LoVoCCS. I. Survey Introduction, Data Processing Pipeline, and Early Science Results
We present the Local Volume Complete Cluster Survey (LoVoCCS; we pronounce it as “low-vox” or “law-vox,” with stress on the second syllable), an NSF’s National Optical-Infrared Astronomy Research Laboratory survey program that uses the Dark Energy Camera to map the dark matter distribution and galax...
Gespeichert in:
| Veröffentlicht in: | The Astrophysical journal 2022-07, Vol.933 (1), p.84 |
|---|---|
| Hauptverfasser: | , , , , , , , , , , , , , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | 1 |
| container_start_page | 84 |
| container_title | The Astrophysical journal |
| container_volume | 933 |
| creator | Fu, Shenming Dell’Antonio, Ian Chary, Ranga-Ram Clowe, Douglas Cooper, M. C. Donahue, Megan Evrard, August Lacy, Mark Lauer, Tod Liu, Binyang McCleary, Jacqueline Meneghetti, Massimo Miyatake, Hironao Montes, Mireia Natarajan, Priyamvada Ntampaka, Michelle Pierpaoli, Elena Postman, Marc Sohn, Jubee Umetsu, Keiichi Utsumi, Yousuke Wilson, Gillian |
| description | We present the Local Volume Complete Cluster Survey (LoVoCCS; we pronounce it as “low-vox” or “law-vox,” with stress on the second syllable), an NSF’s National Optical-Infrared Astronomy Research Laboratory survey program that uses the Dark Energy Camera to map the dark matter distribution and galaxy population in 107 nearby (0.03 <
z
< 0.12) X-ray luminous ([0.1–2.4 keV]
L
X500
> 10
44
erg s
−1
) galaxy clusters that are not obscured by the Milky Way. The survey will reach Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) Year 1–2 depth (for galaxies
r
= 24.5,
i
= 24.0, signal-to-noise ratio (S/N) > 20;
u
= 24.7,
g
= 25.3,
z
= 23.8, S/N > 10) and conclude in ∼2023 (coincident with the beginning of LSST science operations), and will serve as a zeroth-year template for LSST transient studies. We process the data using the LSST Science Pipelines that include state-of-the-art algorithms and analyze the results using our own pipelines, and therefore the catalogs and analysis tools will be compatible with the LSST. We demonstrate the use and performance of our pipeline using three X-ray luminous and observation-time complete LoVoCCS clusters: A3911, A3921, and A85. A3911 and A3921 have not been well studied previously by weak lensing, and we obtain similar lensing analysis results for A85 to previous studies. (We mainly use A3911 to show our pipeline and give more examples in the Appendix.) |
| doi_str_mv | 10.3847/1538-4357/ac68e8 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2685585486</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2685585486</sourcerecordid><originalsourceid>FETCH-LOGICAL-c472t-141f840c32e6d30980bf725eb7cfd1cd2bb27214c77574aaa58f702fd100491f3</originalsourceid><addsrcrecordid>eNp1kM1rGzEQxUVJoY7be48izdFr63OlPQbHSQyGmtotvQlZq21kXGkjaQv-77PLhuSSnoaZ-b3H4wHwFaM5lUwsMKeyYJSLhTaltPIDmLyeLsAEIcSKkorfn8BlSsdhJVU1AftN-BWWy90crudw18V_9gzXPsdQdya74GfwVmcNtzEYm5Lzf-DWtfbkvJ1B7Wu40vF0hjvjrDcW_rCpO-X0GXxs9CnZLy9zCn7erfbLh2Lz_X69vNkUhgmSC8xwIxkylNiypqiS6NAIwu1BmKbGpiaHAxEEMyMEF0xrzWUjEOl_ffoKN3QKrkbfkLJTybhszaMJ3luTFZaSYMF76NsItTE8dTZldQxd9H0uRUrJueRMlj2FRsrEkFK0jWqj-6vjWWGkhoLV0KYa2lRjwb3kepS40L556vaoKkoVVpKpth5Czt7B_uv6DEjShqs</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2685585486</pqid></control><display><type>article</type><title>LoVoCCS. I. Survey Introduction, Data Processing