Zobrazeno 1 - 10
of 819
pro vyhledávání: '"Sacchi N"'
Autor:
Sacchi, N., Ciceri, F., Bonifazi, F., Algeri, M., Gallina, A., Pollichieni, S., Raggio, E., Hadj-Amar, B., Lombardini, L., Pupella, S., Liumbruno, G., Cardillo, M.
Publikováno v:
In Human Immunology October 2021 82(10):758-766
Autor:
Davies, J. I., Wilson, C. D., Auld, R., Baes, M., Barlow, M. J., Bendo, G. J., Bock, J. J., Boselli, A., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Cortese, L., Dwek, E., Eales, S. A., Elbaz, D., Galametz, M., Galliano, F., Gear, W. K., Glenn, J., Gomez, H. L., Griffin, M., Hony, S., Isaak, K. G., Levenson, L. R., Lu, N., Madden, S., O'Halloran, B., Okumura, K., Oliver, S., Page, M. J., Panuzzo, P., Papageorgiou, A., Parkin, T. J., Perez-Fournon, I., Pohlen, M., Rangwala, N., Rigby, E. E., Roussel, H., Rykala, A., Sacchi, N., Sauvage, M., Schulz, B., Schirm, M. R. P., Smith, M. W. L., Spinoglio, L., Stevens, J. A., Srinivasan, S., Symeonidis, M., Trichas, M., Vaccari, M., Vigroux, L., Wozniak, H., Wright, G. S., Zeilinger, W. W.
Galactic cirrus emission at far-infrared wavelengths affects many extragalactic observations. Separating this emission from that associated with extragalactic objects is both important and difficult. In this paper we discuss a particular case, the M8
Externí odkaz:
http://arxiv.org/abs/1010.4770
Autor:
Pohlen, M., Cortese, L., Smith, M. W. L., Eales, S. A., Boselli, A., Bendo, G. J., Gomez, H. L., Papageorgiou, A., Auld, R., Baes, M., Bock, J. J., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Dwek, E., Elbaz, D., Galametz, M., Galliano, F., Gear, W. K., Glenn, J., Griffin, M., Hony, S., Isaak, K. G., Levenson, L. R., Lu, N., Madden, S., O'Halloran, B., Okumura, K., Oliver, S., Page, M. J., Panuzzo, P., Parkin, T. J., Perez-Fournon, I., Rangwala, N., Rigby, E. E., Roussel, H., Rykala, A., Sacchi, N., Sauvage, M., Schulz, B., Schirm, M. R. P., Spinoglio, L., Stevens, J. A., Srinivasan, S., Symeonidis, M., Trichas, M., Vaccari, M., Vigroux, L., Wilson, C. D., Wozniak, H., Wright, G. S., Zeiliner, W. W.
By combining Herschel-SPIRE data with archival Spitzer, HI, and CO maps, we investigate the spatial distribution of gas and dust in the two famous grand-design spirals M99 and M100 in the Virgo cluster. Thanks to the unique resolution and sensitivity
Externí odkaz:
http://arxiv.org/abs/1005.5476
Autor:
Cortese, L., Bendo, G. J., Boselli, A., Davies, J. I., Gomez, H. L., Pohlen, M., Auld, R., Baes, M., Bock, J. J., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Dwek, E., Eales, S. A., Elbaz, D., Galametz, M., Galliano, F., Gear, W. K., Glenn, J., Griffin, M., Hony, S., Isaak, K. G., Levenson, L. R., Lu, N., Madden, S., O'Halloran, B., Okumura, K., Oliver, S., Page, M. J., Panuzzo, P., Papageorgiou, A., Parkin, T. J., Perez-Fournon, I., Rangwala, N., Rigby, E. E., Roussel, H., Rykala, A., Sacchi, N., Sauvage, M., Schulz, B., Schirm, M. R. P., Smith, M. W. L., Spinoglio, L., Stevens, J. A., Srinivasan, S., Symeonidis, M., Trichas, M., Vaccari, M., Vigroux, L., Wilson, C. D., Wozniak, H., Wright, G. S., Zeilinger, W. W.
