VizieR Online Data Catalog: The SPTpol Extended Cluster Survey (Bleem+, 2020)

L. E. Bleem; S. Bocquet; B. Stalder; M. D. Gladders; P. A. R. Ade; S. W. Allen; A. J. Anderson; J. Annis; M. L. N. Ashby; J. E. Austermann; S. Avila; J. S. Avva; M. Bayliss; J. A. Beall; K. Bechtol; A. N. Bender; B. A. Benson; E. Bertin; F. Bianchini; C. Blake; M. Brodwin; D. Brooks; E. Buckley-Geer; D. L. Burke; J. E. Carlstrom; A. Carnero Rosell; M. Carrasco Kind; J. Carretero; C. L. Chang; H. C. Chiang; R. Citron; C. Corbett Moran; M. Costanzi; T. M. Crawford; A. T. Crites; L. N. da Costa; T. de Haan; Vicente J. de; S. Desai; H. T. Diehl; J. P. Dietrich; M. A. Dobbs; T. F. Eifler; W. Everett; B. Flaugher; B. Floyd; J. Frieman; J. Gallicchio; J. Garcia-Bellido; E. M. George; D. W. Gerdes; A. Gilbert; D. Gruen; R. A. Gruendl; J. Gschwend; N. Gupta; G. Gutierrez; N. W. Halverson; N. Harrington; J. W. Henning; C. Heymans; G. P. Holder; D. L. Hollowood; W. L. Holzapfel; K. Honscheid; J. D. Hrubes; N. Huang; J. Hubmayr; K. D. Irwin; D. J. James; T. Jeltema; S. Joudaki; G. Khullar; M. Klein; L. Knox; N. N. Kuropatki!; A. T. Lee; D. Li; C. Lidman; A. Lowitz; N. Maccrann; G. Mahler; M. A. G. Maia; J. L. Marshall; M. McDonald; J. J. McMahon; P. Melchior; F. Menanteau; S. S. Meyer; R. Miquel; L. M. Mocanu; J. J. Mohr; J. Montgomery; A. Nadolski; T. Natoli; J. P. Nibarger; G. Noble; V. Novosad; S. Padin; A. Palmese; D. Parkinson; S. Patil; F. Paz-Chinchon; A. A. Plazas; C. Pryke; N. S. Ramachandra; C. L. Reichardt; J. D. Remolina Gonzalez; A. K. Romer; A. Roodman; J. E. Ruhl; E. S. Rykoff; B. R. Saliwanchik; E. Sanchez; A. Saro; J. T. Sayre; K. K. Schaffer; T. Schrabback; S. Serrano; K. Sharon; C. Sievers; G. Smecher; M. Smith; M. Soares-Santos; A. A. Stark; K. T. Story; E. Suchyta; G. Tarle; C. Tucker; K. Vanderlinde; T. Veach; J. D. Vieira; G. Wang; J. Weller; N. Whitehorn; W. L. K. Wu; V. Yefremenko; Y. Zhang

doi:10.26093/cds/vizier.22470025

VizieR Online Data Catalog: The SPTpol Extended Cluster Survey (Bleem+, 2020)

