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20212026
most citedMultiplicity of Galactic Cepheids from long-baseline interferometry V. High-accuracy orbital parallax and mass of SU Cygni

6 citations · 17 across the 19 of their papers we have counts for

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Showing 2022Show all

5 papers · 1 filter

astro-ph.IM2022

Gaussian phase autocorrelation as an accurate compensator for FFT-based atmospheric phase screen simulations

Sorabh Chhabra, Jyotirmay Paul, A. N. Ramaprakash +1

Accurately simulating the atmospheric turbulence behaviour is always challenging. The well-known FFT based method falls short in correctly predicting both the low and high frequenc…

astro-ph.IM2022

Speckle simulation tool for automated modelling of a large range of telescope aperture to fried parameter ratios

Sorabh Chhabra, Abhay A. Kohok, Bhushan S. Joshi +3

The Speckle Imager via MUlti Layer Atmospheric Turbulence Object Reconstructor (SIMULATOR) is a lab-based testbed instrument developed to test for speckle correlation-based techniq…

astro-ph.IM2022★ 2 cited

Spectrograph design for the Asgard/BIFROST spectro-interferometric instrument for the VLTI

Sorabh Chhabra, Michele Frangiamore, Stefan Kraus +4

The BIFROST instrument will be the first VLTI instrument optimised for high spectral resolution up to R=25,000 and operate between 1.05 and 1.7 m. A key component of the instrum…

astro-ph.IM2022★ 1 cited

Beam combiner for the Asgard/BIFROST instrument

Daniel J. Mortimer, Sorabh Chhabra, Stefan Kraus +4

BIFROST will be a short-wavelength ( = 1.0 - 1.7m) beam combiner for the VLT Interferometer, combining both high spatial (/2B = 0.8 mas) and spectral (up to R = 25,000) re…

astro-ph.IM2022★ 2 cited

High spectral-resolution interferometry down to 1 micron with Asgard/BIFROST at VLTI: Science drivers and project overview

Stefan Kraus, Daniel Mortimer, Sorabh Chhabra +10

We present science cases and instrument design considerations for the BIFROST instrument that will open the short-wavelength (Y/J/H-band), high spectral dispersion (up to R=25,000)…