We present Herschel-SPIRE observations of the perturbed galaxy NGC4438 in the Virgo cluster. These images reveal the presence of extra-planar dust up to ~4-5 kpc away from the galaxy's disk. The dust closely follows the distribution of the stripped a
Externí odkaz:
http://arxiv.org/abs/1005.2331
Autor:
O'Halloran, B., Galametz, M., Madden, S. C., Galliano, F., Hony, S., Sauvage, M., Pohlen, M., Bendo, G. J., Auld, R., Baes, M., Barlow, M. J., Bock, J. J., Boselli, A., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Cortese, L., Davies, J. I., Dwek, E., Eales, S. A., Elbaz, D., Gear, W. K., Glenn, J., Gomez, H. L., Griffin, M., Isaak, K. G., Levenson, L. R., Lu, N., Okumura, K., Oliver, S., Page, M. J., Panuzzo, P., Papageorgiou, A., Parkin, T. J., Perez-Fournon, I., Rangwala, N., Rigby, E. E., Roussel, H., Rykala, A., Sacchi, N., Schulz, B., Schirm, M. R. P., Smith, M. W. L., Spinoglio, L., Stevens, J. A., Sundar, S., Symeonidis, M., Trichas, M., Vaccari, M., Vigroux, L., Wilson, C. D., Wozniak, H., Wright, G. S., Zeilinger, W. W.
We present Herschel SPIRE and PACS photometeric observations of the low metallicity (Z ~ 0.35 solar) nearby dwarf galaxy, NGC 1705, in six wavelength bands as part of the Dwarf Galaxy Survey guaranteed time Herschel Key Program. We confirm the presen
Externí odkaz:
http://arxiv.org/abs/1005.2091
Autor:
Eales, S. A., Smith, M. W. L., Wilson, C. D., Bendo, G. J., Cortese, L., Pohlen, M., Boselli, A., Gomez, H. L., Auld, R., Baes, M., Barlow, M. J., Bock, J. J., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Davies, J. I., Dwek, E., Elbaz, D., Galametz, M., Galliano, F., Gear, W. K., Glenn, J., Griffin, M., Hony, S., Isaak, K. G., Levenson, L. R., Lu, N., Madden, S., O'Halloran, B., Okumura, K., Oliver, S., Page, M. J., Panuzzo, P., Papageorgiou, A., Parkin, T. J., Perez-Fournon, I., Rangwala, N., Rigby, E. E., Roussel, H., Rykala, A., Sacchi, N., Sauvage, M., Schulz, B., Schirm, M. R. P., Spinoglio, L., Srinivasan, S., Stevens, J. A., Symeonidis, M., Trichas, M., Vaccari, M., Vigroux, L., Wozniak, H., Wright, G. S., Zeilinger, W. W.
The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with current telescopes to galaxies in the nearby universe. In this letter,
Externí odkaz:
http://arxiv.org/abs/1005.2113
Autor:
Galametz, M., Madden, S. C., Galliano, F., Hony, S., Sauvage, M., Pohlen, M., Bendo, G. J., Auld, R., Baes, M., Barlow, M. J., Bock, J. J., Boselli, A., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Cortese, L., Davies, J. I., Dwek, E., Eales, S. A., Elbaz, D., Gear, W. K., Glenn, J., Gomez, H. L., Griffin, M., Isaak, K. G., Levenson, L. R., Lu, N., O'Halloran, B., Okumura, K., Oliver, S., Page, M. J., Panuzzo, P., Papageorgiou, A., Parkin, T. J., Perez-Fournon, I., Rangwala, N., Rigby, E. E., Roussel, H., Rykala, A., Sacchi, N., Schulz, B., Schirm, M. R. P., Smith, M. W. L., Spinoglio, L., Stevens, J. A., Sundar, S., Symeonidis, M., Trichas, M., Vaccari, M., Vigroux, L., Wilson, C. D., Wozniak, H., Wright, G. S., Zeilinger, W. W.
