{"status":"public","citation":{"ieee":"R. A. Marino <i>et al.</i>, “A giant Lyα nebula and a small-scale clumpy outflow in the system of the exotic quasar J0952+0114 unveiled by MUSE,” <i>The Astrophysical Journal</i>, vol. 880, no. 1. IOP Publishing, 2019.","ista":"Marino RA, Cantalupo S, Pezzulli G, Lilly SJ, Gallego S, Mackenzie R, Matthee JJ, Brinchmann J, Bouché N, Feltre A, Muzahid S, Schroetter I, Johnson SD, Nanayakkara T. 2019. A giant Lyα nebula and a small-scale clumpy outflow in the system of the exotic quasar J0952+0114 unveiled by MUSE. The Astrophysical Journal. 880(1), 47.","mla":"Marino, Raffaella Anna, et al. “A Giant Lyα Nebula and a Small-Scale Clumpy Outflow in the System of the Exotic Quasar J0952+0114 Unveiled by MUSE.” <i>The Astrophysical Journal</i>, vol. 880, no. 1, 47, IOP Publishing, 2019, doi:<a href=\"https://doi.org/10.3847/1538-4357/ab2881\">10.3847/1538-4357/ab2881</a>.","chicago":"Marino, Raffaella Anna, Sebastiano Cantalupo, Gabriele Pezzulli, Simon J. Lilly, Sofia Gallego, Ruari Mackenzie, Jorryt J Matthee, et al. “A Giant Lyα Nebula and a Small-Scale Clumpy Outflow in the System of the Exotic Quasar J0952+0114 Unveiled by MUSE.” <i>The Astrophysical Journal</i>. IOP Publishing, 2019. <a href=\"https://doi.org/10.3847/1538-4357/ab2881\">https://doi.org/10.3847/1538-4357/ab2881</a>.","apa":"Marino, R. A., Cantalupo, S., Pezzulli, G., Lilly, S. J., Gallego, S., Mackenzie, R., … Nanayakkara, T. (2019). A giant Lyα nebula and a small-scale clumpy outflow in the system of the exotic quasar J0952+0114 unveiled by MUSE. <i>The Astrophysical Journal</i>. IOP Publishing. <a href=\"https://doi.org/10.3847/1538-4357/ab2881\">https://doi.org/10.3847/1538-4357/ab2881</a>","ama":"Marino RA, Cantalupo S, Pezzulli G, et al. A giant Lyα nebula and a small-scale clumpy outflow in the system of the exotic quasar J0952+0114 unveiled by MUSE. <i>The Astrophysical Journal</i>. 2019;880(1). doi:<a href=\"https://doi.org/10.3847/1538-4357/ab2881\">10.3847/1538-4357/ab2881</a>","short":"R.A. Marino, S. Cantalupo, G. Pezzulli, S.J. Lilly, S. Gallego, R. Mackenzie, J.J. Matthee, J. Brinchmann, N. Bouché, A. Feltre, S. Muzahid, I. Schroetter, S.D. Johnson, T. Nanayakkara, The Astrophysical Journal 880 (2019)."},"title":"A giant Lyα nebula and a small-scale clumpy outflow in the system of the exotic quasar J0952+0114 unveiled by MUSE","type":"journal_article","year":"2019","external_id":{"arxiv":["1906.06347"]},"author":[{"last_name":"Marino","first_name":"Raffaella Anna","full_name":"Marino, Raffaella Anna"},{"full_name":"Cantalupo, Sebastiano","first_name":"Sebastiano","last_name":"Cantalupo"},{"full_name":"Pezzulli, Gabriele","last_name":"Pezzulli","first_name":"Gabriele"},{"last_name":"Lilly","first_name":"Simon J.","full_name":"Lilly, Simon J."},{"last_name":"Gallego","first_name":"Sofia","full_name":"Gallego, Sofia"},{"full_name":"Mackenzie, Ruari","first_name":"Ruari","last_name":"Mackenzie"},{"id":"7439a258-f3c0-11ec-9501-9df22fe06720","orcid":"0000-0003-2871-127X","first_name":"Jorryt J","last_name":"Matthee","full_name":"Matthee, Jorryt J"},{"last_name":"Brinchmann","first_name":"Jarle","full_name":"Brinchmann, Jarle"},{"last_name":"Bouché","first_name":"Nicolas","full_name":"Bouché, Nicolas"},{"last_name":"Feltre","first_name":"Anna","full_name":"Feltre, Anna"},{"full_name":"Muzahid, Sowgat","first_name":"Sowgat","last_name":"Muzahid"},{"last_name":"Schroetter","first_name":"Ilane","full_name":"Schroetter, Ilane"},{"full_name":"Johnson, Sean D.","last_name":"Johnson","first_name":"Sean D."