1.2-m @ PRL

The 1.2-m telescope was designed and built indigenously by the SHAR Center of ISRO.
The telescope is on a fork mounted equatorially. All the original electronics has been
replaced by PRL's engineers in recent times and the current version of the electronics
and control/drive system is controlled by a Linux PC. The software is also developed
in house. Apart from normal 'sidereal' tracking, it is also possible to have non sidereal
rate tracking for observing fast moving objects like comets and asteroids.
The telescope is operational since December 1994.
(website)
Location Details
Location | Mount Abu Observatory (Gurushikhar, Mount Abu, India) |
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Coordinates | 24°39′17.34″N 72°46′45.18″E |
Altitude | 1680m |
Type | Optical fork-equatorial mount |
Size | 1.2m |
Operated by | PRL (Mount Abu Observatory, India) |
Instruments | PARAS, MFOSC-P, NICS, LNC CCD camera, EMPOL, LISA, PRLPOL |
PRL Advanced Radial velocity All Sky Search (PARAS)
- type: echelle spectrograph
- spectral coverage: 3800–9500 Å
- peak effiency: 5000-6500 Å
- spectral resolution: R∼67,000
- camera: CCD
Mt. Abu Faint Object Spectrograph and Camera – Pathfinder (MFOSC-P)
- detector: 1K×1K pixels CCD Camera
- pixel size: 13micron
- Field-of-view: 5.2×5.2 square arcmin
- Filters (broad): Bessell's B,V,R,I
- filter (narrow): H-alpha
Near Infrared Camera/Spectrograph (NICS)
- detector: 1K×1K pixels (HAWAI-1 from teledyne)
- pixel scale: 0.5 arcsec/pixel
- Field-of-view: 8×8 square arcmin
- Filter wheel 1 : Open, Y, J, H, K, Ks, (Barr-new MKO)
- filter wheel 2 : Open, IJ, JH, HK, NB1(Brγ), NB2(H2 1-OS(1))
Liquid Nitrogen cooled CCD Camera (LNC CCD)
- Array format: 1296 x 1152 pixels
- pixel size: 22 micron
- Pixel Scale: 0.29 arcsec/pixel
- Field-of-view: 6.5 x 5.5 square arcmin
- Filters (broad): U, B, V, R, I (Johnson-Cousins filter set)
- filter (narrow): Hale-Bopp comet filter set
EMCCD based Optical Imaging Polarimeter (EMPOL)
- detector: 1Kx1K Andor iXon
- Field-of-view: 3 x 3 square arcmin
- Filters: B, V, R, I (Johnson-Cousins filter set) ; SDSS (g, r, i, z) filters, and (blue, green, red) continuum filters.
Low Resolution Spectroscope (LISA)
- spectral resolution: R∼1,000
- wavelength range: 380 nm to 690 nm
- platescale: 0.326 arcsec/pixel