… Taking advantage of the short-wavelength coverage, we are able to study the so-called
big blue bump, the region in which the energy output peaks, in detail. Most objects exhibit a …

… ABSTRACT We discuss several models of quasar big blue bump … of the big blue bump: (1)
IR/VIS color represents the … color shows the slope of the big blue bump (in a region where it …

… -IR polarized flux as an indication of the blue underlying continuum, we seem to be sketching
in the true spectrum of the quasar big blue bump. The results so far look more intelligible …

… of a quasar (Ton 202)… big blue bump emission. In this case, the existence of the Balmer-edge
feature, seen in absorption in the shorter wavelength side, indicates that the big blue bump …

… ABSTRACT We discuss several models of quasar big blue bump … of the big blue bump: (1)
IR/VIS color represents the … shows the slope of the big blue bump (in a region where it domi- …

We determined the spin value of supermassive black hole (SMBH) in active galactic nuclei (AGN)
with investigated ultraviolet-to-optical spectral energy distribution, presented in the …

… quasar Big Blue Bump generally lead to bound-free continuum features, which may be in
absorption or emission. Searches for Lyman edges attributable to quasar … Small Blue Bump) …

… bump seems similar to that of 3C 273 but shifted to lower frequency—more of a big green
bump than a big blue bump… luminous quasars, leading one to speculate that it too has a bump, …

… We hypothesise that these red, strong-lined quasars have intrinsically weak Big Blue Bumps…
We therefore hypothesise that these quasars have intrinsically weak Big Blue Bumps. Note, …

… optically thin thermal, hypothesis for the optical/UV big blue bump (BBB) in active galactic
nuclei (AGNs). The most basic … quasars should avoid the shot noise in the IUE data, as well as …