Podcasts about gaasp

Paul en Wouter spraken met Carina van Leeuwen, de drijvende kracht achter het Amsterdamse coldcaseteam. Welke memorabele zaken zijn haar bijgebleven? Hoe gaat dit team te werk? En wie is toch die deels in cement gegoten dode vrouw die in de rivier de Gaasp werd gevonden? Verder zit 'Sontje' B. van Zone 6 opnieuw vast voor marteling, nu in de 'Keulse drugsoorlog' En alleen al in Nederland zijn 30 verdachten gearresteerd voor geweldsgolf na rip 1400 kilo cocaïne. Presentatie: Corrie GerritsmaJournalisten: Paul Vugts en Hanneloes PenProductie en montage: Verena VerhoevenEindredactie: Josien WolthuizenMuziek: Kloaq Audio Design Schrijf je hier in voor de wekelijkse Misdaadnieuwsbrief. Reageren of vragen?Mail: misdaad@parool.nlWhatsapp en Signal: 06 27 19 33 64 Meer lezen? Zij leidt het coldcaseteam van de Amsterdamse politie: ‘Wij zitten te rommelen in een verleden waar soms al lang een deken overheen is gegooid’ ‘Sontje’ B. van rapformatie Zone 6 opnieuw vast, nu voor marteling in ‘Keulse drugsoorlog’ Alleen in Nederland al 30 verdachten gearresteerd voor geweldsgolf na rip 1400 kilo cocaïne Dankzij deze forensisch onderzoeker hebben drie onbekende doden nu een naam Support the show: https://www.kiosk.nl/See omnystudio.com/listener for privacy information.

Neste episódio, nossa convidada, Sandra Quintino a Psicanalista especializada em Adoção; Voluntária no GAASP no grupo de Pós – Adoção; Personal e Profissional Coach com Pós-Graduação em Comunicação; Administradora com ênfase em Marketing e Palestrante. Batemos um papo, ainda sobre o luto da infertilidade: Tabus, dúvidas e questões pertinentes a esse assunto que por vezes necessitam de orientação e ajuda profissional. Bora ouvir!!! --- Send in a voice message: https://anchor.fm/adocaoemais/message

New releases from AXEGRINDER, CRUCIFIX, DECOMP, GAASP, GRIT, NO PROBLEM and WARCHILD.

Utilizing a pinhole-plane imaging concept, ZEISS Airyscan allows for simultaneous improvement in resolution and signal-to-noise by capitalizing on an innovative 32-channel GaAsP photomultiplier tube (PMT) array detector. Each detection channel functions as a very small pinhole to increase resolution while the overall detector design delivers better signal-to-noise than traditional GaAsP-based confocal systems. In the past, a stack of at least five z-slices had to be deconvolved to get usable images with an optical section thinner than one Airy unit. Now, the new 2D Superresolution mode for ZEISS Airyscan delivers images with the thinnest optical section (0.2 Airy units) from a single image while maintaining the light collection efficiency of a much larger 1.25 Airy unit pinhole.

The Fast Module for ZEISS LSM 880 with Airyscan: Confocal Superresolution Imaging with Four Times the Speed and Improved Signal-to-Noise Ratio First introduced in August 2014, the Airyscan detector from ZEISS represents a new detector concept for laser scanning microscopy (LSM) that enables a simultaneous resolution and signal-to-noise (SNR) increase over traditional LSM imaging. The Airyscan detector design substitutes the conventional LSM detector and pinhole scheme for an array of 32 sensitive GaAsP detector elements, arranged in a compound eye fashion that resides in the pinhole-plane while still generating an optical section. The new detection geometry allows for the collection of the spatial distribution of light originating from every point of a microscopic fluorescent object at the pinhole allowing access to higher frequency information and while additionally collecting more light for ultra-efficient imaging. Based on the Airyscan detection concept, the next innovation from ZEISS has been developed with the introduction of the Fast mode for Airyscan. The Fast mode concept utilizes the Airyscan detector technology in combination with an illumination shaping approach to enhance acquisition speeds by four times while simultaneously increasing SNR and resolution overcoming the traditional compromises of confocal imaging.

Blazars, a subclass of active galactic nuclei in which the jet is aligned very close to our line of sight, can accelerate charged particles to relativistic energies in the jet. Electromagnetic emission from this class of sources can be observed from radio up to TeV energies. The MAGIC telescope is an Imaging Atmospheric Cherenkov Telescope with a 17-m diameter dish, located on the Canary Island of La Palma, in operation for exploring a new window of very high energy (VHE) gamma-ray bands, above 50 GeV. Searching for new VHE gamma-ray blazars, BL Lacertae was observed with the MAGIC telescope in 2005 and 2006. A VHE gamma-ray signal was discovered with a 5.1 sigma excess in the 2005 data. This discovery established a new class of VHE gamma-ray emitters, "low-frequency peaked BL Lac objects". On the other hand, the 2006 data showed no significant excess. This drop in flux followed the observed trend in the optical activity. The MAGIC telescope continuously observed the bright known blazars Mkn501, 1ES1959+650 and Mkn421. In particular, extensive simultaneous multiwavelength observations with the MAGIC telescope and the X-ray Satellite Suzaku were carried out for Mkn501 in July 2006 and for 1ES1959+650 in May 2006. VHE gamma-ray signals from about 100 GeV to a few TeV were clearly detected. For the first time, the VHE gamma-ray spectra were simultaneously obtained with the X-ray spectra during their low states of activity. Long term observations of Mkn421 in 2006 showed a strong variability in VHE gamma-ray emission. The spectral energy distributions (SEDs) of these four blazars could be well explained by a homogeneous one-zone synchrotron self-Compton model. This model suggests that the variation of the injected electron population in the jet is responsible for observed variations of the SEDs of the blazars. For all sources, the derived magnetic field strength in the jet and the Doppler beaming factor showed similar values. A contribution on the hardware sector is also presented in this thesis. For further lowering energy threshold in the MAGIC project, a new type of photosensor, "HPDs with an 18-mm diameter GaAsP photocathode", were developed. A quantum efficiency of the photocathode could reach over 50 %. Compared to the PMTs currently used in MAGIC, the new photosensors would improve the overall Cherenkov photon conversion efficiency by a factor of 2. Other performance values including lifetime also fulfilled the requirements of photosensors to be used in the MAGIC telescope.