Zobrazeno 1 - 10
of 36
pro vyhledávání: '"Alacid, J. M."'
Autor:
Lafarga, M., Ribas, I., Lovis, C., Perger, M., Zechmeister, M., Bauer, F. F., Kürster, M., Cortés-Contreras, M., Morales, J. C., Herrero, E., Rosich, A., Baroch, D., Reiners, A., Caballer, J. A., Quirrenbach, A., Amado, P. J., Alacid, J. M., Béjar, V. J. S., Dreizler, S., Hatzes, A. P., Henning, T., Jeffers, S. V., Kaminski, A., Montes, D., Pedraz, S., Rodríguez-López, C., Schmitt, J. H. M. M.
Publikováno v:
A&A 636, A36 (2020)
For years, the standard procedure to measure radial velocities (RVs) of spectral observations consisted in cross-correlating the spectra with a binary mask, that is, a simple stellar template that contains information on the position and strength of
Externí odkaz:
http://arxiv.org/abs/2003.07471
Autor:
Simón-Díaz, S., Negueruela, I., Apellániz, J. Maíz, Castro, N., Herrero, A., Garcia, M., Pérez-Prieto, J. A., Caon, N., Alacid, J. M., Camacho, I., Dorda, R., Godart, M., González-Fernández, C., Holgado, G., Rübke, K.
The IACOB project is an ambitious long-term project which is contributing to step forward in our knowledge about the physical properties and evolution of Galactic massive stars. The project aims at building a large database of high-resolution, multi-
Externí odkaz:
http://arxiv.org/abs/1504.04257
The observation of blank fields, defined as regions of the sky that are devoid of stars down to a given threshold magnitude, constitutes one of the most relevant calibration procedures required for the proper reduction of astronomical data obtained f
Externí odkaz:
http://arxiv.org/abs/1209.4861
The observation of blank fields, regions of the sky devoid of stars down to a given threshold magnitude, constitutes one of the typical important calibration procedures required for the proper reduction of astronomical data obtained in imaging mode.
Externí odkaz:
http://arxiv.org/abs/1107.3949
Autor:
Mathews, G. S., Dent, W. R. F., Williams, J. P., Howard, C. D., Meeus, G., Riaz, B., Roberge, A., Sandell, G., Vandenbussche, B., Duchêne, G., Kamp, I., Ménard, F., Montesinos, B., Pinte, C., Thi, W. F., Woitke, P., Alacid, J. M., Andrews, S. M., Ardila, D. R., Aresu, G., Augereau, J. C., Barrado, D., Brittain, S., Ciardi, D. R., Danchi, W., Eiroa, C., Fedele, D., Grady, C. A., de Gregorio-Monsalvo, I., Heras, A., Huelamo, N., Krivov, A., Lebreton, J., Liseau, R., Martin-Zaidi, C., Mendigutía, I., Mora, A., Morales-Calderon, M., Nomura, H., Pantin, E., Pascucci, I., Phillips, N., Podio, L., Poelman, D. R., Ramsay, S., Rice, K., Riviere-Marichalar, P., Solano, E., Tilling, I., Walker, H., White, G. J., Wright, G., Collaboration, the GASPS
Context - Circumstellar discs are ubiquitous around young stars, but rapidly dissipate their gas and dust on timescales of a few Myr. The Herschel space observatory allows for the study of the warm disc atmosphere, using far-infrared spectroscopy to
Externí odkaz:
http://arxiv.org/abs/1005.3864
Autor:
Pinte, C., Woitke, P., Menard, F., Duchene, G., Kamp, I., Meeus, G., Mathews, G. S., Howard, C. D., Grady, C. A., Thi, W. -F., Tilling, I., Augereau, J. -C., Dent, W. R. F., Alacid, J. M., Andrews, S., Ardila, D. R., Aresu, G., Barrado, D., Brittain, S., Ciardi, D. R., Danchi, W., Eiroa, C., Fedele, D., de Gregorio-Monsalvo, I., Heras, A., Huelamo, N., Krivov, A., Lebreton, J., Liseau, R., Martin-Zaidi, C., Mendigutia, I., Montesinos, B., Mora, A., Morales-Calderon, M., Nomura, H., Pantin, E., Pascucci, I., Phillips, N., Podio, L., Poelman, D. R., Ramsay, S., Riaz, B., Rice, K., Riviere-Marichalar, P., Roberge, A., Sandell, G., Solano, E., Vandenbussche, B., Walker, H., Williams, J. P., White, G. J., Wright, G.
The Herschel GASPS Key Program is a survey of the gas phase of protoplanetary discs, targeting 240 objects which cover a large range of ages, spectral types, and disc properties. To interpret this large quantity of data and initiate self-consistent a
Externí odkaz:
http://arxiv.org/abs/1005.3826
Autor:
Thi, W. F., Mathews, G., Ménard, F., Woitke, P., Meeus, G., Riviere-Marichalar, P., Pinte, C., Howard, C. D., Roberge, A., Sandell, G., Pascucci, I., Riaz, B., Grady, C. A., Dent, W. R. F., Kamp, I., Duchêne, G., Augereau, J. C., Pantin, E., Vandenbussche, B., Tilling, I., Williams, J. P., Eiroa, C., Barrado, D., Alacid, J. M., Andrews, S., Ardila, D. R., Aresu, G., Brittain, S., Ciardi, D. R., Danchi, W., Fedele, D., de Gregorio-Monsalvo, I., Heras, A., Huelamo, N., Krivov, A., Lebreton, J., Liseau, R., Martin-Zaidi, C., Mendigutía, I., Montesinos, B., Mora, A., Morales-Calderon, M., Nomura, H., Phillips, N., Podio, L., Poelman, D. R., Ramsay, S., Rice, K., Solano, E., Walker, H., White, G. J., Wright, G.
Planets are formed in disks around young stars. With an age of ~10 Myr, TW Hya is one of the nearest T Tauri stars that is still surrounded by a relatively massive disk. In addition a large number of molecules has been found in the TW Hya disk, makin
Externí odkaz:
http://arxiv.org/abs/1005.3830
Autor:
Meeus, G., Pinte, C., Woitke, P., Montesinos, B., Mendigutía, I., Riviere-Marichalar, P., Eiroa, C., Mathews, G. S., Vandenbussche, B., Howard, C. D., Roberge, A., Sandell, G., Duchêne, G., Ménard, F., Grady, C. A., Dent, W. R. F., Kamp, I., Augereau, J. C., Thi, W. F., Tilling, I., Alacid, J. M., Andrews, S., Ardila, D. R., Aresu, G., Barrado, D., Brittain, S., Ciardi, D. R., Danchi, W., Fedele, D., de Gregorio-Monsalvo, I., Heras, A., Huelamo, N., Krivov, A., Lebreton, J., Liseau, R., Martin-Zaidi, C., Mora, A., Morales-Calderon, M., Nomura, H., Pantin, E., Pascucci, I., Phillips, N., Podio, L., Poelman, D. R., Ramsay, S., Riaz, B., Rice, K., Solano, E., Walker, H., White, G. J., Williams, J. P., Wright, G., Collaboration, the GASPS
In an effort to simultaneously study the gas and dust components of the disc surrounding the young Herbig Ae star HD 169142, we present far-IR observations obtained with the PACS instrument onboard the Herschel Space Observatory. This work is part of
Externí odkaz:
http://arxiv.org/abs/1005.3828
Akademický článek
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Publikováno v:
ASP Conference Series; 2016, Vol. 512, p181-184, 4p
