白崎 正人

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研究者氏名
白崎 正人

研究分野

 
 

経歴

 
2017年9月
 - 
現在
国立天文台 特任助教
 
2015年4月
 - 
2017年8月
国立天文台 学術振興会特別研究員PD
 
2012年4月
 - 
2015年3月
東京大学大学院 学術振興会特別研究員DC1
 

受賞

 
2017年2月
井上科学振興財団 第33回井上研究奨励賞
 
2015年3月
東京大学大学院理学系研究科物理学専攻 研究奨励賞
 

論文

 
Chiaki Hikage, Masamune Oguri, Takashi Hamana, Surhud More, Rachel Mandelbaum, Masahiro Takada, Fabian Köhlinger, Hironao Miyatake, Atsushi J. Nishizawa, Hiroaki Aihara, Robert Armstrong, James Bosch, Jean Coupon, Anne Ducout, Bau-Ching Hsieh, Yutaka Komiyama, François Lanusse, Alexie Leauthaud, Elinor Medezinski, Sogo Mineo, Satoshi Miyazaki, Ryoma Murata, Hitoshi Murayama, Masato Shirasaki, Cristóbal Sifón, Melanie Simet, Joshua Speagle, David N. Spergel, Michael A. Strauss, Naoshi Sugiyama, Masayuki Tanaka, Shiang-Yu Wang
   2018年9月
We measure cosmic weak lensing shear power spectra with the Subaru Hyper
Suprime-Cam (HSC) survey first-year shear catalog covering 137degTex of the
sky. Thanks to the high effective galaxy number density of 16.5 arcminTex
even after conserva...
Masato Shirasaki
   2018年7月
Cross correlation with thermal Sunyaev-Zel'dovich (tSZ) effect in cosmic
microwave background observation and weak gravitational lensing effect in
galaxy imaging survey opens a new window on constraining matter contents in the
Universe at redshift...
Ryuichi Takahashi, Takahiro Nishimichi, Masahiro Takada, Masato Shirasaki, Kosei Shiroyama
   2018年5月
In this study, we measure the response of matter and halo projected power
spectra Tex (X, Y are matter and/or halos), to a
large-scale density contrast, Tex, using separate universe
simulations. We show that the f...
Daiki Hashimoto, Atsushi J. Nishizawa, Masato Shirasaki, Oscar Macias, Shunsaku Horiuchi, Hiroyuki Tashiro, Masamune Oguri
   2018年5月
The cross-correlation study of the unresolved Tex-ray background (UGRB)
with galaxy clusters has a potential to reveal the nature of the UGRB. In this
paper, we perform a cross-correlation analysis between Tex-ray data by the
Fermi Large...
Hironao Miyatake, Nicholas Battaglia, Matt Hilton, Elinor Medezinski, Atsushi J. Nishizawa, Surhud More, Simone Aiola, Neta Bahcall, J. Richard Bond, Erminia Calabrese, Steve K. Choi, Mark J. Devlin, Joanna Dunkley, Rolando Dunner, Brittany Fuzia, Patricio Gallardo, Megan Gralla, Matthew Hasselfield, Mark Halpern, Chiaki Hikage, J. Colin Hill, Adam D. Hincks, Renée Hložek, Kevin Huffenberger, John P. Hughes, Brian Koopman, Arthur Kosowsky, Thibaut Louis, Mathew S. Madhavacheril, Jeff McMahon, Rachel Mandelbaum, Tobias A. Marriage, Loïc Maurin, Satoshi Miyazaki, Kavilan Moodley, Ryoma Murata, Sigurd Naess, Laura Newburgh, Michael D. Niemack, Takahiro Nishimichi, Nobuhiro Okabe, Masamune Oguri, Ken Osato, Lyman Page, Bruce Partridge, Naomi Robertson, Neelima Sehgal, Masato Shirasaki, Jonathan Sievers, Cristóbal Sifón, Sara Simon, Blake Sherwin, David N. Spergel, Suzanne T. Staggs, George Stein, Masahiro Takada, Hy Trac, Keiichi Umetsu, Alex van Engelen, Edward J. Wollack
   2018年4月
We present weak-lensing measurements using the first-year data from the Hyper
Suprime-Cam Strategic Survey Program on the Subaru telescope for eight galaxy
clusters selected through their thermal Sunyaev-Zel'dovich (SZ) signal measured
at 148 GHz ...

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