@article{rudie_unique_2017,
	title = {A {Unique} {View} of {AGN}-{Driven} {Molecular} {Outflows}: {The} {Discovery} of a {Massive} {Galaxy} {Counterpart} to a \$z=2.4\$ {High}-{Metallicity} {Damped} {Lyman}-\${\textbackslash}alpha\$ {Absorber}},
	volume = {1703},
	shorttitle = {A {Unique} {View} of {AGN}-{Driven} {Molecular} {Outflows}},
	url = {http://adsabs.harvard.edu/abs/2017arXiv170303807R},
	abstract = {We report the discovery of massive 
\${\textbackslash}log(M/M\_{\textbackslash}odot)=10.74{\textasciicircum}\{+0.18\}\_\{-0.16\}\$ galaxy at the same redshift as a
carbon-monoxide bearing sub-damped Lyman \${\textbackslash}alpha\$ absorber (sub-DLA)
seen in the spectrum of the QSO J1439+1117. The galaxy, J1439B, is
located 4.7" from the QSO sightline, a projected distance of 38 physical
kpc at \$z=2.4189\$, and exhibits broad optical emission lines
(\${\textbackslash}sigma\_\{{\textbackslash}rm\{[O III]\}\}=303 {\textbackslash}pm 12\$ km s\${\textasciicircum}\{-1\}\$) with ratios
characteristic of excitation by an active galactic nucleus (AGN). The
galaxy has a factor of \${\textbackslash}sim\$10 lower star formation than is typical of
star-forming galaxies of the same mass and redshift. The nearby DLA is
highly enriched, suggesting its galactic counterpart must be massive if
it follows the \$z{\textbackslash}sim2\$ mass-metallicity relationship. Metallic
absorption associated with the DLA is spread over a velocity range
\${\textbackslash}Delta v {\textgreater} 1000\$ km s\${\textasciicircum}\{-1\}\$, suggesting an energetic origin. We
explore the possibility that a different galaxy could be responsible for
the rare absorber, and conclude it is unlikely based on imaging,
integral field spectroscopy, and high-\$z\$ massive galaxy pair
statistics. We argue that the gas seen in absorption against the QSO was
likely ejected from the galaxy J1439B and therefore provides a unique
observational probe of AGN feedback in the distant universe.},
	urldate = {2017-03-15},
	journal = {ArXiv e-prints},
	author = {Rudie, Gwen C. and Newman, Andrew B. and Murphy, Michael T.},
	month = mar,
	year = {2017},
	keywords = {Astrophysics - Astrophysics of Galaxies},
	pages = {arXiv:1703.03807},
}

{"_id":"76A7X2ThrpNuzvyqj","bibbaseid":"rudie-newman-murphy-auniqueviewofagndrivenmolecularoutflowsthediscoveryofamassivegalaxycounterparttoaz24highmetallicitydampedlymantextbackslashalphaabsorber-2017","author_short":["Rudie, G. C.","Newman, A. B.","Murphy, M. T."],"bibdata":{"bibtype":"article","type":"article","title":"A Unique View of AGN-Driven Molecular Outflows: The Discovery of a Massive Galaxy Counterpart to a \\$z=2.4\\$ High-Metallicity Damped Lyman-\\${\\textbackslash}alpha\\$ Absorber","volume":"1703","shorttitle":"A Unique View of AGN-Driven Molecular Outflows","url":"http://adsabs.harvard.edu/abs/2017arXiv170303807R","abstract":"We report the discovery of massive \\${\\textbackslash}log(M/M_{\\textbackslash}odot)=10.74{\\textasciicircum}\\{+0.18\\}_\\{-0.16\\}\\$ galaxy at the same redshift as a carbon-monoxide bearing sub-damped Lyman \\${\\textbackslash}alpha\\$ absorber (sub-DLA) seen in the spectrum of the QSO J1439+1117. The galaxy, J1439B, is located 4.7\" from the QSO sightline, a projected distance of 38 physical kpc at \\$z=2.4189\\$, and exhibits broad optical emission lines (\\${\\textbackslash}sigma_\\{{\\textbackslash}rm\\{[O III]\\}\\}=303 {\\textbackslash}pm 12\\$ km s\\${\\textasciicircum}\\{-1\\}\\$) with ratios characteristic of excitation by an active galactic nucleus (AGN). The galaxy has a factor of \\${\\textbackslash}sim\\$10 lower star formation than is typical of star-forming galaxies of the same mass and redshift. The nearby DLA is highly enriched, suggesting its galactic counterpart must be massive if it follows the \\$z{\\textbackslash}sim2\\$ mass-metallicity relationship. Metallic absorption associated with the DLA is spread over a velocity range \\${\\textbackslash}Delta v {\\textgreater} 1000\\$ km s\\${\\textasciicircum}\\{-1\\}\\$, suggesting an energetic origin. We explore the possibility that a different galaxy could be responsible