MUSE-ALMA Haloes VII: Survey Science Goals & Design, Data Processing and Final Catalogues
Monthly Notices of the Royal Astronomical Society, Volume 516, Issue 4, November 2022, Pages 5618-5636 November 2022 The gas cycling in the circumgalactic regions of galaxies is known to be multi-phase. The MUSE-ALMA Haloes survey gathers a large multi-wavelength observational sample of absorption a...
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| creator | Péroux, Céline Weng, Simon Karki, Arjun Augustin, Ramona Kulkarni, Varsha P Szakacs, Roland Klitsch, Anne Hamanowicz, Aleksandra Fresco, Alejandra Y Zwaan, Martin A Biggs, Andrew Fox, Andrew J Hayes, Mattjew Howk, J. Christopher Kacprzak, Glenn G Kassin, Susan Kuntschner, Harald Nelson, Dylan Pettini, Max |
| description | Monthly Notices of the Royal Astronomical Society, Volume 516,
Issue 4, November 2022, Pages 5618-5636 November 2022 The gas cycling in the circumgalactic regions of galaxies is known to be
multi-phase. The MUSE-ALMA Haloes survey gathers a large multi-wavelength
observational sample of absorption and emission data with the goal to
significantly advance our understanding of the physical properties of such CGM
gas. A key component of the MUSE-ALMA Haloes survey is the multi-facility
observational campaign conducted with VLT/MUSE, ALMA and HST. MUSE-ALMA Haloes
targets comprise 19 VLT/MUSE IFS quasar fields, including 32 $z_{\rm abs} |
| doi_str_mv | 10.48550/arxiv.2211.16517 |
| format | Article |
| fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_2211_16517</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2211_16517</sourcerecordid><originalsourceid>FETCH-arxiv_primary_2211_165173</originalsourceid><addsrcrecordid>eNpjYJA0NNAzsTA1NdBPLKrILNMzMjI01DM0MzU052SI9A0NdtV19PF1VPBIzMlPLVYI8_S0UgguLSpLrVQITs5MzUtOVXDPT8wpVlBTcEktzkzP01FwSSxJVAgoyk9OLS7OzEtXSMxLUXDLzEvMUXAGyuTkp5emFvMwsKYBdaXyQmluBnk31xBnD12wI-ILijJzE4sq40GOiQc7xpiwCgC-FT0B</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>MUSE-ALMA Haloes VII: Survey Science Goals & Design, Data Processing and Final Catalogues</title><source>arXiv.org</source><creator>Péroux, Céline ; Weng, Simon ; Karki, Arjun ; Augustin, Ramona ; Kulkarni, Varsha P ; Szakacs, Roland ; Klitsch, Anne ; Hamanowicz, Aleksandra ; Fresco, Alejandra Y ; Zwaan, Martin A ; Biggs, Andrew ; Fox, Andrew J ; Hayes, Mattjew ; Howk, J. Christopher ; Kacprzak, Glenn G ; Kassin, Susan ; Kuntschner, Harald ; Nelson, Dylan ; Pettini, Max</creator><creatorcontrib>Péroux, Céline ; Weng, Simon ; Karki, Arjun ; Augustin, Ramona ; Kulkarni, Varsha P ; Szakacs, Roland ; Klitsch, Anne ; Hamanowicz, Aleksandra ; Fresco, Alejandra Y ; Zwaan, Martin A ; Biggs, Andrew ; Fox, Andrew J ; Hayes, Mattjew ; Howk, J. Christopher ; Kacprzak, Glenn G ; Kassin, Susan ; Kuntschner, Harald ; Nelson, Dylan ; Pettini, Max</creatorcontrib><description>Monthly Notices of the Royal Astronomical Society, Volume 516,
Issue 4, November 2022, Pages 5618-5636 November 2022 The gas cycling in the circumgalactic regions of galaxies is known to be
multi-phase. The MUSE-ALMA Haloes survey gathers a large multi-wavelength
observational sample of absorption and emission data with the goal to
significantly advance our understanding of the physical properties of such CGM
gas. A key component of the MUSE-ALMA Haloes survey is the multi-facility
observational campaign conducted with VLT/MUSE, ALMA and HST. MUSE-ALMA Haloes
targets comprise 19 VLT/MUSE IFS quasar fields, including 32 $z_{\rm abs}<$0.85
strong absorbers with measured N$_{HI}$ $\geq 10^{18}$ cm$^{\rm -2}$ from
UV-spectroscopy. We additionally use a new complementary HST medium program to
characterise the stellar content of the galaxies through a 40-orbit three-band
UVIS and IR WFC3 imaging. Beyond the absorber-selected targets, we detect 3658
sources all fields combined, including 703 objects with spectroscopic
redshifts. This galaxy-selected sample constitutes the main focus of the
current paper. We have secured millimeter ALMA observations of some of the
fields to probe the molecular gas properties of these objects. Here, we present
the overall survey science goals, target selection, observational strategy,
data processing and source identification of the full sample. Furthermore, we
provide catalogues of magnitude measurements for all objects detected in
VLT/MUSE, ALMA and HST broad-band images and associated spectroscopic redshifts
derived from VLT/MUSE observations. Together, this data set provides robust
