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| WoS | SCOPUS | Document Type | Document Title | Abstract | Authors | Affiliation | ResearcherID (WoS) | AuthorsID (SCOPUS) | Author Email(s) | Journal Name | JCR Abbreviation | ISSN | eISSN | Volume | Issue | WoS Edition | WoS Category | JCR Year | IF | JCR (%) | FWCI | FWCI Update Date | WoS Citation | SCOPUS Citation | Keywords (WoS) | KeywordsPlus (WoS) | Keywords (SCOPUS) | KeywordsPlus (SCOPUS) | Language | Publication Stage | Publication Year | Publication Date | DOI | JCR Link | DOI Link | WOS Link | SCOPUS Link |
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| ○ | ○ | Article | How neutral nitrogen-containing compounds are oxidized in oxidative-denitrogenation of liquid fuel with TiO2@carbon | Oxidative-denitrogenation (ODN) of indole (IND) and methyl-substituted INDs (methyl-INDs), representative neutral nitrogen-containing compounds (NCCs), was carried out with TiO2@C and H2O2 as heterogeneous catalyst and oxidant, respectively, under ultrasound irradiation. The oxidation of INDs progressed through radical formation, as evidenced by electron spin resonance and radical scavenger experiments. The oxidized position of INDs in the ODN process was checked via characterization of the obtained products. It was observed that the oxidation finally occurred on the carbon rather than on the nitrogen atom of INDs, unlike the oxidation of basic NCCs (e.g., oxidation on the nitrogen atom, as respective N-oxides were formed) and sulfur-containing compounds. To understand the relative reactivity and oxidation position, electron density (ED) on the nitrogen atom of the studied INDs and relative stability of representative intermediates/products were calculated. It could be confirmed that ED on the nitrogen atom of the INDs is very important in the oxidation of INDs since the ODN reactivity of INDs was enhanced with increasing ED on the nitrogen atom of the investigated INDs. Moreover, theoretical analyses of the relative stability of substrate and intermediates/products (especially for IND) can explain the route for the observed final products in ODN. In other words, oxygen on the nitrogen atom, obtained via the first step of oxidation (electrophilic addition of an active oxygen atom on nitrogen), moves to the nearby carbon atom, because of the relative stability of the intermediates and products. | Bhadra, Biswa Nath; Baek, Yong Su; Choi, Cheol Ho; Jhung, Sung Hwa | Kyungpook Natl Univ, Dept Chem, Daegu 41566, South Korea; Kyungpook Natl Univ, Greennano Mat Res Ctr, Daegu 41566, South Korea | ; Jhung, Sung/AAO-6683-2021; Bhadra, Biswa/ABG-6935-2021; Bhadra, Biswa Nath/ABG-6935-2021; Choi, Cheol Ho/AAA-4705-2020 | 56982844300; 57201976608; 7402958948; 6701659467 | cchoi@knu.ac.kr;sung@knu.ac.kr; | PHYSICAL CHEMISTRY CHEMICAL PHYSICS | PHYS CHEM CHEM PHYS | 1463-9076 | 1463-9084 | 23 | 14 | SCIE | CHEMISTRY, PHYSICAL;PHYSICS, ATOMIC, MOLECULAR & CHEMICAL | 2021 | 3.945 | 23.6 | 0.3 | 2025-07-30 | 6 | 6 | METAL-ORGANIC FRAMEWORK; LIGHT GAS OIL; ADSORPTIVE REMOVAL; HYDROGEN-PEROXIDE; VISIBLE-LIGHT; DESULFURIZATION; DESULFURIZATION/DENITRIFICATION; COMPOSITE; ADSORBENT; CATALYSTS | Atoms; Carbon; Ionization of gases; Magnetic moments; Oxidation; Oxide minerals; Oxygen; Sulfur compounds; Titanium dioxide; Electrophilic additions; Heterogeneous catalyst; Oxidative denitrogenation; Radical scavengers; Relative reactivities; Relative stabilities; Sulfur containing compound; Ultrasound irradiation; Reaction intermediates | English | 2021 | 2021-04-14 | 10.1039/d1cp00633a | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |||
| ○ | ○ | Article | Tunnel barrier engineering of spin-polarized mild band gap vertical ternary heterostructures | The atomic and electronic structures and properties of advanced 2D ternary vertical spin-polarized semiconducting heterostructures based on mild band gap graphitic carbon nitride g-C3N4 and ferromagnetic single-layer CrI3 fragments, namely CrI3/g-C3N4/CrI3 and g-C3N4/CrI3/g-C3N4, were proposed and examined using the ab initio GGA PBE PBC technique. Both possible ferromagnetic (FM) and antiferromagnetic (AFM) spin ordering configurations of CrI3/g-C3N4/CrI3 were considered and found to be energetically degenerated, being significantly different in the density of states. Electronic structure calculations revealed that weak van der Waals interactions between the fragments are responsible for the main features of the atomic and electronic structures of both the types of heterostructures. The combination of flat valence and conduction bands and conductivity channels localized at spin-polarized semiconducting CrI3 fragments makes proposed heterostructures as magnetic tunnel junctions for spin- and photo-related applications such as spintronics, magnetoresistive random-access memory, photocatalysis, and as elements for highly efficient spin-polarized photovoltaic nanodevices. | Melchakova, Iu; Avramov, P. | Kyungpook Natl Univ, Dept Chem, Daegu, South Korea | Melchakova, Iuliia/KGM-5967-2024 | 57206720228; 7004322420 | paul.veniaminovich@knu.ac.kr; | PHYSICAL CHEMISTRY CHEMICAL PHYSICS | PHYS CHEM CHEM PHYS | 1463-9076 | 1463-9084 | 23 | 39 | SCIE | CHEMISTRY, PHYSICAL;PHYSICS, ATOMIC, MOLECULAR & CHEMICAL | 2021 | 3.945 | 23.6 | 0.08 | 2025-07-30 | 1 | 1 | INITIO MOLECULAR-DYNAMICS; GIANT MAGNETORESISTANCE; DEVICES; ENERGY | Antiferromagnetism; Calculations; Chromium compounds; Electronic structure; Ferromagnetic materials; Ferromagnetism; Spin polarization; Tunnel junctions; Van der Waals forces; Antiferromagnetic spin ordering; Barrier engineering; Electronic.structure; Ferromagnetic and anti-ferromagnetic; Ferromagnetic spin ordering; Graphitic carbon nitrides; Single layer; Spin-polarized; Structures and properties; Tunnel barrier; Energy gap | English | 2021 | 2021-10-13 | 10.1039/d1cp02051j | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |||
| ○ | ○ | Article | LeuO, a LysR-Type Transcriptional Regulator, Is Involved in Biofilm Formation and Virulence of Acinetobacter baumannii | Acinetobacter baumannii is an important nosocomial pathogen that can survive in different environmental conditions and poses a severe threat to public health due to its multidrug resistance properties. Research on transcriptional regulators, which play an essential role in adjusting to new environments, could provide new insights into A. baumannii pathogenesis. LysR-type transcriptional regulators (LTTRs) are structurally conserved among bacterial species and regulate virulence in many pathogens. We identified a novel LTTR, designated as LeuO encoded in the A. baumannii genome. After construction of LeuO mutant strain, transcriptome analysis showed that LeuO regulates the expression of 194 upregulated genes and 108 downregulated genes responsible for various functions and our qPCR validation of several differentially expressed genes support transcriptome data. Our results demonstrated that disruption of LeuO led to increased biofilm formation and increased pathogenicity in an animal model. However, the adherence and surface motility of the LeuO mutant were reduced compared with those of the wild-type strain. We observed some mutations on amino acids sequence of LeuO in clinical isolates. These mutations in the A. baumannii biofilm regulator LeuO may cause hyper-biofilm in the tested clinical isolates. This study is the first to demonstrate the association between the LTTR member LeuO and virulence traits of A. baumannii. | Islam, Md. Maidul; Kim, Kyeongmin; Lee, Je Chul; Shin, Minsang | Kyungpook Natl Univ, Sch Med, Dept Microbiol, Daegu, South Korea | Islam, Md. Maidul/AAE-6691-2022 | 57216605059; 57216604095; 