نتایج جستجو برای: astronomical observatory
تعداد نتایج: 21523 فیلتر نتایج به سال:
[email protected] Gunma Astronomical Observatory, 6860-86 Nakayama, Takayama-mura, Agatsuma-gun, Gunma 377-0702 Gunma Study Center, The University of the Air, 1-13-2 Wakamiya-cho, Maebashi, Gunma 371-0032 Liberal Arts Education Center, Tokai University, 1117 Kitakaname, Hiratsuka, Kanagawa 259-1292 Department of Physics, Faculty of Science, Graduate School of Tokai University, 1117 Kitakaname,
Xinglong Tan, Jian Wang, Shuanggen Jin and Xiaolin Meng (School of Environment and Spatial Informatics, China University of Mining and Technology, Xuzhou, China) (Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, China) (Department of Geomatics Engineering, Bulent Ecevit University, Zonguldak, Turkey) (Institute of Engineering Surveying and Space Geodesy (IESSG), The Uni...
1 INAF, Osservatorio Astronomico di Padova, Padua, Italy, 2 Instituto de Astronomía, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico, 3 Instituto de Astrofísica de Andalucía (CSIC), Granada, Spain, 4 Dipartimento di Fisica e Astronomia “Galileo Galilei”, Università di Padova, Padova, Italy, 5 Belgrade Astronomical Observatory, Belgrade, Serbia, 6 INAF, Osservatorio di Astrofisica e...
1 Shanghai Key Laboratory of Space Navigation and Positioning Techniques, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China; [email protected] 2 Department of Geomatics Engineering, Bulent Ecevit University, Zonguldak 67100, Turkey; [email protected] 3 University of Chinese Academy of Sciences, Beijing 100047, China * Correspondence: [email protected] or s...
Large gravitational wave interferometric detectors, like Virgo and LIGO, demonstrated the capability to reach their design sensitivity, but to transform these machines into an effective observational instrument for gravitational wave astronomy a large improvement in sensitivity is required. Advanced detectors in the near future and third-generation observatories in more than one decade will ope...
We describe work investigating how astronomical simulation data can be effectively incorporated into the Virtual Observatory. We focus specifically on determining whether the data query, access and retrieval standards being developed by the International Virtual Observatory Alliance for observational data can be similarly applied to, and fully support, the requirements of data extracted from as...
Abstract CASA, the Common Astronomy Software Applications, is primary data processing software for Atacama Large Millimeter/submillimeter Array (ALMA) and Karl G. Jansky Very (VLA), frequently used also other radio telescopes. The CASA can handle from single-dish, aperture-synthesis, Long Baseline Interferometery (VLBI) One of its core functionalities to support calibration imaging pipelines AL...
We present results of optical spectroscopic observations of candidates of Lyman Break Galaxies (LBGs) at z ∼ 5 in the region including the GOODS-N and the J0053+1234 region by using GMOS-N and GMOS-S, respectively. Among 25 candidates, five objects are identified to be at z ∼ 5 (two of them were already identified by an earlier study) and one object very close to the color-selection window turn...
High angular resolution and sensitive aperture synthesis observations of CS (J = 2−1) and CS (J = 3−2) emissions toward L1551 NE, the second brightest protostar in the Taurus Molecular Cloud, made with the Nobeyama Millimeter Array are presented. L1551 NE is categorized as a class 0 object deeply embedded in the red-shifted outflow lobe of L1551 IRS 5. Previous studies of the L1551 NE region in...
NBI, Astronomical Observatory, University of Copenhagen, Juliane Maries Vej 30, DK–2100 Copenhagen Ø, Denmark Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA Instituto de Astrof́ısica de Andalućıa, IAA-CSIC, Granada, Spain European Southern Observatory, Casilla 19001, Santiago 19, Chile Research Associate, National Fund for Scientific Research (FNRS), Belgium E...
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