Zobrazeno 1 - 10
of 794
pro vyhledávání: '"PUECH, M."'
Autor:
Hammer, F., Morris, S., Cuby, J. G., Kaper, L., Steinmetz, M., Afonso, J., Barbuy, B., Bergin, E., Finogenov, A., Gallego, J., Kassin, S., Miller, C., Ostlin, G., Penterricci, L., Schaerer, D., Ziegler, B., Chemla, F., Dalton, G., De Frondat, F., Evans, C., Mignant, D. Le, Puech, M., Rodrigues, M., Sanchez-Janssen, R., Taburet, S., Tasca, L., Yang, Y. B., Zanchetta, S., Dohlen, K., Dubbeldam, M., Hadi, K. El, Janssen, A., Kelz, A., Larrieu, M., Lewis, I., MacIntosh, M., Morris, T., Navarro, R., Seifert, W.
The powerful combination of the cutting-edge multi-object spectrograph MOSAIC with the world largest telescope, the ELT, will allow us to probe deeper into the Universe than was possible. MOSAIC is an extremely efficient instrument in providing spect
Externí odkaz:
http://arxiv.org/abs/2011.03549
Autor:
Japelj, J., Laigle, C., Puech, M., Pichon, C., Rahmani, H., Dubois, Y., Devriendt, J. E. G., Petitjean, P., Hammer, F., Gendron, E., Kaper, L., Morris, S., Pirzkal, N., Sánchez-Janssen, R., Slyz, A., Vergani, S. D., Yang, Y.
Publikováno v:
A&A 632, A94 (2019)
Mapping of the large-scale structure through cosmic time has numerous applications in the studies of cosmology and galaxy evolution. At $z > 2$, the structure can be traced by the neutral intergalactic medium (IGM) by way of observing the Ly$\alpha$,
Externí odkaz:
http://arxiv.org/abs/1911.00021
We have found that the high velocity dispersions of dwarf spheroidal galaxies (dSphs) can be well explained by Milky Way (MW) tidal shocks, which reproduce precisely the gravitational acceleration previously attributed to dark matter (DM). Here we su
Externí odkaz:
http://arxiv.org/abs/1909.07979
Quantitative spectroscopy of O-type stars in galaxies beyond 1 Mpc requires the unprecedented sensitivity of the so-called Extremely Large Telescopes. Visible spectroscopy with these exciting new facilities will give us the first chance to explore th
Externí odkaz:
http://arxiv.org/abs/1810.01738
Autor:
Evans, C. J., Barbuy, B., Castilho, B., Smiljanic, R., Melendez, J., Japelj, J., Cristiani, S., Snodgrass, C., Bonifacio, P., Puech, M., Quirrenbach, A.
In the era of Extremely Large Telescopes, the current generation of 8-10m facilities are likely to remain competitive at far-blue visible wavelengths for the foreseeable future. High-efficiency (>20%) observations of the ground UV (300-400 nm) at med
Externí odkaz:
http://arxiv.org/abs/1806.11173
Autor:
Puech, M., Evans, C. J., Disseau, K., Japelj, J., Ramírez-Agudelo, O. H., Rahmani, H., Trevisan, M., Wang, J. L., Rodrigues, M., Sánchez-Janssen, R., Yang, Y., Hammer, F., Kaper, L., Morris, S. L., Barbuy, B., Cuby, J. -G., Dalton, G., Fitzsimons, E., Jagourel, P., Team, the MOSAIC Science
We present the consolidated scientific case for multi-object spectroscopy with the MOSAIC concept on the European ELT. The cases span the full range of ELT science and require either 'high multiplex' or 'high definition' observations to best exploit
Externí odkaz:
http://arxiv.org/abs/1806.03296
Recent observations of our neighbouring galaxy M31 have revealed that its disk was shaped by widespread events. The evidence for this includes the high dispersion ($V/\sigma$ $\le$ 3) of stars older than 2 Gyr, and a global star formation episode, 2-
Externí odkaz:
http://arxiv.org/abs/1801.04279
Autor:
