... The Large-Scale Polarization Explorer (LSPE)," in SPIE Astronomical Telescopes+ Instrument., 2012, p. 84467A. [5] M. Salatino, P. de Bernardis, L. Kuzmin, S. Mahashabde, and S. Masi, "Sensitivity to cosmic rays of cold electron bolometers for space ...
... Current leads made from Nb were attached to the larger angles of rhombus and had the width of 510 µm. Details of detector preparation are given in [4]. ...
... Since the flatness (parallelism) of the Si substrates is quite good (the thickness variation is well below 5 µm over 100 mm wafer size), the acoustic wave is reflected back to the point of emission with an accuracy much better than 0.1 µm. At frequencies ...
... Sweden 6 Spectra of the phase-locked FFO for different delay in the PL loop FFO LW = 3.4 MHz initial SR = 67 % Extra Cable : 2 3 4 5 6 7 8 mmmmmmm April 4, 2008 BjЖrkliden, Sweden 7 SR value on the delay in PL loop 0 -1 100 o Loop length, 0 0 1 2 3 ...
... 4] H. B. Wang et al., Phys. Rev. Lett. 105, 057002 (2010). [5] M. Tsujimoto et al., Phys. Rev. Lett. 105, 037005 (2010). [6] T. Kashiwagi et al., ...
... 4] H. B. Wang et al., Phys. Rev. Lett. 105, 057002 (2010). [5] M. Tsujimoto et al., Phys. Rev. Lett. 105, 037005 (2010). [6] T. Kashiwagi et al., ...
... prediction of the formation of strain-minimizing textures during film thickening is supported by the recent experimental observations of Oh and Je13 for 1.5m thick TiN films deposited by reactive rf-magnetron sputtering in a pure nitrogen atmosphere ...