@article{munoz-elgueta_apex_2022,
	title = {{APEX} at the {QSO} {MUSEUM}: molecular gas reservoirs associated with \$z{\textbackslash}sim\$3 quasars and their link to the extended {Ly}\${\textbackslash}alpha\$ emission},
	shorttitle = {{APEX} at the {QSO} {MUSEUM}},
	url = {https://arxiv.org/abs/2201.11660v1},
	doi = {10.1093/mnras/stac041},
	abstract = {Cool gas (T\${\textbackslash}sim\$10\${\textasciicircum}\{4\}\${\textasciitilde}K) traced by hydrogen Ly\${\textbackslash}alpha\$ emission is now routinely detected around \$z{\textbackslash}sim3\$ quasars, but little is known about their molecular gas reservoirs. Here, we present an APEX spectroscopic survey of the CO(6-5), CO(7-6) and [CI](2-1) emission lines for 9 quasars from the QSO MUSEUM survey which have similar UV luminosities, but very diverse Ly\${\textbackslash}alpha\$ nebulae. These observations (\${\textbackslash}langle{\textasciitilde}{\textbackslash}rm rms{\textasciitilde}{\textbackslash}rangle=2.6\${\textasciitilde}mJy in 300{\textasciitilde}km{\textasciitilde}s\${\textasciicircum}\{-1\}\$) detected three CO(6-5) lines with 3.4\${\textbackslash}leq I\_\{{\textbackslash}rm CO(6-5)\} {\textbackslash}leq\$5.1{\textasciitilde}Jy{\textasciitilde}km{\textasciitilde}s\${\textasciicircum}\{-1\}\$, 620\${\textbackslash}leq\$FWHM\${\textbackslash}leq\$707{\textasciitilde}km{\textasciitilde}s\${\textasciicircum}\{-1\}\$, and three [CI](2-1) lines with 2.3\${\textbackslash}leq I\_\{{\textbackslash}rm [CI](2-1)\} {\textbackslash}leq\$15.7{\textasciitilde}Jy{\textasciitilde}km{\textasciitilde}s\${\textasciicircum}\{-1\}\$, 329\${\textbackslash}leq\$FWHM\${\textbackslash}leq\$943{\textasciitilde}km{\textasciitilde}s\${\textasciicircum}\{-1\}\$. For the CO and [CI] detected sources, we constrain the molecular gas reservoirs to be \${\textbackslash}rm M\_\{H\_\{2\}\} = (0.4-6.9) {\textbackslash}times 10{\textasciicircum}\{11\} M\_\{{\textbackslash}odot\}\$, while the non-detections imply \${\textbackslash}rm M\_\{H\_\{2\}\} {\textless} 1.1{\textbackslash}times 10{\textasciicircum}\{11\} M\_\{{\textbackslash}odot\}\$. We compare our observations with the extended Ly\${\textbackslash}alpha\$ properties to understand the link between the cool and the molecular gas phases. We find large velocity shifts between the bulk of Ly\${\textbackslash}alpha\$ and the molecular gas systemic redshift in five sources (from \${\textbackslash}sim\$-400 to \${\textbackslash}sim+\$1200{\textasciitilde}km{\textasciitilde}s\${\textasciicircum}\{-1\}\$). The sources with the largest shifts have the largest Ly\${\textbackslash}alpha\$ line widths in the sample, suggesting more turbulent gas conditions and/or large-scale inflows/outflows around these quasars. We also find that the brightest (\$I\_\{{\textbackslash}rm[CI](2-1)\}=15.7{\textbackslash}pm3.7{\textasciitilde}{\textbackslash}rm Jy{\textasciitilde}km{\textasciitilde}s{\textasciicircum}\{-1\}\$) and the widest (FWHM\${\textbackslash}sim\$900{\textasciitilde}km{\textasciitilde}s\${\textasciicircum}\{-1\}\$) lines are detected for the smallest and dimmest Ly\${\textbackslash}alpha\$ nebulae. From this, we speculate that host galaxy obscuration can play an important role in reducing the ionizing and Ly\${\textbackslash}alpha\$ photons able to escape to halo scales, and/or that these systems are hosted by more massive halos.},
