Zobrazeno 1 - 10
of 172
pro vyhledávání: '"Fabbri J"'
Autor:
Dark Energy Survey Collaboration, Abbott, T., Abdalla, F. B., Aleksic, J., Allam, S., Amara, A., Bacon, D., Balbinot, E., Banerji, M., Bechtol, K., Benoit-Levy, A., Bernstein, G. M., Bertin, E., Blazek, J., Bonnett, C., Bridle, S., Brooks, D., Brunner, R. J., Buckley-Geer, E., Burke, D. L., Caminha, G. B., Capozzi, D., Carlsen, J., Carnero-Rosell, A., Carollo, M., Carrasco-Kind, M., Carretero, J., Castander, F. J., Clerkin, L., Collett, T., Conselice, C., Crocce, M., Cunha, C. E., D'Andrea, C. B., da Costa, L. N., Davis, T. M., Desai, S., Diehl, H. T., Dietrich, J. P., Dodelson, S., Doel, P., Drlica-Wagner, A., Estrada, J., Etherington, J., Evrard, A. E., Fabbri, J., Finley, D. A., Flaugher, B., Foley, R. J., Rosalba, P., Frieman, J., Garcia-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Goldstein, D. A., Gruen, D., Gruendl, R. A., Guarnieri, P., Gutierrez, G., Hartley, W., Honscheid, K., Jain, B., James, D. J., Jeltema, T., Jouvel, S., Kessler, R., King, A., Kirk, D., Kron, R., Kuehn, K., Kuropatkin, N., Lahav, O., Li, T. S., Lima, M., Lin, H., Maia, M. A. G., Makler, M., Manera, M., Maraston, C., Marshall, J. L., Martini, P., McMahon, R. G., Melchior, P., Merson, A., Miller, C. J., Miquel, R., Mohr, J. J., Morice-Atkinson, X., Naidoo, K., Neilsen, E., Nichol, R. C., Nord, B., Ogando, R., Ostrovski, F., Palmese, A., Papadopoulos, A., Peiris, H., Peoples, J., Percival, W. J., Plazas, A. A., Reed, S. L., Refregier, A., Romer, A. K., Roodman, A., Ross, A., Rozo, E., Rykoff, E. S., Sadeh, I., Sako, M., Sanchez, C., Sanchez, E., Santiago, B., Scarpine, V., Schubnell, M., Sevilla-Noarbe, I., Sheldon, E., Smith, M., Smith, R. C., Soares-Santos, M., Sobreira, F., Soumagnac, M., Suchyta, E., Sullivan, M., Swanson, M., Tarle, G., Thaler, J., Thomas, D., Thomas, R. C., Tucker, D., Vieira, J. D., Vikram, V., Walker, A. R., Wechsler, R. H., Weller, J., Wester, W., Whiteway, L., Wilcox, H., Yanny, B., Zhang, Y., Zuntz, J.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 460 (2016) no. 2, 1270-1299
This overview article describes the legacy prospect and discovery potential of the Dark Energy Survey (DES) beyond cosmological studies, illustrating it with examples from the DES early data. DES is using a wide-field camera (DECam) on the 4m Blanco
Externí odkaz:
http://arxiv.org/abs/1601.00329
Autor:
Gallagher, Joseph S., Sugerman, B. E. K., Clayton, Geoffrey C., Andrews, J. E., Clem, J., Barlow, M. J., Ercolano, B., Fabbri, J., Otsuka, M., Wesson, R., Meixner, M.
We present nebular phase optical imaging and spectroscopy and near/mid-IR imaging of the Type II SN 2006bc. Observations reveal the central wavelength of the symmetric H$\alpha$ line profile to be red-shifted with respect to the host galaxy H$\alpha$
Externí odkaz:
http://arxiv.org/abs/1205.5517
Autor:
Fabbri, J., Otsuka, M., Barlow, M. J., Gallagher, Joseph S., Wesson, R., Sugerman, B. E. K., Clayton, Geoffrey C., Meixner, M., Andrews, J. E., Welch, D. L., Ercolano, B.
We present an analysis of multi-epoch observations of the Type II-P supernova SN 2004et. New and archival optical spectra of SN 2004et are used to study the evolution of the Halpha and [O I] 6300A line profiles between days 259 and 646. Mid-infrared
Externí odkaz:
http://arxiv.org/abs/1110.3166
Autor:
Andrews, J. E., Clayton, Geoffrey C., Wesson, R., Sugerman, B. E. K., Barlow, M. J., Clem, J., Ercolano, B., Fabbri, J., Gallagher, J. S., Landolt, A., Meixner, M., Otsuka, M., Riebel, D., Welch, D. L.
SN 2010jl was an extremely bright, Type IIn SNe which showed a significant IR excess no later than 90 days after explosion. We have obtained Spitzer 3.6 and 4.5 \mum and JHK observations of SN 2010jl \sim90 days post explosion. Little to no reddening
Externí odkaz:
http://arxiv.org/abs/1106.0537
Autor:
Andrews, J. E., Sugerman, B. E. K, Clayton, Geoffrey, Gallagher, J. S., Barlow, M. J., Clem, J., Ercolano, B., Fabbri, J., Meixner, M., Otsuka, M., Welch, D. L., Wesson, R.
SN 2007it is a bright, Type IIP supernova which shows indications of both pre-existing and newly formed dust. The visible photometry shows a bright late-time luminosity, powered by the 0.09 M$_{\sun}$ of $^{56}$Ni present in the ejecta. There is also
Externí odkaz:
http://arxiv.org/abs/1102.2431
Autor:
Andrews, J. E., Gallagher, J. S., Clayton, Geoffrey C., Sugerman, B. E. K., Chatelain, J. P., Clem, J., Welch, D. L., Barlow, M. J., Ercolano, B., Fabbri, J., Wesson, R., Meixner, M.
SN 2007od exhibits characteristics that have rarely been seen in a Type IIP supernova (SN). Optical V band photometry reveals a very steep brightness decline between the plateau and nebular phases of ~4.5 mag, likely due to SN 2007od containing a low
Externí odkaz:
http://arxiv.org/abs/1004.1209
Autor:
Wesson, R., Barlow, M. J., Ercolano, B., Andrews, J. E., Clayton, Geoffrey C., Fabbri, J., Gallagher, Joseph S., Meixner, M., Sugerman, B. E. K., Welch, D. L., Stock, D. J.
SN 2008S erupted in early 2008 in the grand design spiral galaxy NGC 6946. The progenitor was detected by Prieto et al. in Spitzer Space Telescope images taken over the four years prior to the explosion, but was not detected in deep optical images, f
Externí odkaz:
http://arxiv.org/abs/0907.0246
Autor:
Barlow, M. J., Sugerman, B. E. K., Fabbri, J., Meixner, M., Fisher, R. S., Bowey, J. E., Panagia, N., Ercolano, B., Clayton, G. C., Cohen, M., Gledhill, T. M., Gordon, K., Tielens, A. G. G. M., Zijlstra, A. A.
Dust emission from the Type II supernova SN 2002hh in NGC 6946 has been detected at mid-infrared wavelengths by the Spitzer Space Telescope from 590 to 758 days after outburst and confirmed by higher angular resolution Gemini-N mid-IR observations. T
Externí odkaz:
http://arxiv.org/abs/astro-ph/0506542
Autor:
Martinez, E., Saidi, B., Veillerot, M., Caubet, P., Fabbri, J-M., Piallat, F., Gassilloud, R., Schamm-Chardon, S.
Publikováno v:
In Journal of Electron Spectroscopy and Related Phenomena August 2015 203:1-7
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