Search Results - "Peel, M W"

Revisiting the Distance to Radio Loops I and IV Using Gaia and Radio/Optical Polarization Data by Panopoulou, G. V., Dickinson, C., Readhead, A. C. S., Pearson, T. J., Peel, M. W.

“…Abstract Galactic synchrotron emission exhibits large angular scale features known as radio spurs and loops. Determining the physical size of these structures…”
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The C-Band All-Sky Survey (C-BASS): design and capabilities by 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-polarization survey at a frequency of 5 GHz, designed to provide complementary data to the all-sky…”
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The C-Band All-Sky Survey (C-BASS): constraining diffuse Galactic radio emission in the North Celestial Pole region by 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

“…ABSTRACT 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…”
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Statistical properties of polarized radio sources at high frequency and their impact on cosmic microwave background polarization measurements by Battye, R. A., Browne, I. W. A., Peel, M. W., Jackson, N. J., Dickinson, C.

“…We have studied the implications of high-sensitivity polarization measurements of objects from the Wilkinson Microwave Anisotropy Probe (WMAP) point source…”
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Template fitting of WMAP 7-year data: anomalous dust or flattening synchrotron emission? by Peel, M. W., Dickinson, C., Davies, R. D., Banday, A. J., Jaffe, T. R., Jonas, J. L.

“…Abstract Anomalous microwave emission at 20-40 GHz has been detected across our Galactic sky. It is highly correlated with thermal dust emission and hence it…”
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One Centimetre Receiver Array-prototype observations of the CRATES sources at 30 GHz by Peel, M. W., Gawroński, M. P., Battye, R. A., Birkinshaw, M., Browne, I. W. A., Davis, R. J., Feiler, R., Kus, A. J., Lancaster, K., Lowe, S. R., Pazderska, B. M., Pazderski, E., Roukema, B. F., Wilkinson, P. N.

“…Knowledge of the population of radio sources in the range ∼2-200 GHz is important for understanding their effects on measurements of the cosmic microwave…”
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QUIJOTE scientific results – IV. A northern sky survey in intensity and polarization at 10–20 GHz with the multifrequency instrument by Rubiño-Martín, J A, Guidi, F, Génova-Santos, R T, Harper, S E, Herranz, D, Hoyland, R J, Lasenby, A N, Poidevin, F, Rebolo, R, Ruiz-Granados, B, Vansyngel, F, Vielva, P, Watson, R A, Artal, E, Ashdown, M, Barreiro, R B, Bilbao-Ahedo, J D, Casas, F J, Casaponsa, B, Cepeda-Arroita, R, de la Hoz, E, Dickinson, C, Fernández-Cobos, R, Fernández-Torreiro, M, González-González, R, Hernández-Monteagudo, C, López-Caniego, M, López-Caraballo, C, Martínez-González, E, Peel, M W, Peláez-Santos, A E, Perrott, Y, Piccirillo, L, Razavi-Ghods, N, Scott, P, Titterington, D, Tramonte, D, Vignaga, R

“…ABSTRACT We present QUIJOTE intensity and polarization maps in four frequency bands centred around 11, 13, 17, and 19 GHz, and covering approximately 29 000…”
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30 GHz observations of sources in the Very Small Array fields by Gawroński, M. P., Peel, M. W., Lancaster, K., Battye, R. A., Birkinshaw, M., Browne, I. W. A., Davies, M. L., Davis, R. J., Feiler, R., Franzen, T. M. O., Génova-Santos, R., Kus, A. J., Lowe, S. R., Pazderska, B. M., Pazderski, E., Pooley, G. G., Roukema, B. F., Waldram, E. M., Wilkinson, P. N.