Pipeline, and Early Science Results</title><source>IOP Publishing Free Content</source><source>DOAJ Directory of Open Access Journals</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>Alma/SFX Local Collection</source><creator>Fu, Shenming ; Dell’Antonio, Ian ; Chary, Ranga-Ram ; Clowe, Douglas ; Cooper, M. C. ; Donahue, Megan ; Evrard, August ; Lacy, Mark ; Lauer, Tod ; Liu, Binyang ; McCleary, Jacqueline ; Meneghetti, Massimo ; Miyatake, Hironao ; Montes, Mireia ; Natarajan, Priyamvada ; Ntampaka, Michelle ; Pierpaoli, Elena ; Postman, Marc ; Sohn, Jubee ; Umetsu, Keiichi ; Utsumi, Yousuke ; Wilson, Gillian</creator><creatorcontrib>Fu, Shenming ; Dell’Antonio, Ian ; Chary, Ranga-Ram ; Clowe, Douglas ; Cooper, M. C. ; Donahue, Megan ; Evrard, August ; Lacy, Mark ; Lauer, Tod ; Liu, Binyang ; McCleary, Jacqueline ; Meneghetti, Massimo ; Miyatake, Hironao ; Montes, Mireia ; Natarajan, Priyamvada ; Ntampaka, Michelle ; Pierpaoli, Elena ; Postman, Marc ; Sohn, Jubee ; Umetsu, Keiichi ; Utsumi, Yousuke ; Wilson, Gillian ; SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)</creatorcontrib><description>We present the Local Volume Complete Cluster Survey (LoVoCCS; we pronounce it as “low-vox” or “law-vox,” with stress on the second syllable), an NSF’s National Optical-Infrared Astronomy Research Laboratory survey program that uses the Dark Energy Camera to map the dark matter distribution and galaxy population in 107 nearby (0.03 <
z
< 0.12) X-ray luminous ([0.1–2.4 keV]
L
X500
> 10
44
erg s
−1
) galaxy clusters that are not obscured by the Milky Way. The survey will reach Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) Year 1–2 depth (for galaxies
r
= 24.5,
i
= 24.0, signal-to-noise ratio (S/N) > 20;
u
= 24.7,
g
= 25.3,
z
= 23.8, S/N > 10) and conclude in ∼2023 (coincident with the beginning of LSST science operations), and will serve as a zeroth-year template for LSST transient studies. We process the data using the LSST Science Pipelines that include state-of-the-art algorithms and analyze the results using our own pipelines, and therefore the catalogs and analysis tools will be compatible with the LSST. We demonstrate the use and performance of our pipeline using three X-ray luminous and observation-time complete LoVoCCS clusters: A3911, A3921, and A85. A3911 and A3921 have not been well studied previously by weak lensing, and we obtain similar lensing analysis results for A85 to previous studies. (We mainly use A3911 to show our pipeline and give more examples in the Appendix.)</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.3847/1538-4357/ac68e8</identifier><language>eng</language><publisher>Philadelphia: The American Astronomical Society</publisher><subject>Algorithms ; Astronomy ; ASTRONOMY AND ASTROPHYSICS ; Astronomy data analysis ; Astrophysics ; Dark energy ; Dark matter ; Data processing ; Galactic clusters ; Galaxies ; Galaxy clusters ; Galaxy distribution ; Infrared astronomy ; Milky Way ; Observational cosmology ; Pipelines ; Polls & surveys ; Signal to noise ratio ; Surveys ; Weak gravitational lensing ; X-ray astronomy</subject><ispartof>The Astrophysical journal, 2022-07, Vol.933 (1), p.84</ispartof><rights>2022. The Author(s). Published by the American Astronomical Society.</rights><rights>2022. