Masafumi Ishigaki

Precise Strong Lensing Mass Modeling of Four Hubble frontier Field Clusters and a Sample of Magnified High-redshift Galaxies

We conduct precise strong lensing mass modeling of four

ALMA Census of Faint 1.2 mm Sources Down to ~0.02 mJy: Extragalactic Background Light and Dust-Poor High-z Galaxies

{\it Hubble}

Evolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data

Frontier Fields (HFF) clusters, Abell

Full-data Results of Hubble Frontier Fields: UV Luminosity Functions at z ∼ 6–10 and a Consistent Picture of Cosmic Reionization

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The Frontier Fields lens modelling comparison project

2744, MACS

Size–Luminosity Relations and UV Luminosity Functions at z = 6–9 Simultaneously Derived from the Complete Hubble Frontier Fields Data

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Line identification and photometric history of the hot post-AGB star Hen 3−1013 (IRAS 14331−6435)

J0416.1

HUBBLE FRONTIER FIELDS FIRST COMPLETE CLUSTER DATA: FAINT GALAXIES AT z ∼ 5-10 FOR UV LUMINOSITY FUNCTIONS AND COSMIC REIONIZATION

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THE SIZES OF z ? 6?8 LENSED GALAXIES FROM THE HUBBLE FRONTIER FIELDS ABELL 2744 DATA

2403, MACS

rEFSDAL MEETS POPPER: COMPARING PREDICTIONS of the RE-APPEARANCE of the MULTIPLY IMAGED SUPERNOVA behind MACSJ1149.5+2223

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