25930392000; 7401536650 | shinms@knu.ac.kr; | FRONTIERS IN CELLULAR AND INFECTION MICROBIOLOGY | FRONT CELL INFECT MI | 2235-2988 | 11 | SCIE | IMMUNOLOGY;MICROBIOLOGY | 2021 | 6.073 | 23.7 | 1.22 | 2025-07-30 | 18 | 17 | Acinetobacter baumannii; LeuO; transcriptome (RNA-seq); biofilm; virulence; adherence | STAPHYLOCOCCUS-AUREUS-CIDABC; ANTIMICROBIAL RESISTANCE; EPITHELIAL-CELLS; EXPRESSION; MOTILITY; EFFLUX; GENES; PATHOGENESIS; SECRETION; ADHERENCE | Acinetobacter baumannii; adherence; biofilm; LeuO; transcriptome (RNA-seq); virulence | Acinetobacter baumannii; Animals; Biofilms; Virulence; ampicillin; chloramphenicol; crystal violet; cyclophosphamide; kanamycin; transcriptome; Acinetobacter baumannii; amino acid sequence; animal experiment; animal model; Article; bacterial growth; bacterial strain; bacterial virulence; bacterium adherence; biofilm; cell motility; colony forming unit; controlled study; differential gene expression; female; gene expression; gene mutation; mouse; multidrug resistance; nonhuman; pathogenicity; public health; quality control; real time polymerase chain reaction; RNA sequencing; animal; biofilm; genetics; virulence | English | 2021 | 2021-10-11 | 10.3389/fcimb.2021.738706 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |||
| ○ | ○ | Review | Review on Stress Tolerance in Campylobacter jejuni | Campylobacter spp. are the leading global cause of bacterial colon infections in humans. Enteropathogens are subjected to several stress conditions in the host colon, food complexes, and the environment. Species of the genus Campylobacter, in collective interactions with certain enteropathogens, can manage and survive such stress conditions. The stress-adaptation mechanisms of Campylobacter spp. diverge from other enteropathogenic bacteria, such as Escherichia coli, Salmonella enterica serovar Typhi, S. enterica ser. Paratyphi, S. enterica ser. Typhimurium, and species of the genera Klebsiella and Shigella. This review summarizes the different mechanisms of various stress-adaptive factors on the basis of species diversity in Campylobacter, including their response to various stress conditions that enhance their ability to survive on different types of food and in adverse environmental conditions. Understanding how these stress adaptation mechanisms in Campylobacter, and other enteric bacteria, are used to overcome various challenging environments facilitates the fight against resistance mechanisms in Campylobacter spp., and aids the development of novel therapeutics to control Campylobacter in both veterinary and human populations. | Kim, Se-Hun; Chelliah, Ramachandran; Ramakrishnan, Sudha Rani; Perumal, Ayyappasamy Sudalaiyadum; Bang, Woo-Suk; Rubab, Momna; Daliri, Eric Banan-Mwine; Barathikannan, Kaliyan; Elahi, Fazle; Park, Eunji; Jo, Hyeon Yeong; Hwang, Su-Bin; Oh, Deog Hwan | Natl Inst Food & Drug Safety Evaluat, Food Microbiol Div, Food Safety Evaluat Dept, Cheongju, South Korea; Kangwon Natl Univ, Coll Agr & Life Sci, Chunchon, South Korea; Kyungpook Natl Univ, Sch Food Sci, Dept Food Sci & Biotechnol, Coll Agr & Life Sci, Daegu, South Korea; McGill Univ, Dept Bioresource Engn, Montreal, PQ, Canada; Yeungnam Univ, Dept Food & Nutr, Coll Human Ecol & Kinesiol, Gyongsan, South Korea | BARATHIKANNAN, KALIYAN/U-3027-2019; Ghimire, Madhav/AAT-3026-2021; Ramakrishnan, Sudha/V-6342-2017; Oh, Deog-Hwan/AHE-4751-2022; Elahi, Fazle/AAW-2559-2020; Daliri, Eric Banan-Mwine/JQV-7944-2023 | 57195906431; 55954049700; 57190606907; 57226403821; 7004161569; 57200441377; 56483260100; 57190745599; 57213854802; 57204561374; 57200685458; 57200989607; 7203001812 | hoonye77@naver.com;ramachandran865@gmail.com;deoghwa@kangwon.ac.kr; | FRONTIERS IN CELLULAR AND INFECTION MICROBIOLOGY | FRONT CELL INFECT MI | 2235-2988 | 10 | SCIE | IMMUNOLOGY;MICROBIOLOGY | 2021 | 6.073 | 23.7 | 1.12 | 2025-07-30 | 42 | 39 | Campylobacter; stress; resistance mechanisms; stress adaptation; enteric bacteria | 4 DEGREES-C; BIOFILM FORMATION; LISTERIA-MONOCYTOGENES; ANTIBIOTIC-RESISTANCE; CROSS-PROTECTION; HEAT-SHOCK; ANTIMICROBIAL RESISTANCE; FOODBORNE PATHOGENS; SALMONELLA-ENTERICA; HELICOBACTER-PYLORI | Campylobacter; enteric bacteria; resistance mechanisms; stress; stress adaptation | Campylobacter; Campylobacter Infections; Campylobacter jejuni; Enterobacteriaceae; Humans; Shigella; Campylobacter jejuni; enteropathogen; Escherichia coli; human; Klebsiella; nonhuman; physiological stress; review; Salmonella enterica serovar Typhi; Shigella; species diversity; veterinary medicine; Campylobacter; campylobacteriosis; Enterobacteriaceae; Shigella | English | 2021 | 2021-02-04 | 10.3389/fcimb.2020.596570 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |||
| ○ | ○ | Article | Response of epilithic diatom assemblages to weir construction on the Nakdong River, Republic of Korea | In South Korea, sixteen multifunctional weirs were constructed on four major rivers (Han, Nakdong, Geum, Yeongsan) from 2009 to 2012. Hydrological changes resulting from weir construction altered the physical, chemical, and biological characteristics of natural large rivers. We aimed to investigate the variation in epilithic assemblages responding to changes in physicochemical, meteorological, and hydrological variables in the eight weir (lentic) sections of the Nakdong River, which is the longest river in South Korea. Sampling was conducted to determine the influence of environmental parameters on community composition, and to monitor the seasonality of environmental and biological patterns. A total of 173 taxa including 26 major epilithic diatom taxa were identified. Among them, nutrient-tolerant diatom species were characterized by Cyclostephanos dubius, Navicula gregaria, Fragilaria crotonensis, Aulacoseira granulata, Melosira varians, Navicula minima, Nitzschia amphibia, Amphora pediculus, and Nitzschia inconspicua. These species were primarily dominant in the midstream and downstream weir sections of the river adjacent to urban-industrial land use zones relating to nutrient enrichment. Moreover, preference for longer hydraulic retention time (HRT) was identified in C. dubius, N. gregaria, and F. crotonensis, in addition to its tolerance for high nutrition. Redundancy analysis based on the relative abundance of diatom taxa demonstrated that the diatom assemblage composition was closely related to total nitrogen (TN), total phosphorus (TP), phosphate phosphorus (PO4-P), electrical conductivity, precipitation, water discharge, and HRT. Variation partitioning analysis further revealed that hydrological-meteorological variables play a synergistic role in enhancing the function of physical and chemical variables in structuring diatom assemblage composition soon after weir construction. A generalized linear model using the Akaike?s information criterion also suggests that the trophic diatom index (TDI) could indicate the water quality status in the weir sections, as the TDI was positively correlated (p < 0.05) with nutrients (TN and PO4-P). Our findings inform the applicability of using the TDI for efficiently monitoring and managing the water quality of consecutive weir sections of the Nakdong River and the weir systems of other rivers in temperate regions. | Lee, Kyung-Lak; Choi, Jae Sin; Lee, Jae-Hak; Jung, Kang-Young; Kim, Han Soon | Natl Inst Environm Res, Water Environm Engn Res Div, Incheon 22689, South Korea; Kyungpook Natl Univ, Dept Biol, Daegu 41566, South Korea; Natl Inst Environm Res, Yeongsan River Environm Res Ctr, Gwangju 61011, South Korea | 57201446081; 57199098900; 55690077600; 57194539617; 7410135359 | kimhsu@knu.ac.kr; | ECOLOGICAL INDICATORS | ECOL INDIC | 1470-160X | 1872-7034 | 126 | SCIE | ENVIRONMENTAL SCIENCES | 2021 | 6.263 | 23.8 | 0.78 | 2025-07-30 | 7 | 10 | Weir; Nakdong River; Epilithic diatom; Hydraulic retention time; Land use; Diatom trophic index | WATER-QUALITY ASSESSMENT; ECOLOGICAL STATUS; FLOWING WATER; STREAM; COMMUNITIES; DISTURBANCE; INDICATORS; MANAGEMENT; INDEXES; MACROINVERTEBRATE | Diatom trophic index; Epilithic diatom; Hydraulic retention time; Land use; Nakdong River; Weir | Nakdong River; South Korea; Amphora ovalis pediculus; Aulacoseira granulata; Bacillariophyta; Cyclostephanos dubius; Fragilaria crotonensis; Melosira varians; Navicula gregaria; Navicula minima; Nitzschia amphibia; Nitzschia inconspicua; Varanidae; Nutrients; Phosphorus; Precipitation (chemical); Rivers; Water quality; Weirs; Diatom assemblage; Diatom indices; Diatom trophic index; Epilithic diatom; Hydraulic retention; Hydraulic retention time; Meteorological variables; Nakdong river; South Korea; Weir; assembly rule; community composition; diatom; epilithon; hydrological response; relative abundance; seasonality; water quality; weir; Land use | English | 2021 | 2021-07 | 10.1016/j.ecolind.2021.107711 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |||
| ○ | ○ | Article | An active galactic nucleus recognition model based on deep neural network | To understand the cosmic accretion history of supermassive black holes, separating the radiation from active galactic nuclei (AGNs) and star-forming galaxies (SFGs) is critical. However, a reliable solution on photometrically recognizing AGNs still remains unsolved. In this work, we present a novel AGN recognition method based on Deep Neural Network (Neural Net; NN). The main goals of this work are (i) to test if the AGN recognition problem in the North Ecliptic Pole Wide (NEPW) field could be solved by NN; (ii) to show that NN exhibits an improvement in the performance compared with the traditional, standard spectral energy distribution (SED) fitting method in our testing samples; and (iii) to publicly release a reliable AGN/SFG catalogue to the astronomical community using the best available NEPW data, and propose a better method that helps future researchers plan an advanced NEPW data base. Finally, according to our experimental result, the NN recognition accuracy is around 80.29 per cent-85.15 per cent, with AGN completeness around 85.42 per cent-88.53 per cent and SFG completeness around 81.17 per cent-85.09 per cent. | Chen, Bo Han; Goto, Tomotsugu; Kim, Seong Jin; Wang, Ting Wen; Santos, Daryl Joe D.; Ho, Simon C-C; Hashimoto, Tetsuya; Poliszczuk, Artem; Pollo, Agnieszka; Trippe, Sascha; Miyaji, Takamitsu; Toba, Yoshiki; Malkan, Matthew; Serjeant, Stephen; Pearson, Chris; Hwang, Ho Seong; Kim, Eunbin; Shim, Hyunjin; Lu, Ting Yi; Hsiao, Yu-Yang; Huang, Ting-Chi; Herrera-Endoqui, Martin; Bravo-Navarro, Blanca; Matsuhara, Hideo | Natl Tsing Hua Univ, Dept Phys, 101,Sect 2,Kuang Fu Rd, Hsinchu 30013, Taiwan; Natl Tsing Hua Univ, Inst Astron, 101,Sect 2,Kuang Fu Rd, Hsinchu 30013, Taiwan; Natl Tsing Hua Univ, Ctr Informat & Computat Astron CICA, 101,Sect 2,Kuang Fu Rd, Hsinchu 30013, Taiwan; Natl Ctr Nucl Res, Ul Pasteura 7, PL-02093 Warsaw, Poland; Jagiellonian Univ, Astron Observ, Ul Orla 171, PL-30244 Krakow, Poland; Seoul Natl Univ, Dept Phys & Astron, 1 Gwanak Rd, Seoul 08826, South Korea; Univ Nacinal Autonoma Mexico IA UNAM E, Inst Astrn Sede Ensenada, Km 107, Ensenada 22860, Baja California, Mexico; Leibnitz Inst Fiir Astrophys AIP, Sternwarte 16, D-14482 Potsdam, Germany; Kyoto Univ, Dept Astron, Sakyo Ku, Kitashirakawa Oiwake Cho, Kyoto 6068502, Japan; Acad Sinica, Inst Astron & Astrophys, 11 Astron Math Bldg,1,Sect 4,Roosevelt Rd, Taipei 10617, Taiwan; Ehime Univ, Res Ctr Space & Cosm Evolut, 2-5 Bunkyo Cho, Matsuyama, Ehime 7908577, Japan; UCLA, Dept Phys & Astron, 475 Portola Plaza, Los Angeles, CA 90095 USA; Open Univ, Dept Phys Sci, Milton Keynes MK7 6AA, Bucks, England; STEC Rutherford Appleton Lab, RAL Space, Didcot OX11 0QX, Oxon, England; Open Univ, Milton Keynes MK7 6AA, Bucks, England; Univ Oxford, Keble Rd, Oxford OX1 3RH, England; Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 34055, South Korea; Kyungpook Natl Univ, Dept Earth Sci Educ, 80 Daehak Ro, Daegu 41566, South Korea; Grad Univ Adv Studies, SOKENDA1, Dept Space & Astronaut Sci, Miura, Kanagawa 2400193, Japan; Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan; Univ Autonoma Baja California, Ingn Aerosp, Blvd Univ 1000 Valle Las Palmas, Tijuana 22260, BC, Mexico | ; Malkan, Matthew/IWM-5356-2023; Serjeant, Stephen/AAN-1908-2021; Shim, Hyunjin/LZI-7486-2025; Hashimoto, Tetsuya/ABG-3643-2021; HWANG, Ho/AAS-6010-2020 | 57221833663; 57151800100; 57070819300; 57211574957; 57218278835; 57216812477; 24518043000; 57192100278; 56234075800; 8559107900; 57203194972; 37068332400; 7006872661; 7003485288; 55531949600; 57207581761; 55202031200; 14061137700; 57207966444; 57221836434; 57203623570; 56045884200; 57221830943; 7003505733 | 369grant2@gmail.com; | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | MON NOT R ASTRON SOC | 0035-8711 | 1365-2966 | 501 | 3 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.235 | 23.9 | 0.84 | 2025-07-30 | 14 | 13 | methods: data analysis; infrared: galaxies; submillimetre: galaxies; ultraviolet: galaxies | POLE WIDE SURVEY; SOURCE CATALOG; X-RAY; AKARI; SELECTION; FIELD; CLASSIFICATION; STARS | infrared: Galaxies; methods: Data analysis; submillimetre: Galaxies; ultraviolet: Galaxies | Cosmology; Deep neural networks; Stars; Active galactic nuclei; Cosmics; Infrared galaxies; Methods. Data analysis; Model-based OPC; Recognition models; Star forming galaxy; Submillimeter: galaxies; Supermassive black holes; Ultraviolet:galaxies; Active Galactic Nuclei | English | 2021 | 2021-01-14 | 10.1093/mnras/staa3865 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |
| ○ | Article | Environmental effects on AGN activity via extinction-free mid-infrared census | How does the environment affect active galactic nucleus (AGN) activity? We investigated this question in an extinction-free way by selecting 1120 infrared (IR) galaxies in the AKARI North Ecliptic Pole Wide field at redshift z ≤ 1.2. A unique feature of the AKARI satellite is its continuous nine-band IR filter coverage, providing us with an unprecedentedly large sample of IR spectral energy distributions (SEDs) of galaxies. By taking advantage of this, for the first time, we explored the AGN activity derived from SED modelling as a function of redshift, luminosity, and environment. We quantified AGN activity in two ways: AGN contribution fraction (ratio of AGN luminosity to the total IR luminosity), and AGN number fraction (ratio of number of AGNs to the total galaxy sample). We found that galaxy environment (normalized local density) does not greatly affect either definitions of AGN activity of our IRG/LIRG samples (log LTIR ≤ 12). However, we found a different behaviour for ULIRGs (log LTIR > 12). At our highest redshift bin (0.7 ≤ z ≤ 1.2), AGN activity increases with denser environments, but at the intermediate redshift bin (0.3 ≤ z ≤ 0.7), the opposite is observed. These results may hint at a different physical mechanism for ULIRGs. The trends are not statistically significant (p ≥ 0.060 at the intermediate redshift bin, and p ≥ 0.139 at the highest redshift bin). Possible different behaviour of ULIRGs is a key direction to explore further with future space missions (e.g. JWST, Euclid, SPHEREx). © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. | Santos, Daryl Joe D; Goto, Tomotsugu; Kim, Seong Jin; Wang, Ting-Wen; Ho, Simon C-C; Hashimoto, Tetsuya; Huang, Ting-Chi; Lu, Ting-Yi; On, Alvina Y. L; Wong, Yi-Hang