{"paper":{"title":"Faint millimeter NIKA2 dusty star-forming galaxies: finding the high-redshift population","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Beelen, A. Beno\\^it, A. Catalano, A. Gomez, A. J. Rigby, A. Maury, A. Monfardini, A. Ritacco, A. Sievers, B. Ladjelate, C. Kramer, C. Romero, C. Tucker, D.-Z. Liu, E. Artis, E. F. C. Driessen, F. K\\'eruzor\\'e, F. Mayet, F. Ruppin, F.-X. D\\'esert, G. Lagache, G. Pisano, H. Ajeddig, H. Aussel, H. Roussel, J.-F. Lestrade, J. F. Mac\\'ias-P\\'erez, J. Goupy, K. Schuster, L.-J. Bing, L. Perotto, M. B\\'ethermin, M. Calvo, M. De Petris, M. Mu\\~noz-Echeverr\\'ia, M.-Y. Xiao, N. Ponthieu, O. Bourrion, P. Ade, P. Andr\\'e, P. Mauskopf, R. Adam, R. Neri, R. Zylka, S. Berta, S. Doyle, S. Leclercq, S. Shu, V. Rev\\'eret","submitted_at":"2024-03-01T19:00:06Z","abstract_excerpt":"We develop a new framework to constrain the source redshift. The method jointly accounts for the detection/non-detection of spectral lines and the prior information from the photometric redshift and total infrared luminosity from spectral energy distribution analysis. The method uses the estimated total infrared luminosity to predict the line fluxes at given redshifts and generates model spectra. The redshift-dependent spectral models are then compared with the observed spectra to find the redshift. Results. We apply the aforementioned joint redshift analysis method to four high-z dusty star-f"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.00911","kind":"arxiv","version":1},"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/2403.00911/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"}