Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/6808
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Sharma, T. K | - |
dc.contributor.author | Parihar, P. S | - |
dc.contributor.author | Banyal, R. K | - |
dc.contributor.author | Ahmad Dar, Ajaz | - |
dc.contributor.author | Kemkar, P. M. M | - |
dc.contributor.author | Stanzin, U | - |
dc.contributor.author | Anupama, G. C | - |
dc.date.accessioned | 2020-11-10T13:55:49Z | - |
dc.date.available | 2020-11-10T13:55:49Z | - |
dc.date.issued | 2017-08 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society, Vol. 470, No. 1, pp. 1091–1100 | en_US |
dc.identifier.issn | 1365-2966 | - |
dc.identifier.uri | http://prints.iiap.res.in/handle/2248/6808 | - |
dc.description | Restricted Access © Royal Astronomical Society https://doi.org/10.1093/mnras/stx1259 | en_US |
dc.description.abstract | We have developed a simple and portable device that makes precise and automated measurements of night sky extinction. Our instrument uses a commercially available telephoto lens for light collection, which is retrofitted to a custom-built telescope mount, a thermoelectrically cooled CCD for imaging, and a compact enclosure with electronic control to facilitate remote observations. The instrument is also capable of measuring the sky brightness and detecting the presence of thin clouds that otherwise would remain unnoticed. The measurements of sky brightness made by our simple device are more accurate than those made using a large telescope. Another capability of the device is that it can provide an instantaneous measurement of atmospheric extinction, which is extremely useful for exploring the nature of short-term extinction variation. The instrument was designed and developed primarily in order to characterize and investigate thoroughly the Indian Astronomical Observatory (IAO), Hanle for the establishment of India’s future large-telescope project. The device was installed at the IAO, Hanle in 2014 May. In this paper, we present he instrument details and discuss the results of extinction data collected for about 250 nights. | en_US |
dc.language.iso | en | en_US |
dc.publisher | Oxford University Press on behalf of the Royal Astronomical Society | en_US |
dc.subject | Atmospheric effects | en_US |
dc.subject | Instrumentation: photometers | en_US |
dc.subject | Site testing | en_US |
dc.subject | Telescopes | en_US |
dc.title | An automated extinction and sky brightness monitor for the Indian Astronomical Observatory, Hanle | en_US |
dc.type | Article | en_US |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
An automated extinction and sky brightness monitor for the Indian Astronomical Observatory, Hanle.pdf Restricted Access | Restricted Access | 1.29 MB | Adobe PDF | View/Open Request a copy |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.