“…Small angular scale (high ℓ) studies of cosmic microwave background (CMB) anisotropies require accurate knowledge of the statistical properties of…”
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The C-Band All-Sky Survey (C-BASS): new constraints on the integrated radio spectrum of M 31 by Harper, Stuart E, Barr, Adam, Dickinson, C, Peel, M W, Cepeda-Arroita, Roke, Copley, C J, Grumitt, R D P, Leahy, J Patrick, Jonas, J L, Jones, Michael E, Leech, J, Pearson, T J, Readhead, A C S, Taylor, Angela C

“…ABSTRACT The Andromeda galaxy (M 31) is our closest neighbouring spiral galaxy, making it an ideal target for studying the physics of the interstellar medium…”
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The C-Band All-Sky Survey (C-BASS): template fitting of diffuse galactic microwave emission in the northern sky by Harper, S E, Dickinson, C, Barr, A, Cepeda-Arroita, R, Grumitt, R D P, Heilgendorff, H M, Jew, L, Jonas, J L, Jones, M E, Leahy, J P, Leech, J, Pearson, T J, Peel, M W, Readhead, A C S, Taylor, A C

“…ABSTRACT The C-Band All-Sky Survey (C-BASS) has observed the Galaxy at 4.76 GHz with an angular resolution of 0${_{.}^{\circ}}$73 full-width half-maximum, and…”
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Detection of spectral variations of Anomalous Microwave Emission with QUIJOTE and C-BASS by Cepeda-Arroita, R, Harper, S E, Dickinson, C, Rubiño-Martín, J A, Génova-Santos, R T, Taylor, Angela C, Pearson, T J, Ashdown, M, Barr, A, Barreiro, R B, Casaponsa, B, Casas, F J, Chiang, H C, Fernandez-Cobos, R, Grumitt, R D P, Guidi, F, Heilgendorff, H M, Herranz, D, Jew, L R P, Jonas, J L, Jones, Michael E, Lasenby, A, Leech, J, Leahy, J P, Martínez-González, E, Peel, M W, Piccirillo, L, Poidevin, F, Readhead, A C S, Rebolo, R, Ruiz-Granados, B, Sievers, J, Vansyngel, F, Vielva, P, Watson, R A

“…ABSTRACT Anomalous Microwave Emission (AME) is a significant component of Galactic diffuse emission in the frequency range 10–$60\, \mathrm{GHz}$ and a new…”
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A Forecast of the Sensitivity on the Measurement of the Optical Depth to Reionization with the GroundBIRD Experiment by Lee, K., Génova-Santos, R. T., Hazumi, M., Honda, S., Kutsuma, H., Oguri, S., Otani, C., Peel, M. W., Sueno, Y., Suzuki, J., Tajima, O., Won, E.

“…Abstract We compute the expected sensitivity on measurements of optical depth to reionization for a ground-based experiment at Teide Observatory. We simulate…”
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QUIJOTE scientific results – V. The microwave intensity and polarization spectra of the Galactic regions W49, W51 and IC443 by Tramonte, D, Génova-Santos, R T, Rubiño-Martín, J A, Vielva, P, Poidevin, F, López-Caraballo, C H, Peel, M W, Ashdown, M, Artal, E, Barreiro, R B, Casas, F J, de la Hoz, E, Fernández-Torreiro, M, Guidi, F, Herranz, D, Hoyland, R J, Lasenby, A N, Martinez-Gonzalez, E, Piccirillo, L, Rebolo, R, Ruiz-Granados, B, Vansyngel, F, Watson, R A

“…ABSTRACT We present new intensity and polarization maps obtained with the QUIJOTE experiment towards the Galactic regions W49, W51 and IC443, covering the…”
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QUIJOTE scientific results – X. Spatial variations of Anomalous Microwave Emission along the Galactic plane by Fernández-Torreiro, M, Rubiño-Martín, J A, López-Caraballo, C H, Génova-Santos, R T, Peel, M W, Guidi, F, Harper, S E, Artal, E, Ashdown, M, Barreiro, R B, Casas, F J, de la Hoz, E, Herranz, D, Hoyland, R, Lasenby, A, Martínez-Gonzalez, E, Piccirillo, L, Poidevin, F, Rebolo, R, Ruiz-Granados, B, Tramonte, D, Vansyngel, F, Vielva, P, Watson, R A

“…ABSTRACT Anomalous microwave emission (AME) is an important emission component between 10 and 60 GHz that is not yet fully understood. It seems to be…”
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QUIJOTE Scientific Results – XVII. Studying the anomalous microwave emission in the Andromeda Galaxy with QUIJOTE-MFI by Fernández-Torreiro, M, Génova-Santos, R T, Rubiño-Martín, J A, López-Caraballo, C H, Peel, M W, Arce-Tord, C, Rebolo, R, Artal, E, Ashdown, M, Barreiro, R B, Casas, F J, de la Hoz, E, Guidi, F, Herranz, D, Hoyland, R, Lasenby, A, Martínez-Gonzalez, E, Piccirillo, L, Poidevin, F, Ruiz-Granados, B, Tramonte, D, Vansyngel, F, Vielva, P, Watson, R A