L. E. Bleem, S. Bocquet, B. Stalder, M. D. Gladders, P. A. R. Ade, S. W. Allen, A. J. Anderson, J. Annis, M. L. N. Ashby, J. E. Austermann, S. Avila, J. S. Avva, M. Bayliss, J. A. Beall, K. Bechtol, A. N. Bender, B. A. Benson, E. Bertin, F. Bianchini, C. BlakeM. Brodwin, D. Brooks, E. Buckley-Geer, D. L. Burke, J. E. Carlstrom, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, C. L. Chang, H. C. Chiang, R. Citron, C. Corbett Moran, M. Costanzi, T. M. Crawford, A. T. Crites, L. N. da Costa, T. de Haan, Vicente J. de, S. Desai, H. T. Diehl, J. P. Dietrich, M. A. Dobbs, T. F. Eifler, W. Everett, B. Flaugher, B. Floyd, J. Frieman, J. Gallicchio, J. Garcia-Bellido, E. M. George, D. W. Gerdes, A. Gilbert, D. Gruen, R. A. Gruendl, J. Gschwend, N. Gupta, G. Gutierrez, N. W. Halverson, N. Harrington, J. W. Henning, C. Heymans, G. P. Holder, D. L. Hollowood, W. L. Holzapfel, K. Honscheid, J. D. Hrubes, N. Huang, J. Hubmayr, K. D. Irwin, D. J. James, T. Jeltema, S. Joudaki, G. Khullar, M. Klein, L. Knox, N. N. Kuropatki!, A. T. Lee, D. Li, C. Lidman, A. Lowitz, N. Maccrann, G. Mahler, M. A. G. Maia, J. L. Marshall, M. McDonald, J. J. McMahon, P. Melchior, F. Menanteau, S. S. Meyer, R. Miquel, L. M. Mocanu, J. J. Mohr, J. Montgomery, A. Nadolski, T. Natoli, J. P. Nibarger, G. Noble, V. Novosad, S. Padin, A. Palmese, D. Parkinson, S. Patil, F. Paz-Chinchon, A. A. Plazas, C. Pryke, N. S. Ramachandra, C. L. Reichardt, J. D. Remolina Gonzalez, A. K. Romer, A. Roodman, J. E. Ruhl, E. S. Rykoff, B. R. Saliwanchik, E. Sanchez, A. Saro, J. T. Sayre, K. K. Schaffer, T. Schrabback, S. Serrano, K. Sharon, C. Sievers, G. Smecher, M. Smith, M. Soares-Santos, A. A. Stark, K. T. Story, E. Suchyta, G. Tarle, C. Tucker, K. Vanderlinde, T. Veach, J. D. Vieira, G. Wang, J. Weller, N. Whitehorn, W. L. K. Wu, V. Yefremenko, Y. Zhang

Research output: Other contribution

Abstract

The SPTpol Extended Cluster Survey (SPT-ECS) is a 2770deg² that covers two separate regions of sky with low dust emission that lie north of previous areas surveyed using the South Pole Telescope (SPT): a 2200deg² region bounded in right ascension (RA) and decl. (DEC) by 22h2 region bounded by 10hThe survey was conducted using the SPTpol receiver that was installed on the 10m South Pole Telescope (SPT) from 2012 to 2016. The survey is composed of 10 separate ~250-270deg² "fields," each imaged to noise levels of ~30-40μK arcmin at 150GHz. See Section 2 for further explanations.

To confirm the SZ candidates as galaxy clusters, we make use of targeted optical and NIR follow-up observations, data drawn from the wide-area DES (see II/357), the Pan-STARRS1 survey (Chambers+ 2016, II/349), the all sky Wide-field Infrared Survey Explorer (WISE) data set (see II/328), and the literature.

We use the Parallel Imager for Southern Cosmology Observations (PISCO) --a new imager with a 9' field of view installed on the 6.5m Magellan/Clay telescope at Las Campanas Observatory in Chile-- to obtain approximately uniform depth griz' imaging data for over 500 SPT-selected clusters and cluster candidates. See Section 4.1.2.

(5 data files).

Original language	English
Publisher	American Astronomical Society
Place of Publication	Online
DOIs	https://doi.org/10.26093/cds/vizier.22470025
Publication status	Published - 1 May 2020

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10.26093/cds/vizier.22470025

https://ui.adsabs.harvard.edu/abs/2020yCat..22470025B

Cite this

Bleem, L. E., Bocquet, S., Stalder, B., Gladders, M. D., Ade, P. A. R., Allen, S. W., Anderson, A. J., Annis, J., Ashby, M. L. N., Austermann, J. E., Avila, S., Avva, J. S., Bayliss, M., Beall, J. A., Bechtol, K., Bender, A. N., Benson, B. A., Bertin, E., Bianchini, F., ... Zhang, Y. (2020, May 1). VizieR Online Data Catalog: The SPTpol Extended Cluster Survey (Bleem+, 2020). American Astronomical Society. https://doi.org/10.26093/cds/vizier.22470025