Valerie; Hsiao, Tiger Yu-Yang; Pollo, Agnieszka; Malkan, Matthew A; Miyaji, Takamitsu; Toba, Yoshiki; Kilerci-Eser, Ece; Małek, Katarzyna; Hwang, Ho Seong; Jeong, Woong-Seob; Shim, Hyunjin; Pearson, Chris; Poliszczuk, Artem; Chen, Bo Han | Institute of Astronomy, National Tsing Hua University, No. 101, Section 2, Kuang-Fu Road, Hsinchu City, 30013, Taiwan; Institute of Astronomy, National Tsing Hua University, No. 101, Section 2, Kuang-Fu Road, Hsinchu City, 30013, Taiwan; Institute of Astronomy, National Tsing Hua University, No. 101, Section 2, Kuang-Fu Road, Hsinchu City, 30013, Taiwan; Institute of Astronomy, National Tsing Hua University, No. 101, Section 2, Kuang-Fu Road, Hsinchu City, 30013, Taiwan; Institute of Astronomy, National Tsing Hua University, No. 101, Section 2, Kuang-Fu Road, Hsinchu City, 30013, Taiwan; Institute of Astronomy, National Tsing Hua University, No. 101, Section 2, Kuang-Fu Road, Hsinchu City, 30013, Taiwan, Centre for Informatics and Computation in Astronomy (CICA), National Tsing Hua University, 101, Section 2. Kuang-Fu Road, Hsinchu, 30013, Taiwan, Department of Physics, National Chung Hsing University, 145 Xingda Rd., South Dist., Taichung, 40227, Taiwan; Department of Space and Astronautical Science, Graduate University for Advanced Studies, Sokendai, Shonankokusaimura, Hayama, Miura District, Kanagawa, 240-0193, Japan, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa, 252-5210, Japan; Institute of Astronomy, National Tsing Hua University, No. 101, Section 2, Kuang-Fu Road, Hsinchu City, 30013, Taiwan; Institute of Astronomy, National Tsing Hua University, No. 101, Section 2, Kuang-Fu Road, Hsinchu City, 30013, Taiwan, Centre for Informatics and Computation in Astronomy (CICA), National Tsing Hua University, 101, Section 2. Kuang-Fu Road, Hsinchu, 30013, Taiwan, Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, United Kingdom; Institute of Astronomy, National Tsing Hua University, No. 101, Section 2, Kuang-Fu Road, Hsinchu City, 30013, Taiwan; Institute of Astronomy, National Tsing Hua University, No. 101, Section 2, Kuang-Fu Road, Hsinchu City, 30013, Taiwan; National Centre for Nuclear Research, ul. Pasteura 7, Warsaw, PL-02-093, Poland, Astronomical Observatory of the Jagiellonian University, ul. Orla 171, Cracow, PL-30-244, Poland; Department of Physics and Astronomy, Ucla, 475 Portola Plaza, Los Angeles, 90095, CA, United States; Instituto de Astronomía, Universidad Nacional Autónoma de México, AP 106, Ensenada, 22860, Mexico; Department of Astronomy, Kyoto University, Kitashirakawa-Oiwake-cho, Sakyo-ku, Kyoto, 606-8502, Japan, Academia Sinica Institute of Astronomy and Astrophysics, 11F of Astronomy-Mathematics Building, AS/NTU, No.1, Section 4, Roosevelt Road, Taipei, 10617, Taiwan, Research Center for Space and Cosmic Evolution, Ehime University, 2-5 Bunkyo-cho, Matsuyama, Ehime, 790-8577, Japan; Sabancl University, Faculty of Engineering and Natural Sciences, Istanbul, 34956, Turkey; National Centre for Nuclear Research, ul. Pasteura 7, Warsaw, PL-02-093, Poland, Aix Marseille Univ. Cnrs, Cnes, Marseille, LAM, France; Astronomy Program, Department of Physics and Astronomy, Seoul National University, 1 Gwanak-ro, Gwanak-gu, Seoul, 08826, South Korea, Snu Astronomy Research Center, Seoul National University, 1 Gwanak-ro, Gwanak-gu, Seoul, 08826, South Korea; Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu, Daejeon, 34055, South Korea, Korea University of Science and Technology, 217 Gajeong-ro, Yuseong-gu, Daejeon, 34113, South Korea; Department of Earth Science Education, Kyungpook National University, 80 Daehak-ro, Buk-gu, Daegu, 41566, South Korea; Ral Space, Stfc Rutherford Appleton Laboratory, Didcot, Oxon, OX11 0QX, United Kingdom, Open University, Milton Keynes, MK7 6AA, United Kingdom, University of Oxford, Keble Rd, Oxford, OX1 3RH, United Kingdom; National Centre for Nuclear Research, ul. Pasteura 7, Warsaw, PL-02-093, Poland; Department of Physics, National Tsing Hua University, No. 101, Section 2, Kuang-Fu Road, Hsinchu City, 30013, Taiwan | 57218278835; 57151800100; 57070819300; 57211574957; 57216812477; 24518043000; 57203623570; 57207966444; 57214263438; 57191345120; 57218282309; 56234075800; 7006872661; 57203194972; 37068332400; 55961627300; 56210521800; 15131707100; 7102145940; 14061137700; 55531949600; 57192100278; 57221833663 | daryl_santos@gapp.nthu.edu.tw; | Monthly Notices of the Royal Astronomical Society | MON NOT R ASTRON SOC | 0035-8711 | 1365-2966 | 507 | 2 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.235 | 23.9 | 0.49 | 2025-07-30 | 9 | galaxies: active; infrared: galaxies | English | Final | 2021 | 10.1093/mnras/stab2352 | 바로가기 | 바로가기 | 바로가기 | ||||||||
| ○ | ○ | Article | gzK-colour-selected star-forming galaxies in the AKARI NEP-Deep Field | We study the clustering property and physical parameters of gzK-colour-selected star-forming galaxies (sgzKs) based on the Canada-France-Hawaii Telescope surveys over 0.55 deg(2) in the AKARI North Ecliptic Pole-Deep Field. Two-point correlation functions for two magnitude-limited cases, K-s < 21.1 (N = 234) and K-s < 21.5 (N = 428), are estimated using a single powerlaw function with the fixed slope of 0.8. The bias factors of sgzKs with K-s < 21.1 and 21.5 are 5.79 +/- 1.07 and 4.00 +/- 0.67, respectively, representing that sgzKs with z similar to 1.7 reside in dark matter haloes more massive than 10(13) M-circle dot. We find that haloes hosting sgzKs with K-s < 21.5 evolve into haloes that host local massive galaxies with similar to 6 L*. This suggests that sgzKs with K-s < 21.5 are likely to be predecessors of local massive galaxies. The evolutionary track of bias factor for host haloes of the bright sgzKs is similar to that of the bright passive extremely red objects, implying a possible connection between the two populations of galaxies. From the spectral energy distribution fitting, we estimate physical parameters and active galactic nucleus (AGN) contribution for 75 mid-infrared (MIR)-detected sgzKs with K-s < 21.5. The median values of stellar mass and star formation rate are 9.5 x 10(10) M-circle dot and 162 M-circle dot yr(-1), respectively. MIR-detected sgzKs have a variety of AGN contributions ranging from 0 to 80 per cent. The number ratio of sgzKs with larger AGN contribution than 10 per cent is 30 per cent. | Seo, Hyunjong; Jeong, Woong-Seob; Shim, Hyunjin; Kim, Minjin; Ko, Jongwan; Pyo, Jeonghyun; Pearson, Chris; Oi, Nagisa; Goto, Tomotsugu; Miyaji, Takamitsu | Korea Astron & Space Sci Inst KASI, 776 Daedeok Daero, Daejeon 34055, South Korea; Korea Univ Sci & Technol, 217 Gajeong Ro, Daejeon 305350, South Korea; Kyungpook Natl Univ, Dept Earth Sci Educ, 80 Daehakro, Daegu 41566, South Korea; Kyungpook Natl Univ, Dept Astron & Atmospher Sci, Daegu 702701, South Korea; STFC Rutherford Appleton Lab, RAL Space, Didcot OX11 0QX, Oxon, England; Open Univ, Sch Phys Sci, Milton Keynes MK7 6AA, Bucks, England; Univ Oxford, Oxford Astrophys, Keble Rd, Oxford OX1 3RH, England; Tokyo Univ Sci, Shinjuku Ku, 1-3 Kagurazaka, Tokyo 1628601, Japan; Natl Tsing Hua Univ, Inst Astron, 101,Sect 2,Kuang Fu Rd, Hsinchu 30013, Taiwan; Univ Nacl Autonoma Mexico, Inst Astron, Km 107 Carret Tij Ens, Ensenada 22860, Baja California, Mexico; Leibniz Inst Astrophys Potsdam AIP, Stentwarte 16, D-14482 Potsdam, Germany; 45 Gungdong Ro, Daejeon 34137, South Korea | ; Shim, Hyunjin/LZI-7486-2025; Kim, Minjin/AAU-9910-2020 | 35278506600; 7102145940; 14061137700; 56898213300; 18434193800; 22036293900; 55531949600; 23968436800; 57151800100; 57203194972 | hyunjongseo11@gmail.com; | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | MON NOT R ASTRON SOC | 0035-8711 | 1365-2966 | 502 | 2 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.235 | 23.9 | 0 | 2025-07-30 | 0 | 0 | galaxies: evolution; galaxies: formation; galaxies: high-redshift | SUPERMASSIVE BLACK-HOLES; ACTIVE GALACTIC NUCLEI; DUST-OBSCURED GALAXIES; LUMINOSITY FUNCTION; SCALING RELATIONS; MASSIVE GALAXIES; HOST GALAXIES; STELLAR MASS; EVOLUTION; POPULATION | galaxies: evolution; galaxies: formation; galaxies: high-redshift | Active Galactic Nuclei; Cosmology; Red Shift; Active galactic nuclei; Bias factor; Clustering properties; Galaxies:high-redshift; Galaxy evolution; Galaxy formations; Midinfrared; Physical parameters; Star forming galaxy; Two-point correlation function; Stars | English | 2021 | 2021-04 | 10.1093/mnras/stab052 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |
