dc.contributor.author |
Anupama, G. C |
|
dc.contributor.author |
Maheswar, G |
|
dc.contributor.author |
Sriram, S |
|
dc.contributor.author |
Sivarani, T |
|
dc.contributor.author |
Parihar, P. S |
|
dc.contributor.author |
Nagabhushana, S |
|
dc.contributor.author |
Angchuk, D |
|
dc.contributor.author |
Barway, Sudhanshu |
|
dc.contributor.author |
Bhatt, B. C |
|
dc.contributor.author |
Banyal, R. K |
|
dc.contributor.author |
Basheer, Alikhan |
|
dc.contributor.author |
Prasanna, Deshmukh |
|
dc.contributor.author |
Divakar, D. K |
|
dc.contributor.author |
Dorjai, T |
|
dc.contributor.author |
Goswami, A |
|
dc.contributor.author |
Govinda, K. V |
|
dc.contributor.author |
Jorphail, S |
|
dc.contributor.author |
Kamath, U. S |
|
dc.contributor.author |
Kemkar, P. M. M |
|
dc.contributor.author |
Mahay, T. T |
|
dc.contributor.author |
Muneer, S |
|
dc.contributor.author |
Muthumariappan, C |
|
dc.contributor.author |
Shantikumar, N. S |
|
dc.contributor.author |
Pandey, G |
|
dc.contributor.author |
Reddy, B. E |
|
dc.contributor.author |
Sahu, D. K |
|
dc.contributor.author |
Sandeep, D. S |
|
dc.contributor.author |
Ramya, S |
|
dc.contributor.author |
Stalin, C. S |
|
dc.contributor.author |
Subramanian, S |
|
dc.contributor.author |
Tsewang, Stanzin |
|
dc.contributor.author |
Subramaniam, A |
|
dc.date.accessioned |
2022-08-24T05:23:20Z |
|
dc.date.available |
2022-08-24T05:23:20Z |
|
dc.date.issued |
2022-06 |
|
dc.identifier.citation |
Journal of Astrophysics and Astronomy, Vol. 43, No. 1, 32 |
en_US |
dc.identifier.issn |
0973-7758 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/8021 |
|
dc.description |
Restricted Access |
en_US |
dc.description |
The original publication is available at springerlink.com |
|
dc.description.abstract |
An observatory class national large optical-IR telescope (NLOT), is proposed to be built and
located in the country. The telescope consists of a 10–12 m segmented primary. In order to cater to a
diversity of observational programs, the telescope is designed with high throughput in both the optical and IR
regions (0.3–5 μm). It should perform reasonably well up to 30 μm. The telescope and instruments should
have remote operations capability, allowing for the queue as well as classical scheduling and high reliability
and robustness. This article provides a brief description of the science cases that drive the telescope
requirements, activities related to optics design and some thoughts on the instruments. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Indian Academy of Science |
en_US |
dc.relation.uri |
https://doi.org/10.1007/s12036-022-09819-6 |
|
dc.rights |
© Indian Academy of Sciences |
|
dc.subject |
General: Optical-infrared astronomy |
en_US |
dc.subject |
Instrumentation: segmented mirror telescopes |
en_US |
dc.subject |
Telescope optics design |
en_US |
dc.subject |
Astronomical instruments |
en_US |
dc.title |
A 10-m class national large optical-IR telescope |
en_US |
dc.type |
Article |
en_US |