@misc{9d7bafbab8ab45148cd60e16fe83262b,

title = "VizieR Online Data Catalog: The SPTpol Extended Cluster Survey (Bleem+, 2020)",

abstract = "The SPTpol Extended Cluster Survey (SPT-ECS) is a 2770deg2 that covers two separate regions of sky with low dust emission that lie north of previous areas surveyed using the South Pole Telescope (SPT): a 2200deg2 region bounded in right ascension (RA) and decl. (DEC) by 22h2 region bounded by 10hThe survey was conducted using the SPTpol receiver that was installed on the 10m South Pole Telescope (SPT) from 2012 to 2016. The survey is composed of 10 separate ~250-270deg2 {"}fields,{"} each imaged to noise levels of ~30-40μK arcmin at 150GHz. See Section 2 for further explanations. To confirm the SZ candidates as galaxy clusters, we make use of targeted optical and NIR follow-up observations, data drawn from the wide-area DES (see II/357), the Pan-STARRS1 survey (Chambers+ 2016, II/349), the all sky Wide-field Infrared Survey Explorer (WISE) data set (see II/328), and the literature. We use the Parallel Imager for Southern Cosmology Observations (PISCO) --a new imager with a 9' field of view installed on the 6.5m Magellan/Clay telescope at Las Campanas Observatory in Chile-- to obtain approximately uniform depth griz' imaging data for over 500 SPT-selected clusters and cluster candidates. See Section 4.1.2. (5 data files).",

keywords = "Clusters: galaxy, Redshifts, Radio sources",

author = "Bleem, {L. E.} and S. Bocquet and B. Stalder and Gladders, {M. D.} and Ade, {P. A. R.} and Allen, {S. W.} and Anderson, {A. J.} and J. Annis and Ashby, {M. L. N.} and Austermann, {J. E.} and S. Avila and Avva, {J. S.} and M. Bayliss and Beall, {J. A.} and K. Bechtol and Bender, {A. N.} and Benson, {B. A.} and E. Bertin and F. Bianchini and C. Blake and M. Brodwin and D. Brooks and E. Buckley-Geer and Burke, {D. L.} and Carlstrom, {J. E.} and {Carnero Rosell}, A. and {Carrasco Kind}, M. and J. Carretero and Chang, {C. L.} and Chiang, {H. C.} and R. Citron and {Corbett Moran}, C. and M. Costanzi and Crawford, {T. M.} and Crites, {A. T.} and {da Costa}, {L. N.} and {de Haan}, T. and de, {Vicente J.} and S. Desai and Diehl, {H. T.} and Dietrich, {J. P.} and Dobbs, {M. A.} and Eifler, {T. F.} and W. Everett and B. Flaugher and B. Floyd and J. Frieman and J. Gallicchio and J. Garcia-Bellido and George, {E. M.} and Gerdes, {D. W.} and A. Gilbert and D. Gruen and Gruendl, {R. A.} and J. Gschwend and N. Gupta and G. Gutierrez and Halverson, {N. W.} and N. Harrington and Henning, {J. W.} and C. Heymans and Holder, {G. P.} and Hollowood, {D. L.} and Holzapfel, {W. L.} and K. Honscheid and Hrubes, {J. D.} and N. Huang and J. Hubmayr and Irwin, {K. D.} and James, {D. J.} and T. Jeltema and S. Joudaki and G. Khullar and M. Klein and L. Knox and Kuropatki!, {N. N.} and Lee, {A. T.} and D. Li and C. Lidman and A. Lowitz and N. Maccrann and G. Mahler and Maia, {M. A. G.} and Marshall, {J. L.} and M. McDonald and McMahon, {J. J.} and P. Melchior and F. Menanteau and Meyer, {S. S.} and R. Miquel and Mocanu, {L. M.} and Mohr, {J. J.} and J. Montgomery and A. Nadolski and T. Natoli and Nibarger, {J. P.} and G. Noble and V. Novosad and S. Padin and A. Palmese and D. Parkinson and S. Patil and F. Paz-Chinchon and Plazas, {A. A.} and C. Pryke and Ramachandra, {N. S.} and Reichardt, {C. L.} and {Remolina Gonzalez}, {J. D.} and Romer, {A. K.} and A. Roodman and Ruhl, {J. E.} and Rykoff, {E. S.} and Saliwanchik, {B. R.} and E. Sanchez and A. Saro and Sayre, {J. T.} and Schaffer, {K. K.} and T. Schrabback and S. Serrano and K. Sharon and C. Sievers and G. Smecher and M. Smith and M. Soares-Santos and Stark, {A. A.} and Story, {K. T.} and E. Suchyta and G. Tarle and C. Tucker and K. Vanderlinde and T. Veach and Vieira, {J. D.} and G. Wang and J. Weller and N. Whitehorn and Wu, {W. L. K.} and V. Yefremenko and Y. Zhang",

