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Welcome to my home page. Here you will be able to access information about me, and the work I am doing here at the University Sternwarte, part of the Ludwig Maximilian University in Munich.

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Welcome to my home page. Here you will be able to access information about me, and the work I am doing here at the University Sternwarte, part of the Ludwig Maximilian University in Munich.

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To obtain the Galaxy Zoo2 bar length measurement data, as published in this recent paper,, please follow this link

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To obtain the Galaxy Zoo2 bar length measurement data, as published in this recent paper, please follow this link

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My main research interests include mass measurements and correlation function of galaxy clusters. In particular I use optical, X-ray data & SZ selected clusters. I use clusters and correlation functions to constrain cosmological models and parameters using the cluster mass function, and the abundance of extreme clusters. I am also interested in large scale data analysis in Cosmology, involving correlating large surveys such as SDSS, XCS (see links opposite) and VESPA. I also work in astrophysics with Galaxy Zoo, in particular bar length and width measurements, and correlating bar properties with host galaxy properties. Combining astrophysics, statistics and cosmology, I have used VESPA to constrain homogeneity and isotropy of the Universe using the Star Formation Rate Histories of Luminous Red Galaxies as a proxy for homogeneity.

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My main research interests include machine learning photometric redshift estimation, exploring parameter space, and mass measurements and correlation function of galaxy clusters. In particular I use optical, X-ray data & SZ selected clusters. I use clusters and correlation functions to constrain cosmological models and parameters using the cluster mass function, and the abundance of extreme clusters. I am also interested in large scale data analysis in Cosmology, involving correlating large surveys such as SDSS, XCS (see links opposite) and VESPA. I also work in astrophysics with Galaxy Zoo, in particular bar length and width measurements, and correlating bar properties with host galaxy properties. Combining astrophysics, statistics and cosmology, I have used VESPA to constrain homogeneity and isotropy of the Universe using the Star Formation Rate Histories of Luminous Red Galaxies as a proxy for homogeneity.

To access the machine learning photometric redshift code follow this link

April 02, 2013, at 10:57 AM EST by 138.246.87.202 -
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My main research interests include mass measurements of galaxy clusters using optical & X-ray data or weak lensing measurements. Constraining cosmological models using the cluster mass function, and the abundance of extreme clusters. Data analysis in Cosmology, involving correlating large surveys such as SDSS, XCS (see links opposite) and VESPA. Astrophysics with Galaxy Zoo, in particular bar length and width measurements, and correlating bar properties with host galaxy properties. And using VESPA to constrain homogeneity and isotropy.

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My main research interests include mass measurements and correlation function of galaxy clusters. In particular I use optical, X-ray data & SZ selected clusters. I use clusters and correlation functions to constrain cosmological models and parameters using the cluster mass function, and the abundance of extreme clusters. I am also interested in large scale data analysis in Cosmology, involving correlating large surveys such as SDSS, XCS (see links opposite) and VESPA. I also work in astrophysics with Galaxy Zoo, in particular bar length and width measurements, and correlating bar properties with host galaxy properties. Combining astrophysics, statistics and cosmology, I have used VESPA to constrain homogeneity and isotropy of the Universe using the Star Formation Rate Histories of Luminous Red Galaxies as a proxy for homogeneity.

April 02, 2013, at 10:52 AM EST by 138.246.87.202 -
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Welcome to my home page. Here you will be able to access information about me, and the work I am doing here at the University of Barcelona.

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Welcome to my home page. Here you will be able to access information about me, and the work I am doing here at the University Sternwarte, part of the Ludwig Maximilian University in Munich.

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My main research interests include mass measurements of galaxy clusters using optical & X-ray data or weak lensing measurements. Constraining cosmological models using the cluster mass function, and the abundance of extreme clusters. Data analysis in Cosmology, involving correlating large surveys such as SDSS, XCS (see links opposite) and VESPA. Astrophysics with Galaxy Zoo, in particular bar length and width measurements, and correlating bar properties with host galaxy properties.

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My main research interests include mass measurements of galaxy clusters using optical & X-ray data or weak lensing measurements. Constraining cosmological models using the cluster mass function, and the abundance of extreme clusters. Data analysis in Cosmology, involving correlating large surveys such as SDSS, XCS (see links opposite) and VESPA. Astrophysics with Galaxy Zoo, in particular bar length and width measurements, and correlating bar properties with host galaxy properties. And using VESPA to constrain homogeneity and isotropy.

