33 citations · 107 across the 7 of their papers we have counts for
7 papers
Chandra Survey in the AKARI North Ecliptic Pole Deep Field Optical/Infrared Identifications of X-ray Sources
T. Miyaji, B. A. Bravo-Navarro, J. Díaz Tello +17
We present a catalog of optical and infrared identifications (ID) of X-ray sources in the AKARI North Ecliptic Pole (NEP) Deep field detected with Chandra covering $\sim 0.34\,{\rm…
Effects of galaxy environment on merger fraction
W. J. Pearson, D. J. D. Santos, T. Goto +13
Aims. In this work, we intend to examine how environment influences the merger fraction, from the low density field environment to higher density groups and clusters. We also aim t…
Variation of optical and infrared properties of galaxies with their surface brightness
Junais, K. Małek, S. Boissier +12
Although low surface brightness galaxies (LSBs) contribute a large fraction to the number density of galaxies, their properties are still poorly known. LSBs are often considered du…
North Ecliptic Pole merging galaxy catalogue
W. J. Pearson, L. E. Suelves, S. C. -C. Ho +17
We aim to generate a catalogue of merging galaxies within the 5.4 sq. deg. North Ecliptic Pole over the redshift range . To do this, imaging data from the Hyper Supr…
The 2 to 24 micron source counts from the AKARI North Ecliptic Pole survey
K. Murata, C. P. Pearson, T. Goto +3
We present herein galaxy number counts of the nine bands in the 2-24 micron range on the basis of the AKARI North Ecliptic Pole (NEP) surveys. The number counts are derived from NE…
The First Source Counts at 18 microns from the AKARI NEP Survey
Chris Pearson, S. Serjeant, S. Oyabu +9
We present the first galaxy counts at 18 microns using the Japanese AKARI satellite's survey at the North Ecliptic Pole (NEP), produced from the images from the NEP-Deep and NEP-Wi…
Source Counts at 15 microns from the AKARI NEP Survey
C. P. Pearson, S. Oyabu, T. Wada +11
We present galaxy counts at 15 microns using the Japanese AKARI satellite's NEP-deep and NEP-wide legacy surveys at the North Ecliptic Pole. The total number of sources detected ar…