papers

Publications (49)

astro-ph2006

Note on Redshift Distortion in Fourier Space

Yan-Chuan Cai, Jun Pan

We explore features of redshift distortion in Fourier analysis of N-body simulations. The phases of the Fourier modes of the dark matter density fluctuation are generally shifted b…

astro-ph.GA2018

SDSS-IV MaNGA: A Distinct Mass Distribution Explored in Slow-Rotating Early-type Galaxies

Yu Rong, Hongyu Li, Jie Wang +8

We study the radial acceleration relation (RAR) for early-type galaxies (ETGs) in the SDSS MaNGA MPL5 dataset. The complete ETG sample show a slightly offset RAR from the relation…

cs.CV2026

DeTracker: Motion-decoupled Vehicle Detection and Tracking in Unstabilized Satellite Videos

Jiajun Chen, Jing Xiao, Shaohan Cao +4

Satellite videos provide continuous observations of surface dynamics but pose significant challenges for multi-object tracking (MOT), especially under unstabilized conditions where…

astro-ph2007

Scale Transformations, Tree-level Perturbation Theory, and the Cosmological Matter Bispectrum

Jun Pan, Peter Coles, Istvan Szapudi

Scale transformations have played an extremely successful role in studies of cosmological large-scale structure by relating the non-linear spectrum of cosmological density fluctuat…

astro-ph2000

Large-scale Cosmic Homogeneity from a Multifractal Analysis of the PSCz Catalogue

Jun Pan, Peter Coles

We investigate the behaviour of galaxy clustering on large scales using the PSCz catalogue. In particular, we ask whether there is any evidence of large-scale fractal behaviour in…

astro-ph2006

The DWT Power Spectrum of the two-degree Field Galaxy Redshift Survey

Yan-Chuan Cai, Jun Pan, Yong-Heng Zhao +2

The power spectrum of the two-degree Field Galaxy Redshift Survey (2dFGRS) sample is estimated with the discrete wavelet transform (DWT) method. The DWT power spectra within $0.04…

astro-ph.CO2013

Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys - I. The Methodology

Pengjie Zhang, Jun Pan, Yi Zheng

Massive spectroscopic surveys will measure the redshift space distortion (RSD) induced by galaxy peculiar velocity to unprecedented accuracy. We develop a new method to improve the…

astro-ph.CO2024

Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics

Shiyu Yue, Longlong Feng, Wenjie Ju +6

This paper presents a novel perspective on correlation functions in the clustering analysis of the large-scale structure of the universe. We first recognise that pair counting in b…

chem-ph1994

Magic Numbers of Silicon Clusters

Jun Pan, Mushti V. Ramakrishna

A structural model for intermediate sized silicon clusters is proposed that is able to generate unique structures without any dangling bonds. This structural model consists of bulk…

chem-ph1995

Chemistry of Nanoscale Semiconductor Clusters

Jun Pan, Atul Bahel, Mushti V. Ramakrishna

The ground state structures of small silicon clusters are determined through exhaustive tight-binding molecular dynamics simulation studies. These simulations revealed that \Si{11}…

astro-ph.GA2026

The FAST Hundred-Deg HI Deep (HD) Survey: Early Results from the Pilot Survey

Chen Xu, Yingjie Jing, Jie Wang +26

The Hundred-deg HI Deep (HD) survey carried out with the Five-hundred-meter Aperture Spherical Telescope (FAST) is planned to map a contiguous region within the DESI DR1 fo…

cs.CV2026

Heterogeneous SAR-optical fusion for near-real-time land use and land cover mapping under cloud contamination: A novel framework and global benchmark dataset

Jiangong Xu, Weibao Xue, Xiaoyu Yu +3

Optical remote sensing imagery is frequently degraded by cloud and cloud-shadow contamination, which limits its reliability for near-real-time land use and land cover (LULC) mappin…

cs.CV2019

Spot Evasion Attacks: Adversarial Examples for License Plate Recognition Systems with Convolutional Neural Networks

Ya-guan Qian, Dan-feng Ma, Bin Wang +5

Recent studies have shown convolution neural networks (CNNs) for image recognition are vulnerable to evasion attacks with carefully manipulated adversarial examples. Previous work…

astro-ph.CO2011

The kinetic SZ tomography with spectroscopic redshift surveys

Jiawei Shao, Pengjie Zhang, Weipeng Lin +2

The kinetic Sunyaev Zel'dovich effect (kSZ) effect is a potentially powerful probe to the missing baryons. However, the kSZ signal is overwhelmed by various contaminations and the…

astro-ph2005

Fast Edge Corrected Measurement of the Two-Point Correlation Function and the Power Spectrum

István Szapudi, Jun Pan, Simon Prunet +1

We present two related techniques to measure the two-point correlation function and the power spectrum with edge correction in any spatial dimensions. The underlying algorithm uses…

astro-ph.GA2017

A Universe of Ultra-Diffuse Galaxies: Theoretical Predictions from CDM Simulations

