Zobrazeno 1 - 10
of 161
pro vyhledávání: '"Davies, Rod"'
Autor:
Traficante, Alessio, Paladini, Roberta, Compiegne, Mathieu, Alves, Marta I. R., Cambresy, Laurent, Gibson, Steven J., Tibbs, Christopher T., Noriega-Crespo, Alberto, Molinari, Sergio, Carey, Sean J., Ingalls, Jim G., Natoli, Paolo, Davies, Rod D., Davis, Richard J., Dickinson, Clive, Fuller, Gary A.
Herschel FIR continuum data obtained as part of the Hi-GAL survey have been used, together with the GLIMPSE 8 $\mu$m and MIPSGAL 24 $\mu$m data, to attempt the first 3D-decomposition of dust emission associated with atomic, molecular and ionized gas
Externí odkaz:
http://arxiv.org/abs/1403.3327
Autor:
Ghosh, Tuhin, Banday, A. J., Jaffe, Tess, Dickinson, Clive, Davies, Rod, Davis, Richard, Gorski, Krzysztof
Publikováno v:
Mon.Not.Roy.Astron.Soc.422:3617-3642,2012
WMAP data when combined with ancillary data on free-free, synchrotron and dust allow an improved understanding of the spectrum of emission from each of these components. Here we examine the sky variation at intermediate and high latitudes using a cro
Externí odkaz:
http://arxiv.org/abs/1112.0509
Autor:
King, Oliver G., Copley, Charles, Davies, Rod, Davis, Richard, Dickinson, Clive, Hafez, Yaser A., Holler, Christian, John, Jaya John, Jonas, Justin L., Jones, Michael E., Leahy, J. Patrick, Muchovej, Stephen J. C., Pearson, Timothy J., Readhead, Anthony C. S., Stevenson, Matthew A., Taylor, Angela C.
Publikováno v:
Proceedings of SPIE MIllimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V (2010)
The C-Band All-Sky Survey (C-BASS) aims to produce sensitive, all-sky maps of diffuse Galactic emission at 5 GHz in total intensity and linear polarization. These maps will be used (with other surveys) to separate the several astrophysical components
Externí odkaz:
http://arxiv.org/abs/1008.4082
Autor:
Franzen, Thomas M. O., Davies, Matthew L., Davies, Rod D., Davis, Richard J., Feroz, Farhan, Genova-Santos, Ricardo, Grainge, Keith J. B., Green, David A., Hobson, Michael P., Hurley-Walker, Natasha, Lasenby, Anthony N., Lopez-Caniego, Marcos, Olamaie, Malak, Padilla-Torres, Carmen P., Pooley, Guy G., Rebolo, Rafael, Rodriguez-Gonzalvez, Carmen, Saunders, Richard D. E., Scaife, Anna M. M., Scott, Paul F., Shimwell, Timothy W., Titterington, David J., Waldram, Elizabeth M., Watson, Robert A., Zwart, Jonathan T. L.
Using the Arcminute Microkelvin Imager (AMI) at 16 GHz and the Very Small Array (VSA) at 33 GHz to make follow-up observations of sources in the New Extragalactic WMAP Point Source Catalogue, we have investigated the flux-density variability in a com
Externí odkaz:
http://arxiv.org/abs/0907.3843
Autor:
Davies, Matthew L., Franzen, Thomas M. O., Davies, Rod D., Davis, Richard J., Feroz, Farhan, Genova-Santos, Ricardo, Grainge, Keith J. B., Green, David A., Hobson, Michael P., Hurley-Walker, Natasha, Lasenby, Anthony N., Lopez-Caniego, Marcos, Olamaie, Malak, Padilla-Torres, Carmen P., Pooley, Guy G., Rebolo, Rafael, Rodriguez-Gonzalvez, Carmen, Saunders, Richard D. E., Scaife, Anna M. M., Scott, Paul F., Shimwell, Timothy W., Titterington, David J., Waldram, Elizabeth M., Watson, Robert A., Zwart, Jonathan T. L.
We present follow-up observations of 97 point sources from the Wilkinson Microwave Anisotropy Probe (WMAP) 3-year data, contained within the New Extragalactic WMAP Point Source (NEWPS) catalogue between declinations of -4 and +60 degrees; the sources
Externí odkaz:
http://arxiv.org/abs/0907.3707
Autor:
Hafez, Yaser A., Davies, Rod D., Davis, Richard J., Dickinson, Clive, Battistelli, Elia S., Blanco, Francisco, Cleary, Kieran, Franzen, Thomas, Genova-Santos, Ricardo, Grainge, Keith, Hobson, Michael P., Jones, Michael E., Lancaster, Katy, Lasenby, Anthony N., Padilla-Torres, Carmen P., Rubino-Martin, Jose Alberto, Rebolo, Rafael, Saunders, Richard D. E., Scott, Paul F., Taylor, Angela C., Titterington, David, Tucci, Marco, Watson, Robert A.
Accurate calibration of data is essential for the current generation of CMB experiments. Using data from the Very Small Array (VSA), we describe procedures which will lead to an accuracy of 1 percent or better for experiments such as the VSA and CBI.
Externí odkaz:
http://arxiv.org/abs/0804.2853
Autor:
Genova-Santos, Ricardo, Rubino-Martin, Jose Alberto, Rebolo, Rafael, Battye, Richard A., Blanco, Francisco, Davies, Rod D., Davis, Richard J., Franzen, Thomas, Grainge, Keith, Hobson, Michael P., Lasenby, Anthony, Padilla-Torres, Carmen P., Pooley, Guy G., Saunders, Richard D. E., Scaife, Anna, Scott, Paul F., Titterington, David, Tucci, Marco, Watson, Robert A.
Publikováno v:
Mon.Not.Roy.Astron.Soc.391:1127,2008
We present interferometric imaging at 33 GHz, with the new superextended configuration of the Very Small Array (VSA), of a very deep decrement in the cosmic microwave background (CMB) temperature. This decrement is located in the direction of the Cor
Externí odkaz:
http://arxiv.org/abs/0804.0199
Publikováno v:
Mon.Not.Roy.Astron.Soc.383:150-160,2008
We discuss the possibility of performing a substantial spectroscopic galaxy redshift survey selected via the 21cm emission from neutral hydrogen using the Five-hundred metre Aperture Spherical Telescope (FAST) to be built in China. We consider issues
Externí odkaz:
http://arxiv.org/abs/0707.2316
Autor:
Scaife, Anna, Green, David A., Battye, Richard A., Davies, Rod D., Davis, Richard J., Dickinson, Clive, Franzen, Thomas, Genova-Santos, Ricardo, Grainge, Keith, Hafez, Yaser A., Hobson, Michael P., Lasenby, Anthony, Pooley, Guy G., Rajguru, Nutan, Rebolo, Rafael, Rubino-Martin, Jose Alberto, Saunders, Richard D. E., Scott, Paul F., Titterington, David, Waldram, Elizabeth, Watson, Robert A.
Publikováno v:
Mon.Not.Roy.Astron.Soc.Lett.377:L69-L73,2007
We present results from observations made at 33 GHz with the Very Small Array (VSA) telescope towards potential candidates in the Galactic plane for spinning dust emission. In the cases of the diffuse HII regions LPH96 and NRAO591 we find no evidence
Externí odkaz:
http://arxiv.org/abs/astro-ph/0702473