76 citations · 310 across the 10 of their papers we have counts for
10 papers
H emission in the outskirts of galaxies at z=0.4
Rhythm Shimakawa, Masayuki Tanaka, Satoshi Kikuta +1
This paper reports detections of H emission and stellar continuum out to approximately 30 physical kpc, and H directionality in the outskirts of H-emitting galaxies (H…
Constraining the Movement of the Spiral Features and the Locations of Planetary Bodies within the AB Aur System
Jamie R. Lomax, John P. Wisniewski, Carol A. Grady +54
We present new analysis of multi-epoch, H-band, scattered light images of the AB Aur system. We used a Monte Carlo, radiative transfer code to simultaneously model the system's SED…
Enhanced Star Formation of Less Massive Galaxies in a Proto-Cluster at z=2.5
Masao Hayashi, Tadayuki Kodama, Ichi Tanaka +5
We investigate a correlation between star-formation rate (SFR) and stellar mass for Halpha emission line galaxies (HAEs) in one of the richest proto-clusters ever known at z~2.5, U…
[OIII] emission line as a tracer of star-forming galaxies at high redshifts: Comparison between H and [OIII] emitters at =2.23 in HiZELS
T. L. Suzuki, T. Kodama, D. Sobral +10
We investigate the properties of =2.23 H and [OIII]5007 emitters using the narrow-band-selected samples obtained from the High- Emission Line Survey (HiZELS: Sobral et…
Similarities and uniqueness of Ly emitters among star-forming galaxies at z=2.5
Rhythm Shimakawa, Tadayuki Kodama, Takatoshi Shibuya +8
We conducted a deep narrow-band imaging survey with the Subaru Prime Focus Camera on the Subaru Telescope and constructed a sample of Ly emitters (LAEs) at z=2.53 in the UDS-CAN…
Correlation between star formation activity and electron density of ionized gas at z=2.5
Rhythm Shimakawa, Tadayuki Kodama, Charles C. Steidel +7
In the redshift interval of , the physical conditions of the inter-stellar medium (ISM) in star-forming galaxies are likely to be different from those in the local Universe…