TL
Ting-Yi Lu
astro-ph.GAastro-ph.COastro-ph.HEgr-qcastro-ph.IMphysics.ed-phphysics.pop-ph
On Valency
published · living versionsW_unu28bt7·v1 · currentpublished
Why a Multi-Cycle Treasury Program is Essential to Maximize JWST's Scientific Contributions to Galaxy Formation
with Genesis Community, Alice Shapley, Steven L. Finkelstein, Rachel S. Somerville +416
1 version
Preprints & journals
30 papers in the corpus · 2009–2025Deep JWST spectroscopy of galaxies in a candidate ionized bubble at : probing reionization at pMpc scales with Ly emission2510.12019v2 · Lily Whitler, Daniel P. Stark, Charlotte A. Mason et al.2025 · 2 citationsMon Not R Astron Soc (2026)
The Impact of Galaxy Overdensities and Ionized Bubbles on Ly Emission at 2505.24080v2 · Zuyi Chen, Daniel P. Stark, Charlotte A. Mason et al.2025 · 1 citationarXiv
Constraints on the intergalactic medium from JWST spectroscopy of Lyman-alpha damping wings in galaxies2501.11702v2 · Charlotte A. Mason, Zuyi Chen, Daniel P. Stark et al.2025 · 22 citationsA&A 705, A114 (2026)
Mapping reionization bubbles in the JWST era II: inferring the position and characteristic size of individual bubbles2501.07980v2 · Ivan Nikoli'c, Andrei Mesinger, Charlotte A. Mason et al.2025 · 10 citationsA&A 699, A323 (2025)
Mapping reionization bubbles in the JWST era I: empirical edge detection with Lyman alpha emission from galaxies2411.04176v1 · Ting-Yi Lu, Charlotte A. Mason, Andrei Mesinger et al.2024 · 12 citationsA&A 697, A69 (2025)
The reionising bubble size distribution around galaxies2304.11192v1 · Ting-Yi Lu, Charlotte Mason, Anne Hutter et al.2023 · 6 citationsarXiv
JWST/NIRSpec Spectroscopy of Star Forming Galaxies with CEERS: New Insight into Bright Ly Emitters in Ionized Bubbles2301.07072v5 · Mengtao Tang, Daniel P. Stark, Zuyi Chen et al.2023 · 186 citationsarXiv
Early results from GLASS-JWST. XIV: A spectroscopically confirmed protocluster 650 million years after the Big Bang2211.09097v3 · Takahiro Morishita, Guido Roberts-Borsani, Tommaso Treu et al.2022 · 127 citationsarXiv
Constraining the Hubble constant and its lower limit from the proper motion of extragalactic radio jets2209.05008v1 · Tiger Yu-Yang Hsiao, Tomotsugu Goto, Tetsuya Hashimoto et al.2022 · 2 citationsarXiv
Can luminous Lyman alpha emitters at 5.7 and 6.6 suppress star formation?2209.02405v1 · Daryl Joe D. Santos, Tomotsugu Goto, Tetsuya Hashimoto et al.2022 · 1 citationarXiv
ALMA [O III] and [C II] Detections of A1689-zD1 at 2202.13613v1 · Yi Hang Valerie Wong, Poya Wang, Tetsuya Hashimoto et al.2022 · 2 citationsarXiv
Upper limits on Einstein's weak equivalence principle placed by uncertainties of dispersion measures of fast radio bursts2111.11447v2 · Tetsuya Hashimoto, Tomotsugu Goto, Daryl Joe D. Santos et al.2021 · 8 citationsarXiv
Constraining violations of the Weak Equivalence Principle Using CHIME FRBs2111.11451v1 · Kaustubha Sen, Tetsuya Hashimoto, Tomotsugu Goto et al.2021 · 3 citationsarXiv
Uncloaking hidden repeating fast radio bursts with unsupervised machine learning2110.09440v1 · Bo Han Chen, Tetsuya Hashimoto, Tomotsugu Goto et al.2021 · 49 citationsarXiv
