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1.
A. V. Moiseev 《Astrophysical Bulletin》2008,63(1):70-82
We analyze factors that affect the accuracy of stellar line-of-sight velocities measured from the spectra obtained with the SCORPIO instrument attached to the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. We show that nonuniform illumination of the spectrograph slit combined with the effect of differential atmospheric refractionmay result in substantial systematic errors in the inferred line-of-sight velocities, and formulate recommendations concerning the methodology of observations, which allow the errors of line-of-sight velocity measurements to be minimized. 相似文献
2.
V. L. Afanasiev S. N. Dodonov V. R. Amirkhanyan A. V. Moiseev 《Astrophysical Bulletin》2016,71(4):479-488
We describe the design of a suspended low- and medium-resolution spectrograph (R ≈ 300–1300) designed and made at the Special Astrophysical Observatory of the Russian Academy of Sciences for the 1.6-m AZT-33IK telescope of Sayan Observatory of the Institute of Solar-Terrestrial Physics of the Siberian Branch of the Russian Academy of Sciences. We report the results of laboratory measurements of the parameters of the instrument and tests performed on the 1-m Zeiss-1000 telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. We measured the total quantum efficiency of the “spectrograph + telescope + detector” system on AZT-33IK telescope, which at its maximum reaches 56%. Such a hight transparency of the spectrograph allows it to be used with the 1.6-m telescope to determine the types and redshifts of objects with integrated magnitudes mAB ≈ 20–21, and this result was confirmed by actual observations. 相似文献
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本文介绍了云南天文台一米望远镜附属的一台低色散光谱仪实验装置,介绍了该装置的设计原理、系统结构参数及试观测情况,并讨论了存在的问题和解决问题的设想。我们已用该装置观测到19m左右的具有大红移的类星体光谱。该类低色散光谱仪,将为我国星系研究工作者提供实测条件。 相似文献
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Dodin A. V. Potanin S. A. Shatsky N. I. Belinski A. A. Atapin K. E. Burlak M. A. Egorov O. V. Tatarnikov A. M. Postnov K. A. Belvedersky M. I. Burenin R. A. Gilfanov M. R. Medvedev P. S. Meshcheryakov A. V. Sazonov S. Yu. Khorunzhev G. A. Sunyaev R. A. 《Astronomy Letters》2020,46(7):429-438
Astronomy Letters - Based on observations with the new transient double-beam spectrograph (TDS) at the 2.5-m telescope of the Caucasus Mountain Observatory of SAI MSU, we have determined the types... 相似文献
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Dodin A. V. Shatsky N. I. Belinski A. A. Atapin K. E. Burlak M. A. Zheltoukhov S. G. Tatarnikov A. M. Postnov K. A. Cherepashchuk A. M. Belvedersky M. I. Borisov V. D. Burenin R. A. Gilfanov M. R. Krivonos R. A. Medvedev P. S. Meshcheryakov A. V. Sazonov S. Yu. Sunyaev R. A. Khorunzhev G. A. 《Astronomy Letters》2021,47(10):661-673
Astronomy Letters - Based on observations with the transient double-beam spectrograph (TDS) at the 2.5-m telescope of the Caucasus Mountain Observatory of SAI MSU, we have determined the redshifts... 相似文献
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R. A. Burenin A. L. Amvrosov M. V. Eselevich V. M. Grigor’ev V. A. Aref’ev V. S. Vorob’ev A. A. Lutovinov M. G. Revnivtsev S. Yu. Sazonov A. Yu. Tkachenko G. A. Khorunzhev A. L. Yaskovich M. N. Pavlinsky 《Astronomy Letters》2016,42(5):295-306
The capabilities of the new medium- and low-resolution spectrograph installed recently on the 1.6-m AZT-33IK telescope at the Sayan Observatory of the Institute of Solar–Terrestrial Physics to solve the problems of ground-based optical support for the future all-skyX-ray survey of the SRGobservatory are discussed. Results of the test observations of galaxy clusters, active galactic nuclei (AGNs) and quasars, and cataclysmic variables performed immediately after the installation of the spectrograph on the telescope are presented. The results of these observations show that the AZT-33IK telescope equipped with the new medium- and low-resolution spectrograph can provide a substantial fraction of the necessary optical observations in the program of ground-based optical support for the all-sky survey of the SRG observatory. 相似文献
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In astronomical observations at optical wavelengths, a fast image tracking system can be adopted to reduce the effects of the atmospheric seeing and telescopic tracking error, and therefore improve the observing efficiency. Aiming at the need of astronomical observations, totally 5 kinds of algorithms in two categories were selected to make a comparative study on their accuracies and stabilities under different noise conditions by both numerical experiment and laboratory test. The results indicate that the normalized cross-correlation method and barycenter method have not only a higher accuracy but also a better reliability against interferences, they will be applied to the high-resolution spectrograph of the Xinglong 2.16 m telescope and the scienti?c instruments of the SONG (Stellar Observations Network Group) project, respectively. 相似文献
9.