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c472t-141f840c32e6d30980bf725eb7cfd1cd2bb27214c77574aaa58f702fd100491f3</citedby><cites>FETCH-LOGICAL-c472t-141f840c32e6d30980bf725eb7cfd1cd2bb27214c77574aaa58f702fd100491f3</cites><orcidid>0000-0001-7847-0393 ; 0000-0001-6161-8988 ; 0000-0002-5554-8896 ; 0000-0001-5422-1958 ; 0000-0002-9883-7460 ; 0000-0002-9365-7989 ; 0000-0003-1225-7084 ; 0000-0003-1371-6019 ; 0000-0003-3234-7247 ; 0000-0002-9254-144X ; 0000-0002-7196-4822 ; 0000-0002-0144-387X ; 0000-0002-2808-0853 ; 0000-0002-3032-1783 ; 0000-0002-6572-7089 ; 0000-0002-7957-8993 ; 0000-0001-7583-0621 ; 0000-0003-0751-7312 ; 0000-0002-4876-956X ; 0000-0001-7964-9766 ; 000000029254144X ; 0000000230321783 ; 0000000255548896 ; 0000000178470393 ; 0000000271964822 ; 0000000161618988 ; 0000000175830621 ; 0000000332347247 ; 0000000312257084 ; 0000000228080853 ; 0000000307517312 ; 0000000179649766 ; 0000000298837460 ; 000000020144387X ; 000000024876956X ; 0000000279578993 ; 0000000313716019 ; 0000000293657989 ; 0000000154221958 ; 0000000265727089</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/1538-4357/ac68e8/pdf$$EPDF$$P50$$Giop$$Hfree_for_read</linktopdf><link.rule.ids>230,314,776,780,860,881,27902,27903,38868,53844</link.rule.ids><backlink>$$Uhttps://www.osti.gov/servlets/purl/1882175$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Fu, Shenming</creatorcontrib><creatorcontrib>Dell’Antonio, Ian</creatorcontrib><creatorcontrib>Chary, Ranga-Ram</creatorcontrib><creatorcontrib>Clowe, Douglas</creatorcontrib><creatorcontrib>Cooper, M. C.</creatorcontrib><creatorcontrib>Donahue, Megan</creatorcontrib><creatorcontrib>Evrard, August</creatorcontrib><creatorcontrib>Lacy, Mark</creatorcontrib><creatorcontrib>Lauer, Tod</creatorcontrib><creatorcontrib>Liu, Binyang</creatorcontrib><creatorcontrib>McCleary, Jacqueline</creatorcontrib><creatorcontrib>Meneghetti, Massimo</creatorcontrib><creatorcontrib>Miyatake, Hironao</creatorcontrib><creatorcontrib>Montes, Mireia</creatorcontrib><creatorcontrib>Natarajan, Priyamvada</creatorcontrib><creatorcontrib>Ntampaka, Michelle</creatorcontrib><creatorcontrib>Pierpaoli, Elena</creatorcontrib><creatorcontrib>Postman, Marc</creatorcontrib><creatorcontrib>Sohn, Jubee</creatorcontrib><creatorcontrib>Umetsu, Keiichi</creatorcontrib><creatorcontrib>Utsumi, Yousuke</creatorcontrib><creatorcontrib>Wilson, Gillian</creatorcontrib><creatorcontrib>SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)</creatorcontrib><title>LoVoCCS. I. Survey Introduction, Data Processing Pipeline, and Early Science Results</title><title>The Astrophysical journal</title><addtitle>APJ</addtitle><addtitle>Astrophys. J</addtitle><description>We present the Local Volume Complete Cluster Survey (LoVoCCS; we pronounce it as “low-vox” or “law-vox,” with stress on the second syllable), an NSF’s National Optical-Infrared Astronomy Research Laboratory survey program that uses the Dark Energy Camera to map the dark matter distribution and galaxy population in 107 nearby (0.03 <
z
< 0.12) X-ray luminous ([0.1–2.4 keV]
L
X500
> 10
44
erg s
−1
) galaxy clusters that are not obscured by the Milky Way. The survey will reach Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) Year 1–2 depth (for galaxies
r
= 24.5,
i
= 24.0, signal-to-noise ratio (S/N) > 20;
u
= 24.7,
g
= 25.3,
z
