Zobrazeno 1 - 10
of 437
pro vyhledávání: '"Walsh, J R"'
Publikováno v:
A&A 690, A264 (2024)
The optical line and continuum emission in the very high ionization Galactic planetary nebula (PN) NGC 4361 (PN G294.1 +43.6), has been mapped with VLT MUSE Wide Field normal mode (4750-9300A) commissioning observations. The PN is larger than a singl
Externí odkaz:
http://arxiv.org/abs/2408.02381
Autor:
Akras, S., Monteiro, H., Walsh, J. R., García-Rojas, J., Aleman, I., Boffin, H., Boumis, P., Chiotellis, A., Corradi, R. M. L., Gonçalves, D. R., Gutiérrez-Soto, L. A., Jones, D., Morisset, C., Papanikolaou, X.
Integral field spectroscopy (IFS) provides a unique capability to spectroscopically study extended sources over a 2D field of view, but it also requires new techniques and tools. In this paper, we present an automatic code, Spectroscopic Analysis Too
Externí odkaz:
http://arxiv.org/abs/2203.06175
Autor:
Walsh, J. R., Monreal-Ibero, A.
The Multi-Unit Spectroscopic Explorer (MUSE) is a large integral field unit mounted on the ESO Very Large Telescope. Its spatial (60 arcsecond field) and wavelength (4800-9300A) coverage is well suited to detailed imaging spectroscopy of extended pla
Externí odkaz:
http://arxiv.org/abs/2004.03182
Akademický článek
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Autor:
Walsh, J. R., Monreal-Ibero, A., Barlow, M. J., Ueta, T., Wesson, R., Zijlstra, A. A., Kimeswenger, S., Leal-Ferreira, M. L., Otsuka, M.
Publikováno v:
A&A 620, A169 (2018)
The spatial structure of the emission lines and continuum over the 50 arcsecond extent of the nearby, O-rich, planetary nebula NGC 7009 (Saturn Nebula) have been observed with the MUSE integral field spectrograph on the ESO Very Large Telescope. Scie
Externí odkaz:
http://arxiv.org/abs/1810.03984
Autor:
Beccari, G., Petr-Gotzens, M. G., Boffin, H. M. J., Romaniello, M., Fedele, D., Carraro, G., De Marchi, G., de Wit, W. -J., Drew, J. E., Kalari, V. M., Manara, C. F., Martin, E. L., Mieske, S., Panagia, N., Testi, L., Vink, J. S., Walsh, J. R., Wright, N. J.
Publikováno v:
A&A 604, A22 (2017)
As part of the Accretion Discs in H$\alpha$ with OmegaCAM (ADHOC) survey, we imaged in r, i and H-alpha a region of 12x8 square degrees around the Orion Nebula Cluster. Thanks to the high-quality photometry obtained, we discovered three well-separate
Externí odkaz:
http://arxiv.org/abs/1705.09496
Autor:
Golling, T., Hance, M., Harris, P., Mangano, M. L., McCullough, M., Moortgat, F., Schwaller, P., Torre, R., Agrawal, P., Alves, D. S. M., Antusch, S., Arbey, A., Auerbach, B., Bambhaniya, G., Battaglia, M., Bauer, M., Dev, P. S. Bhupal, Boveia, A., Bramante, J., Buchmueller, O., Buschmann, M., Chakrabortty, J., Chala, M., Chekanov, S., Chen, C. -Y., Cheng, H. -C., Cirelli, M., Citron, M., Cohen, T., Craig, N., Curtin, D., D'Agnolo, R. T., Doglioni, C., Dror, J. A., Pree, T. du, Dylewsky, D., Ellis, J., Ellis, S. A. R., Essig, R., Fan, J. J., Farina, M., Feng, J. L., Fox, P. J., Galloway, J., Giudice, G., Gluza, J., Gori, S., Guha, S., Hahn, K., Han, T., Helsens, C., Henriques, A., Iwamoto, S., Jelinski, T., Jung, S., Kahlhoefer, F., Khoze, V. V., Kim, D., Kopp, J., Kotwal, A., Kraemer, M., Lindert, J. M., Liu, J., Lou, H. K., Love, J., Low, M., Machado, P. A. N., Mahmoudi, F., Marrouche, J., Martin, A., Mohan, K., Mohapatra, R. N., Nardini, G., Olive, K. A., Ostdiek, B., Panico, G., Plehn, T., Proudfoot, J., Qian, Z., Reece, M., Rizzo, T., Roskas, C., Ruderman, J., Ruiz, R., Sala, F., Salvioni, E., Saraswat, P., Schell, T., Schmidt-Hoberg, K., Serra, J., Shadmi, Y., Shelton, J., Solans, C., Spannowsky, M., Srivastava, T., Stolarski, D., Szafron, R., Taoso, M., Tarem, S., Thalapillil, A., Thamm, A., Tsai, Y., Verhaaren, C., Vignaroli, N., Walsh, J. R., Wang, L. T., Weiland, C., Wells, J., Williams, C., Wulzer, A., Xue, W., Yu, F., Zheng, B., Zheng, J.
This report summarises the physics opportunities in the search and study of physics beyond the Standard Model at a 100 TeV pp collider.
Comment: 196 pages, 114 figures. Chapter 3 of the "Physics at the FCC-hh" Report
Comment: 196 pages, 114 figures. Chapter 3 of the "Physics at the FCC-hh" Report
Externí odkaz:
http://arxiv.org/abs/1606.00947
The large field and wavelength range of MUSE is well suited to mapping Galactic planetary nebulae (PN). The bright PN NGC 7009 was observed with MUSE on the VLT during the Science Verification of the instrument in seeing of 0.6". Emission line maps i
Externí odkaz:
http://arxiv.org/abs/1602.06788
Publikováno v:
A&A 574, A109 (2015)
Imaging and spectroscopic observations of planetary nebulae (PNe) in the nearest large elliptical galaxy NGC 5128 (Centaurus A), were obtained to find more PNe and measure their radial velocities. NTT imaging was obtained in 15 fields in NGC 5128 ove
Externí odkaz:
http://arxiv.org/abs/1501.01853
Publikováno v:
Progress in Additive Manufacturing; Aug2024, Vol. 9 Issue 4, p1025-1038, 14p