Zobrazeno 1 - 10
of 178
pro vyhledávání: '"Lim, T. L."'
Autor:
Brandeker, A., Cataldi, G., Olofsson, G., Vandenbussche, B., Acke, B., Barlow, M. J., Blommaert, J. A. D. L., Cohen, M., Dent, W. R. F., Dominik, C., Di Francesco, J., Fridlund, M., Gear, W. K., Glauser, A. M., Greaves, J. S., Harvey, P. M., Heras, A. M., Hogerheijde, M. R., Holland, W. S., Huygen, R., Ivison, R. J., Leeks, S. J., Lim, T. L., Liseau, R., Matthews, B. C., Pantin, E., Pilbratt, G. L., Royer, P., Sibthorpe, B., Waelkens, C., Walker, H. J.
Publikováno v:
A&A 591, A27 (2016)
The young star beta Pictoris is well known for its dusty debris disk, produced through the grinding down by collisions of planetesimals, kilometre-sized bodies in orbit around the star. In addition to dust, small amounts of gas are also known to orbi
Externí odkaz:
http://arxiv.org/abs/1604.07418
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:
Etxaluze, M., Cernicharo, J., Goicoechea, J. R., van Hoof, P. A. M., Swinyard, B. M., Barlow, M. J., van de Steene, G. C., Groenewegen, M. A. T., Kerschbaum, F., Lim, T. L., Lique, F., Matsuura, M., Pearson, C., Polehampton, E. T., Royer, P., Ueta, T.
The Helix Nebula (NGC 7293) is the closest planetary nebulae. Therefore, it is an ideal template for photochemical studies at small spatial scales in planetary nebulae. We aim to study the spatial distribution of the atomic and the molecular gas, and
Externí odkaz:
http://arxiv.org/abs/1404.2177
Autor:
Swinyard, B. M., Polehampton, E. T., Hopwood, R., Valtchanov, I., Lu, N., Fulton, T., Benielli, D., Imhof, P., Marchili, N., Baluteau, J. -P., Bendo, G. J., Ferlet, M., Griffin, M. J., Lim, T. L., Makiwa, G., Naylor, D. A., Orton, G. S., Papageorgiou, A., Pearson, C. P., Schulz, B., Sidher, S. D., Spencer, L. D., van der Wiel, M. H. D., Wu, R.
The Herschel SPIRE instrument consists of an imaging photometric camera and an imaging Fourier Transform Spectrometer (FTS), both operating over a frequency range of 450-1550 GHz. In this paper, we briefly review the FTS design, operation, and data r
Externí odkaz:
http://arxiv.org/abs/1403.1107
Autor:
Focardi, M., Di Giorgio, A. M., Farina, M., Pancrazzi, M., Ottensamer, R., Lim, T. L., Pezzuto, S., Micela, G., Pace, E.
EChO is a three-modules (VNIR, SWIR, MWIR), highly integrated spectrometer, covering the wavelength range from 0.55 $\mu$m, to 11.0 $\mu$m. The baseline design includes the goal wavelength extension to 0.4 $\mu$m while an optional LWIR module extends
Externí odkaz:
http://arxiv.org/abs/1401.2977
Autor:
Barlow, M. J., Swinyard, B. M., Owen, P. J., Cernicharo, J., Gomez, H. L., Ivison, R. J., Krause, O., Lim, T. L., Matsuura, M., Miller, S., Olofsson, G., Polehampton, E. T.
Publikováno v:
Science, 342, 1343-1345 (2013)
Noble gas molecules have not hitherto been detected in space. From spectra obtained with the Herschel Space Observatory, we report the detection of emission in the 617.5 GHz and 1234.6 GHz J = 1-0 and 2-1 rotational lines of {36}ArH^+ at several posi
Externí odkaz:
http://arxiv.org/abs/1312.4843