Skip to main content
Log in

Indian spectroscopic and imaging space telescope (INSIST): An optics design trade-off study

  • Published:
Journal of Astrophysics and Astronomy Aims and scope Submit manuscript

Abstract

Large ground and space-based surveys in optical and near-infrared (NIR) wavelengths will revolutionize astronomy in the coming decade. Unfortunately, no ultraviolet (UV) facilities are planned to complement these surveys, which is crucial for studying the most active phase of the Universe that includes star formation in galaxies, active galactic nuclei (AGN), galaxy clusters, etc. A dedicated UV mission, the Indian Spectroscopic and Imaging Space Telescope (INSIST), is proposed to observe the UV sky. The compelling science objectives defined a set of high-level mission requirements. According to which, the INSIST is to have a wide field-of-view (\(\textrm{FoV} \approx 0.25\) square degree) comparable to India’s Ultraviolet Imaging Telescope (UVIT) and about two orders of magnitude larger than that of the Hubble Space Telescope, simultaneous imaging of the FoV in UV (150–300 nm), u (300–400 nm) and g (400–550 nm) bands, a Multi-Object-Slit medium resolution spectroscopy in a narrow FoV in UV and a simultaneous slitless spectroscopic capability in UV and u bands. To achieve these requirements, several optical design configurations were explored. Here, we present an optical design trade study conducted on various optical design configurations to achieve a sensitivity limit of \(m_{\textrm{AB}}> 26\) mag, in the UV band and a spatial resolution better than 0.2\(^{\prime \prime }\), using a 1-m size telescope aperture. We also present results from our fabrication and alignment tolerance analysis of the selected optical designs, and the design performance that meets the design requirements. Critical parameters like the encircled energy concentration, point spread function (its stability over the field), effects of the spiders supporting the secondary, etc., are explored during the design phase. Based on the trade study conducted in reference to various performance matrices, we down-selected the most optimal optical design for the INSIST.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Fig. 1
Fig. 2
Fig. 3
Fig. 4
Fig. 5
Fig. 6
Fig. 7
Fig. 8
Fig. 9
Fig. 10
Fig. 11
Fig. 12
Fig. 13
Fig. 14
Fig. 15
Fig. 16
Fig. 17
Fig. 18
Fig. 19
Fig. 20
Fig. 21
Fig. 22

Similar content being viewed by others

References

  • Abell P. A., Allison J., Anderson S. F., et al. 2009, 0912.0201

  • Agrawal P. C. 2005, ICRC, 4, 171

    Google Scholar 

  • Alsing J., Kirk D., Heavens A., Jaffe A. H. 2015, MNRAS, 452, 1202

    Article  ADS  Google Scholar 

  • Amara A., Refrégier A. 2007, MNRAS, 381, 1018

    Article  ADS  Google Scholar 

  • Amiaux J., Scaramella R., Mellier Y., et al. 2012, SPIE, 8442, 84420Z

    Google Scholar 

  • Appenzeller I., Wolf B. 1979, A &A, 75, 164

    ADS  Google Scholar 

  • Barstow M. A., WSO Team 2003, ASIB, 105, 407

  • Bertaux J.-L., Leblanc F., Witasse O., et al. 2005, Nature, 435, 790

    Article  ADS  Google Scholar 

  • Campbell M. A., Evans C. J., Mackey A. D., et al. 2010, MNRAS, 405, 421

    ADS  Google Scholar 

  • Cook L. G. 1979, SPIE, 183, 207

    ADS  Google Scholar 

  • Crowther P. A., Caballero-Nieves S. M., Bostroem K. A., et al. 2016, MNRAS, 458, 624

    Article  ADS  Google Scholar 

  • Cuzzi J., Clark R., Filacchione G., et al. 2009, Ring Particle Composition and Size Distribution, eds Dougherty M. K., Esposito L. W., Krimigis S. M., 459

  • Cuzzi J. N., French R. G., Hendrix A. R., et al. 2018, Icarus, 309, 363

    Article  ADS  Google Scholar 

  • Cuzzi J. N., Burns J. A., Charnoz S., et al. 2010, Science, 327, 1470

    Article  ADS  Google Scholar 

  • Cypriano E. S., Amara A., Voigt L. M., et al. 2010, MNRAS, 405, 494

    ADS  Google Scholar 

  • de Vries W. H., Olivier S. S., Asztalos S. J., Rosenberg L. J., Baker K. L. 2007, ApJ, 662, 744