for the rare absorber, and conclude it is unlikely based on imaging, integral field spectroscopy, and high-\\$z\\$ massive galaxy pair statistics. We argue that the gas seen in absorption against the QSO was likely ejected from the galaxy J1439B and therefore provides a unique observational probe of AGN feedback in the distant universe.","urldate":"2017-03-15","journal":"ArXiv e-prints","author":[{"propositions":[],"lastnames":["Rudie"],"firstnames":["Gwen","C."],"suffixes":[]},{"propositions":[],"lastnames":["Newman"],"firstnames":["Andrew","B."],"suffixes":[]},{"propositions":[],"lastnames":["Murphy"],"firstnames":["Michael","T."],"suffixes":[]}],"month":"March","year":"2017","keywords":"Astrophysics - Astrophysics of Galaxies","pages":"arXiv:1703.03807","bibtex":"@article{rudie_unique_2017,\n\ttitle = {A {Unique} {View} of {AGN}-{Driven} {Molecular} {Outflows}: {The} {Discovery} of a {Massive} {Galaxy} {Counterpart} to a \\$z=2.4\\$ {High}-{Metallicity} {Damped} {Lyman}-\\${\\textbackslash}alpha\\$ {Absorber}},\n\tvolume = {1703},\n\tshorttitle = {A {Unique} {View} of {AGN}-{Driven} {Molecular} {Outflows}},\n\turl = {http://adsabs.harvard.edu/abs/2017arXiv170303807R},\n\tabstract = {We report the discovery of massive \n\\${\\textbackslash}log(M/M\\_{\\textbackslash}odot)=10.74{\\textasciicircum}\\{+0.18\\}\\_\\{-0.16\\}\\$ galaxy at the same redshift as a\ncarbon-monoxide bearing sub-damped Lyman \\${\\textbackslash}alpha\\$ absorber (sub-DLA)\nseen in the spectrum of the QSO J1439+1117. The galaxy, J1439B, is\nlocated 4.7\" from the QSO sightline, a projected distance of 38 physical\nkpc at \\$z=2.4189\\$, and exhibits broad optical emission lines\n(\\${\\textbackslash}sigma\\_\\{{\\textbackslash}rm\\{[O III]\\}\\}=303 {\\textbackslash}pm 12\\$ km s\\${\\textasciicircum}\\{-1\\}\\$) with ratios\ncharacteristic of excitation by an active galactic nucleus (AGN). The\ngalaxy has a factor of \\${\\textbackslash}sim\\$10 lower star formation than is typical of\nstar-forming galaxies of the same mass and redshift. The nearby DLA is\nhighly enriched, suggesting its galactic counterpart must be massive if\nit follows the \\$z{\\textbackslash}sim2\\$ mass-metallicity relationship. Metallic\nabsorption associated with the DLA is spread over a velocity range\n\\${\\textbackslash}Delta v {\\textgreater} 1000\\$ km s\\${\\textasciicircum}\\{-1\\}\\$, suggesting an energetic origin. We\nexplore the possibility that a different galaxy could be responsible for\nthe rare absorber, and conclude it is unlikely based on imaging,\nintegral field spectroscopy, and high-\\$z\\$ massive galaxy pair\nstatistics. We argue that the gas seen in absorption against the QSO was\nlikely ejected from the galaxy J1439B and therefore provides a unique\nobservational probe of AGN feedback in the distant universe.},\n\turldate = {2017-03-15},\n\tjournal = {ArXiv e-prints},\n\tauthor = {Rudie, Gwen C. and Newman, Andrew B. and Murphy, Michael T.},\n\tmonth = mar,\n\tyear = {2017},\n\tkeywords = {Astrophysics - Astrophysics of Galaxies},\n\tpages = {arXiv:1703.03807},\n}\n\n","author_short":["Rudie, G. C.","Newman, A. B.","Murphy, M. T."],"key":"rudie_unique_2017","id":"rudie_unique_2017","bibbaseid":"rudie-newman-murphy-auniqueviewofagndrivenmolecularoutflowsthediscoveryofamassivegalaxycounterparttoaz24highmetallicitydampedlymantextbackslashalphaabsorber-2017","role":"author","urls":{"Paper":"http://adsabs.harvard.edu/abs/2017arXiv170303807R"},"keyword":["Astrophysics - Astrophysics of Galaxies"],"metadata":{"authorlinks":{}}},"bibtype":"article","biburl":"https://bibbase.org/zotero/polyphant","dataSources":["7gvjSdWrEu7z5vjjj"],"keywords":["astrophysics - astrophysics of galaxies"],"search_terms":["unique","view","agn","driven","molecular","outflows","discovery","massive","galaxy","counterpart","high","metallicity","damped","lyman","textbackslash","alpha","absorber","rudie","newman","murphy"],"title":"A Unique View of AGN-Driven Molecular Outflows: The Discovery of a Massive Galaxy Counterpart to a \\$z=2.4\\$ High-Metallicity Damped Lyman-\\${\\textbackslash}alpha\\$ Absorber","year":2017}