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11篇 您的检索式：作者名="Serabyn"

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		题名	作者	年代	出处	被引量
	1	Submillimeter atmospheric transmission measurements on Mauna Kea during extremely dry El Ni?o conditions: implications for broadband opacity contributions显示文摘	J.R Pardo E Serabyn J Cernicharo	2001	Journal of Quantitative Spectroscopy and Radiative Transfer2001，，4：	2
	2	Improved high-contrast imaging with on-axis telescopes using a multistage vortex coronagraph 显示文摘	Mawet D Serabyn E Wallace J K	2011	Optics Letters2011，36，8：	1
	3	Atmospheric transmission at microwaves ( ATM ) : improved model for millimetersub millimeter applieations显示文摘	PARDO J R CERNICHARO J and SERABYN E	2001	IEEE Transaction on Antennas and Propagation2001，49，12：	1
	4	Optical vectorial vortex coronagraphs using liquid crystal polymers:theory,manufacturing and laboratory demonstration显示文摘	MAWET D SERABYN E LIEWER K	2009	Optics Express2009，17，3：	1
	5	Atmospheric transmission at microwaves (ATM): an improved model for millimeter/ submillimeter applications 显示文摘	Pardo J R Cernicharo J Serabyn E	2001	IEEE Transacti on on Antennas and Propagation2001，49，12：	1
	6	查看详情显示文摘	Serabyn E Mawet D Burruss R		0，，：	1
	7	Submillimeter atmospheric transmission measurements on Mauna Kea during extremelydry El Ni-o conditions:implications for broadband opacity contributions显示文摘	Pardo J R Serabyn E R Cernicharo J	2001	Journal of Quantitative Spectroscopy and RadiativeTransfer2001，68，4：	1
	8	Atmospheric transmission at microwaves(ATM):An improved model for mm/submm applications显示文摘	Pardo J R Cernicharo J Serabyn E		0，，12：	1
	9	Atmospheric transmission at microwaves (ATM): an improved model for millimeter Isubmillimeter applications显示文摘	PardoJ R CernicharoJ Serabyn E	2001	IEEE Trans on Antennas and Propagation2001，49，12：	1
	10	Atmospheric transmission at microwaves(ATM):An improved model for millimeter/sub millimeter applications显示文摘	Pardo J R Cernicharo J Serabyn E	2001	IEEE Trans on Antennas and Propagation2001，49，12：	1
	11	Near-infrared polarimetry of the GG Tauri A binary system显示文摘A high angular resolution near-infrared image that shows the intensity of polarization for the GG Tau A binary system was obtained with the Subaru Telescope.The image shows a circumbinary disk scattering the light from the central binary. The azimuthal profile of the intensity of polarization for the circumbinary disk is roughly reproduced by a simple disk model with the Henyey-Greenstein phase function and the Rayleigh function, indicating there are small dust grains at the surface of the disk.Combined with a previous observation of the circumbinary disk, our image indicates that the gap structure in the circumbinary disk orbits counterclockwise, but material in the disk orbits clockwise. We propose that there is a shadow caused by material located between the central binary and the circumbinary disk. The separations and position angles of the stellar components of the binary in the past 20 yr are consistent with the binary orbit with a = 33.4 AU and e = 0.34.	Yoichi Itoh Yumiko Oasa Tomoyuki Kudo Nobuhiko Kusakabe Jun Hashimoto Lyu Abe Wolfgang Brandner Timothy D.Brandt Joseph C.Carson Sebastian Egner Markus Feldt Carol A.Grady Olivier Guyon Yutaka Hayano Masahiko Hayashi Saeko S.Hayashi Thomas Henning Klaus W.Hodapp Miki Ishii Masanori Iye Markus Janson Ryo Kandori Gillian R.Knapp Masayuki Kuzuhara Jungmi Kwon Taro Matsuo Michael W.McElwain Shoken Miyama Jun-Ichi Morino Amaya Moro-Martin Tetsuo Nishimura Tae-Soo Pyo Eugene Serabyn Takuya Suenaga Hiroshi Suto Ryuji Suzuki Yasuhiro H.Takahashi Naruhisa Takato Hiroshi Terada Christian Thalmann Daigo Tomono Edwin L.Turner Makoto Watanabe John Wisniewski Toru Yamada Satoshi Mayama Thayne Currie Hideki Takami Tomonori Usuda Motohide Tamura	2014	Research in Astronomy and Astrophysics2014，14，11：	0

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