	language = {en},
	urldate = {2022-02-22},
	author = {Muñoz-Elgueta, N. and Battaia, F. Arrigoni and Kauffmann, G. and De Breuck, C. and García-Vergara, C. and Zanella, A. and Farina, E. P. and Decarli, R.},
	month = jan,
	year = {2022},
}

{"_id":"D8v7YbfRrZBL7SPsa","bibbaseid":"muozelgueta-battaia-kauffmann-debreuck-garcavergara-zanella-farina-decarli-apexattheqsomuseummoleculargasreservoirsassociatedwithztextbackslashsim3quasarsandtheirlinktotheextendedlytextbackslashalphaemission-2022","author_short":["Muñoz-Elgueta, N.","Battaia, F. A.","Kauffmann, G.","De Breuck, C.","García-Vergara, C.","Zanella, A.","Farina, E. P.","Decarli, R."],"bibdata":{"bibtype":"article","type":"article","title":"APEX at the QSO MUSEUM: molecular gas reservoirs associated with \\$z{\\textbackslash}sim\\$3 quasars and their link to the extended Ly\\${\\textbackslash}alpha\\$ emission","shorttitle":"APEX at the QSO MUSEUM","url":"https://arxiv.org/abs/2201.11660v1","doi":"10.1093/mnras/stac041","abstract":"Cool gas (T\\${\\textbackslash}sim\\$10\\${\\textasciicircum}\\{4\\}\\$\\textasciitildeK) traced by hydrogen Ly\\${\\textbackslash}alpha\\$ emission is now routinely detected around \\$z{\\textbackslash}sim3\\$ quasars, but little is known about their molecular gas reservoirs. Here, we present an APEX spectroscopic survey of the CO(6-5), CO(7-6) and [CI](2-1) emission lines for 9 quasars from the QSO MUSEUM survey which have similar UV luminosities, but very diverse Ly\\${\\textbackslash}alpha\\$ nebulae. These observations (\\${\\textbackslash}langle{\\textasciitilde}{\\textbackslash}rm rms{\\textasciitilde}{\\textbackslash}rangle=2.6\\$\\textasciitildemJy in 300\\textasciitildekm\\textasciitildes\\${\\textasciicircum}\\{-1\\}\\$) detected three CO(6-5) lines with 3.4\\${\\textbackslash}leq I_\\{{\\textbackslash}rm CO(6-5)\\} {\\textbackslash}leq\\$5.1\\textasciitildeJy\\textasciitildekm\\textasciitildes\\${\\textasciicircum}\\{-1\\}\\$, 620\\${\\textbackslash}leq\\$FWHM\\${\\textbackslash}leq\\$707\\textasciitildekm\\textasciitildes\\${\\textasciicircum}\\{-1\\}\\$, and three [CI](2-1) lines with 2.3\\${\\textbackslash}leq I_\\{{\\textbackslash}rm [CI](2-1)\\} {\\textbackslash}leq\\$15.7\\textasciitildeJy\\textasciitildekm\\textasciitildes\\${\\textasciicircum}\\{-1\\}\\$, 329\\${\\textbackslash}leq\\$FWHM\\${\\textbackslash}leq\\$943\\textasciitildekm\\textasciitildes\\${\\textasciicircum}\\{-1\\}\\$. For the CO and [CI] detected sources, we constrain the molecular gas reservoirs to be \\${\\textbackslash}rm M_\\{H_\\{2\\}\\} = (0.4-6.9) {\\textbackslash}times 10{\\textasciicircum}\\{11\\} M_\\{{\\textbackslash}odot\\}\\$, while the non-detections imply \\${\\textbackslash}rm M_\\{H_\\{2\\}\\} {\\textless} 1.1{\\textbackslash}times 10{\\textasciicircum}\\{11\\} M_\\{{\\textbackslash}odot\\}\\$. We compare our observations with the extended Ly\\${\\textbackslash}alpha\\$ properties to understand the link between the cool and the molecular gas phases. We find large velocity shifts between the bulk of Ly\\${\\textbackslash}alpha\\$ and the molecular gas systemic redshift in five sources (from \\${\\textbackslash}sim\\$-400 to \\${\\textbackslash}sim+\\$1200\\textasciitildekm\\textasciitildes\\${\\textasciicircum}\\{-1\\}\\$). The