{ "id": "2208.00612", "version": "v1", "published": "2022-08-01T05:18:36.000Z", "updated": "2022-08-01T05:18:36.000Z", "title": "Newly discovered $z\\sim5$ quasars based on deep learning and Bayesian information criterion", "authors": [ "Suhyun Shin", "Myungshin Im", "Yongjung Kim", "Linhua Jiang" ], "comment": "8 pages, 5 figures, Accepted for publication in JKAS", "categories": [ "astro-ph.GA" ], "abstract": "We report the discovery of four quasars with $M_{1450} \\gtrsim -25.0$ mag at $z\\sim5$ and supermassive black hole mass measurement for one of the quasars. They were selected as promising high-redshift quasar candidates via deep learning and Bayesian information criterion, which are expected to be effective in discriminating quasars from the late-type stars and high-redshift galaxies. The candidates were observed by the Double Spectrograph on the Palomar 200-inch Hale Telescope. They show clear Ly$\\alpha$ breaks at about 7000-8000 \\r{A}, indicating they are quasars at $4.7 < z < 5.6$. For HSC J233107-001014, we measure the mass of its supermassive black hole (SMBH) using its C\\Romannum{4}$\\lambda 1549$ emission line. The SMBH mass and Eddington ratio of the quasar are found to be $\\sim 10^8 M_{\\odot}$ and $\\sim 0.6$, respectively. This suggests that this quasar possibly harbors a fast growing SMBH near the Eddington limit despite its faintness ($L_{\\rm Bol} < 10^{46}$ erg s$^{-1}$). Our 100 $\\%$ quasar identification rate supports high efficiency of our deep learning and Bayesian information criterion selection method, which can be applied to future surveys to increase high-redshift quasar sample.", "revisions": [ { "version": "v1", "updated": "2022-08-01T05:18:36.000Z" } ], "analyses": { "keywords": [ "deep learning", "black hole mass measurement", "rate supports high efficiency", "quasar identification rate supports high", "bayesian information criterion selection method" ], "note": { "typesetting": "TeX", "pages": 8, "language": "en", "license": "arXiv", "status": "editable" } } }