Alberto Conti | Space Telescope Science Institute (original) (raw)
Papers by Alberto Conti
Arxiv preprint astro-ph/9506069, Jan 1, 1995
The Astronomical …, Jan 1, 1999
Arxiv preprint astro-ph/ …, Jan 1, 2006
The Astronomical …, Jan 1, 2003
The Astrophysical …, Jan 1, 2008
Arxiv preprint arXiv: …, Jan 1, 2007
Arxiv preprint astro-ph/0111001, Jan 1, 2001
... From Correlations of Galaxy Properties to the Physics of Galaxy Formation: A Theoretical Fram... more ... From Correlations of Galaxy Properties to the Physics of Galaxy Formation: A Theoretical Framework Alberto Conti Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260 Barbara S. Ryden & David H. Weinberg ...
American Astronomical …, Jan 1, 2011
Astronomical Data …, Jan 1, 2004
Bulletin of the American …, Jan 1, 1994
NOAO Proposal ID# …, Jan 1, 1999
We propose to obtain identification spectra of high redshift quasar candidates selected from 20 d... more We propose to obtain identification spectra of high redshift quasar candidates selected from 20 deg^2 of multicolor imaging taken with the BTC at the CTIO 4m telescope in November 1997 and November 1998. The primary targets are candidates for quasars at 5 < z < 6 and I < 22 chosen from VIZ imaging data. This allows for quasar selection to M_B < -24, providing a unique data set from which to calculate reliable quasar space densities and differentiate between different proposed forms of evolution in the quasar luminosity function at early epochs.
The challenges facing the developers of user interfaces for astronomy applications has never been... more The challenges facing the developers of user interfaces for astronomy applications has never been greater. Astronomers and engineers often use well-designed commercial and web applications outside their work environment and have come to expect a similar user experience with ...
The …, Jan 1, 2007
... Printed in USA. Statistical Properties of the GALEX-SDSS Matched Source Catalogs, and Classif... more ... Printed in USA. Statistical Properties of the GALEX-SDSS Matched Source Catalogs, and Classification of the UV Sources. Luciana Bianchi,1 Lino Rodriguez-Merino,1 Maurice Viton,2 Michel Laget,2 Boryana Efremova,1 James Herald,1 Alberto Conti,3 Bernie Shiao,3 Armando ...
Galaxies exhibit a wide range of physical properties (eg, luminosities, colors, velocity widths, ... more Galaxies exhibit a wide range of physical properties (eg, luminosities, colors, velocity widths, star formation, gas and stellar content) and the evolutionary processes responsible for these properties are numerous and complex. Understanding which processes shape the ...
Bulletin of the American Astronomical …, Jan 1, 2001
With the new generation of deep, space-based imaging surveys, such as those proposed for the SNAP... more With the new generation of deep, space-based imaging surveys, such as those proposed for the SNAP satellite, we will have an unprecedented opportunity to characterize the evolution of the clustering properties of galaxies across a wide range of look-back times. We consider ...
Arxiv preprint arXiv: …, Jan 1, 2010
NOAO Proposal ID# …, Jan 1, 1999
We propose to obtain identification spectra of high redshift quasar candidates selected from 20 d... more We propose to obtain identification spectra of high redshift quasar candidates selected from 20 deg^2 of multicolor imaging taken with the BTC at the CTIO 4m telescope in November 1997 and November 1998. The primary targets are candidates for quasars at 5 < z < 6 and I < 22 chosen from VIZ imaging data. This allows for quasar selection to M_B < -24, providing a unique data set from which to calculate reliable quasar space densities and differentiate between different proposed forms of evolution in the quasar luminosity function at early epochs.
American …, Jan 1, 2011
Archival science is having a major impact on astronomy and will continue to do so for the foresee... more Archival science is having a major impact on astronomy and will continue to do so for the foreseeable future. The Multi-mission Archive at Space Telescope (MAST) is in the process of developing a new portal aimed specifically at facilitating access to high-quality, comprehensive, multi-wavelength data and related search results. Our goal is to adapt and evolve in response to community
… of SPIE, the International Society for …, Jan 1, 2010
The challenges facing the developers of user interfaces for astronomy applications has never been... more The challenges facing the developers of user interfaces for astronomy applications has never been greater. Astronomers and engineers often use well-designed commercial and web applications outside their work environment and have come to expect a similar user experience with ...
