Publications
Here is a list of publications making use of the CLAUDS data
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The CFHT Large Area U-band Deep Survey (Sawicki et al. 2019) ← project overview paper (READ THIS FIRST)
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HSC-XD 52: An X-Ray Detected AGN in a Low-mass Galaxy at z~0.56 (Halevi et al. 2019)
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Orphan GRB afterglow searches with the Pan-STARRS1 COSMOS survey (Huang et al. 2020)
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Star formation in massive galaxies at redshift z~0.5 (Xu et al. 2020)
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A large massive quiescent galaxy sample at z~1.2 (Xu et al. 2020)
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Evolution of the galaxy merger fraction in the CLAUDS+HSC-SSP deep fields (Thibert et al. 2021)
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Searching for low-redshift faint galaxies with MMT/Hectospec (Cheng et al. 2021a)
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A cautionary tale of fesc estimates from high redshift galaxies (Bassett et al. 2022)
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Group and protocluster candidates in the LAUDS and HSC-SSP joint deep surveys (Li et al. 2022)
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Evaluating Lyα Emission as a Tracer of the Largest Cosmic Structure at z~2.47 (Huang et al. 2022)
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The obscured fraction of quasars at cosmic noon (Vijarnwannaluk et al. 2022)
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Combining the CLAUDS and HSC-SSP surveys. U + grizy(+YJHKs) photometry and photometric redshifts for 18M galaxies in the 20 deg2 of the HSC-SSP Deep and ultraDeep fields (Desprez et al. 2023) ←CATALOGS
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Cluster candidates with massive quiescent galaxies at z∼2 (Kiyota et al. 2024)
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Major merger fraction along the massive galaxy quenching channel at 0.2<z<0.7 (Inoue et al. 2024)
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Environments around quasars at z~3 revealed by wide-field imaging with Subaru HSC and CFHT (Suzuki et al. 2024)
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If you use CLAUDS data...
Please use the following acknowledgement text in your paper:
“These data were obtained and processed as part of the CFHT Large Area U-band Deep Survey (CLAUDS), which is a collaboration between astronomers from Canada, France, and China described in Sawicki et al. (2019, [MNRAS 489, 5202]). CLAUDS data products can be accessed from https://www.clauds.net. CLAUDS is based on observations obtained with MegaPrime/ MegaCam, a joint project of CFHT and CEA/DAPNIA, at the CFHT which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. CLAUDS uses data obtained in part through the Telescope Access Program (TAP), which has been funded by the National Astronomical Observatories, Chinese Academy of Sciences, and the Special Fund for Astronomy from the Ministry of Finance of China. CLAUDS uses data products from TERAPIX and the Canadian Astronomy Data Centre (CADC) and was carried out using resources from Compute Canada and Canadian Advanced Network For Astrophysical Research (CANFAR).”
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And please let us know once your paper is published (or on arXiv) as we love to hear about the different ways people use CLAUDS data!