Zobrazeno 1 - 10
of 4 641
pro vyhledávání: '"Shim, H."'
Autor:
White, Glenn J., Barrufet, L., Serjeant, S., Pearson, C. P., Sedgwick, C., Pal, S., Shimwell, T. W., Sirothia, S. K., Chiu, P., Oi, N., Takagi, T., Shim, H., Matsuhara, H., Patra, D., Malkan, M., Kim, H. K., Nakagawa, T., Malek, K., Burgarella, D., Ishigaki, T.
This paper presents a 610 MHz radio survey covering 1.94 square degrees around the North Ecliptic Pole (NEP), which includes parts of the AKARI (ADF-N) and Euclid, Deep Fields North. The median 5-sigma sensitivity is 28 microJy beam per beam, reachin
Externí odkaz:
http://arxiv.org/abs/2411.03869
Autor:
Pearson, W. J., Santos, D. J. D., Goto, T., Huang, T. -C., Kim, S. J., Matsuhara, H., Pollo, A., Ho, S. C. -C., Hwang, H. S., Małek, K., Nakagawa, T., Romano, M., Serjeant, S., Suelves, L., Shim, H., White, G. J.
Publikováno v:
A&A 686, A94 (2024)
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 to study how the properties of a group or cluster, as well as the posit
Externí odkaz:
http://arxiv.org/abs/2403.11615
Autor:
Garratt, T. K., Geach, J. E., Tamura, Y., Coppin, K. E. K., Franco, M., Ao, Y., Chen, C. -C., Cheng, C., Clements, D. L., Dai, Y. S., Dannerbauer, H., Greve, T. R., Hatsukade, B., Hwang, H. S., Jiang, L., Kohno, K., Koprowski, M. P., Michalowski, M. J., Sawicki, M., Scott, D., Shim, H., Takeuchi, T. T., Wang, W. -H., Xue, Y. Q., Yang, C.
We present 850um imaging of the XMM-LSS field observed for 170 hours as part of the James Clerk Maxwell Telescope SCUBA-2 Large eXtragalactic Survey (S2LXS). S2LXS XMM-LSS maps an area of 9 square degrees, reaching a moderate depth of 1-sigma ~ 4 mJy
Externí odkaz:
http://arxiv.org/abs/2301.10801
Autor:
Shim, H., Lee, D., Kim, Y., Scott, D., Serjeant, S., Ao, Y., Barrufet, L., Chapman, S. C., Clements, D., Conselice, C. J., Goto, T., Greve, T. R., Hwang, H. S., Im, M., Jeong, W. -S., Kim, H. K., Kim, M., Kim, S. J., Kong, A. K. H., Koprowski, M. P., Malkan, M. A., Michalowski, M., Pearson, C., Seo, H., Takagi, T., Toba, Y., White, G. J., Woo, J. -H.
We present the multi-wavelength counterparts of 850-$\mu$m selected submillimetre sources over a 2-deg$^2$ field centred on the North Ecliptic Pole. In order to overcome the large beam size (15 arcsec) of the 850-$\mu$m images, deep optical to near-i
Externí odkaz:
http://arxiv.org/abs/2204.11392
Autor:
Pearson, W. J., Suelves, L. E., Ho, S. C. -C., Oi, N., Brough, S., Holwerda, B. W., Hopkins, A. M., Huang, T. -C., Hwang, H. S., Kelvin, L. S., Kim, S. J., López-Sánchez, Á. R., Małek, K., Pearson, C., Poliszczuk, A., Pollo, A., Rodriguez-Gomez, V., Shim, H., Toba, Y., Wang, L.
We aim to generate a catalogue of merging galaxies within the 5.4 sq. deg. North Ecliptic Pole over the redshift range $0.0 < z < 0.3$. To do this, imaging data from the Hyper Suprime-Cam are used along with morphological parameters derived from thes
Externí odkaz:
http://arxiv.org/abs/2202.10780
Autor:
Huang, T. -C., Matsuhara, H., Goto, T., Santos, D. J. D., Ho, S. C. -C., Kim, S. J., Hashimoto, T., Ikeda, Hiroyuki, Oi, Nagisa, Malkan, M. A., Pearson, W. J., Pollo, A., Serjeant, S., Shim, H., Miyaji, T., Hwang, H. S., Durkalec, A., Poliszczuk, A., Greve, T. R., Pearson, C., Toba, Y., Lee, D., Kim, H. K., Toft, S., Jeong, W. -S., Enokidani, U.
Galaxy clusters provide an excellent probe in various research fields in astrophysics and cosmology. However, the number of galaxy clusters detected so far in the $AKARI$ North Ecliptic Pole (NEP) field is limited. In this work, we provide galaxy clu
Externí odkaz:
http://arxiv.org/abs/2107.10010
Autor:
Dudzevičiūtė, U., Smail, I., Swinbank, A. M., Lim, C. -F., Wang, W. -H., Simpson, J. M., Ao, Y., Chapman, S. C., Chen, C. -C., Clements, D., Dannerbauer, H., Ho, L. C., Hwang, H. S., Koprowski, M., Lee, C. -H., Scott, D., Shim, H., Shirley, R., Toba, Y.
We analyse the physical properties of 121 SNR $\geq$ 5 sub-millimetre galaxies (SMGs) from the STUDIES 450-$\mu$m survey. We model their UV-to-radio spectral energy distributions using MAGPHYS+photo-$z$ and compare the results to similar modelling of
Externí odkaz:
http://arxiv.org/abs/2010.06605
Autor:
Huang, T. -C., Matsuhara, H., Goto, T., Shim, H., Kim, S. J., Malkan, M. A., Hashimoto, T., Hwang, H. S., Oi, N., Toba, Y., Lee, D., Santos, D. J. D., Takagi, T.
The $AKARI$ infrared (IR) space telescope conducted two surveys (Deep and Wide) in the North Ecliptic Pole (NEP) field to find more than 100,000 IR sources using its Infrared Camera (IRC). IRC's 9 filters, which cover wavebands from 2 to 24 $\mu$m co
Externí odkaz:
http://arxiv.org/abs/2008.05224
Autor:
Millard, Jenifer S., Eales, Stephen A., Smith, M. W. L., Gomez, H. L., Małek, K., Simpson, J. M., Peng, Y., Sawicki, M., Beeston, R. A., Bunker, Andrew, Ao, Y., Babul, A., Ho, L. C., Hwang, Ho Seong, Michałowski, M. J., Scoville, N., Shim, H., Toba, Y.
We investigate the evolution of the gas mass fraction for galaxies in the COSMOS field using submillimetre emission from dust at 850$\mu$m. We use stacking methodologies on the 850$\mu$m S2COSMOS map to derive the gas mass fraction of galaxies out to
Externí odkaz:
http://arxiv.org/abs/2003.01727
Publikováno v:
Journal of Inflammation Research, Vol Volume 15, Pp 4623-4636 (2022)
Seung Hoon Lee,1,* Hyung-Jin Kim,1,* Gi-Su Oh,1 Su-Bin Lee,1 Dipendra Khadka,1 Wal Cao,1 Seong-Kyu Choe,1 Hyeok Shim,2 Chang-Deok Kim,3 Tae Hwan Kwak,4 Hong-Seob So1,4 1Department of Microbiology, Wonkwang University School of Medicine, Iksan
Externí odkaz:
https://doaj.org/article/f6a9ad5e0b7f4902a2e23455966cf945
