Zobrazeno 1 - 10
of 12
pro vyhledávání: '"Wei-Leong Tee"'
Autor:
Xiangyu Jin, Jinyi Yang, Xiaohui Fan, Feige Wang, Koki Kakiichi, Romain A. Meyer, George D. Becker, Siwei Zou, Eduardo Bañados, Jaclyn B. Champagne, Valentina D’Odorico, Minghao Yue, Sarah E. I. Bosman, Zheng Cai, Anna-Christina Eilers, Joseph F. Hennawi, Hyunsung D. Jun, Mingyu Li, Zihao Li, Weizhe Liu, Maria Pudoka, Sindhu Satyavolu, Fengwu Sun, Wei Leong Tee, Yunjing Wu
Publikováno v:
The Astrophysical Journal, Vol 976, Iss 1, p 93 (2024)
Understanding when and how reionization happened is crucial for studying the early structure formation and the properties of the first galaxies in the Universe. At z > 5.5, the observed intergalactic medium (IGM) optical depth shows a significant sca
Externí odkaz:
https://doaj.org/article/ecb6fecd511748efb4e90104f9e69cf5
Autor:
Weizhe Liu, Xiaohui Fan, Jinyi Yang, Eduardo Bañados, Feige Wang, Julien Wolf, Aaron J. Barth, Tiago Costa, Roberto Decarli, Anna-Christina Eilers, Federica Loiacono, Yue Shen, Emanuele Paolo Farina, Xiangyu Jin, Hyunsung D. Jun, Mingyu Li, Alessandro Lupi, Madeline A. Marshall, Zhiwei Pan, Maria Pudoka, Ming-Yang Zhuang, Jaclyn B. Champagne, Huan Li, Fengwu Sun, Wei Leong Tee, Andrey Vayner, Haowen Zhang
Publikováno v:
The Astrophysical Journal, Vol 976, Iss 1, p 33 (2024)
The James Webb Space Telescope opens a new window to directly probe luminous quasars powered by billion solar mass black holes in the Epoch of Reionization and their coevolution with massive galaxies with unprecedented details. In this paper, we repo
Externí odkaz:
https://doaj.org/article/5439c601a6de406dbb187cb307c27328
Autor:
Xiaojing Lin, Feige Wang, Xiaohui Fan, Zheng Cai, Jaclyn B. Champagne, Fengwu Sun, Marta Volonteri, Jinyi Yang, Joseph F. Hennawi, Eduardo Bañados, Aaron Barth, Anna-Christina Eilers, Emanuele Paolo Farina, Weizhe Liu, Xiangyu Jin, Hyunsung D. Jun, Alessandro Lupi, Koki Kakiichi, Chiara Mazzucchelli, Masafusa Onoue, Zhiwei Pan, Elia Pizzati, Sofía Rojas-Ruiz, Jan-Torge Schindler, Benny Trakhtenbrot, Yue Shen, Maxime Trebitsch, Ming-Yang Zhuang, Ryan Endsley, Romain A. Meyer, Zihao Li, Mingyu Li, Maria Pudoka, Wei Leong Tee, Yunjing Wu, Haowen Zhang
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 1, p 147 (2024)
Low-luminosity active galactic nuclei (AGNs) with low-mass black holes (BHs) in the early universe are fundamental to understanding the BH growth and their coevolution with the host galaxies. Utilizing JWST NIRCam Wide Field Slitless Spectroscopy, we
Externí odkaz:
https://doaj.org/article/df9925eb61074a36813427e43f3ae1ae
Autor:
Yue Shen, Catherine J. Grier, Keith Horne, Zachary Stone, Jennifer I. Li, Qian Yang, Yasaman Homayouni, Jonathan R. Trump, Scott F. Anderson, W. N. Brandt, Patrick B. Hall, Luis C. Ho, Linhua Jiang, Patrick Petitjean, Donald P. Schneider, Charling Tao, Fergus. R. Donnan, Yusra AlSayyad, Matthew A. Bershady, Michael R. Blanton, Dmitry Bizyaev, Kevin Bundy, Yuguang Chen, Megan C. Davis, Kyle Dawson, Xiaohui Fan, Jenny E. Greene, Hannes Gröller, Yucheng Guo, Héctor Ibarra-Medel, Yuanzhe Jiang, Ryan P. Keenan, Juna A. Kollmeier, Cassandra Lejoly, Zefeng Li, Axel de la Macorra, Maxwell Moe, Jundan Nie, Graziano Rossi, Paul S. Smith, Wei Leong Tee, Anne-Marie Weijmans, Jiachuan Xu, Minghao Yue, Xu Zhou, Zhimin Zhou, Hu Zou
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 272, Iss 2, p 26 (2024)