| ○ | ○ | Article | Identification of AKARI infrared sources by the Deep HSC Optical Survey: construction of a new band-merged catalogue in the North Ecliptic Pole Wide field | The North Ecliptic Pole field is a natural deep-field location for many satellite observations. It has been targeted many times since it was surveyed by the AKARI space telescope with its unique wavelength coverage from the near- to mid-infrared (mid-IR). Many follow-up observations have been carried out, making this field one of the most frequently observed areas with a variety of facilities, accumulating abundant panchromatic data from the X-ray to the radio wavelength range. Recently, a deep optical survey with the Hyper Suprime-Cam (HSC) at the Subaru telescope covered the NEP-Wide (NEPW) field, which enabled us to identify faint sources in the near- and mid-IR bands, and to improve the photometric redshift (photo-z) estimation. In this work, we present newly identified AKARI sources by the HSC survey, along with multiband photometry for 91 861 AKARI sources observed over the NEPW field. We release a new band-merged catalogue combining various photometric data from the GALEX UV to submillimetre (sub-mm) bands (e.g. Herschel/SPIRE, JCMT/SCUBA-2). About similar to 20 000 AKARI sources are newly matched to the HSC data, most of which seem to be faint galaxies in the near- to mid-infrared AKARI bands. This catalogue is motivating a variety of current research, and will be increasingly useful as recently launched (eROSITA/ART-XC) and future space missions (such as JWST, Euclid, and SPHEREx) plan to take deep observations in the NEP field. | Kim, Seong Jin; Oi, Nagisa; Goto, Tomotsugu; Ikeda, Hiroyuki; Ho, Simon C-C; Shim, Hyunjin; Toba, Yoshiki; Hwang, Ho Seong; Hashimoto, Tetsuya; Barrufet, Laia; Malkan, Matthew; Kim, Helen K.; Huang, Ting-Chi; Matsuhara, Hideo; Miyaji, Takamitsu; Pearson, Chris; Serjeant, Stephen; Santos, Daryl Joe D.; Kim, Eunbin; Pollo, Agnieszka; Jeong, Woong-Seob; Wang, Ting-Wen; Momose, Rieko; Takagi, Toshinobu | Natl Tsing Hua Univ, Inst Astron, 101,Sect 2,Kuang Fu Rd, Hsinchu 30013, Taiwan; Tokyo Univ Sci, Fac Sci Div 2, Liberal Arts, Shinjuku Ku, 1-3 Kagurazaka, Tokyo 1628601, Japan; Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan; Wakayama Coll, Natl Inst Technol, 77 Noshima,Nada Cho, Wakayama 6440023, Japan; Kyungpook Natl Univ, Dept Earth Sci Educ, Daegu 41566, South Korea; Kyoto Univ, Dept Astron, Sakyo Ku, Kitashirakawa Oiwake Cho, Kyoto 6068502, Japan; Acad Sinica, Inst Astron & Astrophys, AS NTU, 11 Astron Math Bldg,1,Sect 4,Roosevelt Rd, Taipei 10617, Taiwan; Ehime Univ, Res Ctr Space & Cosm Evolut, 2-5 Bunkyo Cho, Matsuyama, Ehime 7908577, Japan; Korea Astron & Space Sci Inst KASI, 776 Daedeok Daero, Daejeon 34055, South Korea; Natl Tsing Hua Univ, Ctr Informat & Computat Astron CICA, 101,Sect 2,Kuang Fu Rd, Hsinchu 30013, Taiwan; European Space Astronoy Ctr, E-28691 Villanueva De La Canada, Spain; Rutherford Appleton Lab, RAL Space, Didcot OX11 0QX, Oxon, England; Univ Calif Los Angeles, Dept Phys & Astron, 475 Portola Plaza, Los Angeles, CA 90095 USA; Grad Univ Adv Studies, Dept Space & Astronaut Sci, SOKENDAI, Hayama, Kanagawa 2400193, Japan; Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2525210, Japan; Univ Nacl Autonoma Mexico, Inst Astron, Km 107,Carret Tij Ens, Ensenada 22860, Baja California, Mexico; Open Univ, Milton Keynes MK7 6AA, Bucks, England; Univ Oxford, OXford Astrophys, Keble Rd, Oxford OX1 3RH, England; Natl Ctr Nucl Res, Ul Pasteura 7, PL-02093 Warsaw, Poland; Jagiellonian Univ, Astron Observ, Ul Orla 171, PL-30244 Krakow, Poland; Univ Tokyo, Sch Sci, Dept Astron, Bunkyo Ky, 7-3-1 Hongo, Tokyo 1130033, Japan; Japan Space Forum, Chiyoda Ku, 3-2-1 Kandasurugadai, Tokyo 1010062, Japan; Leibniz Inst Astrophys Potsdam ATP, D-14482 Potsdam, Germany | ; Hashimoto, Tetsuya/ABG-3643-2021; Serjeant, Stephen/AAN-1908-2021; HWANG, Ho/AAS-6010-2020; Shim, Hyunjin/LZI-7486-2025; Malkan, Matthew/IWM-5356-2023 | 57070819300; 23968436800; 57151800100; 44561165200; 57216812477; 14061137700; 37068332400; 15131707100; 24518043000; 57201651740; 7006872661; 57203269860; 57203623570; 7003505733; 57203194972; 55531949600; 7003485288; 57218278835; 55202031200; 56234075800; 7102145940; 57211574957; 36615692700; 35405904800 | seongini@gmail.com; | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | MON NOT R ASTRON SOC | 0035-8711 | 1365-2966 | 500 | 3 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.235 | 23.9 | 1.12 | 2025-07-30 | 12 | 17 | catalogues; galaxies: evolution; cosmology: observations; infrared: galaxies | ACTIVE GALACTIC NUCLEI; GALAXIES; EMISSION | Catalogues; Cosmology: Observations; Galaxies: Evolution; Infrared: Galaxies | Galaxies; Image enhancement; Infrared devices; Light sources; Photometry; Poles; Space telescopes; Catalog; Cosmology observations; Galaxy evolution; Infrared galaxies; Infrared source; Midinfrared; Optical-; Satellite observations; Wavelength coverage; Wide-field; Surveys | English | 2021 | 2021-01 | 10.1093/mnras/staa3359 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |
| ○ | ○ | Article | Optically detected galaxy cluster candidates in the AKARI North Ecliptic Pole field based on photometric redshift from the Subaru Hyper Suprime-Cam | 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 cluster candidates in the AKARI NEP field with the minimum requisites based only on the coordinates and photometric redshift (photo-z) of galaxies. We used galaxies detected in five optical bands (g, r, i, z, and Y) by the Subaru Hyper Suprime-Cam (HSC), with additional data from the u band obtained from the Canada-France-Hawaii Telescope (CFHT) MegaPrime/MegaCam, and from the IRAC1 and IRAC2 bands from the Spitzer space telescope for photo-z estimation. We calculated the local density around every galaxy using the 10th-nearest neighbourhood. Cluster candidates were determined by applying the friends-of-friends algorithm to over-densities. A total of 88 cluster candidates containing 4390 member galaxies below redshift 1.1 in 5.4 deg(2) were identified. The reliability of our method was examined through false-detection tests, redshift-uncertainty tests, and applications on the Cosmic Evolution Survey (COSMOS) data, giving false-detection rates of 0.01 to 0.05 and a recovery rate of 0.9 at high richness. Three X-ray clusters previously observed by ROSAT and Chandra were recovered. The cluster galaxies show a higher stellar mass and lower star formation rate compared with the field galaxies in two-sample Z-tests. These cluster candidates are useful for environmental studies of galaxy evolution and future astronomical surveys in the NEP, where AKARI has performed unique nine-band mid-infrared photometry for tens of thousands of galaxies. | Huang, Ting-Chi; Matsuhara, Hideo; Goto, Tomotsugu; Santos, Daryl Joe D.; Ho, Simon C-C; Kim, Seong