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To obtain the Galaxy Zoo2 bar length measurement data, as published in this recent paper, please follow this link

to:

To obtain the Galaxy Zoo2 bar length measurement data, as published in this recent paper,, please follow this link

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My main research interests include mass measurements of galaxy clusters using optical & X-ray data or weak lensing measurements. Constraining cosmological models using the cluster mass function, and the abundance of extreme clusters. Data analysis in Cosmology, involving correlating large surveys such as SDSS, XCS (see links opposite) and VESPA. Astrophysics with galaxy zoo

To acquire the Galaxy Zoo data, as published in follow this link

to:

My main research interests include mass measurements of galaxy clusters using optical & X-ray data or weak lensing measurements. Constraining cosmological models using the cluster mass function, and the abundance of extreme clusters. Data analysis in Cosmology, involving correlating large surveys such as SDSS, XCS (see links opposite) and VESPA. Astrophysics with Galaxy Zoo, in particular bar length and width measurements, and correlating bar properties with host galaxy properties.

To obtain the Galaxy Zoo2 bar length measurement data, as published in this recent paper, please follow this link

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Here is my old home page at the Institute of Cosmology and Gravitation, at the University of Portsmouth.

http://icg.port.ac.uk/~hoyleb/

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My main research interests include Mass measurements of galaxy clusters using optical & X-ray data or weak lensing measurements. Constraining cosmological models using the cluster mass function. Data analysis in Cosmology. Large surveys. Weak lensing. Astrophysics with galaxy zoo

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My main research interests include mass measurements of galaxy clusters using optical & X-ray data or weak lensing measurements. Constraining cosmological models using the cluster mass function, and the abundance of extreme clusters. Data analysis in Cosmology, involving correlating large surveys such as SDSS, XCS (see links opposite) and VESPA. Astrophysics with galaxy zoo

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Below are links to my old home page, and some projects I'm involved in.

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Here is my old home page at the Institute of Cosmology and Gravitation, at the University of Portsmouth.

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http://icg.port.ac.uk/~hoyleb/bars/

http://galaxyzoo.org

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http://www2.clustrmaps.com/stats/maps-no_clusters/icc.ub.edu-~hoyleb--thumb.jpg

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Locations of visitors to this page

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http://www2.clustrmaps.com/stats/maps-no_clusters/icc.ub.edu-~hoyleb--thumb.jpg

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[url=http://www2.clustrmaps.com/user/a39c83f3][img]http://www2.clustrmaps.com/stats/maps-no_clusters/icc.ub.edu-~hoyleb--thumb.jpg[/img][/url]

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[url=http://www2.clustrmaps.com/user/a39c83f3][img]http://www2.clustrmaps.com/stats/maps-no_clusters/icc.ub.edu-~hoyleb--thumb.jpg[/img][/url]

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To acquire the Galaxy Zoo data, as published in follow this link

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[]

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July 02, 2010, at 02:44 AM EST by 192.51.209.56 -
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Research Intrests

My main research interests include Mass measurements of galaxy clusters using optical & X-ray data or weak lensing measurements. Constraining cosmological models using the cluster mass function. Data analysis in Cosmology. Large surveys. Weak lensing. Astrophysics with galaxy zoo

July 01, 2010, at 04:54 AM EST by 192.51.209.56 -
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Welcome to my home page.

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Welcome to my home page. Here you will be able to access information about me, and the work I am doing here at the University of Barcelona.

July 01, 2010, at 04:46 AM EST by 192.51.209.56 -
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Welcome to PmWiki!

A local copy of PmWiki's documentation has been installed along with the software, and is available via the documentation index.

To continue setting up PmWiki, see initial setup tasks.

The basic editing page describes how to create pages in PmWiki. You can practice editing in the wiki sandbox.

More information about PmWiki is available from http://www.pmwiki.org .

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Welcome to my home page.

This site is currently under construction,

Below are links to my old home page, and some projects I'm involved in.

http://icg.port.ac.uk/~hoyleb/

http://icg.port.ac.uk/~hoyleb/bars/

http://galaxyzoo.org

Please check back soon.

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