We present the final data from the Sloan Digital Sky Survey (SDSS) Reverberation Mapping (RM) project, a precursor to the SDSS-V Black Hole Mapper RM program. This data set includes 11 yr photometric and 7 yr spectroscopic light curves for 849 broad-
Externí odkaz:
https://doaj.org/article/6d791eb279de4413b8eae4a884dd70d2
Autor:
Yunjing Wu, Feige Wang, Zheng Cai, Xiaohui Fan, Kristian Finlator, Jinyi Yang, Joseph F. Hennawi, Fengwu Sun, Jaclyn B. Champagne, Xiaojing Lin, Zihao Li, Zuyi Chen, Eduardo Bañados, George D. Becker, Sarah E. I. Bosman, Gustavo Bruzual, Stephane Charlot, Hsiao-Wen Chen, Jacopo Chevallard, Anna-Christina Eilers, Emanuele Paolo Farina, Xiangyu Jin, Hyunsung D. Jun, Koki Kakiichi, Mingyu Li, Weizhe Liu, Maria A. Pudoka, Wei Leong Tee, Zhang-Liang Xie, Siwei Zou
Publikováno v:
The Astrophysical Journal Letters, Vol 956, Iss 2, p L40 (2023)
The launch of JWST opens a new window for studying the connection between metal-line absorbers and galaxies at the end of the Epoch of Reionization. Previous studies have detected absorber–galaxy pairs in limited quantities through ground-based obs
Externí odkaz:
https://doaj.org/article/21d6524d3df84ec483b763434e0fbae8
Autor:
Feige Wang, Jinyi Yang, Joseph F. Hennawi, Xiaohui Fan, Fengwu Sun, Jaclyn B. Champagne, Tiago Costa, Melanie Habouzit, Ryan Endsley, Zihao Li, Xiaojing Lin, Romain A. Meyer, Jan–Torge Schindler, Yunjing Wu, Eduardo Bañados, Aaron J. Barth, Aklant K. Bhowmick, Rebekka Bieri, Laura Blecha, Sarah Bosman, Zheng Cai, Luis Colina, Thomas Connor, Frederick B. Davies, Roberto Decarli, Gisella De Rosa, Alyssa B. Drake, Eiichi Egami, Anna-Christina Eilers, Analis E. Evans, Emanuele Paolo Farina, Zoltan Haiman, Linhua Jiang, Xiangyu Jin, Hyunsung D. Jun, Koki Kakiichi, Yana Khusanova, Girish Kulkarni, Mingyu Li, Weizhe Liu, Federica Loiacono, Alessandro Lupi, Chiara Mazzucchelli, Masafusa Onoue, Maria A. Pudoka, Sofía Rojas-Ruiz, Yue Shen, Michael A. Strauss, Wei Leong Tee, Benny Trakhtenbrot, Maxime Trebitsch, Bram Venemans, Marta Volonteri, Fabian Walter, Zhang-Liang Xie, Minghao Yue, Haowen Zhang, Huanian Zhang, Siwei Zou
Publikováno v:
The Astrophysical Journal Letters, Vol 951, Iss 1, p L4 (2023)
We present the first results from the JWST program A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE). This program represents an imaging and spectroscopic survey of 25 reionization-era quasars and their environments by utilizing
Externí odkaz:
https://doaj.org/article/ddc3cfff06e4420494aa2d447f16d97b
Autor:
Jinyi Yang, Feige Wang, Xiaohui Fan, Joseph F. Hennawi, Aaron J. Barth, Eduardo Bañados, Fengwu Sun, Weizhe Liu, Zheng Cai, Linhua Jiang, Zihao Li, Masafusa Onoue, Jan-Torge Schindler, Yue Shen, Yunjing Wu, Aklant K. Bhowmick, Rebekka Bieri, Laura Blecha, Sarah Bosman, Jaclyn B. Champagne, Luis Colina, Thomas Connor, Tiago Costa, Frederick B. Davies, Roberto Decarli, Gisella De Rosa, Alyssa B. Drake, Eiichi Egami, Anna-Christina Eilers, Analis E. Evans, Emanuele Paolo Farina, Melanie Habouzit, Zoltan Haiman, Xiangyu Jin, Hyunsung D. Jun, Koki Kakiichi, Yana Khusanova, Girish Kulkarni, Federica Loiacono, Alessandro Lupi, Chiara Mazzucchelli, Zhiwei Pan, Sofía Rojas-Ruiz, Michael A. Strauss, Wei Leong Tee, Benny Trakhtenbrot, Maxime Trebitsch, Bram Venemans, Marianne Vestergaard, Marta Volonteri, Fabian Walter, Zhang-Liang Xie, Minghao Yue, Haowen Zhang, Huanian Zhang, Siwei Zou
Publikováno v:
The Astrophysical Journal Letters, Vol 951, Iss 1, p L5 (2023)
Studies of rest-frame optical emission in quasars at z > 6 have historically been limited by the wavelengths accessible by ground-based telescopes. The James Webb Space Telescope (JWST) now offers the opportunity to probe this emission deep into the