Arxiv preprint astro-ph/9506069, Jan 1, 1995
The Astronomical …, Jan 1, 1999
Arxiv preprint astro-ph/ …, Jan 1, 2006
The Astronomical …, Jan 1, 2003
The Astrophysical …, Jan 1, 2008
Arxiv preprint arXiv: …, Jan 1, 2007
Arxiv preprint astro-ph/0111001, Jan 1, 2001
... From Correlations of Galaxy Properties to the Physics of Galaxy Formation: A Theoretical Fram... more ... From Correlations of Galaxy Properties to the Physics of Galaxy Formation: A Theoretical Framework Alberto Conti Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260 Barbara S. Ryden & David H. Weinberg ...
American Astronomical …, Jan 1, 2011
Astronomical Data …, Jan 1, 2004
Bulletin of the American …, Jan 1, 1994
NOAO Proposal ID# …, Jan 1, 1999
We propose to obtain identification spectra of high redshift quasar candidates selected from 20 d... more We propose to obtain identification spectra of high redshift quasar candidates selected from 20 deg^2 of multicolor imaging taken with the BTC at the CTIO 4m telescope in November 1997 and November 1998. The primary targets are candidates for quasars at 5 < z < 6 and I < 22 chosen from VIZ imaging data. This allows for quasar selection to M_B < -24, providing a unique data set from which to calculate reliable quasar space densities and differentiate between different proposed forms of evolution in the quasar luminosity function at early epochs.
The challenges facing the developers of user interfaces for astronomy applications has never been... more The challenges facing the developers of user interfaces for astronomy applications has never been greater. Astronomers and engineers often use well-designed commercial and web applications outside their work environment and have come to expect a similar user experience with ...
The …, Jan 1, 2007
... Printed in USA. Statistical Properties of the GALEX-SDSS Matched Source Catalogs, and Classif... more ... Printed in USA. Statistical Properties of the GALEX-SDSS Matched Source Catalogs, and Classification of the UV Sources. Luciana Bianchi,1 Lino Rodriguez-Merino,1 Maurice Viton,2 Michel Laget,2 Boryana Efremova,1 James Herald,1 Alberto Conti,3 Bernie Shiao,3 Armando ...
Galaxies exhibit a wide range of physical properties (eg, luminosities, colors, velocity widths, ... more Galaxies exhibit a wide range of physical properties (eg, luminosities, colors, velocity widths, star formation, gas and stellar content) and the evolutionary processes responsible for these properties are numerous and complex. Understanding which processes shape the ...
Bulletin of the American Astronomical …, Jan 1, 2001
With the new generation of deep, space-based imaging surveys, such as those proposed for the SNAP... more With the new generation of deep, space-based imaging surveys, such as those proposed for the SNAP satellite, we will have an unprecedented opportunity to characterize the evolution of the clustering properties of galaxies across a wide range of look-back times. We consider ...
Arxiv preprint arXiv: …, Jan 1, 2010
NOAO Proposal ID# …, Jan 1, 1999
We propose to obtain identification spectra of high redshift quasar candidates selected from 20 d... more We propose to obtain identification spectra of high redshift quasar candidates selected from 20 deg^2 of multicolor imaging taken with the BTC at the CTIO 4m telescope in November 1997 and November 1998. The primary targets are candidates for quasars at 5 < z < 6 and I < 22 chosen from VIZ imaging data. This allows for quasar selection to M_B < -24, providing a unique data set from which to calculate reliable quasar space densities and differentiate between different proposed forms of evolution in the quasar luminosity function at early epochs.
American …, Jan 1, 2011
Archival science is having a major impact on astronomy and will continue to do so for the foresee... more Archival science is having a major impact on astronomy and will continue to do so for the foreseeable future. The Multi-mission Archive at Space Telescope (MAST) is in the process of developing a new portal aimed specifically at facilitating access to high-quality, comprehensive, multi-wavelength data and related search results. Our goal is to adapt and evolve in response to community
… of SPIE, the International Society for …, Jan 1, 2010
The challenges facing the developers of user interfaces for astronomy applications has never been... more The challenges facing the developers of user interfaces for astronomy applications has never been greater. Astronomers and engineers often use well-designed commercial and web applications outside their work environment and have come to expect a similar user experience with ...