Jin; Hashimoto, Tetsuya; Ikeda, Hiroyuki; Oi, Nagisa; Malkan, Matthew A.; Pearson, William J.; Pollo, Agnieszka; Serjeant, Stephen; Shim, Hyunjin; Miyaji, Takamitsu; Hwang, Ho Seong; Durkalec, Anna; Poliszczuk, Artem; Greve, Thomas R.; Pearson, Chris; Toba, Yoshiki; Lee, Dongseob; Kim, Helen K.; Toft, Sune; Jeong, Woong-Seob; Enokidani, Umi | Grad Univ Adv Studies, Dept Space & Astronaut Sci, SOKENDAI, Hayama, Kanagawa 2400193, Japan; Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan; Natl Tsing Hua Univ, Inst Astron, 101,Sect 2,Kuang Fu Rd, Hsinchu 30013, Taiwan; Natl Tsing Hua Univ, Ctr Informat & Computat Astron CICA, 101,Sect 2,Kuang Fu Rd, Hsinchu 30013, Taiwan; Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan; Wakayama Coll, Natl Inst Technol, 77 Noshima,Nada Cho, Wakayama 6440023, Japan; Tokyo Univ Sci, Shinjuku Ku, 1-3 Kagurazaka, Tokyo 1628601, Japan; UCLA, Dept Phys & Astron, 475 Portola Plaza, Los Angeles, CA 90095 USA; Natl Ctr Nucl Res, Ul Pasteura 7, PL-02093 Warsaw, Poland; Jagiellonian Univ, Astron Observ, Ul Orla 171, PL-30244 Krakow, Poland; Open Univ, Sch Phys Sci, Milton Keynes MK7 6AA, Bucks, England; Kyungpook Natl Univ, Dept Earth Sci Educ, 80 Daehak Ro, Daegu 41566, South Korea; Univ Nacl Autonoma Mexico, Inst Astron, AP 106, Ensenada 22860, Baja California, Mexico; Leibniz Inst Astrophys Potsdam AIP, D-14482 Potsdam, Germany; Seoul Natl Univ, Dept Phys & Astron, Astron Program, 1 Gwanak Ro, Seoul 08826, South Korea; UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England; DTU Space, Cosm Dawn Ctr Dawn, Elektrovej 327, DK-2800 Copenhagen, Denmark; Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark; RAL Space, Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England; Univ Oxford, Oxford Astrophys, Keble Rd, Oxford OX1 3RH, England; Kyoto Univ, Dept Astron, Sakyo Ku, Kitashirakawa Oiwake Cho, Kyoto 6068502, Japan; Acad Sinica Inst Astron & Astrophys, 11F Astron Math Bldg,AS-NTU 1,Sect 4,Roosevelt Rd, Taipei 10617, Taiwan; Ehime Univ, Res Ctr Space & Cosm Evolut, 2-5 Bunkyo Cho, Matsuyama, Ehime 7908577, Japan; Univ Copenhagen, Niels Bohr Inst, Lyngbyvej 2, DK-2100 Copenhagen, Denmark; Korea Astron & Space Sci Inst KASI, 776 Daedeok Daero, Daejeon 34055, South Korea; Natl Chung Hsing Univ, Dept Phys, 145 Xingda Rd, Taichung 40227, Taiwan; Seoul Natl Univ, SNU Astron Res Ctr, 1 Gwanak Ro, Seoul 08826, South Korea | ; Huang, Teddy/ABB-7532-2020; Durkalec, Anna/G-3022-2015; HWANG, Ho/AAS-6010-2020; Shim, Hyunjin/LZI-7486-2025; Hashimoto, Tetsuya/ABG-3643-2021; Serjeant, Stephen/AAN-1908-2021; Malkan, Matthew/IWM-5356-2023; Toft, Sune/JEZ-2766-2023 | 57203623570; 7003505733; 57151800100; 57218278835; 57216812477; 57070819300; 24518043000; 44561165200; 23968436800; 7006872661; 57195032075; 56234075800; 7003485288; 14061137700; 57203194972; 15131707100; 56331194100; 57192100278; 10339159000; 55531949600; 37068332400; 57218674853; 57203269860; 7004109829; 7102145940; 57226334267 | s104022505@m104.nthu.edu.tw; | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | MON NOT R ASTRON SOC | 0035-8711 | 1365-2966 | 506 | 4 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.235 | 23.9 | 0.42 | 2025-07-30 | 6 | 7 | methods: data analysis; galaxies: clusters: general; galaxies: distance and redshifts; galaxies: evolution; galaxies: groups: general | GALACTIC NUCLEI; WIDE SURVEY; DEEP; CATALOG; MASS; MORPHOLOGY; EVOLUTION; STARS; PROBE | Galaxies: Clusters: General; Galaxies: Distance and redshifts; Galaxies: Evolution; Galaxies: Groups: General; Methods: Data analysis | English | 2021 | 2021-10 | 10.1093/mnras/stab2128 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | ||
| ○ | Article | Parenting - It's a life: Where and how youth learn about establishing paternity, child support, and co-parenting | Theory and research suggest the importance of establishing paternity, co-parenting, and child support for positive child and youth development. However, youth's relative knowledge of these topics is not well understood. Thus we examine these in the context of other parenting issues and how this information varied by parents, school/teachers, friends, and social media. We also sought to provide preliminary data on parenting programming to determine if the programming was associated with perceived increases in knowledge about these and other parenting topics. Data from 1713 students in middle and high schools who attended one or more Parenting: It's a Life modules in their school were available for analysis. Youth reported existing knowledge on establishing paternity, co-parenting, and child support relatively low compared to other topics such as peer pressure and healthy relationships. Among the four sources of information surveyed, youth received the most information from parents and caregivers and the least amount of information from social media. Youth reported significant increases in knowledge regarding parenting topics following exposure to Parenting: It's a Life curriculum. The information youth receive on content such as establishing paternity, co-parenting, and child support is relatively low. School-based parenting programs focused on these topics may help educate youth about these important parenting topics before parenthood. | McCurdy, Bethany H.; Weems, Carl F.; Rouse, Heather L.; Jeon, Sesong; Bartel, Maya; Melby, Janet N.; Goudy, Kate; Lee, Jo Ann | Iowa State Univ, Human Dev & Family Studies, Ames, IA 50011 USA; Kyungpook Natl Univ, Coll Human Ecol, Dept Child Dev & Family Studies, Daegu, South Korea | McCurdy, Bethany/JJC-2249-2023; rouse, heather/NFS-7444-2025 | cweems@iastate.edu; | CHILDREN AND YOUTH SERVICES REVIEW | CHILD YOUTH SERV REV | 0190-7409 | 1873-7765 | 126 | SSCI | FAMILY STUDIES;SOCIAL WORK | 2021 | 2.519 | 23.9 | 4 | Establishing paternity; Co-parenting; Child support | TEEN PREGNANCY; FATHER INVOLVEMENT; RESIDENT FATHERS; RISK BEHAVIORS; HEALTH; IMPLEMENTATION; COMMUNICATION; DETERMINANTS; INFORMATION; ACHIEVEMENT | English | 2021 | 2021-07 | 10.1016/j.childyouth.2021.106023 | 바로가기 | 바로가기 | 바로가기 | ||||||||||
| ○ | ○ | Article | Photometric redshifts in the North Ecliptic Pole Wide field based on a deep optical survey with Hyper Suprime-Cam | The AKARI space infrared telescope has performed near-infrared to mid-infrared (MIR) observations on the North Ecliptic Pole Wide (NEPW) field (5.4 deg(2)) for about 1 yr. AKARI took advantage of its continuous nine photometric bands, compared with NASA's Spitzer and Wide-field Infrared Survey Explorer(WISE) space telescopes, which had only four filters with a wide gap in the MIR. The AKARI NEPW field lacked deep and homogeneous optical data, limiting the use of nearly half of the IR sources for extragalactic studies, because of the absence of photometric redshift (photo-z). To remedy this, we have recently obtained deep optical imaging over the NEPW field with five bands (g, r, i, z and Y) of the Hyper Suprime-Camera (HSC) on the Subaru 8-m telescope. We optically identify AKARI-IR sources along with supplementary Spitzer and WISE data as well as pre-existing optical data. In this work, we derive new photo-z using a chi(2) template-fitting method code, PHotometric Analysis for Redshift Estimate (Le Phare) and reliable photometry from 26 selected filters including HSC, AKARI, Canada-France-Hawaii Telescope, Maidanak, Kitt Peak National Observatory, Spitzer and WISE data. We take 2026 spectroscopic redshifts (spec-z) from all available spectroscopic surveys over the NEPW field to calibrate and assess the accuracy of the photo-z. At z < 1.5, we achieve a weighted photo-z dispersion of sigma(Delta z/(1+z)) = 0.053 with eta = 11.3 per cent catastrophic errors. | Ho, Simon