Yu Rong, Qi Guo, Liang Gao +5

A particular population of galaxies have drawn much interest recently, which are as faint as typical dwarf galaxies but have the sizes as large as galaxies, the so called "ul…

astro-ph2005

The Monopole Moment of the Three-Point Correlation Function of the 2-degree Field Galaxy Redshift Survey

Jun Pan, Istvan Szapudi

We measure the monopole moment of the three-point correlation function on scales $1\mpc-70\mpc$ in the Two degree Field Galaxy Redshift Survey (2dFGRS). Volume limited samples are…

astro-ph.CO2017

Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys. II. Dark Matter Velocity Statistics

Yi Zheng, Pengjie Zhang, Yipeng Jing +2

Massive spectroscopic redshift surveys open a promising window to accurately measure peculiar velocity at cosmological distances through redshift space distortion (RSD). In paper I…

astro-ph.CO2012

Influence of baryons on spatial distribution of matter: higher order correlation functions

Xiaojun Zhu, Jun Pan

Baryonic physical processes could leave non-negligible imprint on cosmic matter distribution pattern. Series of high precision simulation data sets with identical initial condition…

chem-ph1995

Growth Pattern of Silicon Clusters

Atul Bahel, Jun Pan, Mushti V. Ramakrishna

Tight-binding molecular dynamics simulated annealing technique is employed to search for the ground state geometries of silicon clusters containing 11-17 atoms. These studies revea…

astro-ph.GA2020

Simulating Kilonovae in the ΛCDM Universe

Zhen Jiang, Jie Wang, Fenghui Zhang +6

Kilonovae are optical flashes produced in the aftermath of neutron star-neutron star mergers (NNMs) or neutron star-black hole mergers (NBMs). In this work, we use the Millennium S…

astro-ph2004

Three-point Correlation Functions of SDSS Galaxies in Redshift Space: Morphology, Color, and Luminosity Dependence

Issha Kayo, Yasushi Suto, Robert C. Nichol +10

We present measurements of the redshift--space three-point correlation function of galaxies in the Sloan Digital Sky Survey (SDSS). For the first time, we analyze the dependence of…

eess.IV2020

Thick Cloud Removal of Remote Sensing Images Using Temporal Smoothness and Sparsity-Regularized Tensor Optimization

Chenxi Duan, Jun Pan, Rui Li

In remote sensing images, the presence of thick cloud accompanying cloud shadow is a high probability event, which can affect the quality of subsequent processing and limit the sce…

astro-ph.GA2019

GABE: Galaxy Assembly with Binary Evolution

Zhen Jiang, Jie Wang, Liang Gao +4

We developed a new semi-analytic galaxy formation model: Galaxy Assembly with Binary Evolution (GABE). For the first time we introduce binary evolution into semi-analytic models of…

astro-ph2005

Cosmological Three-Point Function: Testing The Halo Model Against Simulations

Pablo Fosalba, Jun Pan, Istvan Szapudi +1

We perform detailed comparison of the semi-analytic halo model predictions with measurements in numerical simulations of the two and three point correlation functions (3PCF), as we…

astro-ph2006

The fractional Brownian motion and the halo mass function

Jun Pan

The fractional Brownian motion with index is introduced to construct the fractional excursion set model. A new mass function with single parameter is derived within the f…

astro-ph2008

Effects of correlation between merging steps on the global halo formation

Jun Pan, Yougang Wang, Xuelei Chen +1

The excursion set theory of halo formation is modified by adopting the fractional Brownian motion, to account for possible correlation between merging steps. We worked out analytic…

astro-ph.CO2011

On the fairness of the main galaxy sample of SDSS

Kelai Meng, Bin Ma, Jun Pan +1

Flux-limited and volume-limited galaxy samples are constructed from SDSS data releases DR4, DR6 and DR7 for statistical analysis. The two-point correlation functions , monop…

cond-mat1994

Magic Numbers of Silicon Clusters

Jun Pan, Mushti V. Ramakrishna

A structural model for intermediate sized silicon clusters is proposed that is able to generate unique structures without any dangling bonds. This structural model consists of bulk…

astro-ph2004

Conditional Cumulants in Weakly Non-linear Regime

Jun Pan, Istvan Szapudi

Conditional cumulants form a set of unique statistics which represent a sensible compromise between N-point correlation functions and cumulants measured from moments of counts in c…

astro-ph2006

Colour Dependence of the Distribution of IRAS Galaxies revealed by Multifractal Measures

Jun Pan

Multifractal measures are applied to three IRAS galaxy subsamples selected by colour from the PSCz catalogue. As shown by generalised dimension spectrum, hot IRAS galaxies are foun…

astro-ph.CO2020

Estimating power spectrum of discrete cosmic momentum field with fast Fourier transform

Jun Pan

Fast Fourier transform based estimators are formulated for measuring momentum power spectra, including the auto power spectra of the momentum, the momentum divergence, and the cros…

astro-ph.CO2022

About One-point Statistics of the Ratio of Two Fourier-transformed Cosmic Fields and an Application