characterisation of the neutral atomic gas, molecular gas and stars in the same
objects resulting in the baryon census of condensed matter in complex galaxy
structures.</description><identifier>DOI: 10.48550/arxiv.2211.16517</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies</subject><creationdate>2022-11</creationdate><rights>http://creativecommons.org/licenses/by/4.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2211.16517$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2211.16517$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1093/mnras/stac2546$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Péroux, Céline</creatorcontrib><creatorcontrib>Weng, Simon</creatorcontrib><creatorcontrib>Karki, Arjun</creatorcontrib><creatorcontrib>Augustin, Ramona</creatorcontrib><creatorcontrib>Kulkarni, Varsha P</creatorcontrib><creatorcontrib>Szakacs, Roland</creatorcontrib><creatorcontrib>Klitsch, Anne</creatorcontrib><creatorcontrib>Hamanowicz, Aleksandra</creatorcontrib><creatorcontrib>Fresco, Alejandra Y</creatorcontrib><creatorcontrib>Zwaan, Martin A</creatorcontrib><creatorcontrib>Biggs, Andrew</creatorcontrib><creatorcontrib>Fox, Andrew J</creatorcontrib><creatorcontrib>Hayes, Mattjew</creatorcontrib><creatorcontrib>Howk, J. Christopher</creatorcontrib><creatorcontrib>Kacprzak, Glenn G</creatorcontrib><creatorcontrib>Kassin, Susan</creatorcontrib><creatorcontrib>Kuntschner, Harald</creatorcontrib><creatorcontrib>Nelson, Dylan</creatorcontrib><creatorcontrib>Pettini, Max</creatorcontrib><title>MUSE-ALMA Haloes VII: Survey Science Goals & Design, Data Processing and Final Catalogues</title><description>Monthly Notices of the Royal Astronomical Society, Volume 516,
Issue 4, November 2022, Pages 5618-5636 November 2022 The gas cycling in the circumgalactic regions of galaxies is known to be
multi-phase. The MUSE-ALMA Haloes survey gathers a large multi-wavelength
observational sample of absorption and emission data with the goal to
significantly advance our understanding of the physical properties of such CGM
gas. A key component of the MUSE-ALMA Haloes survey is the multi-facility
observational campaign conducted with VLT/MUSE, ALMA and HST. MUSE-ALMA Haloes
targets comprise 19 VLT/MUSE IFS quasar fields, including 32 $z_{\rm abs}<$0.85
strong absorbers with measured N$_{HI}$ $\geq 10^{18}$ cm$^{\rm -2}$ from
UV-spectroscopy. We additionally use a new complementary HST medium program to
characterise the stellar content of the galaxies through a 40-orbit three-band
UVIS and IR WFC3 imaging. Beyond the absorber-selected targets, we detect 3658
sources all fields combined, including 703 objects with spectroscopic
redshifts. This galaxy-selected sample constitutes the main focus of the
current paper. We have secured millimeter ALMA observations of some of the
fields to probe the molecular gas properties of these objects. Here, we present
the overall survey science goals, target selection, observational strategy,
data processing and source identification of the full sample. Furthermore, we
provide catalogues of magnitude measurements for all objects detected in
VLT/MUSE, ALMA and HST broad-band images and associated spectroscopic redshifts
derived from VLT/MUSE observations. Together, this data set provides robust
characterisation of the neutral atomic gas, molecular gas and stars in the same
objects resulting in the baryon census of condensed matter in complex galaxy
structures.</description><subject>Physics - Astrophysics of Galaxies</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNpjYJA0NNAzsTA1NdBPLKrILNMzMjI01DM0MzU052SI9A0NdtV19PF1VPBIzMlPLVYI8_S0UgguLSpLrVQITs5MzUtOVXDPT8wpVlBTcEktzkzP01FwSSxJVAgoyk9OLS7OzEtXSMxLUXDLzEvMUXAGyuTkp5emFvMwsKYBdaXyQmluBnk31xBnD12wI-ILijJzE4sq40GOiQc7xpiwCgC-FT0B</recordid><startdate>20221129</startdate><enddate>20221129</enddate><creator>Péroux, Céline</creator><creator>Weng, Simon</creator><creator>Karki, Arjun</creator><creator>Augustin, Ramona</creator><creator>Kulkarni, Varsha P</creator><creator>Szakacs, Roland</creator><creator>Klitsch, Anne</creator><creator>Hamanowicz, Aleksandra</creator><creator>Fresco, Alejandra Y</creator><creator>Zwaan, Martin A</creator><creator>Biggs, Andrew</creator><creator>Fox, Andrew J</creator><creator>Hayes, Mattjew</creator><creator>Howk, J. Christopher</creator><creator>Kacprzak, Glenn