D. M. Akhmetov, E. R. Muslimov, D. Yu. Kharitonov, E. G. Ibatullin, N. K. Pavlycheva
{"title":"A Prototype Slitless Spectrograph with a Composite Grism","authors":"D. M. Akhmetov, E. R. Muslimov, D. Yu. Kharitonov, E. G. Ibatullin, N. K. Pavlycheva","doi":"10.1134/S1990341324600790","DOIUrl":null,"url":null,"abstract":"<p>We report the results of laboratory studies of the main optical properties of the slitless spectrograph developed for a small telescope with a 0.5 m-diameter primary mirror and a focal ratio of <span>\\(1:6.8\\)</span>. The spectrograph operates in the 450–950 nm wavelength interval and has a field of <span>\\(35\\overset{\\prime}{.}6\\times 7\\overset{\\prime}{.}2\\)</span>. Its distinctive feature is the use of a composite grism subdivided into two subapertures with independently optimized parameters. Measurements show that the use of such a grism makes it possible to achieve a spectral resolving power <span>\\(R\\)</span> from 461 to 1041 with the grating diffraction efficiency as high as 45<span>\\(\\%\\)</span>. We demonstrate that our solution provides better optical characteristics compared to the classical grism and that our measurements agree well with the results of modeling.</p>","PeriodicalId":478,"journal":{"name":"Astrophysical Bulletin","volume":"79 3","pages":"525 - 534"},"PeriodicalIF":1.3000,"publicationDate":"2024-11-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astrophysical Bulletin","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1134/S1990341324600790","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
We report the results of laboratory studies of the main optical properties of the slitless spectrograph developed for a small telescope with a 0.5 m-diameter primary mirror and a focal ratio of \(1:6.8\). The spectrograph operates in the 450–950 nm wavelength interval and has a field of \(35\overset{\prime}{.}6\times 7\overset{\prime}{.}2\). Its distinctive feature is the use of a composite grism subdivided into two subapertures with independently optimized parameters. Measurements show that the use of such a grism makes it possible to achieve a spectral resolving power \(R\) from 461 to 1041 with the grating diffraction efficiency as high as 45\(\%\). We demonstrate that our solution provides better optical characteristics compared to the classical grism and that our measurements agree well with the results of modeling.
期刊介绍:
Astrophysical Bulletin is an international peer reviewed journal that publishes the results of original research in various areas of modern astronomy and astrophysics, including observational and theoretical astrophysics, physics of the Sun, radio astronomy, stellar astronomy, extragalactic astronomy, cosmology, and astronomy methods and instrumentation.