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Scientific Objectives of the Lunar Millimeter and Submillimeter Observatory
S. F. Likhachev, T. I. Larchenkova, A. S. Andrianov, E. O. Vasiliev, D. A. Litvinov, S. V. Pilipenko, A. G. Rudnitskiy and M. A. Shchurov Astronomy Letters 50(12) 830 (2024) https://doi.org/10.1134/S1063773725700112
Science and Innovation with Stratospheric Balloons: The Olimpo & Lspe/Swipe Projects
Objectives of the Millimetron Space Observatory science program and technical capabilities of its realization
I D Novikov, S F Likhachev, Yu A Shchekinov, A S Andrianov, A M Baryshev, A I Vasyunin, D Z Wiebe, Th de Graauw, A G Doroshkevich, I I Zinchenko, N S Kardashev, V I Kostenko, T I Larchenkova, L N Likhacheva, A O Lyakhovets, D I Novikov, S V Pilipenko, A F Punanova, A G Rudnitsky, A V Smirnov and V I Shematovich Physics-Uspekhi 64(4) 386 (2021) https://doi.org/10.3367/UFNe.2020.12.038898
KISS: a spectrometric imager for millimetre cosmology
The long duration cryogenic system of the OLIMPO balloon–borne experiment: Design and in–flight performance
A. Coppolecchia, L. Lamagna, S. Masi, P.A.R. Ade, G. Amico, E.S. Battistelli, P. de Bernardis, F. Columbro, L. Conversi, G. D’Alessandro, M. De Petris, M. Gervasi, F. Nati, L. Nati, A. Paiella, F. Piacentini, G. Pisano, G. Presta, A. Schillaci, C. Tucker and M. Zannoni Cryogenics 110 103129 (2020) https://doi.org/10.1016/j.cryogenics.2020.103129
In-Flight Performance of the LEKIDs of the OLIMPO Experiment
Absorption and cross-talk in a multipixel receiving system with cold electron bolometers
E A Matrozova, A L Pankratov, A V Gordeeva, A V Chiginev and L S Kuzmin Superconductor Science and Technology 32(8) 084001 (2019) https://doi.org/10.1088/1361-6668/ab151d
Kinetic inductance detectors for the OLIMPO experiment: design and pre-flight characterization
Galaxy clusters as probes for cosmology and dark matter
Elia S. Battistelli, Carlo Burigana, Paolo de Bernardis, et al. International Journal of Modern Physics D 25(10) 1630023 (2016) https://doi.org/10.1142/S0218271816300238
Common-mode rejection in Martin–Puplett spectrometers for astronomical observations at millimeter wavelengths