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Performance of the polarization leakage correction in the PILOT data
The Polarized Instrument for Long-wavelength Observation of the Tenuous interstellar medium ( PILOT ) is a balloon-borne experiment that aims to...
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Design and testing of the Optics for FXT onboard EP satellite
The Einstein Probe (EP) mission is a science mission designed for the time domain astronomy, which is approved by the Chinese Academy of Sciences...
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The structural design and thermo-mechanical performance of the FXT for the EP mission
The Follow-up X-ray Telescope (FXT) is one of the key payloads onboard EP. It is a Wolter-I type X-ray focusing telescope equipped with two telescope...
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The scientific performance of the microchannel X-ray telescope on board the SVOM mission
The Microchannel X-ray Telescope (MXT) will be the first focusing X-ray telescope based on a narrow field “Lobster-Eye” optical design to be flown on...
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Ultra-low-frequency radio astronomy observations from a Seleno-centric orbit
This paper introduces the first results of observations with the Ultra-Long-Wavelength (ULW) —- Low Frequency Interferometer and Spectrometer (LFIS)...
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The Athena X-ray Integral Field Unit: a consolidated design for the system requirement review of the preliminary definition phase
The Athena X-ray Integral Unit (X-IFU) is the high resolution X-ray spectrometer studied since 2015 for flying in the mid-30s on the Athena space...
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Pulsar search acceleration using FPGAs and OpenCL templates
The Square Kilometre Array (SKA) is the world’s largest radio telescope currently under construction, and will employ elaborate signal processing to...
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Hadronic interaction model dependence in cosmic Gamma-ray flux estimation using an extensive air shower array with a muon detector
Observation techniques of high-energy gamma rays using air showers have remarkably progressed via the Tibet AS γ , HAWC, and LHAASO experiments. These...
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A simulation study for the expected performance of Sharjah-Sat-1 payload improved X-Ray Detector (iXRD) in the orbital background radiation
Sharjah-Sat-1 is a 3U cubesat with a CdZnTe based hard X-ray detector, called iXRD (improved X-ray Detector) as a scientific payload with the primary...
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CATCH: chasing all transients constellation hunters space mission
In time-domain astronomy, a substantial number of transients will be discovered by multi-wavelength and multi-messenger observatories, posing a great...
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SULIS: A coronal magnetism explorer for ESA’s Voyage 2050
Magnetism dominates the structure and dynamics of the solar corona. To understand the true nature of the solar corona and the long-standing coronal...
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Modelization of galactic cosmic-ray short-term variations for LISA
The European Space Agency Laser Interferometer Space Antenna (LISA) will be the first mission dedicated to the detection of low-frequency...
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ICARUS: in-situ studies of the solar corona beyond Parker Solar Probe and Solar Orbiter
The primary scientific goal of ICARUS (Investigation of Coronal AcceleRation and heating of solar wind Up to the Sun), a mother-daughter satellite...
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RAPOC : The Rosseland and Planck opacity converterRAPOC (Rosseland and Planck Opacity Converter) is a Python 3 code that calculates Rosseland and Planck mean opacities (RPMs) from...
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Proton irradiation of SiPM arrays for POLAR-2
POLAR-2 is a space-borne polarimeter, built to investigate the polarization of Gamma-Ray Bursts and help elucidate their mechanisms. The instrument...
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The 100-m X-ray test facility at IHEP
The 100-m X-ray Test Facility of the Institute of High Energy Physics (IHEP) was initially proposed in 2012 for the test and calibration of the X-ray...
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Classical novae with CUBES
Among the main science cases that have motivated the proposal of CUBES, a new high-resolution spectrograph for the Very Large Telescope at the...
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New observables of the cosmic microwave background
We introduce new observables of the cosmic microwave background radiation, which can be measured through the detection of high order modes excited...
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Investigation on the cosmic-ray shadow of planets and asteroids
The moon shadow and sun shadow of cosmic rays are commonly used to calibrate the angular resolution of the instrument in extensive air shower...
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The EUSO@TurLab project in the framework of the JEM-EUSO program
The EUSO@TurLab project aims at performing experiments to reproduce Earth UV emissions as seen from a low Earth orbit by the planned missions of the...