Environmental Effects on AGN activity via Extinction-free Mid-Infrared Census2108.06899v1 · Daryl Joe D. Santos, Tomotsugu Goto, Seong Jin Kim et al.2021 · 8 citationsarXiv
A Dyson Sphere around a black hole2106.15181v2 · Tiger Yu-Yang Hsiao, Tomotsugu Goto, Tetsuya Hashimoto et al.2021 · 21 citationsarXiv
Investigative Study on Preprint Journal Club as an Effective Method of Teaching Latest Knowledge in Astronomy2106.01688v1 · Daryl Joe D. Santos, Tomotsugu Goto, Ting-Yi Lu et al.2021 · 1 citationPhys. Rev. Phys. Educ. Res. 17, 010145 (2021)
Revealing the cosmic reionisation history with fast radio bursts in the era of Square Kilometre Array2101.08798v2 · Tetsuya Hashimoto, Tomotsugu Goto, Ting-Yi Lu et al.2021 · 27 citationsarXiv
An Active Galactic Nucleus Recognition Model based on Deep Neural Network2101.06683v1 · Bo Han Chen, Tomotsugu Goto, Seong Jin Kim et al.2021 · 15 citationsMNRAS 501 (2021) 3951-3961
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XI. Proximity Zone Analysis for Faint Quasar Spectra at z~62009.06648v1 · Rikako Ishimoto, Nobunari Kashikawa, Masafusa Onoue et al.2020 · 23 citationsarXiv
No redshift evolution of non-repeating fast radio-burst rates2008.09621v2 · Tetsuya Hashimoto, Tomotsugu Goto, Alvina Y. L. On et al.2020 · 49 citationsarXiv
Fast radio bursts to be detected with the Square Kilometre Array2008.00007v1 · Tetsuya Hashimoto, Tomotsugu Goto, Alvina Y. L. On et al.2020 · 43 citationsarXiv
Far-infrared star-formation rates of six GRB host galaxies with ALMA2007.11874v2 · Tiger Yu-Yang Hsiao, Tetsuya Hashimoto, Jia-Yuan Chang et al.2020 · 5 citationsarXiv
What determines the maximum stellar surface density of galaxies?2006.16738v1 · Chih-Teng Ling, Tetsuya Hashimoto, Tomotsugu Goto et al.2020 · 2 citationsarXiv
Luminosity-duration relations and luminosity functions of repeating and non-repeating fast radio bursts2004.02079v1 · Tetsuya Hashimoto, Tomotsugu Goto, Ting-Wen Wang et al.2020 · 40 citationsarXiv
Rapid Black Hole Growth at the Dawn of the Universe: A Super-Eddington Quasar at z=6.61901.02615v2 · Ji-Jia Tang, Tomotsugu Goto, Youichi Ohyama et al.2019 · 34 citationsarXiv
CFHT Legacy Ultraviolet Extension (CLUE): Witnessing Galaxy Transformations up to 7 Mpc from Rich Cluster Cores1110.3336v1 · Ting Lu, David Gilbank, Sean McGee et al.2011 · 37 citationsarXiv
The stellar and hot gas content of low-mass galaxy clusters1011.0602v3 · Michael L. Balogh, Pasquale Mazzotta, Richard G. Bower et al.2010 · 17 citationsarXiv
Large-scale Structure and Dynamics of the Most X-ray Luminous Galaxy Cluster Known -- RX J1347-11450912.2356v1 · Ting Lu, David G. Gilbank, Michael L. Balogh et al.2009 · 24 citationsarXiv
Recent Arrival of Faint Cluster Galaxies on the Red-sequence: Luminosity Functions from 119 square degrees of CFHTLS0905.3392v1 · Ting Lu, David G. Gilbank, Michael L. Balogh et al.2009 · 43 citationsarXiv
Career total: 38 works. 30 are in this corpus.
Profile built from the corpus for this byline.
Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.