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Discovering Large-scale Structure at 2 < z < 5 in the C3VO Survey
| Indexado |
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| DOI | 10.3847/1538-4357/ADA616 | ||||
| Año | 2025 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
The Charting Cluster Construction with VUDS and ORELSE (C3VO) survey is an ongoing imaging and spectroscopic campaign aiming to map out the growth of structure up to z similar to 5 and was born from the combination of the Visible Multi-Object Spectrograph Ultra Deep Survey and the Observations of Redshift Evolution in Large-Scale Environments (ORELSE) survey. As we previously accomplished with the ORELSE survey, we apply our technique known as Voronoi tessellation Monte Carlo (VMC) mapping to search for serendipitous galaxy overdensities at 2 < z < 5 in the three C3VO fields. We also apply the same technique to mock observations of simulated galaxies with properties derived from the GAlaxy Evolution and Assembly semianalytic model in order to judge the effectiveness of our search algorithm as a function of redshift, total mass, and fraction of spectroscopic redshifts. We find completeness and purity values of the order of 30%-50% for log(M-z=0/M-circle dot)>14 and 2 < z < 4, with a strong dependence on mass and redshift, with values as high as similar to 80% and similar to 70%, respectively, in the best-case scenario for log(M-z=0/M-circle dot)>14.5. In the C3VO fields, we were able to recover many of the previously known structures in the literature as well as find hundreds of new overdensity candidates, once again demonstrating the powerful capabilities of VMC mapping when applied to wide-field optical and infrared galaxy evolution surveys at ever higher redshifts.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Hung, Denise | - |
Univ Hawaii - Estados Unidos
NSF NOIRLab - Estados Unidos University Hawaii Institute for Astronomy - Estados Unidos Gemini Observatory - Estados Unidos |
| 2 | Lemaux, Brian C. | - |
NSF NOIRLab - Estados Unidos
UNIV CALIF DAVIS - Estados Unidos Gemini Observatory - Estados Unidos University of California, Davis - Estados Unidos |
| 3 | Cucciati, Olga | - |
INAF Osservatorio Astrofis & Sci Spazio Bologna - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia |
| 4 | Forrest, Ben | - |
UNIV CALIF DAVIS - Estados Unidos
University of California, Davis - Estados Unidos |
| 5 | Shah, Ekta A. | Mujer |
UNIV CALIF DAVIS - Estados Unidos
University of California, Davis - Estados Unidos |
| 6 | Gal, Roy R. | - |
Univ Hawaii - Estados Unidos
University Hawaii Institute for Astronomy - Estados Unidos |
| 7 | Giddings, Finn | - |
Univ Hawaii - Estados Unidos
University Hawaii Institute for Astronomy - Estados Unidos |
| 8 | Sikorski, Derek | - |
Univ Hawaii - Estados Unidos
University Hawaii Institute for Astronomy - Estados Unidos |
| 9 | Golden-Marx, Emmet | - |
Tsinghua Univ - China
INAF Osservatorio Astron Padova - Italia Tsinghua University - China Osservatorio Astronomico di Padova - Italia |
| 10 | Lubin, Lori M. | - |
UNIV CALIF DAVIS - Estados Unidos
University of California, Davis - Estados Unidos |
| 11 | Hathi, Nimish | - |
Space Telescope Sci Inst - Estados Unidos
Space Telescope Science Institute - Estados Unidos |
| 12 | Zamorani, Giovanni | - |
INAF Osservatorio Astrofis & Sci Spazio Bologna - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia |
| 13 | Shen, Lu | - |
Texas A&M Univ - Estados Unidos
Texas A&M University - Estados Unidos Texas A&M University - Estados Unidos |
| 14 | de la Torre, S. | Hombre |
INAF Osservatorio Astrofis & Sci Spazio Bologna - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia |
| 15 | Cassarà, Letizia P. | - |
INAF IASF Milano - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia |
| 16 | De Lucia, Gabriella | - |
INAF Astron Observ Trieste - Italia
IFPU Inst Fundamental Phys Universe - Italia Osservatorio Astronomico di Trieste - Italia Università degli Studi di Trieste - Italia |
| 17 | Fontanot, Fabio | - |
INAF Astron Observ Trieste - Italia
IFPU Inst Fundamental Phys Universe - Italia Osservatorio Astronomico di Trieste - Italia Università degli Studi di Trieste - Italia |
| 18 | Garilli, Bianca | - |
INAF IASF Milano - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia |
| 19 | Guaita, Lucia | - |
Universidad Nacional Andrés Bello - Chile
|
| 20 | Hirschmann, Michaela Monika | - |
INAF Astron Observ Trieste - Italia
EPFL - Suiza Osservatorio Astronomico di Trieste - Italia Observatoire de Sauverny - Suiza |
| 21 | Lee, Kyoung-Soo | - |
Purdue Univ - Estados Unidos
College of Science - Estados Unidos |
| 21 | Lee, Kyoung Soo | - |
