Optical followup of galaxy clusters detected by the South Pole Telescope

S. Desai; R. Armstrong; M. L.N. Ashby; B. Bayliss; G. Bazin; B. Benson; E. Bertin; L. Bleem; M. Brodwin; A. Clochiatti; R. Foley; M. Gladders; A. H. Gonzalez; F. W. High; J. Liu; J. Mohr; A. Rest; J. Ruel; A. Saro; J. Song; B. Stalder; A. Stanford; C. Stubbs; A. Zenteno

doi:10.1088/1742-6596/375/1/032011

Optical followup of galaxy clusters detected by the South Pole Telescope

S. Desai, R. Armstrong, M. L.N. Ashby, B. Bayliss, G. Bazin, B. Benson, E. Bertin, L. Bleem, M. Brodwin, A. Clochiatti, R. Foley, M. Gladders, A. H. Gonzalez, F. W. High, J. Liu, J. Mohr, A. Rest, J. Ruel, A. Saro, J. SongB. Stalder, A. Stanford, C. Stubbs, A. Zenteno

Research output: Contribution to journal › Conference article › peer-review

Abstract

The South Pole Telescope (SPT) is a 10 meter telescope operating at mm wavelengths. It has recently completed a three-band survey covering 2500 sq. degrees. One of the survey's main goals is to detect galaxy clusters using Sunyaev-Zeldovich effect and use these clusters for a variety of cosmological and astrophysical studies such as the dark energy equation of state, the primordial non-gaussianity and the evolution of galaxy populations. Since 2005, we have been engaged in a comprehensive optical and near-infrared followup program (at wavelengths between 0.4 and 5 μm) to image high-significance SPT clusters, to measure their photometric redshifts, and to estimate the contamination rate of the candidate lists. These clusters are then used for various cosmological and astrophysical studies.

Original language	English (US)
Article number	032011
Journal	Journal of Physics: Conference Series
Volume	375
Issue number	PART 3
DOIs	https://doi.org/10.1088/1742-6596/375/1/032011
State	Published - 2012
Externally published	Yes
Event	12th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2011 - Munich, Germany Duration: Sep 5 2011 → Sep 9 2011

ASJC Scopus subject areas

General Physics and Astronomy

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10.1088/1742-6596/375/1/032011

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Desai, S., Armstrong, R., Ashby, M. L. N., Bayliss, B., Bazin, G., Benson, B., Bertin, E., Bleem, L., Brodwin, M., Clochiatti, A., Foley, R., Gladders, M., Gonzalez, A. H., High, F. W., Liu, J., Mohr, J., Rest, A., Ruel, J., Saro, A., ... Zenteno, A. (2012). Optical followup of galaxy clusters detected by the South Pole Telescope. Journal of Physics: Conference Series, 375(PART 3), Article 032011. https://doi.org/10.1088/1742-6596/375/1/032011

Desai, S, Armstrong, R, Ashby, MLN, Bayliss, B, Bazin, G, Benson, B, Bertin, E, Bleem, L, Brodwin, M, Clochiatti, A, Foley, R, Gladders, M, Gonzalez, AH, High, FW, Liu, J, Mohr, J, Rest, A, Ruel, J, Saro, A, Song, J, Stalder, B, Stanford, A, Stubbs, C & Zenteno, A 2012, 'Optical followup of galaxy clusters detected by the South Pole Telescope', Journal of Physics: Conference Series, vol. 375, no. PART 3, 032011. https://doi.org/10.1088/1742-6596/375/1/032011

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abstract = "The South Pole Telescope (SPT) is a 10 meter telescope operating at mm wavelengths. It has recently completed a three-band survey covering 2500 sq. degrees. One of the survey's main goals is to detect galaxy clusters using Sunyaev-Zeldovich effect and use these clusters for a variety of cosmological and astrophysical studies such as the dark energy equation of state, the primordial non-gaussianity and the evolution of galaxy populations. Since 2005, we have been engaged in a comprehensive optical and near-infrared followup program (at wavelengths between 0.4 and 5 μm) to image high-significance SPT clusters, to measure their photometric redshifts, and to estimate the contamination rate of the candidate lists. These clusters are then used for various cosmological and astrophysical studies.",

author = "S. Desai and R. Armstrong and Ashby, {M. L.N.} and B. Bayliss and G. Bazin and B. Benson and E. Bertin and L. Bleem and M. Brodwin and A. Clochiatti and R. Foley and M. Gladders and Gonzalez, {A. H.} and High, {F. W.} and J. Liu and J. Mohr and A. Rest and J. Ruel and A. Saro and J. Song and B. Stalder and A. Stanford and C. Stubbs and A. Zenteno",

year = "2012",

doi = "10.1088/1742-6596/375/1/032011",

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volume = "375",

journal = "Journal of Physics: Conference Series",

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T1 - Optical followup of galaxy clusters detected by the South Pole Telescope

AU - Desai, S.

AU - Armstrong, R.

AU - Ashby, M. L.N.

AU - Bayliss, B.

AU - Bazin, G.

AU - Benson, B.

AU - Bertin, E.

AU - Bleem, L.

AU - Brodwin, M.

AU - Clochiatti, A.

AU - Foley, R.

AU - Gladders, M.

AU - Gonzalez, A. H.

AU - High, F. W.

AU - Liu, J.

AU - Mohr, J.

AU - Rest, A.

AU - Ruel, J.

AU - Saro, A.

AU - Song, J.

AU - Stalder, B.

AU - Stanford, A.

AU - Stubbs, C.

AU - Zenteno, A.

PY - 2012

Y1 - 2012

N2 - The South Pole Telescope (SPT) is a 10 meter telescope operating at mm wavelengths. It has recently completed a three-band survey covering 2500 sq. degrees. One of the survey's main goals is to detect galaxy clusters using Sunyaev-Zeldovich effect and use these clusters for a variety of cosmological and astrophysical studies such as the dark energy equation of state, the primordial non-gaussianity and the evolution of galaxy populations. Since 2005, we have been engaged in a comprehensive optical and near-infrared followup program (at wavelengths between 0.4 and 5 μm) to image high-significance SPT clusters, to measure their photometric redshifts, and to estimate the contamination rate of the candidate lists. These clusters are then used for various cosmological and astrophysical studies.

AB - The South Pole Telescope (SPT) is a 10 meter telescope operating at mm wavelengths. It has recently completed a three-band survey covering 2500 sq. degrees. One of the survey's main goals is to detect galaxy clusters using Sunyaev-Zeldovich effect and use these clusters for a variety of cosmological and astrophysical studies such as the dark energy equation of state, the primordial non-gaussianity and the evolution of galaxy populations. Since 2005, we have been engaged in a comprehensive optical and near-infrared followup program (at wavelengths between 0.4 and 5 μm) to image high-significance SPT clusters, to measure their photometric redshifts, and to estimate the contamination rate of the candidate lists. These clusters are then used for various cosmological and astrophysical studies.

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JO - Journal of Physics: Conference Series

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Y2 - 5 September 2011 through 9 September 2011

ER -

Optical followup of galaxy clusters detected by the South Pole Telescope

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