{"paper":{"title":"Detection of Galactic and Extragalactic Millimeter-Wavelength Transient Sources with SPT-3G","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"A. A. Stark, A. Cukierman, A. E. Gambrel, A. E. Lowitz, A. Foster, A. H. Harke-Hosemann, A. J. Anderson, A. Jones, A. M. Kofman, A. Nadolski, A. N. Bender, A. Rahlin, A. Suzuki, A. T. Lee, B. A. Benson, B. Riedel, B. Thorne, C. Daley, C. Feng, C. L. Chang, C.-L. Kuo, C. L. Reichardt, C. Lu, C. M. Posada, C. Tucker, C. Umilta, D. Dutcher, D. Howe, D. L. Kubik, D. Michalik, D. P. Marrone, D. Riebel, E. Anderes, E. Hivon, E. M. Leitch, E. Schiappucci, E. Shirokoff, E. V. Denison, F. Bianchini, F. R. Bouchet, F. W. Carter, G. Chen, G. C. Hilton, G. I. Noble, G. P. Holder, G. Smecher, G. Wang, H.-M. Cho, H. Nguyen, J. A. Sobrin, J. C. Hood, J. Ding, J. D. Vieira, J. E. Carlstrom, J. E. Ruhl, J.-F. Cliche, J. Fu, J. Montgomery, J. Pearson, J. S. Avva, J. Stephen, J. T. Sayre, J. W. Henning, K. A. Phadke, K. Aylor, K. Benabed, K. Byrum, K. Dibert, K. D. Irwin, K. L. Thompson, K. Prabhu, K. R. Ferguson, K. T. Story, K. W. Yoon, L. Balkenhol, L. Bryant, L. E. Bleem, L. Knox, L. R. Vale, L. Zhang, M. A. Dobbs, M. Archipley, M. Jonas, M. Korman, M. Millea, M. Rouble, M. R. Young, N. Goeckner-Wald, N. Gupta, N. Huang, N. L. Harrington, N. W. Halverson, N. Whitehorn, O. B. Jeong, P. A. R. Ade, P. Chaubal, P. Paschos, P. S. Barry, R. Basu Thakur, R. Gualtieri, R. Guyser, R. W. Gardner, S. Galli, S. Guns, S. Kuhlmann, S. Padin, S. S. Meyer, T. de Haan, T.-L. Chou, T. M. Crawford, T. Natoli, T. S. Khaire, T. W. Cecil, V. Novosad, V. Yefremenko, W. Everett, W. L. Holzapfel, W. L. K. Wu, W. Quan, Y. Omori, Z. Ahmed, Z. Pan","submitted_at":"2021-03-10T16:28:33Z","abstract_excerpt":"High-angular-resolution cosmic microwave background experiments provide a unique opportunity to conduct a survey of time-variable sources at millimeter wavelengths, a population which has primarily been understood through follow-up measurements of detections in other bands. Here we report the first results of an astronomical transient survey with the South Pole Telescope (SPT) using the SPT-3G camera to observe 1500 square degrees of the southern sky. The observations took place from March to November 2020 in three bands centered at 95, 150, and 220 GHz. This survey yielded the detection of fi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2103.06166","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2103.06166/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}