pith. sign in

Chinese Academy of Sciences)

Identifiers

  • name variant Chinese Academy of Sciences) 0.60 · backfill

Papers (70)

  1. VERA monitoring of the radio jet 3C 84 during 2007--2013: detection of non-linear motion astro-ph.GA · 2018 · author #62
  2. Properties of the narrow line Seyfert 1 galaxies revisited astro-ph.GA · 2016 · author #5
  3. Study of compound nucleus formation via bremsstrahlung emission in proton $\alpha$-particle scattering nucl-th · 2016 · author #10
  4. Multicolor Photometry of the Merging Galaxy Cluster A2319: Dynamics and Star Formation Properties astro-ph.GA · 2015 · author #14
  5. Structural Parameters for 10 Halo Globular Clusters in M33 astro-ph.GA · 2015 · author #3
  6. Ongoing growth of the brightest cluster galaxies via major dry mergers in the last ~6 Gyr astro-ph.GA · 2014 · author #11
  7. A search for open cluster Cepheids in the Galactic plane astro-ph.GA · 2014 · author #11
  8. Is radio jet power linearly proportional to the product of central black hole mass and Eddington ratio in AGN? astro-ph.GA · 2014 · author #3
  9. The ONSEN Data Reduction System for the Belle II Pixel Detector physics.ins-det · 2014 · author #10
  10. Creating mock catalogues of stellar haloes from cosmological simulations astro-ph.GA · 2014 · author #10
  11. Ground-based detections of thermal emission from the dense hot Jupiter WASP-43b in H and Ks-bands astro-ph.EP · 2013 · author #11
  12. Structural phase transition below 250 K in superconducting K$_{0.75}$Fe$_{1.75}$Se$_{2}$ cond-mat.supr-con · 2012 · author #14
  13. Paraconductivity of K-doped SrFe2As2 superconductor cond-mat.supr-con · 2012 · author #18
  14. Independent determination of the systematic and random errors of the proper motions in the PPMXL catalog using quasars astro-ph.GA · 2011 · author #4
  15. Abundance gradients in the galactic disk astro-ph.GA · 2011 · author #5
  16. A Decidable Extension of Data Automata cs.FL · 2011 · author #3
  17. Detailed study of B037 based on {\sl HST} images astro-ph.CO · 2011 · author #6
  18. Age and mass constraints for a young massive cluster in M31 based on spectral-energy-distribution fitting astro-ph.CO · 2011 · author #13
  19. The dependence of AGN activity on stellar and halo mass in Semi-Analytic Models astro-ph.CO · 2010 · author #18
  20. The Correlations between the Intrinsic Colors and Spectroscopic Metallicities of M31 Globular Clusters astro-ph.CO · 2010 · author #12
  21. Gamma rays and neutrinos from dark matter annihilation in galaxy clusters astro-ph.HE · 2010 · author #17
  22. Meso-scale phenomena from compromise -- a common challenge, not only for chemical engineering nlin.AO · 2009 · author #5
  23. Spherical-box approach for resonances in presence of Coulomb interaction quant-ph · 2009 · author #2
  24. Neutron halo in deformed nuclei nucl-th · 2009 · author #2
  25. How was the Hubble sequence 6 Gyrs ago? astro-ph.CO · 2009 · author #14
  26. Dark matter annihilation and non-thermal Sunyaev-Zel'dovich effect: I. galaxy cluster astro-ph.CO · 2009 · author #7
  27. Cosmology from very high energy $\gamma$-rays astro-ph · 2008 · author #6
  28. Stellar age versus mass of early-type galaxies in the Virgo Cluster astro-ph · 2008 · author #5
  29. A Multi-wavelength Study of the Massive Star-forming Region S87 astro-ph · 2008 · author #6
  30. Worldwide R&D of Virtual Observatory astro-ph · 2007 · author #3
  31. Thermodynamical properties of dark energy with the equation of state $% \omega =\omega_{0}+\omega_{1}z$ astro-ph · 2007 · author #12
  32. Self-Similar Dynamics of a Magnetized Polytropic Gas astro-ph · 2007 · author #9
  33. The Effects of Metallicity and AGN Activity on the Mid-Infrared Dust Emission of Galaxies astro-ph · 2007 · author #11
  34. J1128+592: a highly variable IDV source astro-ph · 2007 · author #24
  35. The IDV source J1128+5925, a new candidate for annual modulation? astro-ph · 2007 · author #21
  36. Mid-to-Far Infrared Spectral Energy Distribution of Galaxies in Spitzer First Look Survey Field astro-ph · 2007 · author #8
  37. A High-Abundance Arc in the Compact Group of Galaxies HCG 62: An AGN- or Merger-Induced Metal Outflow? astro-ph · 2007 · author #12
  38. Comparison between Windowed FFT and Hilbert-Huang Transform for Analyzing Time Series with Poissonian Fluctuations: A Case Study astro-ph · 2006 · author #9
  39. Color and Metallicity Distributions of M81 Globular Clusters astro-ph · 2005 · author #8
  40. Metallicity Estimates for Old Star Clusters in M33 astro-ph · 2005 · author #4
  41. Constraint on Cosmological Model with Matter Creation Using Complementary Astronomical Observations astro-ph · 2005 · author #8
  42. Reconstruction of the One-point Distribution of Convergence from Weak Lensing by Large-scale Structure astro-ph · 2005 · author #9
  43. Energy Spectra of Anti-nucleons in Finite Nuclei nucl-th · 2004 · author #3
  44. Distribution of Spectral Lags in Gamma Ray Bursts astro-ph · 2004 · author #19