College of Science - Estados Unidos
|
| 22 | Newman, Andrew B. | - |
Carnegie Sci Observ - Estados Unidos
Carnegie Observatories - Estados Unidos |
| 23 | Ramakrishnan, V. | Mujer |
Purdue Univ - Estados Unidos
College of Science - Estados Unidos |
| 24 | Vergani, Daniela | - |
INAF Osservatorio Astrofis & Sci Spazio Bologna - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia |
| 25 | Xie, Lizhi | - |
Tianjin Normal Univ - China
Tianjin Normal University - China |
| 26 | Zucca, Elena | - |
INAF Osservatorio Astrofis & Sci Spazio Bologna - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia |
| Fuente |
|---|
| National Science Foundation |
| University of California |
| U.S. National Science Foundation |
| NASA |
| National Research Council |
| Science and Technology Facilities Council |
| National Aeronautics and Space Administration |
| W. M. Keck Foundation |
| University of Arizona |
| University of California Berkeley |
| National Science Foundation (NSF) |
| Centre National de la Recherche Scientifique |
| California Institute of Technology |
| W.M. Keck Foundation |
| France-Berkeley Fund |
| University of Hawai'i |
| Lockheed Martin Advanced Technology Center |
| ESO Telescopes at the La Silla Paranal Observatory under ESO program |
| NASA's Astrophysics Data Analysis Program |
| European Southern Observatory Very Large Telescope, Paranal, Chile |
| University of California, Davis |
| Institut National des Sciences de l'Univers |
| United States of America |
| International Gemini Observatory |
| NSF NOIRLab |
| Science and Technology Facilities Council of the U.K |
| SMOKA |
| Agradecimiento |
|---|
| We thank the anonymous referee for the valuable comments in improving this work. Some of the material presented in this paper is supported by the National Science Foundation under grant Nos. 1411943 and 1908422. This work was partially supported by NASA's Astrophysics Data Analysis Program under grant No. 80NSSC21K0986. This work was additionally supported by the France-Berkeley Fund, a joint venture between UC Berkeley, UC Davis, and le Centre National de la Recherche Scientifique de France promoting lasting institutional and intellectual cooperation between France and the United States. This study is based, in part, on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under ESO program ID 179.A-2005 and on data products produced by TERAPIX and the Cambridge Astronomy Survey Unit on behalf of the UltraVISTA consortium. This study is based, in part, on data collected at the Subaru Telescope and obtained from the SMOKA, which is operated by the Astronomy Data Center, National Astronomical Observatory of Japan. This work is based, in part, on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. UKIRT is supported by NASA and operated under an agreement among the University of Hawaii, the University of Arizona, and Lockheed Martin Advanced Technology Center; operations are enabled through the cooperation of the East Asian Observatory. When the data reported here were acquired, UKIRT was operated by the Joint Astronomy Centre on behalf of the Science and Technology Facilities Council of the U.K. This study is also based, in part, on observations obtained with WIRCam, a joint project of Taiwan, Korea, Canada, France, and the Canada-France-Hawaii Telescope, which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawai'i. This paper was supported by the international Gemini Observatory, a program of NSF NOIRLab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the U.S. National Science Foundation, on behalf of the Gemini partnership of Argentina, Brazil, Canada, Chile, the Republic of Korea, and the United States of America. Some portion of the spectrographic data presented herein was based on observations obtained with the European Southern Observatory Very Large Telescope, Paranal, Chile, under Large Programs 070.A-9007 and 177.A-0837. The remainder of the spectrographic data presented herein were obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W.M. Keck Foundation. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the Native Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. |
