C
Chris J. Willott
Researcher at National Research Council
Publications - 269
Citations - 16448
Chris J. Willott is an academic researcher from National Research Council. The author has contributed to research in topics: Redshift & Galaxy. The author has an hindex of 68, co-authored 210 publications receiving 15092 citations. Previous affiliations of Chris J. Willott include University of Oxford & IAC.
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Redshift 6.4 host galaxies of 10^8 solar mass black holes: low star formation rate and dynamical mass
TL;DR: In this paper, ALMA observations of rest-frame far-infrared continuum and [CII] line emission in two z = 6.4 quasars with black hole masses of ~10^8 M_sun were presented.
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Star formation and the interstellar medium in z >6 UV-luminous Lyman-break galaxies
TL;DR: In this article, the Atacama Large Millimeter Array (ALMA) detections of atomic carbon line and dust continuum emission in two UV-luminous galaxies at redshift 6.
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Redshift 6.4 host galaxies of 108 solar mass black holes: low star formation rate and dynamical mass
TL;DR: In this article, the Atacama Large Millimeter Array observations of rest-frame far-infrared continuum and [C II] line emission in two z = 6.4 quasars with black hole masses of 108 M ☉ were presented.
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Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV Luminosity Functions at $z \sim 4-7$ Derived with the Half-Million Dropouts on the 100 deg$^2$ Sky
Yoshiaki Ono,Masami Ouchi,Yuichi Harikane,Jun Toshikawa,Michael Rauch,Suraphong Yuma,Marcin Sawicki,Takatoshi Shibuya,Kazuhiro Shimasaku,Masamune Oguri,Chris J. Willott,Mohammad Akhlaghi,Masayuki Akiyama,Jean Coupon,Nobunari Kashikawa,Yutaka Komiyama,Akira Konno,Lihwai Lin,Yoshiki Matsuoka,Satoshi Miyazaki,Tohru Nagao,Kimihiko Nakajima,John D. Silverman,Masayuki Tanaka,Yoshiaki Taniguchi,Shiang-Yu Wang +25 more
TL;DR: In this paper, the authors studied the UV luminosity functions (LFs) at $z\sim 4, $5, $6, and $7$ based on the deep large-area optical images taken by the HSC Subaru strategic program (SSP).
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The bimodal galaxy stellar mass function in the COSMOS survey to z ~ 1: a steep faint end and a new galaxy dichotomy
Niv Drory,Kevin Bundy,Alexie Leauthaud,Alexie Leauthaud,N. Z. Scoville,Peter Capak,Olivier Ilbert,Jeyhan S. Kartaltepe,Jean-Paul Kneib,H. J. McCracken,Mara Salvato,Mara Salvato,David B. Sanders,D. Thompson,Chris J. Willott +14 more
TL;DR: In this paper, the authors present a new analysis of stellar mass functions in the COSMOS field to fainter limits than has been previously probed at z ≤ 1 and observe a dip or plateau at masses ~10^(10) M_⊙, just below the traditional M^*, and an upturn toward a steep faint-end slope of α ~ −1.