المؤلفون: Qin, Sheng-Li, Liu, Tie, Liu, Xunchuan, Goldsmith, Paul F., Li, Di, Zhang, Qizhou, Liu, Hong-Li, Wu, Yuefang, Bronfman, Leonardo, Juvela, Mika, Lee, Chang Won, Garay, Guido, Zhang, Yong, He, Jinhua, Hsu, Shih-Ying, Shen, Zhi-Qiang, Lee, Jeong-Eun, Wang, Ke, Tang, Ningyu, Tang, Mengyao, Zhang, Chao, Yue, Yinghua, Xue, Qiaowei, Li, Shang-Huo, Peng, Yaping, Dutta, Somnath, Jixing, Ge, Xu, Fengwei, Chen, Longfei, Baug, Tapas, dewanggan, Lokesh, Tej, Anandmayee

مصطلحات موضوعية: Astrophysics - Astrophysics of Galaxies

URL الوصول: http://arxiv.org/abs/2201.10044

المؤلفون: Liu, Hong-Li, Liu, Tie, Evans, Neal J., Wang, Ke, Garay, Guido, Qin, Sheng-Li, Li, Shanghuo, Stutz, Amelia, Goldsmith, Paul F., Liu, Sheng-Yuan, Tej, Anandmayee, Zhang, Qizhou, Juvela, Mika, Li, Di, Wang, Jun-Zhi, Bronfman, Leonardo, Ren, Zhiyuan, Wu, Yue-Fang, Kim, Kee-Tae, Lee, Chang-Won, Tatematsu, Kenichi, Cunningham, Maria. R., Liu, Xun-Chuan, Wu, Jing-Wen, Hirota, Tomoya, Lee, Jeong-Eun, Li, Pak-Shing, Kang, Sung-Ju, Mardones, Diego, Ristorcelli, Isabelle, Zhang, Yong, Luo, Qiu-Yi, Toth, L. Viktor, Yi, Hee-weon, Yun, Hyeong-Sik, Peng, Ya-Ping, Li, Juan, Zhu, Feng-Yao, Shen, Zhi-Qiang, Baug, Tapas, Dewangan, Lokesh, Chakali, Eswaraiah, Liu, Rong, Xu, Feng-Wei, Wang, Yu, Zhang, Chao, Li, Jinzeng, Zhou, Jianwen, Tang, Mengyao, Xue, Qiaowei, Issac, Namitha, Soam, Archana, Alvarez-Gutierrez, Rodrigo H.

مصطلحات موضوعية: Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics

URL الوصول: http://arxiv.org/abs/2105.03554

المؤلفون: Qin, Sheng-Li, Liu, Tie, Liu, Xunchuan, Goldsmith, Paul F., Li, Di, Zhang, Qizhou, Liu, Hong-Li, Wu, Yuefang, Bronfman, Leonardo, Juvela, Mika, Lee, Chang Won, Garay, Guido, Zhang, Yong, He, Jinhua, Hsu, Shih-Ying, Shen, Zhi-Qiang, Lee, Jeong-Eun, Wang, Ke, Tang, Ningyu, Tang, Mengyao, Zhang, Chao, Yue, Yinghua, Xue, Qiaowei, Li, Shanghuo, Peng, Yaping, Dutta, Somnath, Ge, Jixing, Xu, Fengwei, Chen, Long-Fei, Baug, Tapas, Dewangan, Lokesh, Tej, Anandmayee

المساهمون: Department of Physics

مصطلحات موضوعية: astrochemistry, stars: formation, ISM: molecules, COMPLEX ORGANIC-MOLECULES, EXTRAORDINARY SOURCES ANALYSIS, HERSCHEL OBSERVATIONS, HIGH-RESOLUTION, ORION-KL, CHEMICAL DIFFERENTIATION, MILLIMETER OBSERVATIONS, MULTILINE OBSERVATIONS, COLOGNE DATABASE, SPECTRAL SURVEY, Physical sciences