= 23.8, S/N > 10) and conclude in ∼2023 (coincident with the beginning of LSST science operations), and will serve as a zeroth-year template for LSST transient studies. We process the data using the LSST Science Pipelines that include state-of-the-art algorithms and analyze the results using our own pipelines, and therefore the catalogs and analysis tools will be compatible with the LSST. We demonstrate the use and performance of our pipeline using three X-ray luminous and observation-time complete LoVoCCS clusters: A3911, A3921, and A85. A3911 and A3921 have not been well studied previously by weak lensing, and we obtain similar lensing analysis results for A85 to previous studies. (We mainly use A3911 to show our pipeline and give more examples in the Appendix.)</description><subject>Algorithms</subject><subject>Astronomy</subject><subject>ASTRONOMY AND ASTROPHYSICS</subject><subject>Astronomy data analysis</subject><subject>Astrophysics</subject><subject>Dark energy</subject><subject>Dark matter</subject><subject>Data processing</subject><subject>Galactic clusters</subject><subject>Galaxies</subject><subject>Galaxy clusters</subject><subject>Galaxy distribution</subject><subject>Infrared astronomy</subject><subject>Milky Way</subject><subject>Observational cosmology</subject><subject>Pipelines</subject><subject>Polls & surveys</subject><subject>Signal to noise ratio</subject><subject>Surveys</subject><subject>Weak gravitational lensing</subject><subject>X-ray astronomy</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>O3W</sourceid><recordid>eNp1kM1rGzEQxUVJoY7be48izdFr63OlPQbHSQyGmtotvQlZq21kXGkjaQv-77PLhuSSnoaZ-b3H4wHwFaM5lUwsMKeyYJSLhTaltPIDmLyeLsAEIcSKkorfn8BlSsdhJVU1AftN-BWWy90crudw18V_9gzXPsdQdya74GfwVmcNtzEYm5Lzf-DWtfbkvJ1B7Wu40vF0hjvjrDcW_rCpO-X0GXxs9CnZLy9zCn7erfbLh2Lz_X69vNkUhgmSC8xwIxkylNiypqiS6NAIwu1BmKbGpiaHAxEEMyMEF0xrzWUjEOl_ffoKN3QKrkbfkLJTybhszaMJ3luTFZaSYMF76NsItTE8dTZldQxd9H0uRUrJueRMlj2FRsrEkFK0jWqj-6vjWWGkhoLV0KYa2lRjwb3kepS40L556vaoKkoVVpKpth5Czt7B_uv6DEjShqs</recordid><startdate>20220701</startdate><enddate>20220701</enddate><creator>Fu, Shenming</creator><creator>Dell’Antonio, Ian</creator><creator>Chary, Ranga-Ram</creator><creator>Clowe, Douglas</creator><creator>Cooper, M. C.</creator><creator>Donahue, Megan</creator><creator>Evrard, August</creator><creator>Lacy, Mark</creator><creator>Lauer, Tod</creator><creator>Liu, Binyang</creator><creator>McCleary, Jacqueline</creator><creator>Meneghetti, Massimo</creator><creator>Miyatake, Hironao</creator><creator>Montes, Mireia</creator><creator>Natarajan, Priyamvada</creator><creator>Ntampaka, Michelle</creator><creator>Pierpaoli, Elena</creator><creator>Postman, Marc</creator><creator>Sohn, Jubee</creator><creator>Umetsu, Keiichi</creator><creator>Utsumi, Yousuke</creator><creator>Wilson, Gillian</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><scope>O3W</scope><scope>TSCCA</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><scope>OIOZB</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0001-7847-0393</orcidid><orcidid>https://orcid.org/0000-0001-6161-8988</orcidid><orcidid>https://orcid.org/0000-0002-5554-8896</orcidid><orcidid>https://orcid.org/0000-0001-5422-1958</orcidid><orcidid>https://orcid.org/0000-0002-9883-7460</orcidid><orcidid>https://orcid.org/0000-0002-9365-7989</orcidid><orcidid>https://orcid.org/0000-0003-1225-7084</orcidid><orcidid>https://orcid.org/0000-0003-1371-6019</orcidid><orcidid>https://orcid.org/0000-0003-3234-7247</orcidid><orcidid>https://orcid.org/0000-0002-9254-144X</orcidid><orcidid>https://orcid.org/0000-0002-7196-4822</orcidid><orcidid>https://orcid.org/0000-0002-0144-387X</orcidid><orcidid>https://