We present the first Herschel PACS and SPIRE images of the low-metallicity galaxy NGC6822 observed from 70 to 500 mu and clearly resolve the HII regions with PACS and SPIRE. We find that the ratio 250/500 is dependent on the 24 mu surface brightness
Externí odkaz:
http://arxiv.org/abs/1005.1730
Autor:
Sauvage, M., Sacchi, N., Bendo, G. J., Boselli, A., Pohlen, M., Wilson, C. D., Auld, R., Baes, M., Barlow, M. J., Bock, J. J., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Cortese, L., Davies, J. I., Dwek, E., Eales, S. A., Elbaz, D., Galametz, M., Galliano, F., Gear, W. K., Glenn, J., Gomez, H. L., Griffin, M., Hony, S., Isaak, K. G., Levenson, L. R., Lu, N., Madden, S. C., O'Halloran, B., Okumura, K., Oliver, S., Page, M. J., Panuzzo, P., Papageorgiou, A., Parkin, T. J., Perez-Fournon, I., Rangwala, N., Rigby, E. E., Roussel, H., Rykala, A., Schulz, B., Schirm, M. R. P., Smith, M. W. L., Spinoglio, L., Stevens, J. A., Srinivasan, S., Symeonidis, M., Trichas, M., Vaccari, M., Vigroux, L., Wozniak, H., Wright, G. S., Zeilinger, W. W.
With appropriate spatial resolution, images of spiral galaxies in thermal infrared (~10 micron and beyond) often reveal a bright central component, distinct from the stellar bulge, superimposed on a disk with prominent spiral arms. ISO and Spitzer st
Externí odkaz:
http://arxiv.org/abs/1005.1848
Autor:
Bendo, G. J., Wilson, C. D., Pohlen, M., Sauvage, M., Auld, R., Baes, M., Barlow, M. J., Bock, J. J., Boselli, A., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Cortese, L., Davies, J. I., Dwek, E., Eales, S. A., Elbaz, D., Galametz, M., Galliano, F., Gear, W. K., Glenn, J., Gomez, H. L., Griffin, M., Hony, S., Isaak, K. G., Levenson, L. R., Lu, N., Madden, S., O'Halloran, B., Okumura, K., Oliver, S., Page, M. J., Panuzzo, P., Papageorgiou, A., Parkin, T. J., Perez-Fournon, I., Rangwala, N., Rigby, E. E., Roussel, H., Rykala, A., Sacchi, N., Schulz, B., Schirm, M. R. P., Smith, M. W. L., Spinoglio, L., Stevens, J. A., Sundar, S., Symeonidis, M., Trichas, M., Vaccari, M., Vigroux, L., Wozniak, H., Wright, G. S., Zeilinger, W. W.
We use Herschel Space Observatory data to place observational constraints on the peak and Rayleigh-Jeans slope of dust emission observed at 70-500 microns in the nearby spiral galaxy M81. We find that the ratios of wave bands between 160 and 500 micr
Externí odkaz:
http://arxiv.org/abs/1005.1889
Autor:
Panuzzo, P., Rangwala, N., Rykala, A., Isaak, K. G., Glenn, J., Wilson, C. D., Auld, R., Baes, M., Barlow, M. J., Bendo, G. J., Bock, J. J., Boselli, A., Bradford, M., Buat, V., Castro-Rodríguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Cortese, L., Davies, J. I., Dwek, E., Eales, S. A., Elbaz, D., Fulton, T., Galametz, M., Galliano, F., Gear, W. K., Gomez, H. L., Griffin, M., Hony, S., Levenson, L. R., Lu, N., Madden, S., O'Halloran, B., Okumura, K., Oliver, S., Page, M. J., Papageorgiou, A., Parkin, T. J., Pérez-Fournon, I., Pohlen, M., Polehampton, E. T., Rigby, E. E., Roussel, H., Sacchi, N., Sauvage, M., Schulz, B., Schirm, M. R. P., Smith, M. W. L., Spinoglio, L., Stevens, J. A., Srinivasan, S., Symeonidis, M., Swinyard, B., Trichas, M., Vaccari, M., Vigroux, L., Wozniak, H., Wright, G. S., Zeilinger, W. W.
We present the observations of the starburst galaxy M82 taken with the Herschel SPIRE Fourier Transform Spectrometer. The spectrum (194-671 {\mu}m) shows a prominent CO rotational ladder from J = 4-3 to 13-12 emitted by the central region of M82. The
Externí odkaz:
http://arxiv.org/abs/1005.1877