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Main Authors:	Archipley, M., Hryciuk, A., Bleem, L. E., Kornoelje, K., Klein, M., Anderson, A. J., Ansarinejad, B., Aravena, M., Balkenhol, L., Barry, P. S., Benabed, K., Bender, A. N., Benson, B. A., Bianchini, F., Bocquet, S., Bouchet, F. R., Camphuis, E., Campitiello, M. G., Carlstrom, J. E., Cathey, J., Chang, C. L., Chapman, S. C., Chaubal, P., Chichura, P. M., Chokshi, A., Chou, T. -L., Coerver, A., Crawford, T. M., Daley, C., de Haan, T., Deane, R. P., Dibert, K. R., Dobbs, M. A., Doohan, M., Doussot, A., Dutcher, D., Everett, W., Feng, C., Ferguson, K. R., Fichman, K., Floyd, B., Foster, A., Galli, S., Gambrel, A. E., Gardner, R. W., Ge, F., Goeckner-Wald, N., Gonzalez, A., Grandis, S., Greve, T. R., Gualtieri, R., Guidi, F., Guns, S., Halverson, N. W., Hill, R., Hivon, E., Holder, G. P., Holzapfel, W. L., Hood, J. C., Huang, N., Kéruzoré, F., Khalife, A. R., Knox, L., Korman, M., Kuo, C. -L., Levy, K., Lowitz, A. E., Lu, C., Lynch, G. P., Maniyar, A., Martsen, E. S., Menanteau, F., Millea, M., Montgomery, J., Nakato, Y., Natoli, T., Noble, G. I., Omori, Y., Ouellette, A., Pan, Z., Phadke, K. A., Pollak, A. W., Prabhu, K., Quan, W., Raghunathan, S., Rahimi, M., Rahlin, A., Reichardt, C. L., Reuter, C., Rouble, M., Ruhl, J. E., Schiappucci, E., Simpson, A., Sobrin, J. A., Stalder, B., Stark, A. A., Sulzenauer, N., Tandoi, C., Thorne, B., Trendafilova, C., Umilta, C., Vieira, J. D., Vitrier, A., Vizgan, D., Wan, Y., Weiß, A., Whitehorn, N., Wu, W. L. K., Young, M. R., Zebrowski, J. A., Zhou, D.
Format:	Preprint
Published:	2025
Subjects:	Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
Online Access:	https://arxiv.org/abs/2506.00298
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author	Archipley, M. Hryciuk, A. Bleem, L. E. Kornoelje, K. Klein, M. Anderson, A. J. Ansarinejad, B. Aravena, M. Balkenhol, L. Barry, P. S. Benabed, K. Bender, A. N. Benson, B. A. Bianchini, F. Bocquet, S. Bouchet, F. R. Camphuis, E. Campitiello, M. G. Carlstrom, J. E. Cathey, J. Chang, C. L. Chapman, S. C. Chaubal, P. Chichura, P. M. Chokshi, A. Chou, T. -L. Coerver, A. Crawford, T. M. Daley, C. de Haan, T. Deane, R. P. Dibert, K. R. Dobbs, M. A. Doohan, M. Doussot, A. Dutcher, D. Everett, W. Feng, C. Ferguson, K. R. Fichman, K. Floyd, B. Foster, A. Galli, S. Gambrel, A. E. Gardner, R. W. Ge, F. Goeckner-Wald, N. Gonzalez, A. Grandis, S. Greve, T. R. Gualtieri, R. Guidi, F. Guns, S. Halverson, N. W. Hill, R. Hivon, E. Holder, G. P. Holzapfel, W. L. Hood, J. C. Huang, N. Kéruzoré, F. Khalife, A. R. Knox, L. Korman, M. Kuo, C. -L. Levy, K. Lowitz, A. E. Lu, C. Lynch, G. P. Maniyar, A. Martsen, E. S. Menanteau, F. Millea, M. Montgomery, J. Nakato, Y. Natoli, T. Noble, G. I. Omori, Y. Ouellette, A. Pan, Z. Phadke, K. A. Pollak, A. W. Prabhu, K. Quan, W. Raghunathan, S. Rahimi, M. Rahlin, A. Reichardt, C. L. Reuter, C. Rouble, M. Ruhl, J. E. Schiappucci, E. Simpson, A. Sobrin, J. A. Stalder, B. Stark, A. A. Sulzenauer, N. Tandoi, C. Thorne, B. Trendafilova, C. Umilta, C. Vieira, J. D. Vitrier, A. Vizgan, D. Wan, Y. Weiß, A. Whitehorn, N. Wu, W. L. K. Young, M. R. Zebrowski, J. A. Zhou, D.