C-C; Goto, Tomotsugu; Oi, Nagisa; Kim, Seong Jin; Malkan, Matthew A.; Pollo, Agnieszka; Hashimoto, Tetsuya; Toba, Yoshiki; Kim, Helen K.; Hwang, Ho Seong; Shim, Hyunjin; Huang, Ting-Chi; Kim, Eunbin; Wang, Ting-Wen; Santos, Daryl Joe D.; Matsuhara, Hideo | Natl Tsing Hua Univ, Inst Astron, Hsinchu, Taiwan; Tokyo Univ Sci, Fac Sci Div 2, Liberal Arts, Shinjuku Ku, 1-3 Kagurazaka, Tokyo 1628601, Japan; UCLA, Dept Phys & Astron, 475 Portola Plaza, Los Angeles, CA 90095 USA; Natl Ctr Nucl Res, Ul Pasteura 7, PL-02093 Warsaw, Poland; Jagiellonian Univ, Astron Observ, Ul Orla 171, PL-30244 Krakow, Poland; Natl Tsing Hua Univ, Ctr Informat & Computat Astron CICA, 101,Sect 2 Kuang Fu Rd, Hsinchu 30013, Taiwan; Kyoto Univ, Dept Astron, Sakyo Ku, Kitashirakawa Oiwake Cho, Kyoto 6068502, Japan; Acad Sinica, Inst Astron & Astrophys, 1F Astron Math Bldg,AS-NTU,1,Sect 4,Roosevelt Rd, Taipei 10617, Taiwan; Ehime Univ, Res Ctr Space & Cosm Evolut, 2-5 Bunkyo Cho, Matsuyama, Ehime 7908577, Japan; Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 34055, South Korea; Kyungpook Natl Univ, Dept Earth Sci Educ, 80 Daehak Ro, Daegu 41566, South Korea; Grad Univ Adv Studies SOKENDAI, Dept Space & Astronaut Sci, Miura, Kanagawa 2400193, Japan; Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan | Shim, Hyunjin/LZI-7486-2025; HWANG, Ho/AAS-6010-2020; Hashimoto, Tetsuya/ABG-3643-2021; Malkan, Matthew/IWM-5356-2023 | 57216812477; 57151800100; 23968436800; 57070819300; 7006872661; 56234075800; 24518043000; 37068332400; 57203269860; 15131707100; 14061137700; 57203623570; 55202031200; 57211574957; 57218278835; 7003505733 | simonsimon259@gapp.nthu.edu.tw;tomo@gapp.nthu.edu.tw; | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | MON NOT R ASTRON SOC | 0035-8711 | 1365-2966 | 502 | 1 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.235 | 23.9 | 0.63 | 2025-07-30 | 9 | 10 | catalogues; galaxies: distances and redshifts; infrared: galaxies | GALAXIES; CATALOG; SUBARU; WISE; ULTRAVIOLET; SPECTRA; SEARCH | catalogues; galaxies: distances and redshifts; infrared: galaxies | Galaxies; Infrared devices; NASA; Photometry; Red Shift; Space telescopes; Surveys; Catalog; Galaxies distances and redshifts; Infrared galaxies; IR source; Midinfrared; Optical data; Photometrics; Red shift; Spitzer; Wide-field; Poles | English | 2021 | 2021-03 | 10.1093/mnras/staa3549 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |
| ○ | ○ | Article | The black hole masses of extremely luminous radio-WISE selected galaxies | We present near-IR photometry and spectroscopy of 30 extremely luminous radio and mid-IR-selected galaxies. With bolometric luminosities exceeding similar to 10(13) and redshifts ranging from z = 0.880 to 2.853, we use Very Large Telescope instruments X-shooter and Infrared Spectrometer and Array Camera to investigate this unique population of galaxies. Broad multicomponent emission lines are detected in 18 galaxies and we measure the near-IR lines H beta,[O III] lambda lambda 4959, 5007 and in 6, 15, and 13 galaxies, respectively, with 10 Ly alpha and 5 CIV lines additionally detected in the UVB arm. We use the broad [O III] lambda 5007 emission lines as a proxy for the bolometric active galactic nucleus luminosity, and derive lower limits to supermassive black hole masses of 10(7.9)-10(9.4)M(circle dot) with expectations of corresponding host masses of 10(10.4)-10(12.0)M(circle dot). We measure lambda(Edd) > 1 for eight of these sources at a 2 sigma significance. Near-IR photometry and SED fitting are used to compare stellar masses directly. We detect both Balmer lines in five galaxies and use these to infer a mean visual extinction of A(V) = 2.68 mag. Due to non-detections and uncertainties in our H beta emission line measurements, we simulate a broad H beta line of FWHM = 1480 kms(-1) to estimate extinction for all sources with measured H alpha emission. We then use this to infer a mean A(V) = 3.62 mag, demonstrating the highly obscured nature of these galaxies, with the consequence of increasing our estimates of black hole masses by a 0.5 orders of magnitude in the most extreme and obscured cases. | Ferris, E. R.; Blain, A. W.; Assef, R. J.; Hatch, N. A.; Kimball, A.; Kim, M.; Sajina, A.; Silva, A.; Stern, D.; Diaz-Santos, T.; Tsai, C-W; Wylezalek, D. | Univ Leicester, Sch Phys & Astron, Univ Rd, Leicester LE1 7RH, Leics, England; Univ Diego Portales, Nucleo Astron Fac Ingn & Ciencias, Av Ejercito Libertador 441, Santiago 8370109, Chile; Univ Nottingham, Sch Phys & Astron, Univ Pk, Nottingham NG7 2RD, England; Natl Radio Astron Observ, 1003 Lopezville Rd, Socorro, NM 87801 USA; Kyungpook Natl Univ, Dept Astron & Atmospher Sci, Daegu 702701, South Korea; Tufts Univ, Dept Phys & Astron, 574 Boston Ave, Medford, MA 02155 USA; Natl Inst Nat Sci, Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan; CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA; Chinese Acad Sci, Natl Astron Observ, Chinese Acad Sci South Amer Ctr Astron CASSACA, Beijing 100101, Peoples R China; Fdn Res & Technol Hellas FORTH, Inst Astrophys, GR-70013 Iraklion, Greece; Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China; Heidelberg Univ, Astron Rech Inst, Zentrum Astron, Monchhofstr 12-14, D-69120 Heidelberg, Germany | ; Assef, Roberto/S-7842-2019; Kim, Minjin/AAU-9910-2020; Diaz-Santos, Tanio/V-1969-2018; Diaz Santos, Tanio/V-1969-2018; Xiao, Ting/HHC-4498-2022; Blain, Andrew/HTN-5718-2023 | 57222073925; 7006989462; 15078033000; 8970939400; 35417434300; 56898213300; 12796129500; 57207299188; 7202386545; 55910071800; 36663120700; 44561692900 | erf5@le.ac.uk; | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | MON NOT R ASTRON SOC | 0035-8711 | 1365-2966 | 502 | 1 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.235 | 23.9 | 0.14 | 2025-07-30 | 3 | 2 | galaxies: active; galaxies: evolution; infrared: galaxies | ACTIVE GALACTIC NUCLEI; STAR-FORMING GALAXIES; FOLLOW-UP; QUASARS; HOT; ACCRETION; OUTFLOWS; II.; AGN; SKY | galaxies: active; galaxies: evolution; infrared: galaxies | English | 2021 | 2021-03 | 10.1093/mnras/stab048 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | ||
| ○ | ○ | Article | The evolution of merger fraction of galaxies at z < 0.6 depending on the star formation mode in the AKARI NEP-Wide Field | We study the galaxy merger fraction and its dependence on star formation mode in the 5.4 deg(2) of the North Ecliptic Pole-Wide Field. We select 6352 galaxies with AKARI 9 m detections, and identify mergers among them using the Gini coefficient and M-20 derived from the Subaru/Hyper Suprime-Cam (HSC) optical images. We obtain the total infrared luminosity and star formation rate of galaxies using the spectral energy distribution templates based on one band, AKARIm. We classify galaxies into three different star formation modes (i.e. starbursts, main-sequence, and quiescent galaxies) and calculate the merger fractions for each. We find that the merger fractions of galaxies increase with redshift at z < 0.6. The merger fractions of starbursts are higher than those of main-sequence and quiescent galaxies in all redshift bins. We also examine the merger fractions of far-infrared-detected galaxies that have at least one detection from Herschel/Spectral and Photometric Imaging Receiver (SPIRE). We find that Herschel-detected galaxies have higher merger fraction compared to non-Herschel-detected galaxies, and both Herschel-detected and non-Herschel-detected galaxies show clearly different merger fractions depending on the star formation modes. | Kim, Eunbin; Hwang, Ho Seong; Jeong, Woong-Seob; Kim, Seong Jin; Burgarella, Denis; Goto, Tomotsugu; Hashimoto, Tetsuya; Jo, Young-Soo; Lee, Jong