Externí odkaz:
https://doaj.org/article/8de574c47d28453a88c84f7344cbf379
Publikováno v:
The Astrophysical Journal, Vol 956, Iss 1, p 52 (2023)
About 70 luminous quasars discovered at z > 6.5 are strongly biased toward the bright end, thus not providing a comprehensive view of quasar abundance beyond the cosmic dawn. We present the predicted results of the Roman/Rubin high-redshift quasar su
Externí odkaz:
https://doaj.org/article/cfc97ef25c104e0188658ec2debe3e79
Autor:
Ian Smail, J. M. Simpson, Wei-Hao Wang, Yiping Ao, Luis C. Ho, Scott Chapman, Thomas R. Greve, Chian-Chou Chen, Douglas Scott, Arif Babul, Andrew Bunker, Ho Seong Hwang, Xinwen Shu, M. P. Koprowski, Yoshiki Toba, Sungwook E. Hong, David L. Clements, Chen-Fatt Lim, Michał J. Michałowski, Hyunjin Shim, Yen-Ting Lin, Yu-Yen Chang, Wei-Leong Tee, Christopher J. Conselice, Yu Gao
We analyze an extremely deep 450 μm image (1σ = 0.56 mJy beam−1) of a sime300 arcmin2 area in the CANDELS/COSMOS field as part of the Sub-millimeter Common User Bolometric Array-2 Ultra Deep Imaging EAO Survey. We select a robust (signal-to-noise
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa528fb0860fe4b14bb27fe6adebd9fe
http://hdl.handle.net/10044/1/80413
http://hdl.handle.net/10044/1/80413
Autor:
James E. Geach, Chen-Fatt Lim, Helmut Dannerbauer, Christopher Harrison, Wei-Hao Wang, Yoshiki Toba, Rob Ivison, James Dunlop, Dominik Riechers, Chian-Chou Chen, Y. Ao, Andrew Bunker, Minju Lee, Ian Smail, X. Z. Zheng, Julian M Simpson, David J. Rosario, Ho Seong Hwang, Tadayuki Kodama, T. Goto, H. Shim, Ho-Gyu Lee, Michał J. Michałowski, Scott Chapman, Chien-Hsiu Lee, A. M. Swinbank, Elisabetta Valiante, X. W. Shu, Junxian Wang, N. Bourne, Wei-Leong Tee
Publikováno v:
Astrophysical journal letters, 2017, Vol.844(1), pp.L10 [Peer Reviewed Journal]
Simpson, J M, Smail, I, Wang, W H, Riechers, D, Dunlop, J S, Ao, Y, Bourne, N, Bunker, A, Chapman, S C, Chen, C C, Dannerbauer, H, Geach, J E, Goto, T, Harrison, C M, Hwang, H S, Ivison, R J, Kodama, T, Lee, C H, Lee, H M, Lee, M, Lim, C F, Michałowski, M J, Rosario, D J, Shim, H, Shu, X W, Swinbank, A M, Tee, W L, Toba, Y, Valiante, E, Wang, J & Zheng, X Z 2017, ' An Imperfectly Passive Nature : Bright Submillimeter Emission from Dust-obscured Star Formation in the z = 3.717 "passive" System, ZF 20115 ', Astrophysical Journal Letters, vol. 844, no. 1, L10 . https://doi.org/10.3847/2041-8213/aa7cf2
Simpson, J M, Smail, I, Wang, W H, Riechers, D, Dunlop, J S, Ao, Y, Bourne, N, Bunker, A, Chapman, S C, Chen, C C, Dannerbauer, H, Geach, J E, Goto, T, Harrison, C M, Hwang, H S, Ivison, R J, Kodama, T, Lee, C H, Lee, H M, Lee, M, Lim, C F, Michałowski, M J, Rosario, D J, Shim, H, Shu, X W, Swinbank, A M, Tee, W L, Toba, Y, Valiante, E, Wang, J & Zheng, X Z 2017, ' An Imperfectly Passive Nature : Bright Submillimeter Emission from Dust-obscured Star Formation in the z = 3.717 "passive" System, ZF 20115 ', Astrophysical Journal Letters, vol. 844, no. 1, L10 . https://doi.org/10.3847/2041-8213/aa7cf2
The identification of high-redshift massive galaxies with old stellar populations may pose challenges to some models of galaxy formation. However, to securely classify a galaxy as quiescent, it is necessary to exclude significant ongoing star formati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::74cf3766e7fccc270fccdb692e64f31b
http://arxiv.org/abs/1704.03868
http://arxiv.org/abs/1704.03868