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PLATO’s signal and noise budget
ESA’s PLATO mission aims the detection and characterization of terrestrial planets around solar-type stars as well as the study of host star...
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Characterization of the eXTP-LAD collimators
The enhanced X-ray Timing and Polarimetry mission (eXTP) is a next-generation flagship X-ray astronomy satellite currently in phase-B study. The...
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Spectral and timing calibration of eXTP-SFA engineering model in 100XF
The spectroscopy focusing array is one of the four main scientific instruments of the enhanced X-ray Timing and Polarimetry mission, tasked with...
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SunbYte: an autonomous pointing framework for low-cost robotic solar telescopes on high altitude balloons
The design and usability of a fully autonomous robotic control system (SunbYte - Sheffield University Balloon “lYfted” TElescope) for solar tracking...
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Simulation of the in-flight background and performance of DRO/GTM
As a new member of the high energy astronomical transient monitoring network, Gamma-ray Transient Monitor (GTM) is an all-sky monitor onboard the...
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A study of cosmic microwave background using non-extensive statistics
The cosmic microwave background (CMB) radiation, the relic afterglow of the Big Bang, has become one of the most useful and precise tools in modern...
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Daksha: on alert for high energy transients
We present Daksha , a proposed high energy transients mission for the study of electromagnetic counterparts of gravitational wave sources, and gamma...
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Science with the Daksha high energy transients mission
We present the science case for the proposed Daksha high energy transients mission. Daksha will comprise of two satellites covering the entire sky...
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The proposed plan of geodetic VLBI in India serving national and global objectives
Project “Saptarshi” was initiated by the National Centre for Geodesy, Indian Institute of Technology Kanpur to set up the modern space geodetic...
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Research and establishment of the X-ray monochromator at the 100XF
The 100-m X-ray Test Facility (100XF) was developed according to the calibration requirement of the first X-ray astronomical satellite Insight -HXMT...
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DSRL: A low-resolution stellar spectral of LAMOST automatic classification method based on discrete wavelet transform and deep learning methods
Automatic classification of stellar spectra contributes to the study of the structure and evolution of the Milky Way and star formation. Currently...
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Life cycle assessment of the Athena X-ray integral field unit
The X-ray Integral Field Unit (X-IFU) is the high-resolution X-ray spectrometer to fly on board the Athena Space Observatory of the European Space...
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Spectroscopic Investigation of Nebular Gas (SING): instrument design, assembly and calibration
The Spectroscopic Investigation of Nebular Gas (SING) is a near-ultraviolet (NUV) low-resolution spectrograph payload designed to operate in the NUV...
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The discovery space of ELT-ANDES. Stars and stellar populations
The ArmazoNes high Dispersion Echelle Spectrograph (ANDES) is the optical and near-infrared high-resolution echelle spectrograph envisioned for the...
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The first cut is the cheapest: optimizing Athena/X-IFU-like TES detectors resolution by filter truncation
The X-ray Integral Field Unit (X-IFU) instrument on the future ESA mission Athena X-ray Observatory is a cryogenic micro-calorimeter array of...
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Forward modelling low-spectral-resolution Cassini/CIRS observations of Titan
The Composite InfraRed Spectrometer (CIRS) instrument onboard the Cassini spacecraft performed 8.4 million spectral observations of Titan at...
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Outdoor fibre link between two telescopes and the lab of the CHARA array at 810 nm. Demonstration of the optical path servo control
In the framework of the ALOHA (Astronomical Light Optical Hybrid Analysis) project, dedicated to high resolution imaging in the L-band using optical...
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How many random observations are needed for good phase coverage of a periodic source?
The specific problem considered is the number of radial velocity measurements required to obtain good estimates of physical parameters of binary...
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Modeling the effects of power efficient approximate multipliers in radio astronomy correlators
Large scale Radio Telescopes for Radio Astronomy highly depend on the availability of large (digital) processing capacities for imaging. Estimates...