year = "2020",

month = may,

day = "1",

doi = "10.26093/cds/vizier.22470025",

language = "English",

publisher = "American Astronomical Society",

address = "United States",

type = "Other",

}

Bleem, LE, Bocquet, S, Stalder, B, Gladders, MD, Ade, PAR, Allen, SW, Anderson, AJ, Annis, J, Ashby, MLN, Austermann, JE, Avila, S, Avva, JS, Bayliss, M, Beall, JA, Bechtol, K, Bender, AN, Benson, BA, Bertin, E, Bianchini, F, Blake, C, Brodwin, M, Brooks, D, Buckley-Geer, E, Burke, DL, Carlstrom, JE, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Chang, CL, Chiang, HC, Citron, R, Corbett Moran, C, Costanzi, M, Crawford, TM, Crites, AT, da Costa, LN, de Haan, T, de, VJ, Desai, S, Diehl, HT, Dietrich, JP, Dobbs, MA, Eifler, TF, Everett, W, Flaugher, B, Floyd, B, Frieman, J, Gallicchio, J, Garcia-Bellido, J, George, EM, Gerdes, DW, Gilbert, A, Gruen, D, Gruendl, RA, Gschwend, J, Gupta, N, Gutierrez, G, Halverson, NW, Harrington, N, Henning, JW, Heymans, C, Holder, GP, Hollowood, DL, Holzapfel, WL, Honscheid, K, Hrubes, JD, Huang, N, Hubmayr, J, Irwin, KD, James, DJ, Jeltema, T, Joudaki, S, Khullar, G, Klein, M, Knox, L, Kuropatki!, NN, Lee, AT, Li, D, Lidman, C, Lowitz, A, Maccrann, N, Mahler, G, Maia, MAG, Marshall, JL, McDonald, M, McMahon, JJ, Melchior, P, Menanteau, F, Meyer, SS, Miquel, R, Mocanu, LM, Mohr, JJ, Montgomery, J, Nadolski, A, Natoli, T, Nibarger, JP, Noble, G, Novosad, V, Padin, S, Palmese, A, Parkinson, D, Patil, S, Paz-Chinchon, F, Plazas, AA, Pryke, C, Ramachandra, NS, Reichardt, CL, Remolina Gonzalez, JD, Romer, AK, Roodman, A, Ruhl, JE, Rykoff, ES, Saliwanchik, BR, Sanchez, E, Saro, A, Sayre, JT, Schaffer, KK, Schrabback, T, Serrano, S, Sharon, K, Sievers, C, Smecher, G, Smith, M, Soares-Santos, M, Stark, AA, Story, KT, Suchyta, E, Tarle, G, Tucker, C, Vanderlinde, K, Veach, T, Vieira, JD, Wang, G, Weller, J, Whitehorn, N, Wu, WLK, Yefremenko, V & Zhang, Y 2020, VizieR Online Data Catalog: The SPTpol Extended Cluster Survey (Bleem+, 2020). American Astronomical Society, Online. https://doi.org/10.26093/cds/vizier.22470025

