MUSE-ALMA haloes VII: survey science goals & design, data processing and final catalogues

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MUSE-ALMA haloes VII : survey science goals & design, data processing and final catalogues. / Peroux, C.; Weng, S.; Karki, A.; Augustin, R.; Kulkarni, V. P.; Szakacs, R.; Klitsch, A.; Hamanowicz, A.; Fresco, A. Y.; Zwaan, M. A.; Biggs, A.; Fox, A. J.; Hayes, M.; Howk, J. C.; Kacprzak, G. G.; Kassin, S.; Kuntschner, H.; Nelson, D.; Pettini, M.

I: Monthly Notices of the Royal Astronomical Society, Bind 516, Nr. 4, 30.09.2022, s. 5618-5636.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Peroux, C, Weng, S, Karki, A, Augustin, R, Kulkarni, VP, Szakacs, R, Klitsch, A, Hamanowicz, A, Fresco, AY, Zwaan, MA, Biggs, A, Fox, AJ, Hayes, M, Howk, JC, Kacprzak, GG, Kassin, S, Kuntschner, H, Nelson, D & Pettini, M 2022, 'MUSE-ALMA haloes VII: survey science goals & design, data processing and final catalogues', Monthly Notices of the Royal Astronomical Society, bind 516, nr. 4, s. 5618-5636. https://doi.org/10.1093/mnras/stac2546

APA

Peroux, C., Weng, S., Karki, A., Augustin, R., Kulkarni, V. P., Szakacs, R., Klitsch, A., Hamanowicz, A., Fresco, A. Y., Zwaan, M. A., Biggs, A., Fox, A. J., Hayes, M., Howk, J. C., Kacprzak, G. G., Kassin, S., Kuntschner, H., Nelson, D., & Pettini, M. (2022). MUSE-ALMA haloes VII: survey science goals & design, data processing and final catalogues. Monthly Notices of the Royal Astronomical Society, 516(4), 5618-5636. https://doi.org/10.1093/mnras/stac2546

Vancouver

Peroux C, Weng S, Karki A, Augustin R, Kulkarni VP, Szakacs R o.a. MUSE-ALMA haloes VII: survey science goals & design, data processing and final catalogues. Monthly Notices of the Royal Astronomical Society. 2022 sep. 30;516(4):5618-5636. https://doi.org/10.1093/mnras/stac2546

Author

Peroux, C. ; Weng, S. ; Karki, A. ; Augustin, R. ; Kulkarni, V. P. ; Szakacs, R. ; Klitsch, A. ; Hamanowicz, A. ; Fresco, A. Y. ; Zwaan, M. A. ; Biggs, A. ; Fox, A. J. ; Hayes, M. ; Howk, J. C. ; Kacprzak, G. G. ; Kassin, S. ; Kuntschner, H. ; Nelson, D. ; Pettini, M. / MUSE-ALMA haloes VII : survey science goals & design, data processing and final catalogues. I: Monthly Notices of the Royal Astronomical Society. 2022 ; Bind 516, Nr. 4. s. 5618-5636.

Bibtex

@article{706617b4df8a4ea48b4507a7712b17f4,
title = "MUSE-ALMA haloes VII: survey science goals & design, data processing and final catalogues",
abstract = "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(abs) = 10(18) cm(-2) from UV-spectroscopy. We additionally use a new complementary HST medium program to characterize 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 characterization 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.",
keywords = "galaxies: evolution, galaxies: formation, galaxies: abundance, galaxies: haloes, quasars: absorption lines, FIELD SPECTROSCOPY SURVEY, LYMAN-ALPHA SYSTEMS, BARYON SURVEY CUBS, MULTIPHASE CIRCUMGALACTIC MEDIUM, STAR-FORMING GALAXIES, H I-ABSORPTION, DAMPED LYMAN, GAS-FLOW, MOLECULAR GAS, PHYSICAL-PROPERTIES",
author = "C. Peroux and S. Weng and A. Karki and R. Augustin and Kulkarni, {V. P.} and R. Szakacs and A. Klitsch and A. Hamanowicz and Fresco, {A. Y.} and Zwaan, {M. A.} and A. Biggs and Fox, {A. J.} and M. Hayes and Howk, {J. C.} and Kacprzak, {G. G.} and S. Kassin and H. Kuntschner and D. Nelson and M. Pettini",
year = "2022",
month = sep,
day = "30",
doi = "10.1093/mnras/stac2546",
language = "English",
volume = "516",
pages = "5618--5636",
journal = "Royal Astronomical Society. Monthly Notices",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "4",

}

RIS

TY - JOUR

T1 - MUSE-ALMA haloes VII

T2 - survey science goals & design, data processing and final catalogues

AU - Peroux, C.

AU - Weng, S.

AU - Karki, A.

AU - Augustin, R.

AU - Kulkarni, V. P.

AU - Szakacs, R.

AU - Klitsch, A.

AU - Hamanowicz, A.

AU - Fresco, A. Y.

AU - Zwaan, M. A.

AU - Biggs, A.

AU - Fox, A. J.

AU - Hayes, M.

AU - Howk, J. C.

AU - Kacprzak, G. G.

AU - Kassin, S.

AU - Kuntschner, H.

AU - Nelson, D.

AU - Pettini, M.

PY - 2022/9/30

Y1 - 2022/9/30

N2 - 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(abs) = 10(18) cm(-2) from UV-spectroscopy. We additionally use a new complementary HST medium program to characterize 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 characterization 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.

AB - 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(abs) = 10(18) cm(-2) from UV-spectroscopy. We additionally use a new complementary HST medium program to characterize 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 characterization 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.

KW - galaxies: evolution

KW - galaxies: formation

KW - galaxies: abundance

KW - galaxies: haloes

KW - quasars: absorption lines

KW - FIELD SPECTROSCOPY SURVEY

KW - LYMAN-ALPHA SYSTEMS

KW - BARYON SURVEY CUBS

KW - MULTIPHASE CIRCUMGALACTIC MEDIUM

KW - STAR-FORMING GALAXIES

KW - H I-ABSORPTION

KW - DAMPED LYMAN

KW - GAS-FLOW

KW - MOLECULAR GAS

KW - PHYSICAL-PROPERTIES

U2 - 10.1093/mnras/stac2546

DO - 10.1093/mnras/stac2546

M3 - Journal article

VL - 516

SP - 5618

EP - 5636

JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

SN - 0035-8711

IS - 4

ER -

ID: 322183432