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From the 1 of 11 papers with an AI index.

most citedGBOT: ground based optical tracking of the Gaia satellite

15 citations

11 papers

astro-ph.IM20268 cited

Quasi-automatic software support for Gaia ground based optical tracking

S. Bouquillon, C. Barache, T. Carlucci +6

The ESA Gaia satellite mission will create a catalog of 1 billion stars with unprecedented astrometric precision. To achieve its aim in terms of astrometric precision, a ground bas…

astro-ph.IM202615 cited

GBOT: ground based optical tracking of the Gaia satellite

Martin Altmann, Sebastien Bouquillon, Francois Taris +6

Gaia, the 1 billion star, high precision, astrometric satellite will revolutionise our understanding in many areas of astronomy ranging from bodies in our Solar System to the forma…

astro-ph.HE2026

X-ray polarization of Z-type neutron star low-mass X-ray binaries -- II. Spectropolarimetric analysis

Andrea Gnarini, Francesco Ursini, Giorgio Matt +8

IXPE has provided for the first time detailed energy- and time-resolved X-ray polarimetry of Z-type neutron star low-mass X-ray binaries (NS-LMXBs) as they move along their color-c…

astro-ph.GA2026

SMGPS: A study of Galactic HII regions with extended morphology

Athanaseus J. T. Ramaila, Mark A. Thompson, Oleg M. Smirnov +7

The paper uses the MeerKAT 1.3 GHz Galactic Plane Survey to identify and characterize 1,327 Galactic H II regions, providing distances, Lyman‑photon fluxes, ionising star spectral…

astro-ph.IM2026

Long-term performance of SiPMs in space environment measured by GRBAlpha, GRBBeta, and VZLUSAT-2 CubeSats

Jakub Ripa, Filip Munz, Marianna Dafcikova +46

In this work, we report the successful application of silicon photomultipliers (SiPMs) in gamma-ray burst (GRB) detectors used in CubeSats operating in the low Earth orbit (LEO) ra…

astro-ph.HE20261 cited

Optical observations of the fast nova V1674 Herculis

Neeraj Singh Rawat, L. S. Sonith, U. S. Kamath +3

We present the evolution of optical spectra and lightcurves of the fast nova V1674 Herculis during 150 days past its eruption. Using the post-eruption AAVSO light curve, we have ca…