Hai Fu's Homepage

Building the Tully-Fisher Relation without Estimating Inclination Angles

Posted on February 23, 2024

Fu, H., ApJL, 963, L19 (2024) “Restoration of the Tully-Fisher Relation by Statistical Rectification” [Read More]

Tags: research

New student papers on dual active galactic nuclei published on the Astrophysical Journal

Posted on March 8, 2023

The following papers concluded two PhD theses in Physics (Astronomy subtrack) at the University of Iowa. Congratulations, Dr. Joshua Steffen and Dr. Arran Gross! [Read More]

Tags: research

Nature paper - A fast radio burst in a complex magnetised environment and a barred galaxy

Posted on September 21, 2022

I am part of an international team who discovered the highly variable magnetised environment of an extremely active fast radio burst in a distant galaxy. I contributed to the analysis of the optical spectra of the host galaxy 1.4 billion lightyears away and the background (possibly lensed) galaxy. I also... [Read More]

Tags: research

A New Longslit Spectrograph for Undergraduate Astronomy Labs

Posted on May 6, 2022

In Fall 2021 and Spring 2022, two undergraduate students helped me commission a longslit spectrograph on the 17-in telescope (PlaneWave CDK17) at the Van Allen Observatory (VAO). The LISA Spectrograph is made by Shelyak Instruments. The spectrograph bundle includes the spectrograph optics, a small CCD camera for target acquisition, a... [Read More]

Tags: teaching

MaNGA Merger Project funded by the NSF (AST-2103251)

Posted on September 27, 2021

The important role played by collisions and mergers in galaxy evolution has been appreciated since the 1970’s. Previous spectroscopic studies of colliding/merging galaxies, while confirming several basic predictions (e.g., elevated nuclear star formation and/or black hole accretion), generally explored only their brighter inner-most regions in a largely non-uniform manner. This... [Read More]

Tags: research news

Researchers detect cold gas pipelines feeding early, massive galaxies

Posted on February 24, 2021

Using absorption lines in the spectra of two background quasars and deep ALMA observations in CO, our group discovered a cold gas stream in a massive dark matter halo. The stream is made of gas that is extremely poor in heavy elements. The detection signifies that massive starburst galaxies existed... [Read More]

Tags: research news

The gas fraction evolution of star-forming galaxies traced by the CO Tully-Fisher relation

Posted on December 10, 2018

For the first time, we used the CO Tully-Fisher relation and a Bayesian statistical method to show the dramatic evolution in gas content of star-forming galaxies, confirming previous result that galaxies were much more gaseous billions of years ago. This new method avoids correcting the inclination angles of the galaxies... [Read More]

Tags: research news

Flat rotation curves measured in ancient dusty starburst galaxies

but they rotate more than 2x faster than the Milky Way

Posted on August 15, 2018

This study utilizes extremely deep high-resolution data from the Atacama Large Millimeter / submillimeter Array (ALMA). Various molecules (e.g., water, carbon monoxide) are detected in a pair of dusty starburst galaxies called ‘HXMM01’, a mega-merger that occurred 10 billion years ago (see news story on Los Angeles Times). In both... [Read More]

Tags: research news

Student-created ‘sandbox’ shows how gravity works

Posted on January 16, 2018

The NSF-funded augmented-reality sandbox, dubbed “Gravbox,” is the first interactive system of its kind to be used for astrophysics. Read the news story. For more information, see the Gravbox Website. [Read More]

Tags: research news