Acero, F., Acquaviva, J. -T., Adam, R., Aghanim, N., Allen, M., Alves, M., Ammanouil, R., Ansari, R., Araudo, A., Armengaud, E., Ascaso, B., Athanassoula, E., Aubert, D., Babak, S., Bacmann, A., Banday, A., Barriere, K., Bellossi, F., Bernard, J. -P., Bernardini, M. G., Béthermin, M., Blanc, E., Blanchet, L., Bobin, J., Boissier, S., Boisson, C., Boselli, A., Bosma, A., Bosse, S., Bottinelli, S., Boulanger, F., Boyer, R., Bracco, A., Briand, C., Bucher, M., Buat, V., Cambresy, L., Caillat, M., Casandjian, J. -M., Caux, E., Célestin, S., Cerruti, M., Charlot, P., Chassande-Mottin, E., Chaty, S., Christensen, N., Ciesla, L., Clerc, N., Cohen-Tanugi, J., Cognard, I., Combes, F., Comis, B., Corbel, S., Cordier, B., Coriat, M., Courtin, R., Courtois, H., Da Silva, B., Daddi, E., Dallier, R., Dartois, E., Demyk, K., Denis, J. -M., Denis, L., Djannati-Ataï, A., Donati, J. -F., Douspis, M., van Driel, W., Korso, M. N. El, Falgarone, E., Fantina, A., Farges, T., Ferrari, A., Ferrari, C., Ferrière, K., Flamary, R., Gac, N., Gauffre, S., Genova, F., Girard, J., Grenier, I., Griessmeier, J. -M., Guillard, P., Guillemot, L., Gulminelli, F., Gusdorf, A., Habart, E., Hammer, F., Hennebelle, P., Herpin, F., Hervet, O., Hughes, A., Ilbert, O., Janvier, M., Josselin, E., Julier, A., Lachaud, C., Lagache, G., Lallement, R., Lambert, S., Lamy, L., Langer, M., Larzabal, P., Lavaux, G., Bertre, T. Le, Fèvre, O. Le, Tiec, A. Le, Lefloch, B., Lehnert, M., Lemoine-Goumard, M., Levrier, F., Limousin, M., Lis, D., López-Sepulcre, A., Macias-Perez, J., Magneville, C., Marcowith, A., Margueron, J., Marquette, G., Marshall, D., Martin, L., Mary, D., Masson, S., Maurogordato, S., Mazauric, C., Mellier, Y., Miville-Deschênes, M. -A., Montier, L., Mottez, F., Mourard, D., Nesvadba, N., Nezan, J. -F., Noterdaeme, P., Novak, J., Ocvirk, P., Oertel, M., Olive, X., Ollier, V., Palanque-Delabrouille, N., Pandey-Pommier, M., Pennec, Y., Pérault, M., Peroux, C., Petit, P., Pétri, J., Petiteau, A., Pety, J., Pratt, G. W., Puech, M., Quertier, B., Raffin, E., Harison, S. Rakotozafy, Rawson, S., Renaud, M., Revenu, B., Richard, C., Richard, J., Rincon, F., Ristorcelli, I., Rodriguez, J., Schultheis, M., Schimd, C., Semelin, B., Sol, H., Starck, J. -L., Tagger, M., Tasse, C., Theureau, G., Torchinsky, S., Vastel, C., Vergani, S. D., Verstraete, L., Vigouroux, X., Vilmer, N., Vilotte, J. -P., Webb, N., Ysard, N., Zarka, P.
The "Square Kilometre Array" (SKA) is a large international radio telescope project characterised, as suggested by its name, by a total collecting area of approximately one square kilometre, and consisting of several interferometric arrays to observe
Externí odkaz:
http://arxiv.org/abs/1712.06950
Most giant spiral galaxies have pseudo or disk-like bulges that are considered to be the result of purely secular processes. This may challenge the hierarchical scenario predicting about one major merger per massive galaxy ($>$$3\times 10^{10} M_{\od
Externí odkaz:
http://arxiv.org/abs/1709.07455
Autor:
Izzo, L., Thöne, C. C., Schulze, S., Mehner, A., Flores, H., Cano, Z., Postigo, A. de Ugarte, Kann, D. A., Amorìn, R., Anderson, J. P., Bauer, F. E., Bensch, K., Christensen, L., Covino, S., Della Valle, M., Fynbo, J. P. U., Jakobsson, P., Klose, S., Kuncarayakti, H., Leloudas, G., Milvang-Jensen, B., Möller, P., Puech, M., Rossi, A., Sànchez-Ramìrez, R., Vergani, S. D.
The low distance, $z=0.0591$, of GRB 100316D and its association with SN 2010bh represent two important motivations for studying this host galaxy and the GRB's immediate environment with the Integral-Field Spectrographs like VLT/MUSE. Its large field
Externí odkaz:
http://arxiv.org/abs/1704.05509