Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Muchovej, S. J."'
Autor:
Stevenson, M. A., Pearson, T. J., Jones, Michael E., Copley, C. J., Dickinson, C., John, J. J., King, O. G., Muchovej, S. J. C., Taylor, Angela C.
Publikováno v:
MNRAS, 484, 5377-5388 (2019 April 21)
The C-Band All-Sky Survey (C-BASS) is an all-sky full-polarization survey at a frequency of 5 GHz, designed to provide data complementary to the all-sky surveys of WMAP and Planck and future CMB B-mode polarization imaging surveys. We describe the de
Externí odkaz:
http://arxiv.org/abs/1811.06124
Autor:
Dickinson, C., Barr, A., Chiang, H. C., Copley, C., Grumitt, R. D. P., Harper, S. E., Heilgendorff, H. M., Jew, L. R. P., Jonas, J. L., Jones, Michael E., Leahy, J. P., Leech, J., Leitch, E. M., Muchovej, S. J. C., Pearson, T. J., Peel, M. W., Readhead, A. C. S., Sievers, J., Stevenson, M. A., Taylor, Angela C.
The C-Band All-Sky Survey C-BASS is a high-sensitivity all-sky radio survey at an angular resolution of 45 arcmin and a frequency of 4.7 GHz. We present a total intensity 4.7 GHz map of the North Celestial Pole (NCP) region of sky, above declination
Externí odkaz:
http://arxiv.org/abs/1810.11681
Autor:
Jones, Michael E., Taylor, Angela C., Aich, Moumita, Copley, C. J., Chiang, H. Cynthia, Davis, R. J., Dickinson, C., Grumitt, R. D. P., Hafez, Yaser, Heilgendorff, Heiko M., Holler, C. M., Irfan, M. O., Jew, Luke R. P., John, J. J., Jonas, J., King, O. G., Leahy, J. P., Leech, J., Leitch, E. M., Muchovej, S. J. C., Pearson, T. J., Peel, M. W., Readhead, A. C. S., Sievers, Jonathan, Stevenson, M. A., Zuntz, J.
The C-Band All-Sky Survey (C-BASS) is an all-sky full-polarisation survey at a frequency of 5 GHz, designed to provide complementary data to the all-sky surveys of WMAP and Planck, and future CMB B-mode polarization imaging surveys. The observing fre
Externí odkaz:
http://arxiv.org/abs/1805.04490
Autor:
Tibbs, C. T., Paladini, R., Cleary, K., Muchovej, S. J. C., Scaife, A. M. M., Stevenson, M. A., Laureijs, R. J., Ysard, N., Grainge, K. J. B., Perrott, Y. C., Rumsey, C., Villadsen, J.
In this analysis we illustrate how the relatively new emission mechanism known as spinning dust can be used to characterize dust grains in the interstellar medium. We demonstrate this by using spinning dust emission observations to constrain the abun
Externí odkaz:
http://arxiv.org/abs/1511.06626
Autor:
Tibbs, C. T., Paladini, R., Cleary, K., Muchovej, S. J. C., Scaife, A. M. M., Stevenson, M. A., Laureijs, R. J., Ysard, N., Grainge, K. J. B., Perrott, Y. C., Rumsey, C., Villadsen, J.
We present the first search for spinning dust emission from a sample of 34 Galactic cold cores, performed using the CARMA interferometer. For each of our cores we use photometric data from the Herschel Space Observatory to constrain N_{H}, T_{d}, n_{
Externí odkaz:
http://arxiv.org/abs/1507.08774
Autor:
Sharon, K., Gladders, M. D., Marrone, D. P., Hoekstra, H., Rasia, E., Bourdin, H., Gifford, D., Hicks, A. K., Greer, C., Mroczkowski, T., Barrientos, L. F., Bayliss, M., Carlstrom, J. E., Gilbank, D. G., Gralla, M., Hlavacek-Larrondo, J., Leitch, E., Mazzotta, P., Miller, C., Muchovej, S. J. C., Schrabback, T., Yee, H. K. C.
We present an initial study of the mass and evolutionary state of a massive and distant cluster, RCS2 J232727.6-020437. This cluster, at z=0.6986, is the richest cluster discovered in the RCS2 project. The mass measurements presented in this paper ar
Externí odkaz:
http://arxiv.org/abs/1503.07188
Autor:
Irfan, M. O., Dickinson, C., Davies, R. D., Copley, C., Davis, R. J., Ferreira, P. G., Holler, C. M., Jonas, J. L., Jones, Michael E., King, O. G., Leahy, J. P., Leech, J., Leitch, E. M., Muchovej, S. J. C., Pearson, T. J., Peel, M. W., Readhead, A. C. S., Stevenson, M. A., Sutton, D., Taylor, Angela C., Zuntz, J.
We present an analysis of the diffuse emission at 5 GHz in the first quadrant of the Galactic plane using two months of preliminary intensity data taken with the C-Band All Sky Survey (C-BASS) northern instrument at the Owens Valley Radio Observatory
Externí odkaz:
http://arxiv.org/abs/1501.06069
Autor:
King, O. G., Jones, Michael E., Copley, C., Davis, R. J., Leahy, J. P., Leech, J., Muchovej, S. J. C., Pearson, T. J., Taylor, Angela C.
Proper modelling of astronomical receivers is vital: it describes the systematic errors in the raw data, guides the receiver design process, and assists data calibration. In this paper we describe a method of analytically modelling the full signal an
Externí odkaz:
http://arxiv.org/abs/1410.5469
Autor:
King, O. G., Jones, Michael E., Blackhurst, E. J., Copley, C., Davis, R. J., Dickinson, C., Holler, C. M., Irfan, M. O., John, J. J., Leahy, J. P., Leech, J., Muchovej, S. J. C., Pearson, T. J., Stevenson, M. A., Taylor, Angela C.
The C-Band All-Sky Survey (C-BASS) is a project to map the full sky in total intensity and linear polarization at 5 GHz. The northern component of the survey uses a broadband single-frequency analogue receiver fitted to a 6.1-m telescope at the Owens
Externí odkaz:
http://arxiv.org/abs/1310.7129
Autor:
Plambeck, R. L., Bolatto, A. D., Carpenter, J. M., Eisner, J. A., Lamb, J. W., Leitch, E. M., Marrone, D. P., Muchovej, S. J., Perez, L. M., Pound, M. W., Teuben, P. J., Volgenau, N. H., Woody, D. P., Wright, M. C. H., Zauderer, B. A.
The 229 GHz (lambda 1.3mm) radio emission from Orion-KL was mapped with up to 0.14" angular resolution with CARMA, allowing measurements of the flux densities of Source I ('SrcI') and the Becklin-Neugebauer Object (BN), the 2 most massive stars in th
Externí odkaz:
http://arxiv.org/abs/1211.0085