The correction of atmospheric dispersion in LAMOST

Atmospheric refraction and dispersion affect the observational quality and efficiency of the Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST). In this paper, by both ZEMAX simulation and numerical calculation, the atmospheric dispersion for LAMOST, which will be installed at the la...

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Published inChinese astronomy and astrophysics Vol. 30; no. 2; pp. 215 - 227
Main Authors Liu, Gen-rong, Yuan, Xiang-yan
Format Journal Article
LanguageEnglish
Published Elsevier B.V 01.04.2006
Subjects
atmospheric effect
telescope
atmospheric effect
telescope
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Abstract Atmospheric refraction and dispersion affect the observational quality and efficiency of the Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST). In this paper, by both ZEMAX simulation and numerical calculation, the atmospheric dispersion for LAMOST, which will be installed at the latitude 40°.4 and has a 20 m focal length and F5 focal ratio, are calculated for the 0.75 h before and after the transit time. Various types of dispersion prism to be used for correcting the atmospheric dispersion in LAMOST were calculated and analyzed, from which one was finally adopted. The secondary spectrum of the dispersion prism, the residual dispersion during tracking of the telescope and the installation errors of the dispersion prism are investigated.
AbstractList Atmospheric refraction and dispersion affect the observational quality and efficiency of the Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST). In this paper, by both ZEMAX simulation and numerical calculation, the atmospheric dispersion for LAMOST, which will be installed at the latitude 40 degree .4 and has a 20 m focal length and F5 focal ratio, are calculated for the 0.75 h before and after the transit time. Various types of dispersion prism to be used for correcting the atmospheric dispersion in LAMOST were calculated and analyzed, from which one was finally adopted. The secondary spectrum of the dispersion prism, the residual dispersion during tracking of the telescope and the installation errors of the dispersion prism are investigated.
Atmospheric refraction and dispersion affect the observational quality and efficiency of the Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST). In this paper, by both ZEMAX simulation and numerical calculation, the atmospheric dispersion for LAMOST, which will be installed at the latitude 40'.4 and has a 20 m focal length and F5 focal ratio, are calculated for the 0.75 h before and after the transit time. Various types of dispersion prism to be used for correcting the atmospheric dispersion in LAMOST were calculated and analyzed, from which one was finally adopted. The secondary spectrum of the dispersion prism, the residual dispersion during tracking of the telescope and the installation errors of the dispersion prism are investigated.
Atmospheric refraction and dispersion affect the observational quality and efficiency of the Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST). In this paper, by both ZEMAX simulation and numerical calculation, the atmospheric dispersion for LAMOST, which will be installed at the latitude 40°.4 and has a 20 m focal length and F5 focal ratio, are calculated for the 0.75 h before and after the transit time. Various types of dispersion prism to be used for correcting the atmospheric dispersion in LAMOST were calculated and analyzed, from which one was finally adopted. The secondary spectrum of the dispersion prism, the residual dispersion during tracking of the telescope and the installation errors of the dispersion prism are investigated.
Author Yuan, Xiang-yan
Liu, Gen-rong
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References Zhang, Jiang (bib5) 2002; 29
Shou-guan, Ding-giang, Yao-quan (bib4) 1996; 35
Wang, Su (bib9) 1990; 232
Su, Cao, Liang (bib6) 1986; 628
Doodrovski (bib7) 1958
Zhang (bib2) 2004.02.12
Zhang, Hu (bib3) 1997; 17
Su, Wang (bib1) 1997; 17
Su (bib8) 1986; 156
Zhang (10.1016/j.chinastron.2006.04.009_bib2) 20040212
Doodrovski (10.1016/j.chinastron.2006.04.009_bib7) 1958
Su (10.1016/j.chinastron.2006.04.009_bib6) 1986; 628
Su (10.1016/j.chinastron.2006.04.009_bib1) 1997; 17
Shou-guan (10.1016/j.chinastron.2006.04.009_bib4) 1996; 35
Zhang (10.1016/j.chinastron.2006.04.009_bib5) 2002; 29
Wang (10.1016/j.chinastron.2006.04.009_bib9) 1990; 232
Zhang (10.1016/j.chinastron.2006.04.009_bib3) 1997; 17
Su (10.1016/j.chinastron.2006.04.009_bib8) 1986; 156
References_xml – year: 1958
  ident: bib7
  article-title: Theory of Optical Instruments
  contributor:
    fullname: Doodrovski
– volume: 156
  start-page: 381
  year: 1986
  ident: bib8
  publication-title: A&A
  contributor:
    fullname: Su
– volume: 17
  start-page: 213
  year: 1997
  ident: bib3
  publication-title: Acta Astrophy. Sinica
  contributor:
    fullname: Hu
– volume: 29
  start-page: 1
  year: 2002
  ident: bib5
  publication-title: Optical-electronic Engineering
  contributor:
    fullname: Jiang
– volume: 232
  start-page: 589
  year: 1990
  ident: bib9
  publication-title: A&A
  contributor:
    fullname: Su
– year: 2004.02.12
  ident: bib2
  publication-title: Technical Report of LAMOST, LAMOST-TR-BAO-L8-006
  contributor:
    fullname: Zhang
– volume: 628
  start-page: 498
  year: 1986
  ident: bib6
  publication-title: SPIE
  contributor:
    fullname: Liang
– volume: 35
  start-page: 5155
  year: 1996
  ident: bib4
  publication-title: Appl. Opt.
  contributor:
    fullname: Yao-quan
– volume: 17
  start-page: 202
  year: 1997
  ident: bib1
  publication-title: Acta Astrophy. Sinica
  contributor:
    fullname: Wang
– volume: 35
  start-page: 5155
  year: 1996
  ident: 10.1016/j.chinastron.2006.04.009_bib4
  publication-title: Appl. Opt.
  doi: 10.1364/AO.35.005155
  contributor:
    fullname: Shou-guan
– year: 20040212
  ident: 10.1016/j.chinastron.2006.04.009_bib2
  publication-title: Technical Report of LAMOST, LAMOST-TR-BAO-L8-006
  contributor:
    fullname: Zhang
– volume: 17
  start-page: 213
  year: 1997
  ident: 10.1016/j.chinastron.2006.04.009_bib3
  publication-title: Acta Astrophy. Sinica
  contributor:
    fullname: Zhang
– volume: 17
  start-page: 202
  year: 1997
  ident: 10.1016/j.chinastron.2006.04.009_bib1
  publication-title: Acta Astrophy. Sinica
  contributor:
    fullname: Su
– volume: 29
  start-page: 1
  year: 2002
  ident: 10.1016/j.chinastron.2006.04.009_bib5
  publication-title: Optical-electronic Engineering
  contributor:
    fullname: Zhang
– volume: 628
  start-page: 498
  year: 1986
  ident: 10.1016/j.chinastron.2006.04.009_bib6
  publication-title: SPIE
  doi: 10.1117/12.963571
  contributor:
    fullname: Su
– volume: 232
  start-page: 589
  year: 1990
  ident: 10.1016/j.chinastron.2006.04.009_bib9
  publication-title: A&A
  contributor:
    fullname: Wang
– year: 1958
  ident: 10.1016/j.chinastron.2006.04.009_bib7
  contributor:
    fullname: Doodrovski
– volume: 156
  start-page: 381
  year: 1986
  ident: 10.1016/j.chinastron.2006.04.009_bib8
  publication-title: A&A
  contributor:
    fullname: Su
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SubjectTerms atmospheric effect
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Title The correction of atmospheric dispersion in LAMOST
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