“…ABSTRACT The Andromeda Galaxy (M31) is the Local Group galaxy that is most similar to the Milky Way (MW). The similarities between the two galaxies make M31…”
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QUIJOTE scientific results – XIII. Intensity and polarization study of the microwave spectra of supernova remnants in the QUIJOTE-MFI wide survey: CTB 80, Cygnus Loop, HB 21, CTA 1, Tycho, and HB 9 by López-Caraballo, C H, Ruiz-Granados, B, Génova-Santos, R T, Fernández-Torreiro, M, Rubiño-Martín, J A, Peel, M W, Poidevin, F, Artal, E, Ashdown, M, Barreiro, R B, Casas, F J, de la Hoz, E, González-González, R, Guidi, F, Herranz, D, Hoyland, R, Lasenby, A, Martínez-González, E, Piccirillo, L, Rebolo, R, Tramonte, D, Vansyngel, F, Vielva, P, Watson, R A

“…ABSTRACT We use the new QUIJOTE-MFI wide survey (11, 13, 17, and 19 GHz) to produce spectral energy distributions (SEDs), on an angular scale of 1°, of the…”
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QUIJOTE scientific results – VIII. Diffuse polarized foregrounds from component separation with QUIJOTE-MFI by de la Hoz, E, Barreiro, R B, Vielva, P, Martínez-González, E, Rubiño-Martín, J A, Casaponsa, B, Guidi, F, Ashdown, M, Génova-Santos, R T, Artal, E, Casas, F J, Fernández-Cobos, R, Fernández-Torreiro, M, Herranz, D, Hoyland, R J, Lasenby, A N, López-Caniego, M, López-Caraballo, C H, Peel, M W, Piccirillo, L, Poidevin, F, Rebolo, R, Ruiz-Granados, B, Tramonte, D, Vansyngel, F, Watson, R A

“…ABSTRACT We derive linearly polarized astrophysical component maps in the Northern Sky from the QUIJOTE-MFI data at 11 and 13 GHz in combination with the…”
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QUIJOTE scientific results – VII. Galactic AME sources in the QUIJOTE-MFI northern hemisphere wide survey by Poidevin, F, Génova-Santos, R T, Rubiño-Martín, J A, López-Caraballo, C H, Watson, R A, Artal, E, Ashdown, M, Barreiro, R B, Casas, F J, de la Hoz, E, Fernández-Torreiro, M, Guidi, F, Herranz, D, Hoyland, R J, Lasenby, A N, Martinez-Gonzalez, E, Peel, M W, Piccirillo, L, Rebolo, R, Ruiz-Granados, B, Tramonte, D, Vansyngel, F, Vielva, P

“…ABSTRACT The QUIJOTE-MFI Northern Hemisphere Wide Survey has provided maps of the sky above declinations −30° at 11, 13, 17, and 19 GHz. These data are…”
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QUIJOTE scientific results – VI. The Haze as seen by QUIJOTE by Guidi, F, Génova-Santos, R T, Rubiño-Martín, J A, Peel, M W, Fernández-Torreiro, M, López-Caraballo, C H, Vignaga, R, de la Hoz, E, Vielva, P, Watson, R A, Ashdown, M, Dickinson, C, Artal, E, Barreiro, R B, Casas, F J, Herranz, D, Hoyland, R J, Lasenby, A N, Martinez-Gonzalez, E, Piccirillo, L, Poidevin, F, Rebolo, R, Ruiz-Granados, B, Tramonte, D, Vansyngel, F

“…ABSTRACT The Haze is an excess of microwave intensity emission surrounding the Galactic Centre. It is spatially correlated with the γ-ray Fermi bubbles, and…”
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Planck observations of M33 by Tibbs, C T, Israel, F P, Laureijs, R J, Tauber, J A, Partridge, B, Peel, M W, Fauvet, L

“…Abstract We have performed a comprehensive investigation of the global integrated flux density of M33 from radio to ultraviolet wavelengths, finding that the…”
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