sources with the largest shifts have the largest Ly\\${\\textbackslash}alpha\\$ line widths in the sample, suggesting more turbulent gas conditions and/or large-scale inflows/outflows around these quasars. We also find that the brightest (\\$I_\\{{\\textbackslash}rm[CI](2-1)\\}=15.7{\\textbackslash}pm3.7{\\textasciitilde}{\\textbackslash}rm Jy{\\textasciitilde}km{\\textasciitilde}s{\\textasciicircum}\\{-1\\}\\$) and the widest (FWHM\\${\\textbackslash}sim\\$900\\textasciitildekm\\textasciitildes\\${\\textasciicircum}\\{-1\\}\\$) lines are detected for the smallest and dimmest Ly\\${\\textbackslash}alpha\\$ nebulae. From this, we speculate that host galaxy obscuration can play an important role in reducing the ionizing and Ly\\${\\textbackslash}alpha\\$ photons able to escape to halo scales, and/or that these systems are hosted by more massive halos.","language":"en","urldate":"2022-02-22","author":[{"propositions":[],"lastnames":["Muñoz-Elgueta"],"firstnames":["N."],"suffixes":[]},{"propositions":[],"lastnames":["Battaia"],"firstnames":["F.","Arrigoni"],"suffixes":[]},{"propositions":[],"lastnames":["Kauffmann"],"firstnames":["G."],"suffixes":[]},{"propositions":[],"lastnames":["De","Breuck"],"firstnames":["C."],"suffixes":[]},{"propositions":[],"lastnames":["García-Vergara"],"firstnames":["C."],"suffixes":[]},{"propositions":[],"lastnames":["Zanella"],"firstnames":["A."],"suffixes":[]},{"propositions":[],"lastnames":["Farina"],"firstnames":["E.","P."],"suffixes":[]},{"propositions":[],"lastnames":["Decarli"],"firstnames":["R."],"suffixes":[]}],"month":"January","year":"2022","bibtex":"@article{munoz-elgueta_apex_2022,\n\ttitle = {{APEX} at the {QSO} {MUSEUM}: molecular gas reservoirs associated with \\$z{\\textbackslash}sim\\$3 quasars and their link to the extended {Ly}\\${\\textbackslash}alpha\\$ emission},\n\tshorttitle = {{APEX} at the {QSO} {MUSEUM}},\n\turl = {https://arxiv.org/abs/2201.11660v1},\n\tdoi = {10.1093/mnras/stac041},\n\tabstract = {Cool gas (T\\${\\textbackslash}sim\\$10\\${\\textasciicircum}\\{4\\}\\${\\textasciitilde}K) traced by hydrogen Ly\\${\\textbackslash}alpha\\$ emission is now routinely detected around \\$z{\\textbackslash}sim3\\$ quasars, but little is known about their molecular gas reservoirs. Here, we present an APEX spectroscopic survey of the CO(6-5), CO(7-6) and [CI](2-1) emission lines for 9 quasars from the QSO MUSEUM survey which have similar UV luminosities, but very diverse Ly\\${\\textbackslash}alpha\\$ nebulae. These observations (\\${\\textbackslash}langle{\\textasciitilde}{\\textbackslash}rm rms{\\textasciitilde}{\\textbackslash}rangle=2.6\\${\\textasciitilde}mJy in 300{\\textasciitilde}km{\\textasciitilde}s\\${\\textasciicircum}\\{-1\\}\\$) detected three CO(6-5) lines with 3.4\\${\\textbackslash}leq I\\_\\{{\\textbackslash}rm CO(6-5)\\} {\\textbackslash}leq\\$5.1{\\textasciitilde}Jy{\\textasciitilde}km{\\textasciitilde}s\\${\\textasciicircum}\\{-1\\}\\$, 620\\${\\textbackslash}leq\\$FWHM\\${\\textbackslash}leq\\$707{\\textasciitilde}km{\\textasciitilde}s\\${\\textasciicircum}\\{-1\\}\\$, and three [CI](2-1) lines with 2.3\\${\\textbackslash}leq I\\_\\{{\\textbackslash}rm [CI](2-1)\\} {\\textbackslash}leq\\$15.7{\\textasciitilde}Jy{\\textasciitilde}km{\\textasciitilde}s\\${\\textasciicircum}\\{-1\\}\\$, 