A. O. Grauzhanina G. G. Valyavin D. R. Gadelshin D. N. Baklanova S. I. Plachinda K. A. Antonyuk N. V. Pit G. A. Galazutdinov A. F. Valeev T. E. Burlakova A. F. Kholtygin 《Astrophysical Bulletin》2017,72(1):67-72
We present first results of spectroscopic observations of transiting exoplanets in the Special Astrophysical Observatory of the Russian Academy of Sciences with the Main Stellar Spectrograph of the 6-m BTA telescope. For the exoplanetWASP-32b, we detected a significant variation of intensity and equivalent width in the Hα spectral line of the parent star at the time of a transit. The equivalent width of the line during transit is by 8–10% larger than outside the planet passage. Residual intensity in the core of the line reveals the following tendency: the line is by 10–15% deeper inside transit than outside it. Observations with the long-slit spectrograph of the Crimean Astrophysical Observatory at the 2.6-m ZTSh telescope also showed a transit event in the Hα line, although, with a smaller amplitude and shape inverted in relation to the data from the 6-m telescope. While in the observations with the BTA the Hα line becomes deeper during the transit, in the ZTSh observations, the residual intensity of the Hα line decreases during the transit. Reducing and analysis of the archive data of WASP-32b observations with the HARPS spectrograph also confirm the Hα line modulation at the time of the transit. The observed data give evidence of the envelope in WASP-32b filling the Roche lobe and a comet-like tail of changing geometry and orientation relative to the observer. These changes determine different depths and shapes of the Hα spectral line at the time of transits. 相似文献
10.
The results of spectroscopic observations of the red dwarf flare star HU Del are given. The observations were made in August 2000 with the 2.6-m telescope of the Byurakan Observatory equipped with a Byu FOSC integral-field spectrograph. A rapid flare evidently occurred on HU Del. 相似文献
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本文概述1991年7月11日日全食时中国日食观测队在墨西哥LaPaz所作的近红外光谱观测情况及得到的初步结果。观测是用一强光力望远镜和一中小色散的光谱仪,配以CCD摄象机、图象处理器、微机等组成的探测系统进行的。日全食时,在λ10712-10972波区共摄得极上层光球和色球的无缝光谱41帧。日面外约1.096R处的有缝光谱35帧。文中还介绍了拍得的色球、日珥资料概况。 相似文献
13.
Jiang Shi-yang 《Chinese Astronomy and Astrophysics》1981,5(3):373-375
Because of the limitations both from the slit width and the slit length of the spectrograph used in high resolution work, the efficiency of a telescope, with an aperture between D0 = 9m and D′0 = 55m, will be no better than that of a telescope with aperture D0. D0 can be identified as the maximum aperture of a ground-based telescope. 相似文献
14.
Zhou Fan Ya-Fang Huang Jin-Zeng Li Xu Zhou Jun Ma Hong Wu Tian-Meng Zhang Yong-Heng Zhao National Astronomical Observatories Chinese Academy of Sciences Beijing China Key Laboratory of Optical Astronomy National Astronomical Observatories 《中国天文和天体物理学报》2011,(11)
We present spectroscopic observations for 11 confirmed globular clusters(GCs) of M31 with the OMR spectrograph on the 2.16 m telescope at the Xinglong site of National Astronomical Observatories,Chinese Academy of Sciences.Nine of our sample clusters are located in the halo of M31 and the most remote one is out to a projected radius of 78.75 kpc from the galactic center.For all our sample clusters,we measured the Lick absorption-line indices and radial velocities.It is noted that most GCs in our sample are ... 相似文献
15.
