Zobrazeno 1 - 10
of 43
pro vyhledávání: '"Yunkun Han"'
Publikováno v:
The Astrophysical Journal, Vol 968, Iss 1, p 13 (2024)
The luminosity and spectral energy distribution of high- z galaxies are sensitive to the stellar-population synthesis (SPS) models. In this paper, we study the effects of different SPS models on the measurements of high- z galaxies and the budget of
Externí odkaz:
https://doaj.org/article/f2d94f6789584b1baa598ed1d5829a41
Publikováno v:
The Astrophysical Journal, Vol 964, Iss 1, p 95 (2024)
We present a UV to millimeter spectral energy distribution (SED) analysis of 16 hyperluminous, dust-obscured quasars at z ∼ 3, selected by the Wide-field Infrared Survey Explorer. We aim to investigate the physical properties of these quasars, with
Externí odkaz:
https://doaj.org/article/681ae9d73b334935936e028e634a4b7c
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 269, Iss 2, p 39 (2023)
The forthcoming Chinese Space Station Telescope (CSST) wide-field multiband imaging survey will produce seven-band photometric spectral energy distributions (SEDs) for billions of galaxies. The effective extraction of astronomical information from th
Externí odkaz:
https://doaj.org/article/3cef301f5d1e48cf945c319e37c4ce78
Publikováno v:
The Astrophysical Journal
WISE J224607.56$-$052634.9 (W2246-0526) is a hyperluminous ($L_{\rm bol}\approx 1.7\times 10^{14}~L_\odot$), dust-obscured and radio-quiet quasar at redshift $z=4.6$. It plays a key role in probing the transition stage between dusty starbursts and un
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::17a75ffc29cf881ab5962a26a682a7c5
Autor:
Xinwen Shu, Lei Yang, Daizhong Liu, Wei-Hao Wang, Tao Wang, Yunkun Han, Xingxing Huang, Chen-Fatt Lim, Yu-Yen Chang, Wei Zheng, XianZhong Zheng, Junxian Wang, Xu Kong
Publikováno v:
The Astrophysical Journal. 926:155
We present ALMA 870um and JCMT SCUBA2 850um dust continuum observations of a sample of optically dark and strongly lensed galaxies in the cluster fields. The ALMA and SCUBA2 observations reach a median rms of about 0.11 mJy and 0.44 mJy, respectively
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5b95c8236976a88a558627d0622c0333
https://doi.org/10.3847/1538-4357/ac3de5
https://doi.org/10.3847/1538-4357/ac3de5
Publikováno v:
Proceedings of the International Astronomical Union. 15:268-270
The massive galaxies and their central supermassive black holes (SMBHs) co-evolution scenario proposes that a gas-rich major merger can trigger the central starburst and feeding the SMBH accretion, and then star formation is eventually quenched by qu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::20cd2a5d4f7c7430d0c8180a57ed10f9
https://doi.org/10.1017/s1743921319001352
https://doi.org/10.1017/s1743921319001352
We present ALMA observations and multiwavelength spectral energy distribution (SED) analysis in a WISE-selected, hyperluminous dust-obscured quasar W0533-3401 at $z=2.9$. We derive its physical properties of each component, such as molecular gas, sta
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::44904c0c100bb99a60fd97d3c80ba5ab
http://arxiv.org/abs/1910.10155
http://arxiv.org/abs/1910.10155
Autor:
Yunkun Han, Zhanwen Han
Publikováno v:
The Astrophysical Journal Supplement Series. 240:3
When modeling and interpreting the spectral energy distributions (SEDs) of galaxies, the simple stellar population (SSP) model, star formation history (SFH) and dust attenuation law (DAL) are three of the most important components. However, each of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3fa97940d285767c803341877b1b5ec3
https://doi.org/10.3847/1538-4365/aaeffa
https://doi.org/10.3847/1538-4365/aaeffa
Autor:
Dandan Zhang, Guanwen Fang, Qiaoqian Wu, Lulu Fan, Xiaoming Jiang, Ying Gao, Jun Yang, Yunkun Han, Zhao Li
Previous studies have shown that WISE-selected hyperluminous, hot dust-obscured galaxies (Hot DOGs) are powered by highly dust-obscured, possibly Compton-thick AGNs. High obscuration provides us a good chance to study the host morphology of the most
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::050bcf381fa9efedbb23cb667713631a
http://arxiv.org/abs/1605.00661
http://arxiv.org/abs/1605.00661
We utilize a Bayesian approach to fit the observed mid-IR-to-submm/mm spectral energy distributions (SEDs) of 22 WISE-selected and submm-detected, hyperluminous hot dust-obscured galaxies. By adopting the Torus+GB model, we decompose the observed IR
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::defd7ccad076cab9a28b4d1a4ec391e9