},{"full_name":"Nanayakkara, Themiya","first_name":"Themiya","last_name":"Nanayakkara"}],"publication_status":"published","main_file_link":[{"url":"https://arxiv.org/abs/1906.06347","open_access":"1"}],"language":[{"iso":"eng"}],"issue":"1","acknowledgement":"We thank Lutz Wisotzki for stimulating discussions. This work is based on observations taken at ESO/VLT in Paranal and we would like to thank the ESO staff for their assistance and support during the MUSE GTO campaigns. This work was supported by the Swiss National Science Foundation. This research made use of Astropy, a community-developed core PYTHON package for astronomy (Astropy Collaboration et al. 2013), NumPy and SciPy (Oliphant 2007), Matplotlib (Hunter 2007), IPython (Perez & Granger 2007), and of the NASA Astrophysics Data System Bibliographic Services. S.C. and G.P. gratefully acknowledge support from Swiss National Science Foundation grant PP00P2−163824. A.F. acknowledges support from the ERC via Advanced Grant under grants agreement no. 339659-MUSICOS. J.B. acknowledges support by FCT/MCTES through national funds by grant UID/FIS/04434/2019 and through Investigador FCT Contract No. IF/01654/2014/CP1215/CT0003. S.D.J. is supported by a NASA Hubble Fellowship (HST-HF2-51375.001-A). T.N. acknowledges the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO) top grant TOP1.16.057.","extern":"1","_id":"11516","date_created":"2022-07-06T13:50:33Z","volume":880,"keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"day":"24","article_type":"original","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","abstract":[{"text":"The well-known quasar SDSS J095253.83+011421.9 (J0952+0114) at z = 3.02 has one of the most peculiar spectra discovered so far, showing the presence of narrow Lyα and broad metal emission lines. Although recent studies have suggested that a proximate damped Lyα absorption (PDLA) system causes this peculiar spectrum, the origin of the gas associated with the PDLA is unknown. Here we report the results of observations with the Multi Unit Spectroscopic Explorer (MUSE) that reveal a new giant (≈100 physical kpc) Lyα nebula. The detailed analysis of the Lyα velocity, velocity dispersion, and surface brightness profiles suggests that the J0952+0114 Lyα nebula shares similar properties with other QSO nebulae previously detected with MUSE, implying that the PDLA in J0952+0144 is covering only a small fraction of the solid angle of the QSO emission. We also detected bright and spectrally narrow C iv λ1550 and He ii λ1640 extended emission around J0952+0114 with velocity centroids similar to the peak of the extended and central narrow Lyα emission. The presence of a peculiarly bright, unresolved, and relatively broad He ii λ1640 emission in the central region at exactly the same PDLA redshift hints at the possibility that the PDLA originates in a clumpy outflow with a bulk velocity of about 500 km s−1. The smaller velocity dispersion of the large-scale Lyα emission suggests that the high-speed outflow is confined to the central region. Lastly, the derived spatially resolved He ii/Lyα and C iv/Lyα maps show a positive gradient with the distance to the QSO, hinting at a non-homogeneous distribution of the ionization parameter.","lang":"eng"}],"oa":1,"publisher":"IOP Publishing","oa_version":"Preprint","month":"07","doi":"10.3847/1538-4357/ab2881","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"publication":"The Astrophysical Journal","quality_controlled":"1","article_number":"47","date_published":"2019-07-24T00:00:00Z","intvolume":"       880","date_updated":"2022-08-18T10:20:18Z","scopus_import":"1","article_processing_charge":"No"}