Zobrazeno 1 - 10
of 294
pro vyhledávání: '"SWINYARD, B. M."'
Autor:
Gull, T. R., Morris, P. W., Black, J. H., Nielsen, K. E., Barlow, M. J., Royer, P., Swinyard, B. M.
The evolved massive binary star Eta Carinae underwent eruptive mass loss events that formed the complex bi-polar Homunculus nebula harboring tens of solar masses of unusually nitrogen-rich gas and dust. Despite expectations for the presence of a sign
Externí odkaz:
http://arxiv.org/abs/2010.02351
Autor:
De Looze, I., Barlow, M. J., Swinyard, B. M., Rho, J., Gomez, H. L., Matsuura, M., Wesson, R.
Theoretical models predict that core-collapse supernovae (CCSNe) can be efficient dust producers (0.1-1.0 Msun), potentially accounting for most of the dust production in the early Universe. Observational evidence for this dust production efficiency
Externí odkaz:
http://arxiv.org/abs/1611.00774
Autor:
Exter, K. M., Cox, N. L. J., Swinyard, B. M., Matsuura, M., Mayer, A., De Beck, E., Decin, L.
Publikováno v:
A&A 596, A96 (2016)
Herschel FIR imaging and spectroscopy were taken at several epochs to probe the central point source and the extended environment of V838 Mon. PACS and SPIRE maps were used to obtain photometry of the near and far dust around V838 Mon. Fitting reveal
Externí odkaz:
http://arxiv.org/abs/1608.08842
Autor:
Molinari, S., Schisano, E., Elia, D., Pestalozzi, M., Traficante, A., Pezzuto, S., Swinyard, B. M., Noriega-Crespo, A., Bally, J., Moore, T. J. T., Plume, R., Zavagno, A., di Giorgio, A. M., Liu, S. J., Pilbratt, G. L., Mottram, J. C., Russeil, D., Piazzo, L., Veneziani, M., Benedettini, M., Calzoletti, L., Faustini, F., Natoli, P., Piacentini, F., Merello, M., Palmese, A., Del Grande, R., Polychroni, D., Rygl, K. L. J., Polenta, G., Barlow, M. J., Bernard, J. -P., Martin, P. G., Testi, L., Ali, B., Andrè, P., Beltrán, M. T., Billot, N., Brunt, C., Carey, S., Cesaroni, R., Compiègne, M., Eden, D., Fukui, Y., Garcia-Lario, P., Hoare, M. G., Huang, M., Joncas, G., Lim, T. L., Lord, S. D., Martinavarro-Armengol, S., Motte, F., Paladini, R., Paradis, D., Peretto, N., Robitaille, T., Schilke, P., Schneider, N., Schulz, B., Sibthorpe, B., Strafella, F., Thompson, M. A., Umana, G., Ward-Thompson, D., Wyrowski, F.
(Abridged) We present the first public release of high-quality data products (DR1) from Hi-GAL, the {\em Herschel} infrared Galactic Plane Survey. Hi-GAL is the keystone of a suite of continuum Galactic Plane surveys from the near-IR to the radio, an
Externí odkaz:
http://arxiv.org/abs/1604.05911
Autor:
Fulton, T., Naylor, D. A., Polehampton, E. T., Valtchanov, I., Hopwood, R., Lu, N., Baluteau, J. -P., Mainetti, G., Pearson, C., Papageorgiou, A., Guest, S., Zhang, L., Imhof, P., Swinyard, B. M., Griffin, M. J., Lim, T. L.
We present the data processing pipeline to generate calibrated data products from the Spectral and Photometric Imaging Receiver (SPIRE) imaging Fourier Transform Spectrometer on the Herschel Space Observatory. The pipeline processes telemetry from SP
Externí odkaz:
http://arxiv.org/abs/1603.00219
Autor:
Hopwood, R., Polehampton, E. T., Valtchanov, I., Swinyard, B. M., Fulton, T., Lu, N., Marchili, N., van der Wiel, M. H. D., Benielli, D., Imhof, P., Baluteau, J. -P., Pearson, C., Clements, D. L., Griffin, M. J., Lim, T. L., Makiwa, G., Naylor, D. A., Noble, G., Puga, E., Spencer, L. D.
