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We fitted all of the several hundred {\it RXTE} PCA spectra of the Crab individually to a simple power-law model; the total number of counts in the composite spectrum is $>10^9$. We then used the spectrum of residuals to derive a…

高能天体物理现象 · 物理学 2015-06-22 Javier Garcia , Jeffrey E. McClintock , James F. Steiner , Ronald A. Remillard , Victoria Grinberg

During its 16 years of service the Rossi X-ray Timing Explorer (RXTE) mission has provided an extensive archive of data, which will serve as a primary source of high cadence observations of variable X-ray sources for fast timing studies. It…

天体物理仪器与方法 · 物理学 2015-06-11 Nikolai Shaposhnikov , Keith Jahoda , Craig Markwardt , Jean Swank , Tod Strohmayer

We present the calibration of the \textit{Nuclear Spectroscopic Telescope Array} (\nustar) X-ray satellite. We used the Crab as the primary effective area calibrator and constructed a piece-wise linear spline function to modify the…

Hard xray data from the RXTE observatory (HEXTE energy range 15 to 240 keV) have been analyzed to obtain a phase coherent timing solution for the Crab pulsar glitch of 15 July 2000. The results are: (1) step change in the rotation frequency…

高能天体物理现象 · 物理学 2016-01-12 M. Vivekanand

Spectral clustering is one of the most popular clustering methods. However, the high computational cost due to the involved eigen-decomposition procedure can immediately hinder its applications in large-scale tasks. In this paper we use…

机器学习 · 计算机科学 2023-01-24 Yongyu Wang

This article is the first in the series that analyze about 1.87 million periods of PSR B0531+21 (Crab pulsar), observed by the PCA detector aboard the RXTE x-ray observatory. The Crab pulsar's x-ray light curve shows little variation over…

天体物理学 · 物理学 2009-11-06 M. Vivekanand

This paper considers a downlink ultra-dense heterogeneous cloud radio access network (H-CRAN) which guarantees seamless coverage and can provide high date rates. In order to reduce channel state information (CSI) feedback overhead,…

信息论 · 计算机科学 2018-04-24 Hao Xu , Cunhua Pan , Wei Xu , Gordon L. Stüber , Jianfeng Shi , Ming Chen

The Crab Nebula is used by many instruments as a calibration source, in particular at high energy, where it is one of the brightest celestial object. The spectrometer INTEGRAL SPI (20 keV - 8 MeV), in operation since October 2002, offers a…

高能天体物理现象 · 物理学 2020-09-02 E. Jourdain , J. P. Roques

We describe a new method to calibrate the relative flux levels in spectra from the HIRES echelle spectrograph on the Keck-I telescope. Standard data reduction techniques that transfer the instrument response between HIRES integrations leave…

天体物理学 · 物理学 2009-11-07 Nao Suzuki , David Tytler , David Kirkman , John M. O'Meara , Dan Lubin

Spectral Clustering is a popular technique to split data points into groups, especially for complex datasets. The algorithms in the Spectral Clustering family typically consist of multiple separate stages (such as similarity matrix…

机器学习 · 计算机科学 2019-11-04 Yifei Wang , Rui Liu , Yong Chen , Hui Zhangs , Zhiwen Ye

The new generation of radio synthesis arrays, such as LOFAR and SKA, have been designed to surpass existing arrays in terms of sensitivity, angular resolution and frequency coverage. This evolution has led to the development of advanced…

天体物理仪器与方法 · 物理学 2013-07-19 Sanaz Kazemi , Sarod Yatawatta , Saleem Zaroubi

We present here the updated calibration of The Nuclear Spectroscopic Telescope ARray NuSTAR, which was performed using data on the Crab accumulated over the last 9 years in orbit. The basis for this new calibration contains over 250ks of…

天体物理仪器与方法 · 物理学 2021-10-25 Kristin K. Madsen , Karl Forster , Brian W. Grefenstette , Fiona A. Harrison , Hiromasa Miyasaka

Spectral clustering is one of the most effective clustering approaches that capture hidden cluster structures in the data. However, it does not scale well to large-scale problems due to its quadratic complexity in constructing similarity…

机器学习 · 计算机科学 2019-11-26 Lingfei Wu , Pin-Yu Chen , Ian En-Hsu Yen , Fangli Xu , Yinglong Xia , Charu Aggarwal

This paper introduces an amendment to radio interferometric calibration of sources below the noise level. The main idea is to employ the information of the stronger sources' measured signals as a plug-in criterion to solve for the weaker…

天体物理仪器与方法 · 物理学 2016-11-15 Sanaz Kazemi , Sarod Yatawatta , Saleem Zaroubi

Context. The Crab nebula has been used as a celestial calibration source of the X-ray flux and spectral shape for many years by X-ray astronomy missions. However, the object is often too bright for current and future missions equipped with…

The Crab Nebula and the Pulsar have been pointed several times by the BeppoSAX satellite. We analysed all these observations, summed together, to study the main spectral properties with a good phase resolution. A new accurate estimate of…

天体物理学 · 物理学 2007-05-23 E. Massaro , G. Cusumano , M. Litterio , T. Mineo

We use the direct Fourier method to calculate the redshift-space power spectrum of the maxBCG cluster catalog (Koester et al. 2007) -- currently by far the largest existing galaxy cluster sample. The total number of clusters used in our…

天体物理学 · 物理学 2007-05-23 Gert Huetsi

The Crab Nebula has long been the standard reference point source for very-high-energy (VHE, E $>$100 GeV) gamma-ray observatories such as VERITAS. It has enabled testing and improvement of analysis methods, validation of techniques, and…

天体物理仪器与方法 · 物理学 2019-08-13 Ralph Bird

Real-world classification domains, such as medicine, health and safety, and finance, often exhibit imbalanced class priors and have asynchronous misclassification costs. In such cases, the classification model must achieve a high recall…

机器学习 · 计算机科学 2021-05-11 Michał Koziarski , Colin Bellinger , Michał Woźniak

We report on X-ray emission properties of the Crab pulsar(PSR B0531+21) using observations by Insight-HXMT during its first year after launch. We obtained high signal-to-noise profiles in the X-ray energy band 11-250 keV. We have confirmed…

高能天体物理现象 · 物理学 2019-06-19 You-Li Tuo , Ming-Yu Ge , Li-Ming Song , Lin-Li Yan , Qing-Cui Bu , Jin-Lu Qu
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