BL Lacertae objects, generalgamma rays, observationsquasars, general X-rays, galaxiesROSAT observations of a large sample of bright gamma-ray (E > 100 MeV) blazars are presented. Results of a detailed spectral analysis in the soft $\\\sim$ 0.1-2.0 keV energy range are discussed in relation...
Things were well, and then gradually and quickly they weren’t, and in March I was admitted to the hospital in early labor at just shy of 24 weeks. Delivery was averted and a sleepless night spent and in the morning we realized, I wasn’t going home. I had a host of problems and ...
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Light comes from the sun.It also comes from flashlights,candles and streetlights.Light is important because it lets us see things.It can pass through clear objects,such as clear glass or clear plastic.But it cannot pass through objects that are not clear.Sunglasses will sto...
As more compression is introduced to the mix, the high dynamic range of the audio (difference between loud explosions and soft footsteps) will get smaller and smaller. While at first glance this might not seem ideal, mixes that include compression allow for MW to be enjoyed on just about any...
Shadows magnify behind strong objects when light is applied. In the brightest light our shadows try their hardest to be seen. Always hiding behind the view, afraid of the brightness that threatens their very existence. In the purest darkness they hide everywhere and in full light they exist onl...
Costumes must fit within the confines of the guest’s ticketed seat and must allow for safe passage of fans through the seating row. Toy or replica weapons are prohibited from entry. Any item that is deemed dangerous or perceived to be dangerous, unsafe (spikes, sharp looking objects, mallet...
Comptonization seen in the soft X-ray band is well explained by the adopted corona model in the case of radio loud objects. However, this Comptonization is much stronger in radio quiet objects and additional ad hoc assumed Comptonizing medium must be present. We speculate that perhaps in ...
If you need finer-grain control and wish to write low-level code to ascertain the strong-naming status of an assembly,you can do that too. Approach #2: Viewing Strong Name Details with IL DASM Visual Studio ships with a handy utility – the Microsoft Intermediate Language Disassembler (...
If the vRL NLSy1 galaxies are part of the population of RBL blazars, then are there XBL analogues to these objects, and if so, why have they not been detected? Acknowledgments: The authors thank GSU for support through the RPE program and the Lowell Observatory and Cerro Tololo Inter...