter

    Eric Schechter (born August 1, 1950) is an American mathematician, retired from Vanderbilt University with the title of professor emeritus. His interests started primarily in analysis but moved into mathematical logic .

  7. File:Schaffer function 2.pdf - Wikipedia

    en.wikipedia.org/wiki/File:Schaffer_function_2.pdf

    You are free: to share – to copy, distribute and transmit the work; to remix – to adapt the work; Under the following conditions: attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made.

  8. File:Schaffer function 2 - multi-objective.pdf - Wikipedia

    en.wikipedia.org/wiki/File:Schaffer_function_2...

    Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts.

  9. Two envelopes problem - Wikipedia

    en.wikipedia.org/wiki/Two_envelopes_problem

    Since the situation is symmetric, it seems obvious that there is no point in switching envelopes. On the other hand, a simple calculation using expected values suggests the opposite conclusion, that it is always beneficial to swap envelopes, since the person stands to gain twice as much money if they switch, while the only risk is halving what ...