  45. Hopf Algebraic Structures in the Cutting Rules hep-th · 2004 · author #2
  46. Automated Clustering Algorithms for Classification of Astronomical Objects astro-ph · 2004 · author #3
  47. Symmetry restoring phase transitions at high density in a 4D Nambu-Jona-Lasinio model with a single order parameter hep-th · 2003 · author #2
  48. Second and first order phase transition in three dimension Gross-Neveu model hep-th · 2003 · author #2
  49. The Power Spectra of Two Classes of Long-duration Gamma-ray Bursts astro-ph · 2003 · author #4
  50. Strong gravitational lensing and galactic bulges astro-ph · 2003 · author #2
  51. Gap equations and effective potentials at finite temperature and chemical potential in D dimensional four-fermion models hep-ph · 2002 · author #2
  52. The Effect of Radiative Cooling on the Sunyaev-Zel'dovich Cluster Counts and Angular Power Spectrum: Analytic Treatment astro-ph · 2002 · author #3
  53. Hopf Algebraic Structures in Proving Perturbative Unitarity hep-th · 2002 · author #2
  54. Chandra observation of Abell 1689: New determination of mass distribution and comparison to lensing measurements astro-ph · 2002 · author #3
  55. Spectroscopic Properties of QSOs Selected from Ultraluminous Infrared Galaxy Samples astro-ph · 2002 · author #12
  56. Damped $\sin(\beta-\alpha)$ of Higgs couplings and the lightest Higgs production at $\gamma\gamma$ colliders in MSSM hep-ph · 2001 · author #3
  57. Intermediate-band Surface Photometry of the Edge-on Galaxy: NGC 4565 astro-ph · 2001 · author #4
  58. Statistical properties of ultraluminous IRAS galaxies from an HST imaging survey astro-ph · 2001 · author #7
  59. Kinetic decoupling of neutralino dark matter astro-ph · 2001 · author #6
  60. Experimental Test of Complementarity by Nuclear Magnetic Resonance Techniques quant-ph · 2000 · author #8
  61. X-ray observations of supernova remnant G54.1+0.3: X-ray spectrum and the discovery of an X-ray jet astro-ph · 2000 · author #5
  62. Photoluminescence Study of Carbon Nanotubes cond-mat.mtrl-sci · 2000 · author #2
  63. $\Lambda_b\to\Sigma_c^{(*)}\pi l{\bar\nu}$ in the heavy quark, chiral, and large $N_c$ limits hep-ph · 1999 · author #3
  64. Turbulent Convection and pulsational Stability of Variable Stars I. Oscillations of Long-Period Variables astro-ph · 1997 · author #5
  65. Turbulent Convection and Pulsational Stability of Variable Stars II. Oscillations of RR Lyrae and Horizontal Branch Red Variable Stars astro-ph · 1997 · author #5
  66. An inverse Compton scattering (ICS) model of pulsar emission astro-ph · 1997 · author #6
  67. $E\otimes e$ Jahn-Teller Effect in $C_{70}^{3-}$ Systems cond-mat.mtrl-sci · 1997 · author #5
  68. Spin Precession and Time-Reversal Symmetry Breaking in Quantum Transport of Electrons Through Mesoscopic Rings cond-mat.mes-hall · 1997 · author #4
  69. Persistent Current From the Competition Between Zeeman Coupling and Spin-Orbit Interaction cond-mat · 1996 · author #4
  70. The Local Stability of Accretion Disks with Advection astro-ph · 1995 · author #3

Mentions

  • 1410.4489 #11 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 1409.1713 #3 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 1406.4028 #10 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 1406.2320 #10 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 1305.1643 #11 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 1209.5718 #14 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 1203.6592 #18 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 1110.1153 #4 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 1108.0721 #5 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 1106.1235 #3 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 1101.1569 #6 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 1101.1567 #13 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 1006.5717 #18 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 1004.1002 #12 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 1002.0197 #17 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 0912.5407 #5 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 0911.1171 #2 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 0909.1600 #2 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 0906.2805 #14 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 0902.4294 #7 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 0809.5124 #6 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 0803.2512 #5 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 0802.2036 #6 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 0711.4378 #3 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 0709.2745 #12 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 0706.3959 #9 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 0706.3257 #11 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 0705.0298 #24 · backfill · confidence 0.70 Chinese Academy of Sciences)
  • 0704.0871 #21 · backfill · confidence 0.70 Chinese Academy of Sciences)

Frequent Coauthors