TY - GEN

T1 - VizieR Online Data Catalog: The SPTpol Extended Cluster Survey (Bleem+, 2020)

AU - Bleem, L. E.

AU - Bocquet, S.

AU - Stalder, B.

AU - Gladders, M. D.

AU - Ade, P. A. R.

AU - Allen, S. W.

AU - Anderson, A. J.

AU - Annis, J.

AU - Ashby, M. L. N.

AU - Austermann, J. E.

AU - Avila, S.

AU - Avva, J. S.

AU - Bayliss, M.

AU - Beall, J. A.

AU - Bechtol, K.

AU - Bender, A. N.

AU - Benson, B. A.

AU - Bertin, E.

AU - Bianchini, F.

AU - Blake, C.

AU - Brodwin, M.

AU - Brooks, D.

AU - Buckley-Geer, E.

AU - Burke, D. L.

AU - Carlstrom, J. E.

AU - Carnero Rosell, A.

AU - Carrasco Kind, M.

AU - Carretero, J.

AU - Chang, C. L.

AU - Chiang, H. C.

AU - Citron, R.

AU - Corbett Moran, C.

AU - Costanzi, M.

AU - Crawford, T. M.

AU - Crites, A. T.

AU - da Costa, L. N.

AU - de Haan, T.

AU - de, Vicente J.

AU - Desai, S.

AU - Diehl, H. T.

AU - Dietrich, J. P.

AU - Dobbs, M. A.

AU - Eifler, T. F.

AU - Everett, W.

AU - Flaugher, B.

AU - Floyd, B.

AU - Frieman, J.

AU - Gallicchio, J.

AU - Garcia-Bellido, J.

AU - George, E. M.

AU - Gerdes, D. W.

AU - Gilbert, A.

AU - Gruen, D.

AU - Gruendl, R. A.

AU - Gschwend, J.

AU - Gupta, N.

AU - Gutierrez, G.

AU - Halverson, N. W.

AU - Harrington, N.

AU - Henning, J. W.

AU - Heymans, C.

AU - Holder, G. P.

AU - Hollowood, D. L.

AU - Holzapfel, W. L.

AU - Honscheid, K.

AU - Hrubes, J. D.

AU - Huang, N.

AU - Hubmayr, J.

AU - Irwin, K. D.

AU - James, D. J.

AU - Jeltema, T.

AU - Joudaki, S.

AU - Khullar, G.

AU - Klein, M.

AU - Knox, L.

AU - Kuropatki!, N. N.

AU - Lee, A. T.

AU - Li, D.

AU - Lidman, C.

AU - Lowitz, A.

AU - Maccrann, N.

AU - Mahler, G.

AU - Maia, M. A. G.

AU - Marshall, J. L.

AU - McDonald, M.

AU - McMahon, J. J.

AU - Melchior, P.

AU - Menanteau, F.

AU - Meyer, S. S.

AU - Miquel, R.

AU - Mocanu, L. M.

AU - Mohr, J. J.

AU - Montgomery, J.

AU - Nadolski, A.

AU - Natoli, T.

AU - Nibarger, J. P.

AU - Noble, G.

AU - Novosad, V.

AU - Padin, S.

AU - Palmese, A.

AU - Parkinson, D.

AU - Patil, S.

AU - Paz-Chinchon, F.

AU - Plazas, A. A.

AU - Pryke, C.

AU - Ramachandra, N. S.

AU - Reichardt, C. L.