A systematic programme of calibration observations was carried out to monitor the performance of the SPIRE FTS instrument on board the Herschel Space Observatory. Observations of planets (including the prime point-source calibrator, Uranus), asteroid
Externí odkaz:
http://arxiv.org/abs/1502.05717
Autor:
Matsuura, M., Dwek, E., Barlow, M. J., Babler, B., Baes, M., Meixner, M., Cernicharo, Jose, Clayton, Geoff C., Dunne, L., Fransson, C., Fritz, Jacopo, Gear, Walter, Gomez, H. L., Groenewegen, M. A. T., Indebetouw, R., Ivison, R. J., Jerkstrand, A., Lebouteiller, V., Lim, T. L., Lundqvist, P., Pearson, C. P., Roman-Duval, J, Royer, P., Staveley-Smith, Lister, Swinyard, B. M., van Hoof, P. A. M., van Loon, J. Th., Verstappen, Joris, Wesson, Roger, Zanardo, Giovanna, Blommaert, Joris A. D. L., Decin, Leen, Reach, W. T., Sonneborn, George, Van de Steene, Griet C., Yates, Jeremy A.
We present new Herschel photometric and spectroscopic observations of Supernova 1987A, carried out in 2012. Our dedicated photometric measurements provide new 70 micron data and improved imaging quality at 100 and 160 micron compared to previous obse
Externí odkaz:
http://arxiv.org/abs/1411.7381
Autor:
Van de Steene, G. C., van Hoof, P. A. M., Exter, K. M., Barlow, M. J., Cernicharo, J., Etxaluze, M., Gear, W. K., Goicoechea, J. R., Gomez, H. L., Groenewegen, M. A. T., Hargrave, P. C., Ivison, R. J., Leeks, S. J., Lim, T. L., Matsuura, M., Olofsson, G., Polehampton, E. T., Swinyard, B. M., Ueta, T., Van Winckel, H., Waelkens, C., Wesson, R.
Publikováno v:
A&A 574, A134 (2015)
In our series of papers presenting the Herschel imaging of evolved planetary nebulae, we present images of the dust distribution in the Helix nebula (NGC 7293). Images at 70, 160, 250, 350, and 500 micron were obtained with the PACS and SPIRE instrum
Externí odkaz:
http://arxiv.org/abs/1411.4429
Autor:
Magdis, Georgios E., Rigopoulou, D., Hopwood, R., Huang, J. -S, Farrah, D., Pearson, C., Alonso-Herrero, A., Bock, J. J., Clements, D., Cooray, A., Griffin, M. J., Oliver, S., Fournon, . Perez, Riechers, D., Swinyard, B. M., Scott, D., Thatte, N., Valtchanov, I., Vaccari, M.
We present Herschel far-IR photometry and spectroscopy as well as ground based CO observations of an intermediate redshift (0.21 < z < 0.88) sample of Herschel-selected (ultra)-luminous infrared galaxies (L_IR > 10^11.5L_sun). With these measurements
Externí odkaz:
http://arxiv.org/abs/1409.5605
Autor:
Pascale, E., Waldmann, I. P., MacTavish, C. J., Papageorgiou, A., Amaral-Rogers, A., Varley, R., de Foresto, V. Coudé, Griffin, M. J., Ollivier, M., Sarkar, S., Spencer, L., Swinyard, B. M., Tessenyi, M., Tinetti, G.
EChOSim is the end-to-end time-domain simulator of the Exoplanet Characterisation Observatory (EChO) space mission. EChOSim has been developed to assess the capability EChO has to detect and characterize the atmospheres of transiting exoplanets, and
Externí odkaz:
http://arxiv.org/abs/1406.3984