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浏览/检索结果: 共3条，第1-3条 帮助 限定条件 发表日期：2019     已选(0)清除 条数/页：5101520253035404550556065707580859095100   排序方式：请选择作者升序作者降序题名升序题名降序发表日期升序发表日期降序提交时间升序提交时间降序 WGDdetector: a pipeline for detecting whole genome duplication events using the genome or transcriptome annotations 期刊论文 BMC BIOINFORMATICS, 2019, 卷号: 20, 期号: x, 页码: - 作者:  Yang, Yongzhi;  Li, Ying;  Chen, Qiao;  Sun, Yongshuai;  Lu, Zhiqiang 收藏  |  浏览/下载：184/0  |  提交时间：2019/04/22 Sequence  Gene  Polyploidy  Protein  Plants  Evolution  Inference  Reveals  Dosage   Targeting slug-mediated non-canonical activation of c-Met to overcome chemo-resistance in metastatic ovarian cancer cells 期刊论文 ACTA PHARMACEUTICA SINICA B, 2019, 卷号: 9 - 收藏  |  浏览/下载：5/0  |  提交时间：2020/10/26 EPITHELIAL-MESENCHYMAL TRANSITION  TUMOR-GROWTH  HETEROGENEITY  AMPLIFICATION  CONTRIBUTES  PROGRESSION  CARCINOMA  REVEALS  PATHWAY  SNAIL  Slug  c-Met  Drug resistance  Ovarian cancer  XL184   Timing analysis of Swift J1658.2-4242's outburst in 2018 with Insight-HXMT, NICER and AstroSat 期刊论文 Journal of High Energy Astrophysics, 2019, 卷号: 24, 页码: 30-40 作者:  HXMT 收藏  |  浏览/下载：41/0  |  提交时间：2022/02/08 Accretion  accretion disks  Black hole physics  X-rays: binaries:  Swift J1658.2-4242  Astrophysics - High Energy Astrophysical Phenomena  Abstract: We present the observational results from a detailed timing analysis of the black hole candidate Swift J1658.2-4242 during its 2018 outburst with the observations of Hard X-ray Modulation Telescope (Insight-HXMT), Neutron Star Interior Composition Explorer (NICER) and AstroSat in 0.1-250 keV. The evolution of intensity, hardness and integrated fractional root mean square (rms) observed by Insight-HXMT and NICER are presented in this paper. Type-C quasi-periodic oscillations (QPOs) observed by NICER (0.8-3.5 Hz) and Insight-HXMT (1-1.6 Hz) are also reported in this work. The features of the QPOs are analyzed with an energy range of 0.5-50 keV. The relations between QPO frequency and other characteristics such as intensity, hardness and QPO rms are carefully studied. The timing and spectral properties indicate that Swift J1658.2-4242 is a black hole binary system. Besides, the rms spectra of the source calculated from the simultaneous observation of Insight-HXMT, NICER and AstroSat support the Lense-Thirring origin of the QPOs. The relation between QPO phase lag and the centroid frequency of Swift J1658.2-4242 reveals a near zero constant when < 4Hz and a soft phase lag at 6.68 Hz. This independence follows the same trend as the high inclination galactic black hole binaries such as MAXI J1659-152.