author_facet	Archipley, M. Hryciuk, A. Bleem, L. E. Kornoelje, K. Klein, M. Anderson, A. J. Ansarinejad, B. Aravena, M. Balkenhol, L. Barry, P. S. Benabed, K. Bender, A. N. Benson, B. A. Bianchini, F. Bocquet, S. Bouchet, F. R. Camphuis, E. Campitiello, M. G. Carlstrom, J. E. Cathey, J. Chang, C. L. Chapman, S. C. Chaubal, P. Chichura, P. M. Chokshi, A. Chou, T. -L. Coerver, A. Crawford, T. M. Daley, C. de Haan, T. Deane, R. P. Dibert, K. R. Dobbs, M. A. Doohan, M. Doussot, A. Dutcher, D. Everett, W. Feng, C. Ferguson, K. R. Fichman, K. Floyd, B. Foster, A. Galli, S. Gambrel, A. E. Gardner, R. W. Ge, F. Goeckner-Wald, N. Gonzalez, A. Grandis, S. Greve, T. R. Gualtieri, R. Guidi, F. Guns, S. Halverson, N. W. Hill, R. Hivon, E. Holder, G. P. Holzapfel, W. L. Hood, J. C. Huang, N. Kéruzoré, F. Khalife, A. R. Knox, L. Korman, M. Kuo, C. -L. Levy, K. Lowitz, A. E. Lu, C. Lynch, G. P. Maniyar, A. Martsen, E. S. Menanteau, F. Millea, M. Montgomery, J. Nakato, Y. Natoli, T. Noble, G. I. Omori, Y. Ouellette, A. Pan, Z. Phadke, K. A. Pollak, A. W. Prabhu, K. Quan, W. Raghunathan, S. Rahimi, M. Rahlin, A. Reichardt, C. L. Reuter, C. Rouble, M. Ruhl, J. E. Schiappucci, E. Simpson, A. Sobrin, J. A. Stalder, B. Stark, A. A. Sulzenauer, N. Tandoi, C. Thorne, B. Trendafilova, C. Umilta, C. Vieira, J. D. Vitrier, A. Vizgan, D. Wan, Y. Weiß, A. Whitehorn, N. Wu, W. L. K. Young, M. R. Zebrowski, J. A. Zhou, D.
contents	Context. The South Pole Telescope third-generation camera (SPT-3G) has observed over 10,000 square degrees of sky at 95, 150, and 220 GHz (3.3, 2.0, 1.4 mm, respectively) and will significantly overlap the ongoing 14,000 square-degree Euclid Wide Survey. The Euclid collaboration recently released Euclid Deep Field South (EDF-S) observations of 23 square degrees at wide field depths in the first quick data release (Q1). Aims. With the goal of releasing complementary millimeter-wave data and encouraging legacy science, we performed dedicated observations of a 57-square-degree field overlapping the EDF-S. Methods. The observing time totaled 20 days, and we reached noise depths of 4.3, 3.8, and 13.2 $μ$K-arcmin at 95, 150, and 220 GHz, respectively. Results. In this work we present the temperature maps and two catalogs constructed from these data. The emissive source catalog contains 601 objects (334 inside EDF-S) with 54% synchrotron-dominated sources and 46% thermal dust emission-dominated sources. The 5$σ$ detection thresholds are 1.7, 2.0, and 6.5 mJy in the three bands. The cluster catalog contains 217 cluster candidates (121 inside EDF-S) with median mass $M_{500c}=2.12 \times 10^{14} M_{\odot}/h_{70}$ and median redshift $z$ = 0.70, corresponding to an order-of-magnitude improvement in cluster density over previous tSZ-selected catalogs in this region (3.81 clusters per square degree). Conclusions. The overlap between SPT and Euclid data will enable a range of multiwavelength studies of the aforementioned source populations. This work serves as the first step toward joint projects between SPT and Euclid and provides a rich dataset containing information on galaxies, clusters, and their environments.
