About: Karl Glazebrook

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Karl Glazebrook FAA (born 1965) is a British astronomer, known for his work on galaxy formation, for playing a key role in developing the "nod and shuffle" technique for doing redshift surveys with large telescopes, and for originating the Perl Data Language (PDL). Glazebrook also developed the open-source Perl Data Language, a perl-based alternative to the commercial IDL. After his move to Australia he played a leading role in the WiggleZ Dark Energy Survey between 2006 and 2011.

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rdfs:label	Karl Glazebrook (de) Karl Glazebrook (es) Karl Glazebrook (fr) Karl Glazebrook (en)
rdfs:comment	Karl Glazebrook (* 11. Mai 1965 in Chatham, Kent) ist ein anglo-australischer Astronom und Kosmologe, der sich mit der Entwicklung von Galaxien und der Natur der Dunklen Energie beschäftigt. In der Öffentlichkeit bekannt wurde Glazebrook mit einer Arbeit zur „Farbe“ des Universums. (de) Karl Glazebrook FAA est un astronome britannique, connu pour ses travaux sur la formation des galaxies, pour avoir joué un rôle clé dans le développement de la technique « nod and shuffle » pour faire des relevés de redshift avec de grands télescopes, et pour avoir créé le langage de données (en). (fr) Karl Glazebrook FAA (born 1965) is a British astronomer, known for his work on galaxy formation, for playing a key role in developing the "nod and shuffle" technique for doing redshift surveys with large telescopes, and for originating the Perl Data Language (PDL). Glazebrook also developed the open-source Perl Data Language, a perl-based alternative to the commercial IDL. After his move to Australia he played a leading role in the WiggleZ Dark Energy Survey between 2006 and 2011. (en) Karl Glazebrook es un astrónomo anglo-australiano, conocido por su trabajo en la formación de galaxias, por desempeñar un papel clave en el desarrollo de la técnica nod and shuffle para hacer espectroscopia con telescopios grandes, y por haber ideado el Perl Data Language (PDL). En 2008, recibió el Premio María y Eric Muhlmann, para el desarrollo de instrumentos de investigación y técnicas innovadoras, de la Sociedad Astronómica del Pacífico. El asteroide (10099) Glazebrook fue nombrado en su honor. * Datos: Q1731257 (es)
dct:subject	Alumni of the University of Edinburgh Living people Academics of Durham University 1965 births Swinburne University of Technology faculty 21st-century Australian astronomers People educated at Chislehurst and Sidcup Grammar School
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Link from a Wikipage to another Wikipage	Hubble Space Telescope Johns Hopkins University Perl Data Language United Kingdom University of Cambridge University of Edinburgh WiggleZ Dark Energy Survey 10099 Glazebrook Alumni of the University of Edinburgh Living people Gemini Observatory Minor Planet Circulars Cosmic latte Redshift survey Academics of Durham University 2dF 1965 births Dark energy Durham University Astronomer Astronomical Society of the Pacific Spacewatch Swinburne University of Technology faculty 21st-century Australian astronomers Swinburne University of Technology People educated at Chislehurst and Sidcup Grammar School Australian Laureate Fellowship Spitzer Space Telescope IDL (programming language) Main-belt Galaxy formation Anglo-Australian Observatory dbr:Gemini_Deep_Deep_Survey
sameAs	Karl Glazebrook Karl Glazebrook Karl Glazebrook Karl Glazebrook Karl Glazebrook Karl Glazebrook Karl Glazebrook Karl Glazebrook Karl Glazebrook Karl Glazebrook
