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Titlebook: Very-high-energy Gamma-ray Observations of Pulsar Wind Nebulae and Cataclysmic Variable Stars with M; Rubén López Coto Book 2017 Springer

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樓主: Entangle
21#
發(fā)表于 2025-3-25 06:39:29 | 只看該作者
22#
發(fā)表于 2025-3-25 07:43:09 | 只看該作者
turn is governed by pharmacokinetic factors, exposure levels, and the balance between activating and deactivating enzymes. The colon may be more susceptible to carcinogens than the liver, since lower levels of deactivating enzymes are present in intestinal cells. Moreover, exposure times to toxic c
23#
發(fā)表于 2025-3-25 14:12:51 | 只看該作者
24#
發(fā)表于 2025-3-25 17:57:19 | 只看該作者
Very-high-energy Gamma-ray Observations of Pulsar Wind Nebulae and Cataclysmic Variable Stars with M
25#
發(fā)表于 2025-3-25 21:28:43 | 只看該作者
26#
發(fā)表于 2025-3-26 02:15:41 | 只看該作者
Nova and Dwarf Nova Observations with MAGICassical Novae and additional outbursts from other Cataclysmic Variables. I will report on the observations performed with the MAGIC telescopes of the symbiotic nova YY Her, the DN ASASSN-13ax, and the Classical Nova V339 Del and present the contemporaneous updated analysis of Fermi-LAT data.
27#
發(fā)表于 2025-3-26 07:37:19 | 只看該作者
The Topo-Trigger: A New Stereo Trigger for Lowering the Energy Threshold of IACTsreshold of the instrument. We simulated the Topo-trigger concept using the standard MAGIC MonteCarlo and tested it with real telescope data. In this chapter I show the concept and results of these tests.
28#
發(fā)表于 2025-3-26 09:17:53 | 只看該作者
Introduction to Pulsar Wind Nebulaeof their broadband emission and an explanation of their two main components: the synchrotron and inverse Compton emission. I also expose the state of the art models predicting gamma-ray emission from these sources.
29#
發(fā)表于 2025-3-26 15:20:39 | 只看該作者
Multiwavelength Campaign on AE Aquarii emission at the spin frequency of the White Dwarf and pulsed emission at different frequencies and did not find any evidence of VHE gamma-ray emission. I established the most constraining upper limits for the steady and pulsed emission for this source and discussed the implication on the state of the art models predicting VHE gamma-ray emission.
30#
發(fā)表于 2025-3-26 20:19:59 | 只看該作者
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