publication
For a complete list of my publication, please visit my personal ADS library or use this query. To search for my refereed first-author papers use this query instead. My papers on the arXiv can be found here.
Here I list the papers produced by me and my group members:
Cosmological Implications of the BIMA 30 GHz Sunyaev-Zeldovich Effect Galaxy Cluster Survey Y.-T. Lin & J. Mohr (2003), ApJ, 582, 574
Near-Infrared Properties of Galaxy Clusters: Luminosity as a Binding Mass Predictor and the State of Cluster Baryons Y.-T. Lin, J. Mohr, & S. Stanford (2003), ApJ, 591, 749
K-Band Properties of Galaxy Clusters and Groups: Luminosity Function, Radial Distribution, and Halo Occupation Number Y.-T. Lin, J. Mohr, & S. Stanford (2004), ApJ, 610, 745
K-band Properties of Galaxy Clusters and Groups: Brightest Cluster Galaxies and Intracluster Light Y.-T. Lin & J. Mohr (2004), ApJ, 617, 879
A beginner’s guide to the theory of CMB temperature and polarization power spectra in the line-of-sight formalism Y.-T. Lin & B. Wandelt (2006), Astroparticle Physics, 25, 151
Evolution of the K-Band Galaxy Cluster Luminosity Function and Scaling Relations Y.-T. Lin, J. Mohr, A. Gonzalez, & S. Stanford (2006), ApJL, 650, L99
Radio Sources in Galaxy Clusters: Radial Distribution, and 1.4 GHz and K-band Bivariate Luminosity Function Y.-T. Lin & J. Mohr (2007), ApJS, 170, 71
Spectral Energy Distribution of Radio Sources in Nearby Clusters of Galaxies: Implications for Sunyaev-Zel'Dovich Effect Surveys Y.-T. Lin et al. (2009), ApJ, 694, 992
A New Test of the Statistical Nature of the Brightest Cluster Galaxies Y.-T. Lin, J. Ostriker, & C. Miller (2010), ApJ, 715, 1486
On the Populations of Radio Galaxies with Extended Morphology at z < 0.3 Y.-T. Lin et al. (2010), ApJ, 723, 1119
Baryon Content of Massive Galaxy Clusters at z = 0-0.6 Y.-T. Lin et al. (2012), ApJL, 734, L3
Modelling colour-dependent galaxy clustering in cosmological simulations S. Masaki, Y.-T. Lin, & N. Yoshida (2013), MNRAS, 436, 2286
The Stellar Mass Growth of Brightest Cluster Galaxies in the IRAC Shallow Cluster Survey Y.-T. Lin et al. (2013), ApJ, 771, 61
Stellar mass assembly of brightest cluster galaxies at late times T. Inagaki, Y.-T. Lin, H.-J. Huang, B.-C. Hsieh, & N. Sugiyama (2015), MNRAS, 446, 1107
Inferring Host Dark Matter Halo Masses of Individual Galaxies from Neighboring Galaxy Counts M. Oguri & Y.-T. Lin (2015), ApJ, 801, 94
On Detecting Halo Assembly Bias with Galaxy Populations Y.-T. Lin et al. (2016), ApJ, 819, 119
First Results on the Cluster Galaxy Population from the Subaru Hyper Suprime-Cam Survey. III. Brightest Cluster Galaxies, Stellar Mass Distribution, and Active Galaxies Y.-T. Lin et al. (2017), ApJ, 851, 139
An Analysis Framework for Understanding the Origin of Nuclear Activity in Low-power Radio Galaxies Y.-T. Lin, H.-J. Huang, & Y.-C. Chen (2018), AJ, 155, 188
The Hidden Giant: Discovery of an Enormous Galactic Dwarf Satellite in Gaia DR2 G. Torrealba et al. (2019), MNRAS, 488, 2743
Mass Bias of Weak-lensing Shear-selected Galaxy Cluster Samples K.-F. Chen, M. Oguri, Y.-T. Lin, & S. Miyazaki (2020), ApJ, 891, 139
Introducing piXedfit: A Spectral Energy Distribution Fitting Code Designed for Resolved Sources Abdurro'uf, Y.-T. Lin, P.-F. Wu, & M. Akiyama (2021), ApJS, 254, 15
Dissecting Nearby Galaxies with piXedfit. I. Spatially Resolved Properties of Stars, Dust, and Gas as Revealed by Panchromatic SED Fitting Abdurro'uf, Y.-T. Lin et al. (2022a), ApJ, 926, 81
SDSS-IV MaNGA: Cannibalism Caught in the Act -- On the Frequency of Occurrence of Multiple Cores in Brightest Cluster Galaxies Y.-H. Hsu, Y.-T. Lin et al. (2022), ApJ. 933, 61
Dissecting Nearby Galaxies with piXedfit. II. Spatially Resolved Scaling Relations among Stars, Dust, and Gas Abdurro'uf, Y.-T. Lin et al. (2022b), ApJ, 935, 98
A Pair of Early- and Late-Forming Galaxy Cluster Samples: a Novel Way of Studying Halo Assembly Bias Assisted by a Constrained Simulation Y.-T. Lin et al. (2022), A&A, 666, A97
A major galaxy cluster merger caught by eROSITA: weak lensing mass distribution and kinematic description R. Monteiro-Oliveira (2022), MNRAS, 515, 3674
A New Stellar Mass Proxy for Subhalo Abundance Matching C.-Y. Chuang & Y.-T. Lin (2023), ApJ, 944, 207
Leaving No Branches Behind: Predicting Baryonic Properties of Galaxies from Merger Trees C.-Y. Chuang, C. Jerspersen, Y.-T. Lin, S. Ho, and S. Genel (2024), ApJ, 965, 101
A Systematic Search of Distant Superclusters with the Subaru Hyper Suprime-Cam Survey T.-C. Chen, Y.-T. Lin et al. (2024), ApJ, submitted (arXiv:2401.10322)