We report on the development of a fast crossed-dispersion spectrograph (CRAB) mounted at the Nasmyth focus of the 6-m telescope. The spectrograph is designed for visible and near-infrared (3800–10 500 Å) CCD observations with the spectral resolution R=4000. We give the basic parameters of the optical scheme and the parameters of the echelle frame. We determined the gain involved in putting the spectrograph into observational practice and discuss the possible range of spectroscopic problems for which the instrument is optimal. 相似文献
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Observations of the dwarf Irr galaxy IC 10 have been performed at the 6-m Special Astrophysical Observatory telescope with the SCORPIO focal reducer in the mode of a slit spectrograph. The ionized-gas emission spectrum in the region of intense current star formation has been investigated. The relative oxygen, N+, and S+ abundances in about twenty H II regions and the synchrotron superbubble have been estimated. The galaxy-averaged oxygen abundance is 12 + log(O/H) = 8.17 ± 0.35 and the metallicity is Z = 0.18 ± 0.14Z ⊙. The metallicity found by comparing diagnostic diagrams with photoionization models is shown to be less reliable than its estimate based on strong oxygen lines. 相似文献
18.
We present new results of our kinematic study of the supernova remnant S8 in the galaxy IC 1613. Based on our observations at the 6-m Special Astrophysical Observatory telescope with the two-dimensional MPFS spectrograph and the SCORPIO focal reducer in the mode of a scanning Fabry-Perot interferometer, we have determined the expansion velocity of the bright optical nebula. Analysis of the 21-cm VLA radio observations for the galaxy confirms our previously suggested model for a supernova explosion in a cavity surrounded by a dense HI shell and a collision of S8 with the shell wall. 相似文献
19.
《天文和天体物理学研究(英文版)》2016,(5)
We report the discovery of an isolated compact galaxy triplet SDSS J084843.45+164417.3, which is first detected by the LAMOST spectral survey and then confirmed by a spectroscopic observation of the BFOSC mounted on the 2.16 meter telescope located at Xinglong Station, which is administered by National Astronomical Observatories, Chinese Academy of Sciences. It is found that this triplet is an isolated and extremely compact system, which has an aligned configuration and very small radial velocity dispersion. The member galaxies have similar colors and show marginal star formation activities. These results support the opinion that the compact triplets are well-evolved systems rather than hierarchically forming structures. This serendipitous discovery reveals the limitations of fiber spectral redshift surveys in studying such a compact system, and demonstrates the necessity of additional observations to complete the current redshift sample. 相似文献
20.
Wei-Kang Zheng Jin-Song Deng Meng Zhai Li-Ping Xin Yu-Lei Qiu Jing Wang Xiao-Meng Lu Jian-Yan Wei Jing-Yao Hu 《中国天文和天体物理学报》2008,8(6)
A gamma-ray burst (GRB) optical photometric follow-up system at the Xinglong Observatory of National Astronomical Observatories of China (NAOC) has been constructed. It uses the 0.8-m Tsinghua-NAOC Telescope (TNT) and the 1-m EST telescope, and can au-tomatically respond to GRB Coordinates Network (GCN) alerts. Both telescopes slew rela-tively fast, being able to point to a new target field within ~ 1 min upon a request. Whenever available, the 2.16-m NAOC telescope is also used. In 2006 the system responded to 15 GRBs and detected seven early afterglows. In 2007 six GRBs have been detected among 18 follow-up observations. TNT observations of the second most distant GRB 060927 (z = 5.5) are shown, which started as early as 91 s after the GRB trigger. The afterglow was detected in the combined image of the first 19 × 20 s unfiltered exposures. This GRB follow-up system has joined the East-Asia GRB Follow-up Observation Network (EAFON). 相似文献