    Article  ADS  Google Scholar 

  • Dolphin A. E. 2016, ApJ, 825, 153

    Article  ADS  Google Scholar 

  • Ercolano B., Pascucci I. 2017, Royal Society Open Science, 4, 170114

    Article  ADS  MathSciNet  Google Scholar 

  • Gardner J. P. 2006, in The Scientific Requirements for Extremely Large Telescopes, eds Whitelock P., Dennefeld M., Leibundgut B., Vol. 232, 87

  • Gentile M., Courbin F., Meylan G. 2013, A &A, 549, A1

    Google Scholar 

  • George K., Poggianti B. M., Bellhouse C. 2019, MNRAS, 487, 3102

    Article  ADS  Google Scholar 

  • Ghosh S. K., Joseph P., Kumar A., et al. 2021, JoAA, 42, 20

    Google Scholar 

  • Gillis B. R., Schrabback T., Marggraf O., et al. 2020, MNRAS, 496, 5017

    Article  ADS  Google Scholar 

  • Grodent D., Bonfond B., Yao Z., et al. 2018, Journal of Geophysical Research (Space Physics), 123, 3299

    Article  ADS  Google Scholar 

  • Guo R. L., Yao Z. H., Grodent D., et al. 2021, Geophys. Res. Lett., 48, e93964

    ADS  Google Scholar 

  • Harvey J. E., Ftaclas C. 1995, ApOpt, 34, 6337

    ADS  Google Scholar 

  • Heymans C., Van Waerbeke L., Bacon D., et al. 2006, MNRAS, 368, 1323

    Article  ADS  Google Scholar 

  • Hodge P. 1989, ARA &A, 27, 139

    ADS  Google Scholar 

  • Hunter D. A., Vacca W. D., Massey P., Lynds R., O’Neil E. J. 1997, AJ, 113, 1691

  • Ivezic Z., Axelrod T., Brandt W. N., et al. 2008, SerAJ, 176, 1

  • Jadhav V. V., Sindhu N., Subramaniam A. 2019, ApJ, 886, 13

    Article  ADS  Google Scholar 

  • Jarvis M., Sheldon E., Zuntz J., et al. 2016, MNRAS, 460, 2245

    Article  ADS  Google Scholar 

  • Jarvis M., Bernstein G. M., Amon A., et al. 2021, MNRAS, 501, 1282

    Article  ADS  Google Scholar 

  • Jee M. J., Tyson J. A. 2011, PASP, 123, 596

    Article  ADS  Google Scholar 

  • Johns-Krull C. M. 2007, ApJ, 664, 975

    Article  ADS  Google Scholar 

  • Koenigl A. 1991, ApJ, 370, L39

    Article  ADS  Google Scholar 

  • Korsch D. 1980, ApOpt, 19, 3640

    ADS  Google Scholar 

  • Kuhn J. R., Hawley S. L. 1999, PASP, 111, 601

    Article  ADS  Google Scholar 

  • Laureijs R., Amiaux J., Arduini S., et al. 2011, 1110.3193

  • Leahy D. A., Postma J., Chen Y., Buick M. 2020, ApJS, 247, 47

    Article  ADS  Google Scholar 

  • Leahy D. A., Postma J., Buick M., et al. 2021, JoAA, 42, 84

    Google Scholar 

  • Lothringer Joshua D., Fu Guangwei, Sing David K., Barman Travis S., 2020, ApJ, 898, 14L

  • Mandelbaum R. 2006, PhD thesis, Princeton University

  • Mandelbaum R., Hirata C.-M., Ishak M., Seljak U., Brinkmann J. 2006, MNRAS, 367, 611