G</creator><creator>Kassin, Susan</creator><creator>Kuntschner, Harald</creator><creator>Nelson, Dylan</creator><creator>Pettini, Max</creator><scope>GOX</scope></search><sort><creationdate>20221129</creationdate><title>MUSE-ALMA Haloes VII: Survey Science Goals & Design, Data Processing and Final Catalogues</title><author>Péroux, Céline ; Weng, Simon ; Karki, Arjun ; Augustin, Ramona ; Kulkarni, Varsha P ; Szakacs, Roland ; Klitsch, Anne ; Hamanowicz, Aleksandra ; Fresco, Alejandra Y ; Zwaan, Martin A ; Biggs, Andrew ; Fox, Andrew J ; Hayes, Mattjew ; Howk, J. Christopher ; Kacprzak, Glenn G ; Kassin, Susan ; Kuntschner, Harald ; Nelson, Dylan ; Pettini, Max</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-arxiv_primary_2211_165173</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Physics - Astrophysics of Galaxies</topic><toplevel>online_resources</toplevel><creatorcontrib>Péroux, Céline</creatorcontrib><creatorcontrib>Weng, Simon</creatorcontrib><creatorcontrib>Karki, Arjun</creatorcontrib><creatorcontrib>Augustin, Ramona</creatorcontrib><creatorcontrib>Kulkarni, Varsha P</creatorcontrib><creatorcontrib>Szakacs, Roland</creatorcontrib><creatorcontrib>Klitsch, Anne</creatorcontrib><creatorcontrib>Hamanowicz, Aleksandra</creatorcontrib><creatorcontrib>Fresco, Alejandra Y</creatorcontrib><creatorcontrib>Zwaan, Martin A</creatorcontrib><creatorcontrib>Biggs, Andrew</creatorcontrib><creatorcontrib>Fox, Andrew J</creatorcontrib><creatorcontrib>Hayes, Mattjew</creatorcontrib><creatorcontrib>Howk, J. Christopher</creatorcontrib><creatorcontrib>Kacprzak, Glenn G</creatorcontrib><creatorcontrib>Kassin, Susan</creatorcontrib><creatorcontrib>Kuntschner, Harald</creatorcontrib><creatorcontrib>Nelson, Dylan</creatorcontrib><creatorcontrib>Pettini, Max</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Péroux, Céline</au><au>Weng, Simon</au><au>Karki, Arjun</au><au>Augustin, Ramona</au><au>Kulkarni, Varsha P</au><au>Szakacs, Roland</au><au>Klitsch, Anne</au><au>Hamanowicz, Aleksandra</au><au>Fresco, Alejandra Y</au><au>Zwaan, Martin A</au><au>Biggs, Andrew</au><au>Fox, Andrew J</au><au>Hayes, Mattjew</au><au>Howk, J. Christopher</au><au>Kacprzak, Glenn G</au><au>Kassin, Susan</au><au>Kuntschner, Harald</au><au>Nelson, Dylan</au><au>Pettini, Max</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>MUSE-ALMA Haloes VII: Survey Science Goals & Design, Data Processing and Final Catalogues</atitle><date>2022-11-29</date><risdate>2022</risdate><abstract>Monthly Notices of the Royal Astronomical Society, Volume 516,
Issue 4, November 2022, Pages 5618-5636 November 2022 The gas cycling in the circumgalactic regions of galaxies is known to be
multi-phase. The MUSE-ALMA Haloes survey gathers a large multi-wavelength
observational sample of absorption and emission data with the goal to
significantly advance our understanding of the physical properties of such CGM
gas. A key component of the MUSE-ALMA Haloes survey is the multi-facility
observational campaign conducted with VLT/MUSE, ALMA and HST. MUSE-ALMA Haloes
targets comprise 19 VLT/MUSE IFS quasar fields, including 32 $z_{\rm abs}<$0.85
strong absorbers with measured N$_{HI}$ $\geq 10^{18}$ cm$^{\rm -2}$ from
UV-spectroscopy. We additionally use a new complementary HST medium program to
characterise the stellar content of the galaxies through a 40-orbit three-band
UVIS and IR WFC3 imaging. Beyond the absorber-selected targets, we detect 3658
sources all fields combined, including 703 objects with spectroscopic
redshifts. This galaxy-selected sample constitutes the main focus of the
current paper. We have secured millimeter ALMA observations of some of the
fields to probe the molecular gas properties of these objects. Here, we present
the overall survey science goals, target selection, observational strategy,
data processing and source identification of the full sample. Furthermore, we
provide catalogues of magnitude measurements for all objects detected in
VLT/MUSE, ALMA and HST broad-band images and associated spectroscopic redshifts
derived from VLT/MUSE observations. Together, this data set provides robust
characterisation of the neutral atomic gas, molecular gas and stars in the same
objects resulting in the baryon census of condensed matter in complex galaxy
structures.</abstract><doi>10.48550/arxiv.2211.16517</doi><oa>free_for_read</oa></addata></record> |
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| title | MUSE-ALMA Haloes VII: Survey Science Goals & Design, Data Processing and Final Catalogues |
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