Ming Li, Jun Pan, Pengjie Zhang +7

The Fourier transformation is an effective and efficient operation of Gaussianization at the one-point level. Using a set of N-body simulation data, we verified that the one-point…

cond-mat.mtrl-sci2017

Synthesis of Single-crystal-like Nanoporous Carbon Membranes and Their Applications in Overall Water Splitting

Hong Wang, Shixiong Min, Chun Ma +17

Nanoporous graphitic carbon membranes with defined chemical composition and pore architecture are novel nanomaterials that are actively pursued. Compared to easy-to-make porous car…

astro-ph.CO2013

An estimation of local bulk flow with the maximum-likelihood method

Yin-Zhe Ma, Jun Pan

A maximum-likelihood method, tested as an unbiased estimator from numerical simulations, is used to estimate cosmic bulk flow from peculiar velocity surveys. The likelihood functio…

astro-ph.GA2024

HiFAST: an HI data calibration and imaging pipeline for FAST

Yingjie Jing, Jie Wang, Chen Xu +30

The Five-hundred-meter Aperture Spherical radio Telescope (FAST) has the largest aperture and a 19-beam L-band receiver, making it powerful for investigating the neutral hydrogen a…

astro-ph.GA2017

Massive Quiescent Galaxies at z>3 in The Millennium Simulation Populated by A Semi-analytic Galaxy Formation Model

Yu Rong, Yingjie Jing, Liang Gao +5

We take advantage of the statistical power of the large-volume dark-matter-only Millennium simulation, combined with a sophisticated semi-analytic galaxy formation model, to explor…

astro-ph2001

Boundary Corrections in Fractal Analysis of Galaxy Surveys

Jun Pan, Peter Coles

The analysis of redshift surveys with fractal tools requires one to apply some form of statistical correction for galaxies lying near the geometric boundary of the sample. In this…

astro-ph.CO2012

Bulk flow of halos in ΛCDM simulation

Ming Li, Jun Pan, Liang Gao +10

Analysis of the Pangu N-body simulation validates that the bulk flow of halos follows a Maxwellian distribution which variance is consistent with the prediction of the linear theor…

astro-ph.GA2019

Comparing galaxy morphology in hydrodynamical simulation and in semi-analytic model

Lan Wang, Dandan Xu, Liang Gao +3

We compare galaxy morphology predicted by the Illustris hydrodynamical simulation and a semi-analytic model (SAM) grafted in the halo merger trees from the Illustris-Dark matter si…

astro-ph.CO2010

The ergodicity bias in the observed galaxy distribution

Jun Pan, Pengjie Zhang

The spatial distribution of galaxies we observed is subject to the given condition that we, human beings are sitting right in a galaxy -- the Milky Way. Thus the ergodicity assumpt…

chem-ph1994

Chemical Reactions of Silicon Clusters

Mushti V. Ramakrishna, Jun Pan

Smalley and co-workers discovered that chemisorption reactivities of silicon clusters vary over three orders of magnitude as a function of cluster size. In particular, they found t…

astro-ph.CO2021

Numerical investigation of non-Gaussianities in the phase and modulus of density Fourier modes

Jian Qin, Jun Pan, Yu Yu +1

We numerically investigate non-Gaussianities in the late-time cosmological density field in Fourier space. We explore various statistics, including the two-point and three-point pr…

astro-ph.GA2018

The Large-scale Effect of Environment on Galactic Conformity

Shuangpeng Sun, Qi Guo, Lan Wang +4

We use a volume-limited galaxy sample from the SDSS Data Release 7 to explore the dependence of galactic conformity on the large-scale environment, measured on 4 Mpc scales.…

chem-ph1995

Structure of Silicon Clusters

Jun Pan, Atul Bahel, Mushti V. Ramakrishna

We determined the structures of silicon clusters in the 11-14 atom size range using the tight-binding molecular dynamics method. These calculations reveal that \Si{11} is an icosah…

astro-ph.CO2009

Clustering of K-band selected local galaxies

Bin Ma, Kelai Meng, Jun Pan +2

We present detailed clustering analysis of a large K-band selected local galaxy sample, which is constructed from the 2MASS and the SDSS and consists of galaxies with $10…

astro-ph.IM2023

Performance of FAST with an Ultra-Wide Bandwidth Receiver at 500-3300 MHz

Chuan-Peng Zhang, Peng Jiang, Ming Zhu +6

The Five-hundred-meter Aperture Spherical radio Telescope (FAST) has been running for several years. A new Ultra-Wide Bandwidth (UWB) receiver, simultaneously covering 500-3300 MHz…

astro-ph.CO2010

A redshift distortion free correlation function at third order in the nonlinear regime

Kelai Meng, Jun Pan, Istvan Szapudi +1

The zeroth-order component of the cosine expansion of the projected three-point correlation function is proposed for clustering analysis of cosmic large scale structure. These func…

astro-ph2003

On Recovering the Nonlinear Bias Function from Counts in Cells Measurements

Istvan Szapudi, Jun Pan

We present a simple and accurate method to constrain galaxy bias based on the distribution of counts in cells. The most unique feature of our technique is that it is applicable to…