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Yuan, Zunli
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1

Constraints on cosmic star formation history via a new mode..:

Wang, Wenjie ; Yuan, Zunli ; Yu, Hongwei.
http://arxiv.org/abs/2311.08975.  , 2023
Link: http://arxiv.org/abs/231..
 
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2

Redshift-evolutionary X-ray and UV luminosity relation of q..:

Wang, Bao ; Liu, Yang ; Yuan, Zunli...
http://arxiv.org/abs/2210.14432.  , 2022
Link: http://arxiv.org/abs/221..
 
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3

A flexible method for estimating luminosity functions via K..:

Yuan, Zunli ; Zhang, Xibin ; Wang, Jiancheng..
http://arxiv.org/abs/2203.06700.  , 2022
Link: http://arxiv.org/abs/220..
 
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4

A flexible method for estimating luminosity functions via k..:

Yuan, Zunli ; Zhang, Xibin ; Wang, Jiancheng..
Yuan , Z , Zhang , X , Wang , J , Cheng , X & Wang , W 2022 , ' A flexible method for estimating luminosity functions via kernel density Estimation. II. Generalization and python implementation ' , The Astrophysical Journal Supplement Series , vol. 260 , 10 . https://doi.org/10.3847/1538-4365/ac596a.  , 2022
Link: https://research.monash...
 
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5

Gamma ray burst constraints on cosmological models from the..:

Liu, Yang ; Liang, Nan ; Xie, Xiaoyao...
http://arxiv.org/abs/2207.00455.  , 2022
Link: http://arxiv.org/abs/220..
 
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6

The improved Amati correlations from Gaussian copula:

Liu, Yang ; Chen, Fuyong ; Liang, Nan...
http://arxiv.org/abs/2203.03178.  , 2022
Link: http://arxiv.org/abs/220..
 
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7

A flexible method for estimating luminosity functions via K..:

Yuan, Zunli ; Jarvis, Matt J ; Wang, Jiancheng
http://arxiv.org/abs/2003.13373.  , 2020
Link: http://arxiv.org/abs/200..
 
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8

Determining the Core Radio Luminosity Function of Radio AGN..:

Yuan, Zunli ; Wang, Jiancheng ; Worrall, D. M..
Yuan , Z , Wang , J , Worrall , D M , Zhang , B-B & Mao , J 2018 , ' Determining the Core Radio Luminosity Function of Radio AGNs via Copula ' , Astrophysical Journal Supplement Series , vol. 239 , no. 2 , 33 . https://doi.org/10.3847/1538-4365/aaed3b.  , 2018
Link: https://hdl.handle.net/1..
 
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9

Determining the core radio luminosity function of radio AGN..:

Yuan, Zunli ; Wang, Jiancheng ; Worrall, D. M..
http://arxiv.org/abs/1810.12713.  , 2018
Link: http://arxiv.org/abs/181..
 
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10

Using the Markov Chain Monte Carlo method to study the phys..:

Qin, Longhua ; Wang, Jiancheng ; Yang, Chuyuan...
http://arxiv.org/abs/1711.10625.  , 2017
Link: http://arxiv.org/abs/171..
 
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11

A mixture evolution scenario of the AGN radio luminosity fu..:

Yuan, Zunli ; Wang, Jiancheng ; Zhou, Ming..
http://arxiv.org/abs/1708.03087.  , 2017
Link: http://arxiv.org/abs/170..
 
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12

Constraining the redshifts of TeV BL Lac objects:

Qin, Longhua ; Wang, Jiancheng ; Yan, Dahai...
http://arxiv.org/abs/1709.03800.  , 2017
Link: http://arxiv.org/abs/170..
 
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13

Effect of spectral index distribution on estimating the AGN..:

Yuan, Zunli ; wang, Jiancheng ; Zhou, Ming.
http://arxiv.org/abs/1607.07046.  , 2016
Link: http://arxiv.org/abs/160..
 
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14

A mixture evolution scenario of the AGN radio luminosity fu..:

Yuan, Zunli ; Wang, Jiancheng ; Zhou, Ming.
http://arxiv.org/abs/1602.04298.  , 2016
Link: http://arxiv.org/abs/160..
 
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15

A graphical analysis of the systematic error of classical b..:

Yuan, Zunli ; Wang, Jiancheng
http://arxiv.org/abs/1302.5887.  , 2013
Link: http://arxiv.org/abs/130..
 
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