H
Hsin-Yi Shih
Researcher at University of Hawaii
Publications - 20
Citations - 634
Hsin-Yi Shih is an academic researcher from University of Hawaii. The author has contributed to research in topics: Galaxy & Radio galaxy. The author has an hindex of 11, co-authored 19 publications receiving 595 citations. Previous affiliations of Hsin-Yi Shih include University of Hawaii at Manoa.
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Journal ArticleDOI
Exclusion of a luminous red giant as a companion star to the progenitor of supernova SN 2011fe
Weidong Li,Joshua S. Bloom,Philipp Podsiadlowski,Adam A. Miller,S. Bradley Cenko,Saurabh Jha,Mark Sullivan,D. Andrew Howell,D. Andrew Howell,Peter Nugent,Peter Nugent,Nathaniel R. Butler,Eran O. Ofek,Eran O. Ofek,Mansi M. Kasliwal,Joseph W. Richards,A. Stockton,Hsin-Yi Shih,Lars Bildsten,Michael M. Shara,Joanne Bibby,Alexei V. Filippenko,Mohan Ganeshalingam,Jeffrey M. Silverman,Shrinivas R. Kulkarni,Nicholas M. Law,Dovi Poznanski,Robert M. Quimby,C. McCully,Brandon Patel,Kate Maguire,Ken J. Shen +31 more
TL;DR: The luminosity of the progenitor system (especially the companion star) is 10–100 times fainter than previous limits on other type Ia supernova progenitors systems, allowing us to rule out luminous red giants and almost all helium stars as the mass-donating companion to the exploding white dwarf.
Journal ArticleDOI
Ionized Outflows from Compact Steep Spectrum Sources
TL;DR: In this article, the emission-line regions around compact-steep-spectrum (CSS) radio galaxies that are younger (103-105 yr old) versions of the FR II radio galaxies are studied.
Journal ArticleDOI
A comparison of the morphological properties between local and z ∼ 1 infrared luminous galaxies: Are local and high-z (U)LIRGs different?
Chao-Ling Hung,Chao-Ling Hung,David B. Sanders,Caitlin M. Casey,Michael Koss,Kirsten L. Larson,Nicholas Lee,Yanxia Li,Kelly E. Lockhart,Hsin-Yi Shih,Joshua E. Barnes,Jeyhan S. Kartaltepe,Howard A. Smith +12 more
TL;DR: In the local universe (z 1), the morphology types of ~30% of (U)LIRGs cannot be determined due to their faintness in the F814W band; thus, the merger fraction measured at z > 1 suffers from large uncertainties as mentioned in this paper.
Journal ArticleDOI
Imaging of Three Possible Low-redshift Analogs to High-redshift Compact Red Galaxies
Hsin-Yi Shih,Alan Stockton +1 more
TL;DR: In this paper, the authors examined the morphologies of three low-redshift compact galaxies drawn from the sample of Trujillo et al. using deeper and higher resolution images, and found faint and relatively extensive outer structures in addition to the compact cores identified in the earlier measurements.
Journal ArticleDOI
A Search for Moderate-redshift Survivors from the Population of Luminous Compact Passive Galaxies at High Redshift
TL;DR: In this paper, a search of a ∼2400 deg{sup 2} region covered by both the Sloan Digital Sky Survey and UKIRT Infrared Deep Sky Survey databases was conducted to identify galaxies at z ∼ 0.5 that are consistent with their being essentially unmodified examples of the luminous passive compact galaxies found at z ≥ 2.5.