C. Shu

发表

Quenching as a Contest between Galaxy Halos and Their Central Black Holes

D. Koo, A. V. D. Wel, H. Ferguson, 2019, The Astrophysical Journal.

Galaxy–Galaxy Weak-lensing Measurements from SDSS. I. Image Processing and Lensing Signals

M. Radovich, L. Fu, H. Mo, 2016, 1607.05406.

THE MORPHOLOGICAL-DEPENDENT TULLY–FISHER RELATION OF SPIRAL GALAXIES

Z. Shao, S. Shen, C. Shu, 2009, 0909.4903.

An Analytic Model of Galactic Winds and Mass Outflows

Cas, H. Mo, C. Shu, 2003, astro-ph/0301035.

Probing Galaxies through Quasar Absorption Lines

B. Ménard, P. Williams, C. Shu, 2005 .

The differences of star formation history between merging galaxies and field galaxies in the early data release of the SDSS

J. Huang, C. Shu, Z. Luo, 2007, astro-ph/0703357.

Dynamical Stability of the Power Law K-essence Dark Energy Model with a New Interaction

C. Shu, W. Fang, Qile Zhang, 2022, 2201.00444.

An Analytic Model of Galactic Winds and Mass Outflows

Cas, H. Mo, C. Shu, 2003, astro-ph/0301035.

AEGIS: Infrared Spectroscopy of an Infrared-luminous Lyman Break Galaxy at z = 3.01

C. Conselice, B. McLeod, C. Willmer, 2006, astro-ph/0608456.

Morphology of Galactic Open Clusters

W. P. Chen, C. Shu, C. W. Chen, 2004, astro-ph/0408021.

The luminosity and mass functions of the Virgo Cluster of galaxies

C. Shu, Jun-liang Zhao, K. Tian, 1996 .

Spitzer Observations of z ~ 3 Lyman Break Galaxies: Stellar Masses and Mid-Infrared Properties

C. Papovich, G. Fazio, P. Barmby, 2006, astro-ph/0605355.

Infrared Luminous Lyman Break Galaxies: A Population that Bridges LBGs and SCUBA Galaxies

C. Conselice, C. Papovich, G. Fazio, 2005, astro-ph/0507685.

Dependence of spiral galaxy distribution on viewing angle in RC3

Jun Ma, C. Shu, G. Song, 2000, astro-ph/0002477.

Stellar and HI Mass Functions Predicted by a Simple Preheating Galaxy Formation Model

Zhijian Luo, C. Shu, 2007 .

Star formation and chemical evolution of damped Lyman α systems

J. Ma, C. Shu, J. Ma, 2001, astro-ph/0103485.

The evolution of globular clusters

Maoan Han, A. Chian, Wen-Ping Chen, 2010 .

The differences of star formation history between merging galaxies and field galaxies in the early data release of the SDSS

J. Huang, C. Shu, Z. Luo, 2007, astro-ph/0703357.

Physical properties of DLAs: Metallicity and neutral hydrogen column density

Shanghai, Taiwan, China., 2003, astro-ph/0310397.

The 2175 Å bump features in FeLoBAL quasars: One indicator of MW-like dust in the nuclear region of quasars

J. Ge, P. Jiang, Shaohua Zhang, 2022, Astronomy & Astrophysics.

Spitzer Observations of z ~ 3 Lyman Break Galaxies: Stellar Masses and Mid-Infrared Properties

C. Papovich, G. Fazio, P. Barmby, 2006, astro-ph/0605355.

Infrared Luminous Lyman Break Galaxies: A Population that Bridges LBGs and SCUBA Galaxies

C. Conselice, C. Papovich, G. Fazio, 2005, astro-ph/0507685.

06 07 46 5 v 1 2 0 Ju l 2 00 6 Color-magnitude relations of late-type galaxies

Z. Shao, S. Shen, C. Shu, 2006 .

Properties and morphologies of Lyman break galaxies at z ∼ 1 in the Chandra Deep Field South, inferred from spectral energy distributions

V. Buat, J.-S. Huang, D. Burgarella, 2013 .

Some statistical properties of spiral galaxies

Jun Ma, Q. Peng, C. Shu, 1999, astro-ph/0002476.

THE MASS-DEPENDENT STAR FORMATION HISTORIES OF DISK GALAXIES: INFALL MODEL VERSUS OBSERVATIONS

S. Shen, C. Shu, R. Chang, 2010, 1008.3045.

MULTI-WAVELENGTH STUDY OF A COMPLETE IRAC 3.6 μm SELECTED GALAXY SAMPLE: A FAIR CENSUS OF RED AND BLUE POPULATIONS AT REDSHIFTS 0.4–1.2

J. Newman, B. Weiner, A. Coil, 2012, 1212.1234.

The planetary–exoplanetary environment: A nonlinear perspective

Maoan Han, J. Valdivia, A. Chian, 2010 .

Metallicity and H I Column Density Properties of Damped Lyα Systems

W. P. Chen, S. Shen, C. Shu, 2005, astro-ph/0501603.

The fundamental plane of spiral galaxies: theoretical expectations

S. Shen, H. Mo, C. Shu, 2001, astro-ph/0105095.

Galaxy–Galaxy Weak-lensing Measurements from SDSS. II. Host Halo Properties of Galaxy Groups

M. Radovich, L. Fu, Nan Li, 2017, The Astrophysical Journal.

Colour–magnitude relations of late-type galaxies

Z. Shao, S. Shen, C. Shu, 2006, astro-ph/0607465.

Probing the slope of cluster mass profile with gravitational Einstein rings : application to Abell 1689

J. Kneib, E. Jullo, M. Limousin, 2007, 0710.2246.

Studies of the open cluster M11. 4. The CM diagram, luminosity function and mass segregation☆

C. Shu, Jun-liang Zhao, K. Tian, 1997 .

Cosmological Perturbations and Quasi-Static Assumptions in f(R) Theories

C. Shu, Hong-Hao Tu, A. Taylor, 2015, 1505.03323.

The host haloes of Lyman-break galaxies and submillimetre sources

Garching, Shude Mao, China, 2001, astro-ph/0102436.

TWO-COMPONENT MODEL FOR CHEMICAL EVOLUTION OF THE GALACTIC DISK

C. Shu, R. Chang, J. Hou, 1999, astro-ph/9903317.

History of Star Formation and Chemical Enrichment in the Milky Way Disk

C. Shu, J. Hou, R. Chang, 2002 .

Dynamical system of scalar field from 2-dimension to 3-D and its cosmological implications

C. Shu, W. Fang, Hong-Hao Tu, 2014, 1402.4045.

Polynomial Hamiltonian systems with a nilpotent critical point

Abraham C.-L. Chian, Maoan Han, Maoan Han, 2010 .

Comparisons between Isothermal and NFW Mass Profiles for Strong-Lensing Galaxy Clusters

Y. Mellier, M. Bartelmann, J. Comerford, 2008, 0805.1148.

Mass Reconstruction of Galaxy-scale Strong Gravitational Lenses Using a Broken Power-law Model

Y. Shu, L. Fu, C. Shu, 2023, The Astrophysical Journal.

Properties and morphologies of Lyman break galaxies at z ∼ 1 in the Chandra Deep Field South, inferred from spectral energy distributions

V. Buat, J.-S. Huang, D. Burgarella, 2013, 1302.3938.