|
Kawamura J, Blundell R, Tong C-YE, Papa DC, Hunter TR, Paine St. N, et al. Superconductive hot-electron bolometer mixer receiver for 800 GHz operation. Vol 48.; 2000.
|
|
Gundlach KH, Schicke M. SIS and bolometer mixers for terahertz frequencies. Supercond. Sci. Technol. 2000;13:181–7.
|
|
Kardashev NS, Andreyanov VV, Buyakas VI, Vinogradov IS, Gvamichava AS, Kotik AI, et al. The Millimetron project. In: Proc. Lebedev Phys. Institute. Vol 228.; 2000.
|
|
Кардашев НС, Андреянов ВВ, Буякас ВИ, Виноградов ИС, Гвамичева АС, Котик АИ, et al. Проект Миллиметрон. Труды ФИАН им. Лебедева. 2000;228.
|
Hansen L, Jørgensen HE, Nørgaard-Nielsen HU, Pedersen K, Goudfrooij P, Linden-Vornle MJD. ISO far-infrared observations of rich galaxy clusters III. Abell 2029, Abell 2052, Abell 2142. A&A. 2000;362(1):133–7.
Abstract: A sample of five rich galaxy clusters has been mapped by ISO at 60 μm, 100 μm, 135 μm, and 200 μm using the PHT-C camera. In previous papers Abell 2670 and Sersic 159-03 were discussed. Here we present the results for Abell 2029, Abell 2052, and Abell 2142. The conclusion of the survey is that the relatively small fields (approximate to 60 square are minutes) are structured with filaments or superpositions of point sources. In some cases point sources (approximate to 0.1 Jy) can be identified with cluster galaxies. An attempt to demonstrate infrared emission from dust in the cooling flows (due to star formation) was inconclusive.
|
