1![From Spitzer to Herschel Extragalactic Surveys The Evolution of the Infrared Luminosity Function and of the Cosmic Star Formation Rate Density Mattia Vaccari - University of the Western Cape From Spitzer to Herschel Extragalactic Surveys The Evolution of the Infrared Luminosity Function and of the Cosmic Star Formation Rate Density Mattia Vaccari - University of the Western Cape](https://www.pdfsearch.io/img/330139c6febb236d2e692deaf60e1f75.jpg) | Add to Reading ListSource URL: www.uwcastro.orgLanguage: English - Date: 2013-01-15 09:49:31
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2![FORMATION AND EVOLUTION OF BLACK HOLES Aspen Center for Physics 2010 Winter Conference on Astrophysics February 14–20, 2010 TITLE: The Evolution of the Hard X-ray Luminosity Function of AGN FORMATION AND EVOLUTION OF BLACK HOLES Aspen Center for Physics 2010 Winter Conference on Astrophysics February 14–20, 2010 TITLE: The Evolution of the Hard X-ray Luminosity Function of AGN](https://www.pdfsearch.io/img/e671e620a2c9319454e41721f6babb14.jpg) | Add to Reading ListSource URL: ciera.northwestern.eduLanguage: English - Date: 2010-02-10 16:19:29
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3![Draft version October 14, 2005 Preprint typeset using LATEX style emulateapj vGALAXIES AT Z ∼ 6: THE REST-FRAME U V LUMINOSITY FUNCTION AND LUMINOSITY DENSITY FROM 506 UDF, UDF-PS, AND GOODS I-DROPOUTS Draft version October 14, 2005 Preprint typeset using LATEX style emulateapj vGALAXIES AT Z ∼ 6: THE REST-FRAME U V LUMINOSITY FUNCTION AND LUMINOSITY DENSITY FROM 506 UDF, UDF-PS, AND GOODS I-DROPOUTS](https://www.pdfsearch.io/img/76636a344b8a15c32fde16e76faec72b.jpg) | Add to Reading ListSource URL: acs.pha.jhu.eduLanguage: English - Date: 2005-12-09 12:39:26
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4![Reionization and the High-Redshift Galaxy UV Luminosity Function with Reionization and the High-Redshift Galaxy UV Luminosity Function with](https://www.pdfsearch.io/img/28e56a25c98447ae49c92f6f61bd2979.jpg) | Add to Reading ListSource URL: firstgalaxies.orgLanguage: English - Date: 2016-03-17 12:45:17
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5![Draft version October 14, 2005 Preprint typeset using LATEX style emulateapj vGALAXIES AT Z ∼ 6: THE REST-FRAME U V LUMINOSITY FUNCTION AND LUMINOSITY DENSITY FROM 506 UDF, UDF-PS, AND GOODS I-DROPOUTS Draft version October 14, 2005 Preprint typeset using LATEX style emulateapj vGALAXIES AT Z ∼ 6: THE REST-FRAME U V LUMINOSITY FUNCTION AND LUMINOSITY DENSITY FROM 506 UDF, UDF-PS, AND GOODS I-DROPOUTS](https://www.pdfsearch.io/img/46d10297218ccccce63ae24e3b66858e.jpg) | Add to Reading ListSource URL: adcam.pha.jhu.eduLanguage: English - Date: 2005-12-09 12:39:26
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6![Answers Research Journal):67–79. www.answersingenesis.org/arj/v9/luminosity_function_galaxies.pdf New Method to Assess the Luminosity Function of Galaxies Jason Lisle, Institute for Creation Research,1806 Royal Answers Research Journal):67–79. www.answersingenesis.org/arj/v9/luminosity_function_galaxies.pdf New Method to Assess the Luminosity Function of Galaxies Jason Lisle, Institute for Creation Research,1806 Royal](https://www.pdfsearch.io/img/c6fa60fa4309ab99d386277a1d889b50.jpg) | Add to Reading ListSource URL: assets.answersingenesis.orgLanguage: English - Date: 2016-03-30 12:05:28
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7![ASTROPHYSICS SEMINAR Wednesday, 19 December 2012 at 11:00 AGN Hard X-ray luminosity function and the Lockman Hole Deep Field ASTROPHYSICS SEMINAR Wednesday, 19 December 2012 at 11:00 AGN Hard X-ray luminosity function and the Lockman Hole Deep Field](https://www.pdfsearch.io/img/1967649c01a22d17755e7cfd2bc4bff1.jpg) | Add to Reading ListSource URL: isdc.unige.chLanguage: English - Date: 2012-12-14 04:58:47
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8![THE LUMINOSITY FUNCTION OF LOW-MASS STARS AND BROWN DWARFS Kelle Lin Cruz A DISSERTATION in Physics and Astronomy THE LUMINOSITY FUNCTION OF LOW-MASS STARS AND BROWN DWARFS Kelle Lin Cruz A DISSERTATION in Physics and Astronomy](https://www.pdfsearch.io/img/0ae9e11d6463f57b6d439ae4569b64d9.jpg) | Add to Reading ListSource URL: www.kellecruz.comLanguage: English - Date: 2010-02-12 13:30:12
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9![Carbon-Enhanced Metal-Poor Stars in SDSS/SEGUE Cumulative frequencies of CEMP stars ([C/Fe] ≥ +0.7) from the SDSS/SEGUE sample, as a function of [Fe/H], for three different luminosity classes: giants (circles), main-s Carbon-Enhanced Metal-Poor Stars in SDSS/SEGUE Cumulative frequencies of CEMP stars ([C/Fe] ≥ +0.7) from the SDSS/SEGUE sample, as a function of [Fe/H], for three different luminosity classes: giants (circles), main-s](https://www.pdfsearch.io/img/d6c0a75771ee343a631e76f298bf7c53.jpg) | Add to Reading ListSource URL: www.jinaweb.orgLanguage: English - Date: 2014-03-07 10:40:33
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10![Ay 124 – Handouts 2 Stellar luminosity classes Disk luminosity function
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