orcid.org/0000-0002-2808-0853</orcidid><orcidid>https://orcid.org/0000-0002-3032-1783</orcidid><orcidid>https://orcid.org/0000-0002-6572-7089</orcidid><orcidid>https://orcid.org/0000-0002-7957-8993</orcidid><orcidid>https://orcid.org/0000-0001-7583-0621</orcidid><orcidid>https://orcid.org/0000-0003-0751-7312</orcidid><orcidid>https://orcid.org/0000-0002-4876-956X</orcidid><orcidid>https://orcid.org/0000-0001-7964-9766</orcidid><orcidid>https://orcid.org/000000029254144X</orcidid><orcidid>https://orcid.org/0000000230321783</orcidid><orcidid>https://orcid.org/0000000255548896</orcidid><orcidid>https://orcid.org/0000000178470393</orcidid><orcidid>https://orcid.org/0000000271964822</orcidid><orcidid>https://orcid.org/0000000161618988</orcidid><orcidid>https://orcid.org/0000000175830621</orcidid><orcidid>https://orcid.org/0000000332347247</orcidid><orcidid>https://orcid.org/0000000312257084</orcidid><orcidid>https://orcid.org/0000000228080853</orcidid><orcidid>https://orcid.org/0000000307517312</orcidid><orcidid>https://orcid.org/0000000179649766</orcidid><orcidid>https://orcid.org/0000000298837460</orcidid><orcidid>https://orcid.org/000000020144387X</orcidid><orcidid>https://orcid.org/000000024876956X</orcidid><orcidid>https://orcid.org/0000000279578993</orcidid><orcidid>https://orcid.org/0000000313716019</orcidid><orcidid>https://orcid.org/0000000293657989</orcidid><orcidid>https://orcid.org/0000000154221958</orcidid><orcidid>https://orcid.org/0000000265727089</orcidid></search><sort><creationdate>20220701</creationdate><title>LoVoCCS. I. Survey Introduction, Data Processing Pipeline, and Early Science Results</title><author>Fu, Shenming ; Dell’Antonio, Ian ; Chary, Ranga-Ram ; Clowe, Douglas ; Cooper, M. C. ; Donahue, Megan ; Evrard, August ; Lacy, Mark ; Lauer, Tod ; Liu, Binyang ; McCleary, Jacqueline ; Meneghetti, Massimo ; Miyatake, Hironao ; Montes, Mireia ; Natarajan, Priyamvada ; Ntampaka, Michelle ; Pierpaoli, Elena ; Postman, Marc ; Sohn, Jubee ; Umetsu, Keiichi ; Utsumi, Yousuke ; Wilson, Gillian</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c472t-141f840c32e6d30980bf725eb7cfd1cd2bb27214c77574aaa58f702fd100491f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Algorithms</topic><topic>Astronomy</topic><topic>ASTRONOMY AND ASTROPHYSICS</topic><topic>Astronomy data analysis</topic><topic>Astrophysics</topic><topic>Dark energy</topic><topic>Dark matter</topic><topic>Data processing</topic><topic>Galactic clusters</topic><topic>Galaxies</topic><topic>Galaxy clusters</topic><topic>Galaxy distribution</topic><topic>Infrared astronomy</topic><topic>Milky Way</topic><topic>Observational cosmology</topic><topic>Pipelines</topic><topic>Polls & surveys</topic><topic>Signal to noise ratio</topic><topic>Surveys</topic><topic>Weak gravitational lensing</topic><topic>X-ray astronomy</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Fu, Shenming</creatorcontrib><creatorcontrib>Dell’Antonio, Ian</creatorcontrib><creatorcontrib>Chary, Ranga-Ram</creatorcontrib><creatorcontrib>Clowe, Douglas</creatorcontrib><creatorcontrib>Cooper, M. C.