| We thank the anonymous referee for the valuable comments in improving this work. Some of the material presented in this paper is supported by the National Science Foundation under grant Nos. 1411943 and 1908422. This work was partially supported by NASA\u2019s Astrophysics Data Analysis Program under grant No. 80NSSC21K0986. This work was additionally supported by the France-Berkeley Fund, a joint venture between UC Berkeley, UC Davis, and le Centre National de la Recherche Scientifique de France promoting lasting institutional and intellectual cooperation between France and the United States. This study is based, in part, on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under ESO program ID 179.A-2005 and on data products produced by TERAPIX and the Cambridge Astronomy Survey Unit on behalf of the UltraVISTA consortium. This study is based, in part, on data collected at the Subaru Telescope and obtained from the SMOKA, which is operated by the Astronomy Data Center, National Astronomical Observatory of Japan. This work is based, in part, on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. UKIRT is supported by NASA and operated under an agreement among the University of Hawaii, the University of Arizona, and Lockheed Martin Advanced Technology Center; operations are enabled through the cooperation of the East Asian Observatory. When the data reported here were acquired, UKIRT was operated by the Joint Astronomy Centre on behalf of the Science and Technology Facilities Council of the U.K. This study is also based, in part, on observations obtained with WIRCam, a joint project of Taiwan, Korea, Canada, France, and the Canada-France-Hawaii Telescope, which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l\u2019Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawai\u2019i. This paper was supported by the international Gemini Observatory, a program of NSF NOIRLab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the U.S. National Science Foundation, on behalf of the Gemini partnership of Argentina, Brazil, Canada, Chile, the Republic of Korea, and the United States of America. Some portion of the spectrographic data presented herein was based on observations obtained with the European Southern Observatory Very Large Telescope, Paranal, Chile, under Large Programs 070.A-9007 and 177.A-0837. The remainder of the spectrographic data presented herein were obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W.M. Keck Foundation. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the Native Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. |
| We thank the anonymous referee for the valuable comments in improving this work. Some of the material presented in this paper is supported by the National Science Foundation under grant Nos. 1411943 and 1908422. This work was partially supported by NASA\u2019s Astrophysics Data Analysis Program under grant No. 80NSSC21K0986. This work was additionally supported by the France-Berkeley Fund, a joint venture between UC Berkeley, UC Davis, and le Centre National de la Recherche Scientifique de France promoting lasting institutional and intellectual cooperation between France and the United States. This study is based, in part, on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under ESO program ID 179.A-2005 and on data products produced by TERAPIX and the Cambridge Astronomy Survey Unit on behalf of the UltraVISTA consortium. This study is based, in part, on data collected at the Subaru Telescope and obtained from the SMOKA, which is operated by the Astronomy Data Center, National Astronomical Observatory of Japan. This work is based, in part, on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. UKIRT is supported by NASA and operated under an agreement among the University of Hawaii, the University of Arizona, and Lockheed Martin Advanced Technology Center; operations are enabled through the cooperation of the East Asian Observatory. When the data reported here were acquired, UKIRT was operated by the Joint Astronomy Centre on behalf of the Science and Technology Facilities Council of the U.K. This study is also based, in part, on observations obtained with WIRCam, a joint project of Taiwan, Korea, Canada, France, and the Canada-France-Hawaii Telescope, which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l\u2019Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawai\u2019i. This paper was supported by the international Gemini Observatory, a program of NSF NOIRLab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the U.S. National Science Foundation, on behalf of the Gemini partnership of Argentina, Brazil, Canada, Chile, the Republic of Korea, and the United States of America. Some portion of the spectrographic data presented herein was based on observations obtained with the European Southern Observatory Very Large Telescope, Paranal, Chile, under Large Programs 070.A-9007 and 177.A-0837. The remainder of the spectrographic data presented herein were obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W.M. Keck Foundation. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the Native Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. |
