Luminosity function

Results: 30



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11Ay 124: Structure and Dynamics of Galaxies

Ay 124: Structure and Dynamics of Galaxies

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Source URL: www.tapir.caltech.edu

Language: English - Date: 2010-01-22 12:30:27
12PHD QUALIFY EXAMINATION —GALACTIC AND EXTRAGALACTIC ASTROPHYSICS September, points) Calculate the order of magnitude of the Sunyaev-Zel’dovich effect for a typical cluster of galaxypoints)

PHD QUALIFY EXAMINATION —GALACTIC AND EXTRAGALACTIC ASTROPHYSICS September, points) Calculate the order of magnitude of the Sunyaev-Zel’dovich effect for a typical cluster of galaxypoints)

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Source URL: www.astro.ncu.edu.tw

Language: English - Date: 2014-05-12 00:06:46
13PHD QUALIFY EXAMINATION — GALACTIC AND EXTRAGALACTIC ASTROPHYSICS 25th September, points) (a) (5 points) What are the luminosity function Φ(M ), the initial luminosity function

PHD QUALIFY EXAMINATION — GALACTIC AND EXTRAGALACTIC ASTROPHYSICS 25th September, points) (a) (5 points) What are the luminosity function Φ(M ), the initial luminosity function

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Source URL: www.astro.ncu.edu.tw

Language: English - Date: 2014-05-12 00:06:46
14The White Dwarf Luminosity Function from SDSS Imaging Data  arXiv:astro-phv1 29 Oct 2005 Hugh C. Harris1,11 , Jeffrey A. Munn1 , Mukremin Kilic2 , James Liebert3 , Kurtis A. Williams3 , Ted von Hippel2 , Stephen

The White Dwarf Luminosity Function from SDSS Imaging Data arXiv:astro-phv1 29 Oct 2005 Hugh C. Harris1,11 , Jeffrey A. Munn1 , Mukremin Kilic2 , James Liebert3 , Kurtis A. Williams3 , Ted von Hippel2 , Stephen

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Source URL: www.as.utexas.edu

Language: English - Date: 2005-11-04 13:01:46
15GMT Science Use Case Measuring the Faint End Slope of the Lyα Luminosity Function at z ~ 6 Abstract: The source of reionization at z > 6 remains uncertain as the present suite of telescopes and instruments appear to be

GMT Science Use Case Measuring the Faint End Slope of the Lyα Luminosity Function at z ~ 6 Abstract: The source of reionization at z > 6 remains uncertain as the present suite of telescopes and instruments appear to be

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Source URL: www.gsmt.noao.edu

Language: English - Date: 2008-04-30 17:22:10
16Probing Star Formation at Early Times Science Use Cases: Lyα Luminosity Function at z ~ 6 Stellar Content of Passive Galaxies at z > 1.5  P. McCarthy

Probing Star Formation at Early Times Science Use Cases: Lyα Luminosity Function at z ~ 6 Stellar Content of Passive Galaxies at z > 1.5 P. McCarthy

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Source URL: www.gsmt.noao.edu

Language: English - Date: 2008-08-15 14:17:20
17Mon. Not. R. Astron. Soc. 000, 1–[removed]Printed 24 June[removed]MN LATEX style file v2.2)

Mon. Not. R. Astron. Soc. 000, 1–[removed]Printed 24 June[removed]MN LATEX style file v2.2)

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Source URL: arxiv.org

Language: English - Date: 2014-06-23 20:26:02
181 Ay 124 Winter 2014 – HOMEWORK #2 Due Friday, Jan 31, 2014 by 5pm, in Steidel’s mailbox in 249 Cahill Problem 1 A galaxy forms stars at a constant rate with an initial mass function

1 Ay 124 Winter 2014 – HOMEWORK #2 Due Friday, Jan 31, 2014 by 5pm, in Steidel’s mailbox in 249 Cahill Problem 1 A galaxy forms stars at a constant rate with an initial mass function

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Source URL: www.astro.caltech.edu

Language: English - Date: 2014-01-24 13:55:03
19Limits on the luminosity function of Ly emitters at z = 7.7

Limits on the luminosity function of Ly emitters at z = 7.7

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Source URL: cds.aanda.org

Language: English
20Limits on the luminosity function of Ly emitters at z = 7.7

Limits on the luminosity function of Ly emitters at z = 7.7

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Source URL: www.aanda.org

Language: English