329\\${\\textbackslash}leq\\$FWHM\\${\\textbackslash}leq\\$943{\\textasciitilde}km{\\textasciitilde}s\\${\\textasciicircum}\\{-1\\}\\$. For the CO and [CI] detected sources, we constrain the molecular gas reservoirs to be \\${\\textbackslash}rm M\\_\\{H\\_\\{2\\}\\} = (0.4-6.9) {\\textbackslash}times 10{\\textasciicircum}\\{11\\} M\\_\\{{\\textbackslash}odot\\}\\$, while the non-detections imply \\${\\textbackslash}rm M\\_\\{H\\_\\{2\\}\\} {\\textless} 1.1{\\textbackslash}times 10{\\textasciicircum}\\{11\\} M\\_\\{{\\textbackslash}odot\\}\\$. We compare our observations with the extended Ly\\${\\textbackslash}alpha\\$ properties to understand the link between the cool and the molecular gas phases. We find large velocity shifts between the bulk of Ly\\${\\textbackslash}alpha\\$ and the molecular gas systemic redshift in five sources (from \\${\\textbackslash}sim\\$-400 to \\${\\textbackslash}sim+\\$1200{\\textasciitilde}km{\\textasciitilde}s\\${\\textasciicircum}\\{-1\\}\\$). The sources with the largest shifts have the largest Ly\\${\\textbackslash}alpha\\$ line widths in the sample, suggesting more turbulent gas conditions and/or large-scale inflows/outflows around these quasars. We also find that the brightest (\\$I\\_\\{{\\textbackslash}rm[CI](2-1)\\}=15.7{\\textbackslash}pm3.7{\\textasciitilde}{\\textbackslash}rm Jy{\\textasciitilde}km{\\textasciitilde}s{\\textasciicircum}\\{-1\\}\\$) and the widest (FWHM\\${\\textbackslash}sim\\$900{\\textasciitilde}km{\\textasciitilde}s\\${\\textasciicircum}\\{-1\\}\\$) lines are detected for the smallest and dimmest Ly\\${\\textbackslash}alpha\\$ nebulae. From this, we speculate that host galaxy obscuration can play an important role in reducing the ionizing and Ly\\${\\textbackslash}alpha\\$ photons able to escape to halo scales, and/or that these systems are hosted by more massive halos.},\n\tlanguage = {en},\n\turldate = {2022-02-22},\n\tauthor = {Muñoz-Elgueta, N. and Battaia, F. Arrigoni and Kauffmann, G. and De Breuck, C. and García-Vergara, C. and Zanella, A. and Farina, E. P. and Decarli, R.},\n\tmonth = jan,\n\tyear = {2022},\n}\n\n","author_short":["Muñoz-Elgueta, N.","Battaia, F. A.","Kauffmann, G.","De Breuck, C.","García-Vergara, C.","Zanella, A.","Farina, E. P.","Decarli, R."],"key":"munoz-elgueta_apex_2022","id":"munoz-elgueta_apex_2022","bibbaseid":"muozelgueta-battaia-kauffmann-debreuck-garcavergara-zanella-farina-decarli-apexattheqsomuseummoleculargasreservoirsassociatedwithztextbackslashsim3quasarsandtheirlinktotheextendedlytextbackslashalphaemission-2022","role":"author","urls":{"Paper":"https://arxiv.org/abs/2201.11660v1"},"metadata":{"authorlinks":{}}},"bibtype":"article","biburl":"https://bibbase.org/zotero/polyphant","dataSources":["7gvjSdWrEu7z5vjjj"],"keywords":[],"search_terms":["apex","qso","museum","molecular","gas","reservoirs","associated","textbackslash","sim","quasars","link","extended","textbackslash","alpha","emission","muñoz-elgueta","battaia","kauffmann","de breuck","garcía-vergara","zanella","farina","decarli"],"title":"APEX at the QSO MUSEUM: molecular gas reservoirs associated with \\$z{\\textbackslash}sim\\$3 quasars and their link to the extended Ly\\${\\textbackslash}alpha\\$ emission","year":2022}