File:Near-infrared spectrum of EM170817 at 4.5 days after binary neutron star merger.jpg

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English: For display purposes, the data have been smoothed using a Savitzky-Golay filter (solid black line), and the unfiltered data are shown in grey. A predicted model macronova spectrum (23) assuming an ejecta mass of Mej = 0.05M☉ and a velocity of v = 0.1c at a phase of 4.5 days post merger is shown in red. The spectra have been corrected for Milky Way extinction assuming reddening E(B – V) = 0.1 (10). Regions of low signal-to-noise ratio from strong telluric absorption by the Earth’s atmosphere between the near-infrared J, H, and K spectral windows are indicated by the vertical dark grey bars. The light grey shaded band is the blackbody which best fits the photometric measurements at 4.5 days (10).
Date
Source https://arxiv.org/abs/1710.05436
Author M. M. Kasliwal, E. Nakar, L. P. Singer, D. L. Kaplan, D. O. Cook, A. Van Sistine, R. M. Lau, C. Fremling, O. Gottlieb, J. E. Jencson, S.M. Adams, U. Feindt, K. Hotokezaka, S. Ghosh, D. A. Perley, P.-C. Yu, T. Piran, J. R. Allison, G. C. Anupama, A.Balasubramanian, K. W Bannister, J. Bally, J. Barnes, S. Barway, E. Bellm, V. Bhalerao, D. Bhattacharya, N. Blagorodnova, J. S. Bloom, P. R. Brady, C. Cannella, D. Chatterjee, S. B. Cenko, B. E. Cobb, C. Copperwheat, A. Corsi, K. De, D. Dobie, S. W. K. Emery, P. A. Evans, O. D. Fox, D. A. Frail, C. Frohmaier, A. Goobar, G. Hallinan, F. Harrison, G. Helou, T. Hinderer, A. Y. Q. Ho, A. Horesh, W.-H. Ip, R. Itoh, D. Kasen, H. Kim, N.P.M. Kuin, T. Kupfer, C. Lynch, K. Madsen, P. A. Mazzali, A. A. Miller, K. Mooley, T. Murphy, C.-C. Ngeow, D. Nichols, S. Nissanke, P. Nugent, E. O. Ofek, H. Qi, R. M. Quimby, S. Rosswog, F. Rusu, E. M. Sadler, P. Schmidt, J. Sollerman, I. Steele, A. R. Williamson, Y. Xu, L. Yan, Y. Yatsu, C. Zhang, W. Zhao


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Date/TimeThumbnailDimensionsUserComment
current00:42, 23 October 2017Thumbnail for version as of 00:42, 23 October 20171,280 × 967 (88 KB)ActiveDendrite (talk | contribs)User created page with UploadWizard

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