155 citations · 185 across the 5 of their papers we have counts for
6 papers
Clumps as multiscale structures in cosmic noon galaxies
Boris S Kalita, Tomoko L Suzuki, Daichi Kashino +31
Star-forming clumps have been found to significantly influence the star formation of gas-rich galaxies. Using public data from JWST/NIRCam (COSMOS-Web) and ALMA (FMOS-COSMOS)…
Evolution of H Equivalent Widths from : implications for star formation and legacy surveys with Roman and Euclid
Ali Ahmad Khostovan, Sangeeta Malhotra, James E. Rhoads +5
We investigate the `intrinsic' H EW distributions of narrowband-selected H samples from HiZELS and DAWN using a forward modeling approach. We find an EW -…
MIGHTEE-HI: HI galaxy properties in the large scale structure environment at z~0.37 from a stacking experiment
Francesco Sinigaglia, Giulia Rodighiero, Ed Elson +20
We present the first measurement of HI mass of star-forming galaxies in different large scale structure environments from a blind survey at . In particular, we carry ou…
CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS COSMOS Survey Field
H. Nayyeri, S. Hemmati, B. Mobasher +36
We present a multi-wavelength photometric catalog in the COSMOS field as part of the observations by the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS). T…
[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…
The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE
Asantha Cooray, Steve Eales, Scott Chapman +247
A large sub-mm survey with Herschel will enable many exciting science opportunities, especially in an era of wide-field optical and radio surveys and high resolution cosmic microwa…