Anna Pancoast et al ApJ This technique features some advantages over classical methods, i. Filippenko , Elinor L. This problem has been solved now with our new flux-calibrated models. This indirectly maps the galaxy morphology, i. Cassisi and Padova tracks have also been chosen because they are different in some key aspects such as the treatment of overshooting or the mixing-length parameter as summarized below. For 2 of these , it was possible to resolve the companions as well.
THE LICK AGN MONITORING PROJECT 2011: DYNAMICAL MODELING OF THE BROAD-LINE REGION IN Mrk 50
The magenta lines are the model based on Padova tracks at high metallicities, and the cyan lines are the model of Schiavon The forbidden zone in the index domain is shaded, according to eq. We identified three major types of Purkinje cells based on their firing patterns during licking behavior. This same value is kept in the tracks with supersolar metallicities Bono et al. A proper fit to the data including the variation of various other element abundance ratios is presented in Paper II. The chamber and head post were secured into place with dental acrylic Teets methyl methacrylate denture material; CoOral-Lite Mfg. He is the co-editor and co-author, with Charles H.
D—F Comparison by response type. Gaussian Processes have been found to be a good model for larger samples of AGN light curves Kelly et al. The histograms in the left column show the lick-spike correlations all licks included for the four units. Examples of acceptable transfer functions for Mrk The key novelty compared to our previous models is that they are now available at the higher spectral resolution of MILES 2.
Member since July, From: For each index, the blue and red sidebands are marked, flanking the relevant feature window. The key novelty compared to our previous models is that they are now available at the higher spectral resolution of MILES 2. Email alerts New issue alert. The Lick group have defined a set of 25 optical absorption-line indices Burstein et al. In addition, we allow for a scaling factor to describe the percentage variability of the emission line compared to that of the continuum. In addition, index re- definition in terms of narrow-band "color" should be preferred over the classical pseudo-equivalent width scheme.