</creatorcontrib><creatorcontrib>Donahue, Megan</creatorcontrib><creatorcontrib>Evrard, August</creatorcontrib><creatorcontrib>Lacy, Mark</creatorcontrib><creatorcontrib>Lauer, Tod</creatorcontrib><creatorcontrib>Liu, Binyang</creatorcontrib><creatorcontrib>McCleary, Jacqueline</creatorcontrib><creatorcontrib>Meneghetti, Massimo</creatorcontrib><creatorcontrib>Miyatake, Hironao</creatorcontrib><creatorcontrib>Montes, Mireia</creatorcontrib><creatorcontrib>Natarajan, Priyamvada</creatorcontrib><creatorcontrib>Ntampaka, Michelle</creatorcontrib><creatorcontrib>Pierpaoli, Elena</creatorcontrib><creatorcontrib>Postman, Marc</creatorcontrib><creatorcontrib>Sohn, Jubee</creatorcontrib><creatorcontrib>Umetsu, Keiichi</creatorcontrib><creatorcontrib>Utsumi, Yousuke</creatorcontrib><creatorcontrib>Wilson, Gillian</creatorcontrib><creatorcontrib>SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)</creatorcontrib><collection>IOP Publishing Free Content</collection><collection>IOPscience (Open Access)</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Fu, Shenming</au><au>Dell’Antonio, Ian</au><au>Chary, Ranga-Ram</au><au>Clowe, Douglas</au><au>Cooper, M. C.</au><au>Donahue, Megan</au><au>Evrard, August</au><au>Lacy, Mark</au><au>Lauer, Tod</au><au>Liu, Binyang</au><au>McCleary, Jacqueline</au><au>Meneghetti, Massimo</au><au>Miyatake, Hironao</au><au>Montes, Mireia</au><au>Natarajan, Priyamvada</au><au>Ntampaka, Michelle</au><au>Pierpaoli, Elena</au><au>Postman, Marc</au><au>Sohn, Jubee</au><au>Umetsu, Keiichi</au><au>Utsumi, Yousuke</au><au>Wilson, Gillian</au><aucorp>SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>LoVoCCS. I. Survey Introduction, Data Processing Pipeline, and Early Science Results</atitle><jtitle>The Astrophysical journal</jtitle><stitle>APJ</stitle><addtitle>Astrophys. J</addtitle><date>2022-07-01</date><risdate>2022</risdate><volume>933</volume><issue>1</issue><spage>84</spage><pages>84-</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>We present the Local Volume Complete Cluster Survey (LoVoCCS; we pronounce it as “low-vox” or “law-vox,” with stress on the second syllable), an NSF’s National Optical-Infrared Astronomy Research Laboratory survey program that uses the Dark Energy Camera to map the dark matter distribution and galaxy population in 107 nearby (0.03 <
z
< 0.12) X-ray luminous ([0.1–2.4 keV]
L
X500
> 10
44
erg s
−1
) galaxy clusters that are not obscured by the Milky Way. The survey will reach Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) Year 1–2 depth (for galaxies
r
= 24.5,
i
= 24.0, signal-to-noise ratio (S/N) > 20;
u
= 24.7,
g
= 25.3,
z
= 23.8, S/N > 10) and conclude in ∼2023 (coincident with the beginning of LSST science operations), and will serve as a zeroth-year template for LSST transient studies. We process the data using the LSST Science Pipelines that include state-of-the-art algorithms and analyze the results using our own pipelines, and therefore the catalogs and analysis tools will be compatible with the LSST. We demonstrate the use and performance of our pipeline using three X-ray luminous and observation-time complete LoVoCCS clusters: A3911, A3921, and A85. A3911 and A3921 have not been well studied previously by weak lensing, and we obtain similar lensing analysis results for A85 to previous studies. (We mainly use A3911 to show our pipeline and give more examples in the Appendix.)