Search Results for author: Tzu-Ching Chang

Found 6 papers, 3 papers with code

HI constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps

no code implementations9 Feb 2021 Laura Wolz, Alkistis Pourtsidou, Kiyoshi W. Masui, Tzu-Ching Chang, Julian E. Bautista, Eva-Maria Mueller, Santiago Avila, David Bacon, Will J. Percival, Steven Cunnington, Chris Anderson, Xuelei Chen, Jean-Paul Kneib, Yi-Chao Li, Yu-Wei Liao, Ue-Li Pen, Jeffrey B. Peterson, Graziano Rossi, Donald P. Schneider, Jaswant Yadav, Gong-Bo Zhao

We present the joint analysis of Neutral Hydrogen (HI) Intensity Mapping observations with three galaxy samples: the Luminous Red Galaxy (LRG) and Emission Line Galaxy (ELG) samples from the eBOSS survey, and the WiggleZ Dark Energy Survey sample.

Cosmology and Nongalactic Astrophysics

Probing Cosmic Reionization and Molecular Gas Growth with TIME

no code implementations16 Dec 2020 Guochao Sun, Tzu-Ching Chang, Bade D. Uzgil, Jamie Bock, Charles M. Bradford, Victoria Butler, Tessalie Caze-Cortes, Yun-Ting Cheng, Asantha Cooray, Abigail T. Crites, Steve Hailey-Dunsheath, Nick Emerson, Clifford Frez, Benjamin L. Hoscheit, Jonathon R. Hunacek, Ryan P. Keenan, Chao-Te Li, Paolo Madonia, Daniel P. Marrone, Lorenzo Moncelsi, Corwin Shiu, Isaac Trumper, Anthony Turner, Alexis Weber, Ta-Shun Wei, Michael Zemcov

The Tomographic Ionized-carbon Mapping Experiment (TIME) will measure the star formation rate (SFR) during cosmic reionization by observing the redshifted [CII] 158$\mu$m line ($6 \lesssim z \lesssim 9$) in the LIM regime.

Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics

Gravitational Wave Detection with Photometric Surveys

1 code implementation5 Oct 2020 Yijun Wang, Kris Pardo, Tzu-Ching Chang, Olivier Doré

While the detection threshold assuming the currently expected performance proves too high for detecting individual GWs in light of the expected supermassive black hole binary population distribution, we show that binaries with chirp mass $M_c>10^{8. 3}~M_\odot$ out to 100 Mpc can be detected if the telescope is able to achieve an astrometric accuracy of 0. 11 mas.

General Relativity and Quantum Cosmology Cosmology and Nongalactic Astrophysics

DAYENU: A Simple Filter of Smooth Foregrounds for Intensity Mapping Power Spectra

2 code implementations23 Apr 2020 Aaron Ewall-Wice, Nicholas Kern, Joshua S. Dillon, Adrian Liu, Aaron Parsons, Saurabh Singh, Adam Lanman, Paul La Plante, Nicolas Fagnoni, Eloy de Lera Acedo, David R. DeBoer, Chuneeta Nunhokee, Philip Bull, Tzu-Ching Chang, T. Joseph Lazio, James Aguirre, Sean Weinberg

We introduce DAYENU, a linear, spectral filter for HI intensity mapping that achieves the desirable foreground mitigation and error minimization properties of inverse co-variance weighting with minimal modeling of the underlying data.

Cosmology and Nongalactic Astrophysics Instrumentation and Methods for Astrophysics

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