AU - Remolina Gonzalez, J. D.

AU - Romer, A. K.

AU - Roodman, A.

AU - Ruhl, J. E.

AU - Rykoff, E. S.

AU - Saliwanchik, B. R.

AU - Sanchez, E.

AU - Saro, A.

AU - Sayre, J. T.

AU - Schaffer, K. K.

AU - Schrabback, T.

AU - Serrano, S.

AU - Sharon, K.

AU - Sievers, C.

AU - Smecher, G.

AU - Smith, M.

AU - Soares-Santos, M.

AU - Stark, A. A.

AU - Story, K. T.

AU - Suchyta, E.

AU - Tarle, G.

AU - Tucker, C.

AU - Vanderlinde, K.

AU - Veach, T.

AU - Vieira, J. D.

AU - Wang, G.

AU - Weller, J.

AU - Whitehorn, N.

AU - Wu, W. L. K.

AU - Yefremenko, V.

AU - Zhang, Y.

PY - 2020/5/1

Y1 - 2020/5/1

N2 - The SPTpol Extended Cluster Survey (SPT-ECS) is a 2770deg2 that covers two separate regions of sky with low dust emission that lie north of previous areas surveyed using the South Pole Telescope (SPT): a 2200deg2 region bounded in right ascension (RA) and decl. (DEC) by 22h2 region bounded by 10hThe survey was conducted using the SPTpol receiver that was installed on the 10m South Pole Telescope (SPT) from 2012 to 2016. The survey is composed of 10 separate ~250-270deg2 "fields," each imaged to noise levels of ~30-40μK arcmin at 150GHz. See Section 2 for further explanations. To confirm the SZ candidates as galaxy clusters, we make use of targeted optical and NIR follow-up observations, data drawn from the wide-area DES (see II/357), the Pan-STARRS1 survey (Chambers+ 2016, II/349), the all sky Wide-field Infrared Survey Explorer (WISE) data set (see II/328), and the literature. We use the Parallel Imager for Southern Cosmology Observations (PISCO) --a new imager with a 9' field of view installed on the 6.5m Magellan/Clay telescope at Las Campanas Observatory in Chile-- to obtain approximately uniform depth griz' imaging data for over 500 SPT-selected clusters and cluster candidates. See Section 4.1.2. (5 data files).

AB - The SPTpol Extended Cluster Survey (SPT-ECS) is a 2770deg2 that covers two separate regions of sky with low dust emission that lie north of previous areas surveyed using the South Pole Telescope (SPT): a 2200deg2 region bounded in right ascension (RA) and decl. (DEC) by 22h2 region bounded by 10hThe survey was conducted using the SPTpol receiver that was installed on the 10m South Pole Telescope (SPT) from 2012 to 2016. The survey is composed of 10 separate ~250-270deg2 "fields," each imaged to noise levels of ~30-40μK arcmin at 150GHz. See Section 2 for further explanations. To confirm the SZ candidates as galaxy clusters, we make use of targeted optical and NIR follow-up observations, data drawn from the wide-area DES (see II/357), the Pan-STARRS1 survey (Chambers+ 2016, II/349), the all sky Wide-field Infrared Survey Explorer (WISE) data set (see II/328), and the literature. We use the Parallel Imager for Southern Cosmology Observations (PISCO) --a new imager with a 9' field of view installed on the 6.5m Magellan/Clay telescope at Las Campanas Observatory in Chile-- to obtain approximately uniform depth griz' imaging data for over 500 SPT-selected clusters and cluster candidates. See Section 4.1.2. (5 data files).

KW - Clusters: galaxy

KW - Redshifts

KW - Radio sources

U2 - 10.26093/cds/vizier.22470025

DO - 10.26093/cds/vizier.22470025

M3 - Other contribution

PB - American Astronomical Society

CY - Online

ER -

VizieR Online Data Catalog: The SPTpol Extended Cluster Survey (Bleem+, 2020)

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