Chul; Malkan, Matthew; Pearson, Chris; Shim, Hyunjin; Toba, Yoshiki; Ho, Simon C-C; Santos, Daryl Joe; Ikeda, Hiroyuki; Kim, Helen K.; Miyaji, Takamitsu; Matsuhara, Hideo; Oi, Nagisa; Takagi, Toshinobu; Wang, Ting-Wen | Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 34055, South Korea; Seoul Natl Univ, Dept Phys & Astron, Astron Program, 1 Gwanak Ro, Seoul 08826, South Korea; Seoul Natl Univ, SNU Astron Res Ctr, 1 Gwanak Ro, Seoul 08826, South Korea; Natl Tsing Hua Univ, Inst Astron, 101,Sect 2,Kuang Fu Rd, Hsinchu 30013, Taiwan; Aix Marseille Univ, CNRS, Lab Astrophys Marseille UMR 7326, F-13388 Marseille, France; Natl Tsing Hua Univ, Ctr Informat & Computat Astron CICA, 101,Sect 2,Kuang Fu Rd, Hsinchu 30013, Taiwan; Univ Calif Los Angeles, Dept Phys & Astron, 475 Portola Plaza, Los Angeles, CA 90095 USA; STFC Rutherford Appleton Lab, RAL Space, Didcot OX11 0QX, Oxon, England; Univ Oxford, Oxford Astrophys, Keble Rd, Oxford OX1 3RH, England; Open Univ, Milton Keynes MK7 6AA, Bucks, England; Kyungpook Natl Univ, Dept Earth Sci Educ, 80 Daehakro, Daegu 41566, South Korea; Kyoto Univ, Dept Astron, Sakyo Ku, Kitashirakawa Oiwake Cho, Kyoto 6068502, Japan; Acad Sinica, Inst Astron & Astrophys, 11F Astron Math Bldg,AS NTU 1,Sect 4,Roosevelt Rd, Taipei 10617, Taiwan; Ehime Univ, Res Ctr Space & Cosm Evolut, 2-5 Bunkyo Cho, Matsuyama, Ehime 7908577, Japan; Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan; Wakayama Coll, Natl Inst Technol, Wakayama 6440023, Japan; Univ Nacl Autonoma Mexico, Inst Astron Sede Ensenada, Km 107,Carrel Tij Ens, Ensenada 22060, Baja California, Mexico; Leibniz Inst Astrophys Potsdam, Sternwarte 16, D-14482 Potsdam, Germany; Grad Univ Adv Studies, SOKENDAI, Dept Space & Astronaut Sci, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan; Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan; Tokyo Univ Sci, Shinjuku Ku, 1-3 Kagurazaka, Tokyo 1628601, Japan; Japan Space Forum, Chiyoda Ku, 3-2-1 Kandasurugadai, Tokyo 1010062, Japan | Shim, Hyunjin/LZI-7486-2025; HWANG, Ho/AAS-6010-2020; Hashimoto, Tetsuya/ABG-3643-2021; Malkan, Matthew/IWM-5356-2023 | 55202031200; 15131707100; 7102145940; 57070819300; 8852232400; 57151800100; 24518043000; 35892221800; 57196138051; 7006872661; 55531949600; 14061137700; 37068332400; 57216812477; 57218278835; 44561165200; 57203269860; 57203194972; 7003505733; 23968436800; 35405904800; 57211574957 | ebkim0925@gmail.com; | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | MON NOT R ASTRON SOC | 0035-8711 | 1365-2966 | 507 | 3 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.235 | 23.9 | 0.49 | 2025-07-30 | 12 | 12 | galaxies: evolution; galaxies: formation; galaxies: spiral; galaxies: starburst; galaxies: star formation; infrared: galaxies | DIGITAL SKY SURVEY; FORMING GALAXIES; MASSIVE GALAXIES; SOURCE CATALOG; PHOTOMETRIC REDSHIFTS; INFRARED GALAXIES; FORMATION HISTORY; DISTANT GALAXIES; MERGING GALAXIES; OPTICAL-IMAGES | galaxies: evolution; galaxies: formation; galaxies: spiral; galaxies: star formation; galaxies: starburst; infrared: galaxies | English | 2021 | 2021-11 | 10.1093/mnras/stab2090 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | ||
| ○ | ○ | Article | Tracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS | We analyse the physical properties of 121 SNR >= 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 850 mu m-selected SMG sample from AS2UDS, to understand the fundamental physical differences between the two populations at the observed depths. The redshift distribution of the 450-mu m sample has a median of z = 1.85 +/- 0.12 and can be described by strong evolution of the far-infrared luminosity function. The fainter 450-mu m sample has similar to 14 times higher space density than the brighter 850-mu m sample at z less than or similar to 2, and a comparable space density at z = 2-3, before rapidly declining, suggesting LIRGs are the main obscured population at z similar to 1-2, while ULIRGs dominate at higher redshifts. We construct rest-frame similar to 180-mu m-selected and dust-mass-matched samples at z = 1-2 and z = 3-4 from the 450 and 850-mu m samples, respectively, to probe the evolution of a uniform sample of galaxies spanning the cosmic noon era. Using far-infrared luminosity, dust masses, and an optically thick dust model, we suggest that higher redshift sources have higher dust densities due to inferred dust continuum sizes which are roughly half of those for the lower redshift population at a given dust mass, leading to higher dust attenuation. We track the evolution in the cosmic dust mass density and suggest that the dust content of galaxies is governed by a combination of both the variation of gas content and dust destruction time-scale. | Dudzeviciute, U.; Smail, Ian; 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. | Univ Durham, Ctr Extragalact Astron, Dept Phys, South Rd, Durham DH1 3LE, England; Natl Taiwan Univ, Grad Inst Astrophys, Taipei 10617, Taiwan; Acad Sinica Inst Astron & Astrophys ASIAA, 1,Sect 4,Roosevelt Rd, Taipei 10617, Taiwan; Chinese Acad Sci, Purple Mt Observ, Nanjing 210033, Peoples R China; Univ British Columbia, Dept Phys & Astron, 6225 Agr Rd, Vancouver, BC V6T 1Z1, Canada; Herzberg Astron & Astrophys, Natl Res Council, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada; Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS B3H 4R2, Canada; European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany; Imperial Coll, Blackett Lab, Prince Consort Rd, London SW7 2AZ, England; Inst Astrofis Canarias, E-38205 Tenerife, Spain; Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain; Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China; Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China; Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 34055, South Korea; Nicolaus Copernicus Univ, Fac Phys Astron & Informat, Inst Astron, Grudziadzka 5, PL-87100 Torun, Poland; NSFs Natl Opt Infrared Astron Res Lab, 950 North Cherry Ave, Tucson, AZ 85719 USA; Kyungpook Natl Univ, Dept Earth Sci Educ, Daegu 41566, South Korea; Kyoto Univ, Dept Astron, Sakyo Ku, Kitashirakawa Oiwake Cho, Kyoto 6068502, Japan; Ehime Univ, Res Ctr Space & Cosm Evolut, 2-5 Bunkyo Cho, Matsuyama, Ehime 7908577, Japan | ; Shirley, Raphael/AAE-2964-2019; Smail, Ian/AAL-9018-2020; Smail, Ian/M-5161-2013; Shim, Hyunjin/LZI-7486-2025; Dannerbauer, Helmut/F-9382-2019; HWANG, Ho/AAS-6010-2020; Koprowski, Maciej/M-7525-2019; CHEN, Chian-Chou (TC)/ABB-2819-2020; Bongiovanni, Angel/J-6176-2012 | 57210119070; 7005932657; 55917471900; 57195235890; 8294170500; 55430490600; 7003967931; 24447889300; 44561018400; 25924805300; 8680454200; 35229428100; 15131707100; 56038935500; 35196197200; 7404952697; 14061137700; 57204707479; 37068332400 | ugne.dudzeviciute2@durham.ac.uk; | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | MON NOT R ASTRON SOC | 0035-8711 | 1365-2966 | 500 | 1 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.235 | 23.9 | 1.68 | 2025-07-30 | 28 | 29 | galaxies: evolution; galaxies: starburst; infrared: galaxies | COSMOLOGY LEGACY SURVEY; DEGREE EXTRAGALACTIC SURVEY; AZTEC/ASTE 1.1-MM SURVEY; STAR-FORMING GALAXIES; DEEP FIELD SOUTH; SOURCE CATALOG; ALMA SURVEY; MU-M; REDSHIFT DISTRIBUTION; LUMINOSITY FUNCTION | galaxies: evolution; galaxies: starburst; infrared: galaxies | Cosmology; Galaxies; Luminance; Far infrared; Galaxies: starbursts; Galaxy evolution; High-redshift; Infrared galaxies; Infrared luminosity; Similar models; Space densities; Spectral energy distribution; Submillimetre; Dust | English | 2021 | 2021-01 | 10.1093/mnras/staa3285 | 바로가기 | 바로가기 | 바로가기 | 바로가기 |
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