Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Anantha Chanumolu"'
Autor:
Yannig Durand, Grégory Bazalgette Courrèges-Lacoste, Charlotte Pachot, Arnaud Pasquet, Anantha Chanumolu, Yasjka Meijer, Valérie Fernandez, Stefan Lesschaeve, David Spilling, Antoine Dussaux, Denis Serre, Frank te Hennepe
Publikováno v:
Sensors, Systems, and Next-Generation Satellites XXVI.
Autor:
Jos Dingjan, Cristina V. Fernandez, Aaldert van Amerongen, Jochen Campo, Jeroen Rietjens, Martijn Smit, Anantha Chanumolu, Raj Nalla, Otto Hasekamp
Publikováno v:
Polarization Science and Remote Sensing IX.
SPEXone is a compact five–angle spectropolarimeter that is being developed as a contributed payload for the NASA Plankton, Aerosol, Cloud and ocean Ecosystem (PACE) observatory, to be launched in 2022. SPEXone will provide accurate atmospheric aero
Autor:
Anantha Chanumolu, Damien Jones, Deon Grobler, Sunetra Giridhar, Sivarani Thirupathi, Robert Jakobsson
Publikováno v:
Experimental Astronomy. 43:39-58
As a continuation to the published work on model based calibration technique with HESP(Hanle Echelle Spectrograph) as a case study, in this paper we present the performance results of the technique. We also describe how the open parameters were chose
Autor:
Angchuk Dorje, Sunetra Giridhar, Amit Kumar, Deon Grobler, M. N. Anand, S. Sriram, S. Kathiravan, Damien Jones, Arun Surya, Tsewang Dorje, Athira Unni, Thirupathi Sivarani, Robert Jakobsson, Tsewang Gyalson, Anantha Chanumolu
Publikováno v:
Ground-based and Airborne Instrumentation for Astronomy VII.
Hanle echelle spectrograph (HESP) is a high resolution, bench mounted, fiber-fed spectrograph at visible wavelengths. The instrument was recently installed at the 2m Himalayan Chandra Telescope (HCT), located at Indian Astronomical Observatory (IAO),
Publikováno v:
Experimental Astronomy. 39:423-443
We present a modelling scheme that predicts the centroids of spectral line features for a high resolution Echelle spectrograph to a high accuracy. Towards this, a computing scheme is used, whereby any astronomical spectrograph can be modelled and con