وصف الملف: application/pdf

Relation: This work has been supported by the National Key R&D Program of China (No. 2017YFA0402701), by the National Natural Science Foundation of China (grant nos 12033005, 12073061, 12122307, 12103045, 11973013, 11973099, and 11873086), and by the international partnership programme of Chinese Academy of Sciences through grant no. 114231KYSB20200009, Shanghai Pujiang Program 20PJ1415500, and the science research grants from the China Manned Space Project with no. CMS-CSST-2021-B06. This research was carried out in part at the Jet Propulsion Laboratory, which is operated by the California Institute of Technology under contract with NASA. J-EL was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT; grant no. 2021R1A2C1011718). CWL is supported by the Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education, Science and Technology (NRF-2019R1A2C1010851). This work is sponsored in part by the Chinese Academy of Sciences (CAS), through a grant to the CAS South America Center for Astronomy (CASSACA) in Santiago, Chile. Chile. G.G. and L.B. acknowledge support by the ANID BASAL project FB210003. SYH acknowledges support from the Ministry of Science and Technology (MoST) with grants 110-2112-M-001-056-. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2019.1.00685.S. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ.; Qin , S-L , Liu , T , Liu , X , Goldsmith , P F , Li , D , Zhang , Q , Liu , H-L , Wu , Y , Bronfman , L , Juvela , M , Lee , C W , Garay , G , Zhang , Y , He , J , Hsu , S-Y , Shen , Z-Q , Lee , J-E , Wang , K , Tang , N , Tang , M , Zhang , C , Yue , Y , Xue , Q , Li , S , Peng , Y , Dutta , S , Ge , J , Xu , F , Chen , L-F , Baug , T , Dewangan , L & Tej , A 2022 , ' ATOMS : ALMA Three-millimeter Observations of Massive Star-forming regions - VIII. A search for hot cores by using C2H5CN, CH3OCHO, and CH3OH lines ' , Monthly Notices of the Royal Astronomical Society , vol. 511 , no. 3 , pp. 3463-3476 . https://doi.org/10.1093/mnras/stac219; ORCID: /0000-0002-5809-4834/work/110389320; http://hdl.handle.net/10138/352552; 8a1938e9-77a6-4aa9-ba45-6e955b467495; 000759087700004

الاتاحة: http://hdl.handle.net/10138/352552

المؤلفون: Liu, Hong-Li, Liu, Tie, Evans II, Neal J., Wang, Ke, Garay, Guido, Qin, Sheng-Li, Li, Shanghuo, Stutz, Amelia, Goldsmith, Paul F., Liu, Sheng-Yuan, Tej, Anandmayee, Zhang, Qizhou, Juvela, Mika, Li, Di, Wang, Jun-Zhi, Bronfman, Leonardo, Ren, Zhiyuan, Wu, Yue-Fang, Kim, Kee-Tae, Lee, Chang Won, Tatematsu, Ken'ichi, Cunningham, Maria R., Liu, Xun-Chuan, Wu, Jing-Wen, Hirota, Tomoya, Lee, Jeong-Eun, Li, Pak-Shing, Kang, Sung-Ju, Mardones, Diego, Ristorcelli, Isabelle, Zhang, Yong, Luo, Qiu-Yi, Toth, L. Viktor, Yi, Hee-weon, Yun, Hyeong-Sik, Peng, Ya-Ping, Li, Juan, Zhu, Feng-Yao, Shen, Zhi-Qiang, Baug, Tapas, Dewangan, L. K., Chakali, Eswaraiah, Liu, Rong, Xu, Feng-Wei, Wang, Yu, Zhang, Chao, Li, Jinzeng, Zhou, Jianwen, Tang, Mengyao, Xue, Qiaowei, Issac, Namitha, Soam, Archana, Alvarez-Gutierrez, Rodrigo H.

