γ-RAY AND PARSEC-SCALE JET PROPERTIES OF A COMPLETE SAMPLE OF BLAZARS FROM THE MOJAVE PROGRAM

著者人数: 145名

Response-based chemotherapy and involved field radiation for intermediate stage Hodgkin disease. A GISL/NHLSG trial

XIPE: the x-ray imaging polarimetry explorer

XIPE, the X-ray Imaging Polarimetry Explorer, is a mission dedicated to X-ray Astronomy. At the time of writing XIPE is in a competitive phase A as fourth medium size mission of ESA (M4). It promises to reopen the polarimetry window in high energy Astrophysics after more than 4 decades thanks to a detector that efficiently exploits the photoelectric effect and to X-ray optics with large effective area. XIPE uniqueness is time-spectrally-spatially- resolved X-ray polarimetry as a breakthrough in high energy astrophysics and fundamental physics. Indeed the payload consists of three Gas Pixel Detectors at the focus of three X-ray optics with a total effective area larger than one XMM mirror bu…

XIPE: the X-ray imaging polarimetry explorer

arXiv:1309.6995v1.-- et al.

CCDC 140070: Experimental Crystal Structure Determination

Related Article: A.Casnati, L.Baldini, N.Pelizzi, K.Rissanen, F.Ugozzoli, R.Ungaro|2000|J.Chem.Soc.,Dalton Trans.||3411|doi:10.1039/B004402O

CCDC 140069: Experimental Crystal Structure Determination

Related Article: A.Casnati, L.Baldini, N.Pelizzi, K.Rissanen, F.Ugozzoli, R.Ungaro|2000|J.Chem.Soc.,Dalton Trans.||3411|doi:10.1039/B004402O

15GHz and jet properties of MOJAVE blazars

We investigate the Fermi Large Area Telescope {gamma}-ray and 15GHz Very Long Baseline Array radio properties of a joint {gamma}-ray and radio-selected sample of active galactic nuclei (AGNs) obtained during the first 11 months of the Fermi mission (2008 August 4-2009 July 5). Our sample contains the brightest 173 AGNs in these bands above declination -30{deg} during this period, and thus probes the full range of {gamma}-ray loudness ({gamma}-ray to radio band luminosity ratio) in the bright blazar population. The latter quantity spans at least 4 orders of magnitude, reflecting a wide range of spectral energy distribution (SED) parameters in the bright blazar population. The BL Lac objects,…

CCDC 140068: Experimental Crystal Structure Determination

Related Article: A.Casnati, L.Baldini, N.Pelizzi, K.Rissanen, F.Ugozzoli, R.Ungaro|2000|J.Chem.Soc.,Dalton Trans.||3411|doi:10.1039/B004402O