Zobrazeno 1 - 10
of 72
pro vyhledávání: '"Chuss, D. T."'
Recent high-resolution 53-$\mu$m polarimetric observations from SOFIA/HAWC+ have revealed the inferred plane-of-the-sky magnetic field (B-field) orientation in the Galactic center's Circum-Nuclear Disk (CND). The B-field is mostly aligned with the st
Externí odkaz:
http://arxiv.org/abs/2304.06823
Autor:
Switzer, E. R., Ade, P. A. R., Baildon, T., Benford, D., Bennett, C. L., Chuss, D. T., Datta, R., Eimer, J. R., Fixsen, D. J., Gandilo, N. N., Essinger-Hileman, T. M., Halpern, M., Hilton, G., Irwin, K., Jhabvala, C., Kimball, M., Kogut, A., Lazear, J., Lowe, L. N., McMahon, J. J., Miller, T. M., Mirel, P., Moseley, S. H., Pawlyk, S., Rodriguez, S., Sharp, E., Shirron, P., Staguhn, J. G., Sullivan, D. F., Taraschi, P., Tucker, C. E., Walts, A., Wollack, E. J.
Publikováno v:
Rev. Sci. Inst 90(9) 2019
The Primordial Inflation Polarization Explorer (PIPER) is a balloon-borne telescope mission to search for inflationary gravitational waves from the early universe. PIPER employs two 32x40 arrays of superconducting transition-edge sensors, which opera
Externí odkaz:
http://arxiv.org/abs/1909.06440
Autor:
Odegard, N., Weiland, J. L., Fixsen, D. J., Chuss, D. T., Dwek, E., Kogut, A., Switzer, E. R.
Publikováno v:
Ap.J. 877, 40 (2019)
New determinations are presented of the cosmic infrared background monopole brightness in the Planck HFI bands from 100 GHz to 857 GHz. Planck was not designed to measure the monopole component of sky brightness, so cross-correlation of the 2015 HFI
Externí odkaz:
http://arxiv.org/abs/1904.11556
Autor:
Chluba, J., Kogut, A., Patil, S. P., Abitbol, M. H., Aghanim, N., Ali-Haimoud, Y., Amin, M. A., Aumont, J., Bartolo, N., Basu, K., Battistelli, E. S., Battye, R., Baumann, D., Ben-Dayan, I., Bolliet, B., Bond, J. R., Bouchet, F. R., Burgess, C. P., Burigana, C., Byrnes, C. T., Cabass, G., Chuss, D. T., Clesse, S., Cole, P. S., Dai, L., de Bernardis, P., Delabrouille, J., Desjacques, V., de Zotti, G., Diacoumis, J. A. D., Dimastrogiovanni, E., Di Valentino, E., Dunkley, J., Durrer, R., Dvorkin, C., Ellis, J., Eriksen, H. K., Fasiello, M., Fixsen, D., Finelli, F., Flauger, R., Galli, S., Garcia-Bellido, J., Gervasi, M., Gluscevic, V., Grin, D., Hart, L., Hernandez-Monteagudo, C., Hill, J. C., Jeong, D., Johnson, B. R., Lagache, G., Lee, E., Lewis, A., Liguori, M., Kamionkowski, M., Khatri, R., Kohri, K., Komatsu, E., Kunze, K. E., Mangilli, A., Masi, S., Mather, J., Matarrese, S., Miville-Deschenes, M. A., Montaruli, T., Munchmeyer, M., Mukherjee, S., Nakama, T., Nati, F., Ota, A., Page, L. A., Pajer, E., Poulin, V., Ravenni, A., Reichardt, C., Remazeilles, M., Rotti, A., Rubino-Martin, J. A., Sarkar, A., Sarkar, S., Savini, G., Scott, D., Serpico, P. D., Silk, J., Souradeep, T., Spergel, D. N., Starobinsky, A. A., Subrahmanyan, R., Sunyaev, R. A., Switzer, E., Tartari, A., Tashiro, H., Thakur, R. Basu, Trombetti, T., Wallisch, B., Wandelt, B. D., Wehus, I. K., Wollack, E. J., Zaldarriaga, M., Zannoni, M.
Following the pioneering observations with COBE in the early 1990s, studies of the cosmic microwave background (CMB) have focused on temperature and polarization anisotropies. CMB spectral distortions - tiny departures of the CMB energy spectrum from
Externí odkaz:
http://arxiv.org/abs/1903.04218
Accurate modeling of the spectrum of thermal dust emission at millimeter wavelengths is important for improving the accuracy of foreground subtraction for CMB measurements, for improving the accuracy with which the contributions of different foregrou
Externí odkaz:
http://arxiv.org/abs/1606.08783
Autor:
Chuss, D. T., Ali, A., Amiri, M., Appel, J., Bennett, C. L., Colazo, F., Denis, K. L., Dünner, R., Essinger-Hileman, T., Eimer, J., Fluxa, P., Gothe, D., Halpern, M., Harrington, K., Hilton, G., Hinshaw, G., Hubmayr, J., Iuliano, J., Marriage, T. A., Miller, N., Moseley, S. H., Mumby, G., Petroff, M., Reintsema, C., Rostem, K., U-Yen, K., Watts, D., Wagner, E., Wollack, E. J., Xu, Z., Zeng, L.
The Cosmology Large Angular Scale Surveyor (CLASS) will measure the polarization of the Cosmic Microwave Background to search for and characterize the polarized signature of inflation. CLASS will operate from the Atacama Desert and observe $\sim$70%
Externí odkaz:
http://arxiv.org/abs/1511.04414
Autor:
Miller, N. J., Chuss, D. T., Marriage, T. A., Wollack, E. J., Appel, J. W., Bennett, C. L., Eimer, J., Essinger-Hileman, T., Fixsen, D. J., Harrington, K., Moseley, S. H., Rostem, K., Switzer, E. R., Watts, D. J.
Publikováno v:
ApJ, 818, 151 (2016)
Variable-delay Polarization Modulators (VPMs) are currently being implemented in experiments designed to measure the polarization of the cosmic microwave background on large angular scales because of their capability for providing rapid, front-end po
Externí odkaz:
http://arxiv.org/abs/1509.04628
We demonstrate that a phonon stopband can be synthesized from an aperiodic structure comprising a discrete set of phononic filter stages. Each element of the set has a dispersion relation that defines a complete bandgap when calculated under a Bloch
Externí odkaz:
http://arxiv.org/abs/1509.03923
Publikováno v:
Rev. Sci. Instrum. 85, 034702 (2014)
We have designed, fabricated and characterized absorptive thermal blocking filters for cryogenic microwave applications. The transmission line filter's input characteristic impedance is designed to match $50\,\Omega$ and its response has been validat
Externí odkaz:
http://arxiv.org/abs/1403.2909
Autor:
Kogut, A., Fixsen, D. J., Chuss, D. T., Dotson, J., Dwek, E., Halpern, M., Hinshaw, G. F., Meyer, S. M., Moseley, S. H., Seiffert, M. D., Spergel, D. N., Wollack, E. J.
The Primordial Inflation Explorer (PIXIE) is an Explorer-class mission to measure the gravity-wave signature of primordial inflation through its distinctive imprint on the linear polarization of the cosmic microwave background. The instrument consist
Externí odkaz:
http://arxiv.org/abs/1105.2044