</abstract><cop>Philadelphia</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4357/ac68e8</doi><tpages>40</tpages><orcidid>https://orcid.org/0000-0001-7847-0393</orcidid><orcidid>https://orcid.org/0000-0001-6161-8988</orcidid><orcidid>https://orcid.org/0000-0002-5554-8896</orcidid><orcidid>https://orcid.org/0000-0001-5422-1958</orcidid><orcidid>https://orcid.org/0000-0002-9883-7460</orcidid><orcidid>https://orcid.org/0000-0002-9365-7989</orcidid><orcidid>https://orcid.org/0000-0003-1225-7084</orcidid><orcidid>https://orcid.org/0000-0003-1371-6019</orcidid><orcidid>https://orcid.org/0000-0003-3234-7247</orcidid><orcidid>https://orcid.org/0000-0002-9254-144X</orcidid><orcidid>https://orcid.org/0000-0002-7196-4822</orcidid><orcidid>https://orcid.org/0000-0002-0144-387X</orcidid><orcidid>https://orcid.org/0000-0002-2808-0853</orcidid><orcidid>https://orcid.org/0000-0002-3032-1783</orcidid><orcidid>https://orcid.org/0000-0002-6572-7089</orcidid><orcidid>https://orcid.org/0000-0002-7957-8993</orcidid><orcidid>https://orcid.org/0000-0001-7583-0621</orcidid><orcidid>https://orcid.org/0000-0003-0751-7312</orcidid><orcidid>https://orcid.org/0000-0002-4876-956X</orcidid><orcidid>https://orcid.org/0000-0001-7964-9766</orcidid><orcidid>https://orcid.org/000000029254144X</orcidid><orcidid>https://orcid.org/0000000230321783</orcidid><orcidid>https://orcid.org/0000000255548896</orcidid><orcidid>https://orcid.org/0000000178470393</orcidid><orcidid>https://orcid.org/0000000271964822</orcidid><orcidid>https://orcid.org/0000000161618988</orcidid><orcidid>https://orcid.org/0000000175830621</orcidid><orcidid>https://orcid.org/0000000332347247</orcidid><orcidid>https://orcid.org/0000000312257084</orcidid><orcidid>https://orcid.org/0000000228080853</orcidid><orcidid>https://orcid.org/0000000307517312</orcidid><orcidid>https://orcid.org/0000000179649766</orcidid><orcidid>https://orcid.org/0000000298837460</orcidid><orcidid>https://orcid.org/000000020144387X</orcidid><orcidid>https://orcid.org/000000024876956X</orcidid><orcidid>https://orcid.org/0000000279578993</orcidid><orcidid>https://orcid.org/0000000313716019</orcidid><orcidid>https://orcid.org/0000000293657989</orcidid><orcidid>https://orcid.org/0000000154221958</orcidid><orcidid>https://orcid.org/0000000265727089</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0004-637X |
| ispartof | The Astrophysical journal, 2022-07, Vol.933 (1), p.84 |
| issn | 0004-637X 1538-4357 |
| language | eng |
| recordid | cdi_proquest_journals_2685585486 |
| source | IOP Publishing Free Content; DOAJ Directory of Open Access Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Alma/SFX Local Collection |
| subjects | Algorithms Astronomy ASTRONOMY AND ASTROPHYSICS Astronomy data analysis Astrophysics Dark energy Dark matter Data processing Galactic clusters Galaxies Galaxy clusters Galaxy distribution Infrared astronomy Milky Way Observational cosmology Pipelines Polls & surveys Signal to noise ratio Surveys Weak gravitational lensing X-ray astronomy |
| title | LoVoCCS. I. Survey Introduction, Data Processing Pipeline, and Early Science Results |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-27T09%3A56%3A42IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=LoVoCCS.%20I.%20Survey%20Introduction,%20Data%20Processing%20Pipeline,%20and%20Early%20Science%20Results&rft.jtitle=The%20Astrophysical%20journal&rft.au=Fu,%20Shenming&rft.aucorp=SLAC%20National%20Accelerator%20Laboratory%20(SLAC),%20Menlo%20Park,%20CA%20(United%20States)&rft.date=2022-07-01&rft.volume=933&rft.issue=1&rft.spage=84&rft.pages=84-&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.3847/1538-4357/ac68e8&rft_dat=%3Cproquest_cross%3E2685585486%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2685585486&rft_id=info:pmid/&rfr_iscdi=true |