المساهمون: Department of Physics

مصطلحات موضوعية: Astronomy, Space science

وصف الملف: application/pdf

Relation: We thank the anonymous referee for comments and suggestions that greatly improved the quality of this paper. H-LL acknowledges funding from a FONDECYT Postdoctoral project (code 3190161). H-LL also thanks Shanghai Astronomical Observatory for providing office facilities that facilitated analysis of this work. TL acknowledges the support from the international partnership program of Chinese Academy of Sciences through grant No.114231KYSB20200009, National Natural Science Foundation of China (NSFC) through grant NSFC No.12073061, and Shanghai Pujiang Program 20PJ1415500. DL acknowledges the support from NSFC 11911530226. GG acknowledges support from ANID project AFB 170002. S-LQ is supported by NSFC under No.12033005. LB acknowledges support from CONICYT project Basal AFB-170002. AS gratefully acknowledges funding support through FONDECYT Regular (project code 1180350) and from Chilean Centro de Excelencia en Astrof ' isica y Tecnolog ' ias Afines (CATA) BASAL grant AFB-170002. RA acknowledges funding support from CONICYT Programa de Astronomia Fondo ALMA-CONICYT 201731170002. This work was carried out in part at the Jet Propulsion Laboratory, which is operated for NASA by the California Institute of Technology. CWL is supported by the Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education, Science and Technology (NRF2019R1A2C1010851). KT was supported by JSPS KAKENHI Grant Number 20H05645. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2019.1.00685.S. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. This research made use of ASTRODENDRO, a PYTHON package to compute dendrograms of Astronomical data (http://www.dendrograms.org/).This research made use of ASTROPY, a community-developed core PYTHON package for Astronomy (Astropy Collaboration 2018).; Liu , H-L , Liu , T , Evans II , N J , Wang , K , Garay , G , Qin , S-L , Li , S , Stutz , A , Goldsmith , P F , Liu , S-Y , Tej , A , Zhang , Q , Juvela , M , Li , D , Wang , J-Z , Bronfman , L , Ren , Z , Wu , Y-F , Kim , K-T , Lee , C W , Tatematsu , K , Cunningham , M R , Liu , X-C , Wu , J-W , Hirota , T , Lee , J-E , Li , P-S , Kang , S-J , Mardones , D , Ristorcelli , I , Zhang , Y , Luo , Q-Y , Toth , L V , Yi , H , Yun , H-S , Peng , Y-P , Li , J , Zhu , F-Y , Shen , Z-Q , Baug , T , Dewangan , L K , Chakali , E , Liu , R , Xu , F-W , Wang , Y , Zhang , C , Li , J , Zhang , C , Zhou , J , Tang , M , Xue , Q , Issac , N , Soam , A & Alvarez-Gutierrez , R H 2021 , ' ATOMS : ALMA three-millimeter observations of massive star-forming regions - III. Catalogues of candidate hot molecular cores and hyper/ultra compact H II regions ' , Monthly Notices of the Royal Astronomical Society , vol. 505 , no. 2 , pp. 2801-2818 . https://doi.org/10.1093/mnras/stab1352; ORCID: /0000-0002-5809-4834/work/98859276; http://hdl.handle.net/10138/341135; d57a9dd6-1e45-4766-8782-62b5ac211dfb; 000672803400092

الاتاحة: http://hdl.handle.net/10138/341135

المؤلفون: Wang, Yuyang¹ (AUTHOR), Xue, Qiaowei² (AUTHOR) xuegh2023@163.com

المصدر: Soft Computing - A Fusion of Foundations, Methodologies & Applications. Feb2024, Vol. 28 Issue 4, p3725-3742. 18p.

مصطلحات موضوعية: *GENERATIVE adversarial networks, *PRODUCT design, *FAULT diagnosis, *FUZZY integrals, *FEATURE extraction, *PIPELINE inspection, *MAGNETIC flux leakage

المؤلفون: Liu, Hong-Li, Liu, Tie, Evans, Neal J., Wang, Ke, Garay, Guido, Qin, Sheng-Li, Li, Shanghuo, Stutz, Amelia, Goldsmith, Paul F., Liu, Sheng-Yuan, Tej, Anandmayee, Zhang, Qizhou, Juvela, Mika, Li, Di, Wang, Jun-Zhi, Bronfman, Leonardo, Ren, Zhiyuan, Wu, Yue-Fang, Kim, Kee-Tae, Lee, Chang-Won, Tatematsu, Ken'Ichi, Cunningham, Maria R., Liu, Xun-Chuan, Wu, Jing-Wen, Hirota, Tomoya, Lee, Jeong-Eun, Li, Pak-Shing, Kang, Sung-Ju, Mardones, Diego, Ristorcelli, Isabelle, Zhang, Yong, Luo, Qiu-Yi, Toth, L. Viktor, Yi, Hee-Weon, Yun, Hyeong-Sik, Peng, Ya-Ping, Li, Juan, Zhu, Feng-Yao, Shen, Zhi-Qiang, Baug, Tapas, Dewangan, L. K., Chakali, Eswaraiah, Liu, Rong, Xu, Feng-Wei, Wang, Yu, Li, Jinzeng, Zhang, Chao, Zhou, Jianwen, Tang, Mengyao, Xue, Qiaowei, Issac, Namitha, Soam, Archana, Álvarez-Gutiérrez, Rodrigo H.

المساهمون: Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS)

المصدر: ISSN: 0035-8711.

مصطلحات موضوعية: errata, addenda, stars: formation, stars: kinematics and dynamics, ISM: clouds, H II regions, [SDU]Sciences of the Universe [physics]

Relation: BIBCODE: 2022MNRAS.511.501L

الاتاحة: https://insu.hal.science/insu-03672038
https://doi.org/10.1093/mnras/stac039