نتایج جستجو برای: psr

تعداد نتایج: 3126  

Journal: :Optics express 2015
Jing Wang Chunghun Lee Ben Niu Haiyang Huang You Li Ming Li Xin Chen Zhen Sheng Aimin Wu Wei Li Xi Wang Shichang Zou Fuwan Gan Minghao Qi

We propose a silicon-on-insulator (SOI) polarization diversity scheme in the mid-infrared wavelength range. In consideration of absorption loss in silicon dioxide (SiO2), the polarization splitter-rotator (PSR) is designed and optimized with silicon nitride (SiN) upper-cladding and SiO2 lower-cladding. This asymmetry allows the PSR, which consists of mode-conversion tapers...

2001
DIEGO F. TORRES YOUSAF M. BUTT FERNANDO CAMILO

We present a correlative study between all unidentified EGRET sources at low Galactic latitudes and the newly discovered pulsars in the released portion of the Parkes multibeam radio survey. We note 14 positional coincidences: eight of these are “Vela-like” pulsars, with relatively small periods, small characteristic ages, and high spin-down luminosities. Three of these coincidences have been i...

2016
Kelly L. Hagberg Svetlana N. Yurgel Monika Mulder Michael L. Kahn

Bacteria have developed various stress response pathways to improve their assimilation and allocation of limited nutrients, such as nitrogen and phosphate. While both the nitrogen stress response (NSR) and phosphate stress response (PSR) have been studied individually, there are few experiments reported that characterize effects of multiple stresses on one or more pathways in Sinorhizobium meli...

2001
Ken’ichi Torii Y. Saito F. Nagase T. Yamagami T. Kamae M. Hirayama N. Kawai I. Sakurai M. Namiki S. Shibata S. Gunji J. P. Finley

ASCA’s long look at the 288 ms radio pulsar PSR J0631 1036 reveals coherent X-ray pulsation from this source for the first time. The source was first detected in a serendipitous Einstein observation and later identified as a radio pulsar. Possible pulsation in the g-ray band has been detected in the Compton Gamma Ray Observatory EGRET data. The X-ray spectrum in the ASCA band is characterized b...

Journal: :Blood 2003
Rory R Koenen Guido Tans René van Oerle Karly Hamulyák Jan Rosing Tilman M Hackeng

Protein S exhibits anticoagulant activity independent of activated protein C (APC). An automated factor Xa-based one-stage clotting assay was developed that enables quantification of the APC-independent activity of protein S in plasma from the ratio of clotting times (protein S ratio [pSR]) determined in the absence and presence of neutralizing antibodies against protein S. The pSR was 1.62 +/-...

2005
Masoumeh T. Izadi Doina Precup

Predictive state representation (PSR), proposed by [Littman et al., 2002; Singh et al., 2004], are a general representation for controlled dynamical systems. We present a sufficient condition under which a linear PSR compresses a POMDP representation.

Journal: :Human reproduction 2006
Shai Shefi Gil Raviv Michael L Eisenberg Ruth Weissenberg Liza Jalalian Jacob Levron Gili Band Paul J Turek Igael Madgar

BACKGROUND Current recommendations regarding posthumous sperm retrieval (PSR) are based on a small number of cases. Our purpose was to determine the time interval from death to a successful procedure. METHODS Seventeen consecutive PSR procedures in 14 deceased and 3 neurologically brain-dead patients at two male infertility centres [Sheba Medical Center (SMC), Tel-Hashomer, Israel and Univers...

2016
Wynn C. G. Ho C.-Y. Ng Andrew G. Lyne Ben W. Stappers Malcolm J. Coe Jules P. Halpern Tyrel J. Johnson Iain A. Steele

The radio and gamma-ray pulsar PSR J2032+4127 was recently found to be in a decadeslong orbit with the Be star MT91 213, with the pulsar moving rapidly toward periastron. This binary shares many similar characteristics with the previously unique binary system PSR B1259−63/LS 2883. Here we describe radio, X-ray, and optical monitoring of PSR J2032+4127/MT91 213. Our extended orbital phase covera...

2003
W. Bednarek

In the recent paper we calculated the γ-ray spectra from pulsar wind nebulae (PWNe), assuming that a significant amount of the pulsar rotational energy is converted into relativistic nuclei. These nuclei accelerate leptons which are responsible for most of the observed electromagnetic emission from PWNe. Small part of nuclei also interact with the matter of the supernova producing γ-rays, which...

2001
T. Yamagami T. Kamae M. Hirayama N. Kawai

ASCA’s long look at the 288 millisecond radio pulsar, PSR J0631+1036, reveals coherent X-ray pulsation from this source for the first time. The source was first detected in the serendipitous Einstein observation and later identified as a radio pulsar. Possible pulsation in the gamma-ray band has been detected from the CGRO EGRET data (Zepka, et al. 1996). The X-ray spectrum in the ASCA band is ...

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