    Article  ADS  Google Scholar 

  • Mandelbaum R. 2018, ARA &A, 56, 393

    ADS  Google Scholar 

  • Martin C., GALEX Science Team 2003, AAS, 203, 96.01

  • Mondal C., Subramaniam A., George K. 2018, AJ, 156, 109

  • Morrissey P., Conrow T., Barlow T. A., et al. 2007, ApJS, 173, 682

    Article  ADS  Google Scholar 

  • O’Connell J. S., Dodge W. R., Lightbody J. W., et al. 1987, PhRvC, 35, 1063

    ADS  Google Scholar 

  • Portegies Zwart S. F., McMillan S. L. W., Gieles M. 2010, ARA &A, 48, 431

    ADS  Google Scholar 

  • Rao N., Kameswara, De Marco O., et al. 2018, A &A, 620, 138

  • Roth L., Saur J., Retherford K. D., et al. 2014, Science, 343, 171

    Article  ADS  Google Scholar 

  • Rowe B. 2010, MNRAS, 404, 350

    ADS  Google Scholar 

  • Sachkov M., Gómez de Castro A. I., Shustov B. 2020, SPIE, 11444E, 73

  • Saha K., Tandon S. N., Simmonds C., et al. 2020, Nature Astronomy, 4, 1185

    Article  ADS  Google Scholar 

  • Schneider P. 1996, MNRAS, 283, 837

    Article  ADS  Google Scholar 

  • Schroeder D. J. 1987, sdap.book

  • Shu F. H., Adams F. C., Lizano S. 1987, ARA &A, 25, 23

  • Sindhu N., Subramaniam A., Jadhav V. V., et al. 2019, ApJ, 882, 43

    Article  ADS  Google Scholar 

  • Sindhu N., Subramaniam A., Geller A. M., et al. 2020, IAUS, 351, 482

    ADS  Google Scholar 

  • Sing D. K., Lecavelier des Etangs A., Fortney J. J., et al. 2013, MNRAS, 436, 2956

  • Sparks W. B., Hand K. P., McGrath M. A., et al. 2016, ApJ, 829, 121

    Article  ADS  Google Scholar 

  • Spergel D., Gehrels N., Baltay C., et al. 2015, arXiv: 1503.03757

  • Stewart A. I., Anderson D. E., Esposito L. W., Barth C. A. 1979, Science, 203, 777

    Article  ADS  Google Scholar 

  • Subramaniam A., Tandon S. N., Hutchings J., et al. 2016, SPIE, 9905, 99051F

    Google Scholar 

  • Swithenbank-Harris B. G., Nichols J. D., Allegrini F., et al. 2021, Journal of Geophysical Research (Space Physics), 126, e28717

    ADS  Google Scholar 

  • Tandon S. N., Subramaniam A., Girish V., et al. 2017, AJ, 154, 128

  • Tandon S. N., Postma J., Joseph P., et al. 2020, AJ, 159, 158

  • Terebizh V. Y. 2011, AN, 332, 714

  • Terebizh V. Y. 2016, AJ, 152, 121

  • Vidal-Madjar A., Lecavelier des Etangs A., Desert J. M., et al. 2003, Nature, 422, 143

  • Weisz D. R., Dolphin A. E., Skillman E. D. et al. 2014, ApJ 789, 147

  • Williams B. F., Lang D., Dalcanton J. J., et al. 2014, ApJS, 215, 9

    Article  ADS  Google Scholar 

  • Wilson R. N. 1996, rtob.book, 233

  • Wittman D. M., Tyson J. A., Kirkman D., Dell’Antonio I., Bernstein G. 2000, Nature, 405, 143

Download references

Acknowledgements

We thank the referee for providing constructive comments that have helped us in improving the work significantly. We gratefully acknowledge the support provided by the INSIST technical and science team. We also thank J. Pazder, Herzberg Astronomy and Astrophysics, for the useful discussions, suggestions and support given during this work. Also, we acknowledge ISRO for providing seed funding for the INSIST mission.

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to S. Sriram.

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Sriram, S., Valsan, V., Subramaniam, A. et al. Indian spectroscopic and imaging space telescope (INSIST): An optics design trade-off study. J Astrophys Astron 44, 55 (2023). https://doi.org/10.1007/s12036-023-09934-y

Download citation

  • Received:

  • Accepted:

  • Published:

  • DOI: https://doi.org/10.1007/s12036-023-09934-y

Keywords

Navigation