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has abstract	Karl Glazebrook (* 11. Mai 1965 in Chatham, Kent) ist ein anglo-australischer Astronom und Kosmologe, der sich mit der Entwicklung von Galaxien und der Natur der Dunklen Energie beschäftigt. In der Öffentlichkeit bekannt wurde Glazebrook mit einer Arbeit zur „Farbe“ des Universums. (de) Karl Glazebrook FAA (born 1965) is a British astronomer, known for his work on galaxy formation, for playing a key role in developing the "nod and shuffle" technique for doing redshift surveys with large telescopes, and for originating the Perl Data Language (PDL). Glazebrook was born in 1965 in the United Kingdom, and educated at the University of Cambridge and the University of Edinburgh (PhD 1992). He held post-doctoral appointments at the University of Durham and University of Cambridge before moving to the Anglo-Australian Observatory, where he played a central role in supporting the 2dF galaxy survey as its instrument scientist. He moved to Johns Hopkins University in 2000 where he was Professor of Astronomy until 2006, at which time he became Professor of Astronomy at Swinburne University of Technology in Melbourne, Australia. His work has been cited over 40,000 times in the literature of astronomy. Glazebrook also developed the open-source Perl Data Language, a perl-based alternative to the commercial IDL. Glazebrook was one of the leaders of the (GDDS) which measured the evolution of galaxies using Gemini Observatory and the Hubble and Spitzer Space Telescopes. The project, along with a number of other studies, determined in 2004 that massive galaxies formed surprisingly early in the distant Universe, explaining why a lot of them appear so remarkably old. As a whimsical side-project Glazebrook also determined that the bulk-averaged color of the Universe is Cosmic latte. Both pieces of work received wide publicity in the international press. The bulk-averaged color earned some additional international publicity because a software bug had initially suggested a pale turquoise instead of the bland beige. He is also well known in the astronomical community for his pioneering work in developing the baryon oscillation technique to use the distribution of galaxies as a probe of dark energy. After his move to Australia he played a leading role in the WiggleZ Dark Energy Survey between 2006 and 2011. (en) Karl Glazebrook es un astrónomo anglo-australiano, conocido por su trabajo en la formación de galaxias, por desempeñar un papel clave en el desarrollo de la técnica nod and shuffle para hacer espectroscopia con telescopios grandes, y por haber ideado el Perl Data Language (PDL). En 2008, recibió el Premio María y Eric Muhlmann, para el desarrollo de instrumentos de investigación y técnicas innovadoras, de la Sociedad Astronómica del Pacífico. Glazebrook nació en 1965 en el Reino Unido, y estudió en la Universidad de Cambridge y en la Universidad de Edimburgo (PhD 1992). Ocupó puestos postdoctorales en la Universidad de Durham y la Universidad de Cambridge antes de pasar al Observatorio Anglo-Australiano, donde desempeñó un papel central en el apoyo a la encuesta 2dF Galaxy Redshift Survey (Sondeo de corrimiento al rojo de galaxias en un campo de 2 grados), como científico de instrumento. Se trasladó a la Universidad Johns Hopkins en 2000, donde fue profesor de Astronomía hasta 2006, año en el cual se convirtió en profesor de Astronomía de la en Melbourne, Australia. Su trabajo ha sido citado más de 10 000 veces en la literatura de astronomía. Glazebrook es coinvestigador principal del estudio Gemini Deep Deep, que (junto con un número de otros estudios) determinó en 2004 que las galaxias masivas se forman sorprendentemente temprano en el universo distante. Como parte del proyecto caprichosa, Glazebrook también se determinó que la mayor parte, un promedio de color del universo es latte cósmico. Ambos trabajos recibieron una amplia publicidad en la prensa internacional. El asteroide (10099) Glazebrook fue nombrado en su honor. * Datos: Q1731257 (es) Karl Glazebrook FAA est un astronome britannique, connu pour ses travaux sur la formation des galaxies, pour avoir joué un rôle clé dans le développement de la technique « nod and shuffle » pour faire des relevés de redshift avec de grands télescopes, et pour avoir créé le langage de données (en). (fr)
gold:hypernym	Astronomer
schema:sameAs	Karl Glazebrook
prov:wasDerivedFrom	wikipedia-en:Karl_Glazebrook?oldid=1080246198&ns=0

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