format	Preprint
id	arxiv_https___arxiv_org_abs_2506_00298
institution	arXiv
publishDate	2025
record_format	arxiv
spellingShingle	Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs Archipley, M. Hryciuk, A. Bleem, L. E. Kornoelje, K. Klein, M. Anderson, A. J. Ansarinejad, B. Aravena, M. Balkenhol, L. Barry, P. S. Benabed, K. Bender, A. N. Benson, B. A. Bianchini, F. Bocquet, S. Bouchet, F. R. Camphuis, E. Campitiello, M. G. Carlstrom, J. E. Cathey, J. Chang, C. L. Chapman, S. C. Chaubal, P. Chichura, P. M. Chokshi, A. Chou, T. -L. Coerver, A. Crawford, T. M. Daley, C. de Haan, T. Deane, R. P. Dibert, K. R. Dobbs, M. A. Doohan, M. Doussot, A. Dutcher, D. Everett, W. Feng, C. Ferguson, K. R. Fichman, K. Floyd, B. Foster, A. Galli, S. Gambrel, A. E. Gardner, R. W. Ge, F. Goeckner-Wald, N. Gonzalez, A. Grandis, S. Greve, T. R. Gualtieri, R. Guidi, F. Guns, S. Halverson, N. W. Hill, R. Hivon, E. Holder, G. P. Holzapfel, W. L. Hood, J. C. Huang, N. Kéruzoré, F. Khalife, A. R. Knox, L. Korman, M. Kuo, C. -L. Levy, K. Lowitz, A. E. Lu, C. Lynch, G. P. Maniyar, A. Martsen, E. S. Menanteau, F. Millea, M. Montgomery, J. Nakato, Y. Natoli, T. Noble, G. I. Omori, Y. Ouellette, A. Pan, Z. Phadke, K. A. Pollak, A. W. Prabhu, K. Quan, W. Raghunathan, S. Rahimi, M. Rahlin, A. Reichardt, C. L. Reuter, C. Rouble, M. Ruhl, J. E. Schiappucci, E. Simpson, A. Sobrin, J. A. Stalder, B. Stark, A. A. Sulzenauer, N. Tandoi, C. Thorne, B. Trendafilova, C. Umilta, C. Vieira, J. D. Vitrier, A. Vizgan, D. Wan, Y. Weiß, A. Whitehorn, N. Wu, W. L. K. Young, M. R. Zebrowski, J. A. Zhou, D. Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics Context. The South Pole Telescope third-generation camera (SPT-3G) has observed over 10,000 square degrees of sky at 95, 150, and 220 GHz (3.3, 2.0, 1.4 mm, respectively) and will significantly overlap the ongoing 14,000 square-degree Euclid Wide Survey. The Euclid collaboration recently released Euclid Deep Field South (EDF-S) observations of 23 square degrees at wide field depths in the first quick data release (Q1). Aims. With the goal of releasing complementary millimeter-wave data and encouraging legacy science, we performed dedicated observations of a 57-square-degree field overlapping the EDF-S. Methods. The observing time totaled 20 days, and we reached noise depths of 4.3, 3.8, and 13.2 $μ$K-arcmin at 95, 150, and 220 GHz, respectively. Results. In this work we present the temperature maps and two catalogs constructed from these data. The emissive source catalog contains 601 objects (334 inside EDF-S) with 54% synchrotron-dominated sources and 46% thermal dust emission-dominated sources. The 5$σ$ detection thresholds are 1.7, 2.0, and 6.5 mJy in the three bands. The cluster catalog contains 217 cluster candidates (121 inside EDF-S) with median mass $M_{500c}=2.12 \times 10^{14} M_{\odot}/h_{70}$ and median redshift $z$ = 0.70, corresponding to an order-of-magnitude improvement in cluster density over previous tSZ-selected catalogs in this region (3.81 clusters per square degree). Conclusions. The overlap between SPT and Euclid data will enable a range of multiwavelength studies of the aforementioned source populations. This work serves as the first step toward joint projects between SPT and Euclid and provides a rich dataset containing information on galaxies, clusters, and their environments.
title	Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs
topic	Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
url	https://arxiv.org/abs/2506.00298

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