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Browsing by Author "Chapman, Scott"

Browsing by Author "Chapman, Scott"

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  • Webb, Tracy; Noble, Allison; DeGroot, Andrew; Wilson, Gillian; Muzzin, Adam; Bonaventura, Nina; Cooper, Mike; Delahaye, Anna; Foltz, Ryan; Lidman, Chris; Surace, Jason; Yee, H. K. C.; Chapman, Scott; Dunne, Loretta; Geach, James; Hayden, Brian; Hildebrandt, Hendrik; Huang, Jiasheng; Pope, Alexandra; Smith, Matthew W. L.; Perlmutter, Saul; Tudorica, Alex (2015)
    We have discovered an optically rich galaxy cluster at z = 1.7089 with star formation occurring in close proximity to the central galaxy. The system, SpARCS104922.6+564032.5, was detected within the Spitzer Adaptation of ...
  • Smith, Matthew W. L.; Eales, Stephen A.; Williams, Thomas G.; Lee, Bumhyun; Li, Zongnan; Barmby, Pauline; Bureau, Martin; Chapman, Scott; Cho, Brian S.; Chung, Aeree; Chung, Eun Jung; Chung, Hui-Hsuan; Clark, Christopher J. R.; Clements, David L.; Davis, Timothy A.; De Looze, Ilse; Eden, David J.; Athikkat-Eknath, Gayathri; Ford, George P.; Gao, Yu; Gear, Walter; Gomez, Haley L.; de Grijs, Richard; He, Jinhua; Ho, Luis C.; Hughes, Thomas M.; Jiao, Sihan; Li, Zhiyuan; Kemper, Francisca; Kirchschlager, Florian; Koch, Eric W.; Kong, Albert K. H.; Lee, Chien-Hsiu; Lin, En-Tzu; Mairs, Steve; Michalowski, Michal J.; Pattle, Kate; Peng, Yingjie; Ragan, Sarah E.; Rawlings, Mark G.; Rigopoulou, Dimitra; Saintonge, Amelie; Schruba, Andreas; Tang, Xindi; Wang, Junfeng; Whitworth, Anthony P.; Wilson, Christine D.; Yim, Kijeong; Zhu, Ming (2021)
    Observing nearby galaxies with submillimeter telescopes on the ground has two major challenges. First, the brightness is significantly reduced at long submillimeter wavelengths compared to the brightness at the peak of the ...
  • Herczeg, Gregory J.; Johnstone, Doug; Mairs, Steve; Hatchell, Jennifer; Lee, Jeong-Eun; Bower, Geoffrey C.; Chen, Huei-Ru Vivien; Aikawa, Yuri; Yoo, Hyunju; Kang, Sung-Ju; Kang, Miju; Chen, Wen-Ping; Williams, Jonathan P.; Bae, Jaehan; Dunham, Michael M.; Vorobyov, Eduard I.; Zhu, Zhaohuan; Rao, Ramprasad; Kirk, Helen; Takahashi, Satoko; Morata, Oscar; Lacaille, Kevin; Lane, James; Pon, Andy; Scholz, Aleks; Samal, Manash R.; Bell, Graham S.; Graves, Sarah; Lee, E. 'lisa M.; Parsons, Harriet; He, Yuxin; Zhou, Jianjun; Kim, Mi-Ryang; Chapman, Scott; Drabek-Maunder, Emily; Chung, Eun Jung; Eyres, Stewart P. S.; Forbrich, Jan; Hillenbrand, Lynne A.; Inutsuka, Shu-ichiro; Kim, Gwanjeong; Kim, Kyoung Hee; Kuan, Yi-Jehng; Kwon, Woojin; Lai, Shih-Ping; Lalchand, Bhavana; Lee, Chang Won; Lee, Chin-Fei; Long, Feng; Lyo, A. -Ran; Qian, Lei; Scicluna, Peter; Soam, Archana; Stamatellos, Dimitris; Takakuwa, Shigehisa; Tang, Ya-Wen; Wang, Hongchi; Wang, Yiren (2017)
    Most protostars have luminosities that are fainter than expected from steady accretion over the protostellar lifetime. The solution to this problem may lie in episodic mass accretion-prolonged periods of very low accretion ...
  • Hill, Ryley; Chapman, Scott; Scott, Douglas; Apostolovski, Yordanka; Aravena, Manuel; Béthermin, Matthieu; Bradford, C. M.; Canning, Rebecca E. A.; De Breuck, Carlos; Dong, Chenxing; Gonzalez, Anthony; Greve, Thomas R.; Hayward, Christopher C.; Hezaveh, Yashar; Litke, Katrina; Malkan, Matt; Marrone, Daniel P.; Phadke, Kedar; Reuter, Cassie; Rotermund, Kaja; Spilker, Justin; Vieira, Joaquin D.; Weiß, Axel (2020)
    We present an extensive ALMA spectroscopic follow-up programme of the $z\, {=}\, 4.3$ structure SPT2349-56, one of the most actively star-forming protocluster cores known, to identify additional members using their [C II] ...
  • O'Sullivan, Ewan; Combes, Françoise; Babul, Arif; Chapman, Scott; Phadke, Kedar A.; Schellenberger, Gerrit; Salomé, Philippe (2021)
    We present Northern Extended Millimeter Array (NOEMA) CO(2-1) maps of the z = 0.4418 cluster-central quasi-stellar object (QSO) IRAS 09104+4109, which trace ~4.5 × 10<SUP>10</SUP> M<SUB>?</SUB> of molecular gas in and ...
  • Hill, Ryley; Chapman, Scott; Phadke, Kedar A.; Aravena, Manuel; Archipley, Melanie; Ashby, Matthew L. N.; Béthermin, Matthieu; Canning, Rebecca E. A.; Gonzalez, Anthony; Greve, Thomas R.; Gururajan, Gayathri; Hayward, Christopher C.; Hezaveh, Yashar; Jarugula, Sreevani; MacIntyre, Duncan; Marrone, Daniel P.; Miller, Tim; Rennehan, Douglas; Reuter, Cassie; Rotermund, Kaja M.; Scott, Douglas; Spilker, Justin; Vieira, Joaquin D.; Wang, George; Weiß, Axel (2022)
    The protocluster SPT2349-56 at $z = 4.3$ contains one of the most actively star-forming cores known, yet constraints on the total stellar mass of this system are highly uncertain. We have therefore carried out deep optical ...
  • Liu, Tie; Kim, Kee-Tae; Juvela, Mika; Wang, Ke; Tatematsu, Ken'ichi; Di Francesco, James; Liu, Sheng-Yuan; Wu, Yuefang; Thompson, Mark; Fuller, Gary; Eden, David; Li, Di; Ristorcelli, I.; Kang, Sung-ju; Lin, Yuxin; Johnstone, D.; He, J. H.; Koch, P. M.; Sanhueza, Patricio; Qin, Sheng-Li; Zhang, Qizhou; Hirano, N.; Goldsmith, Paul F.; Evans, Neal J., II; White, Glenn J.; Choi, Minho; Lee, Chang Won; Toth, L. V.; Mairs, Steve; Yi, H. -W; Tang, Mengyao; Soam, Archana; Peretto, N.; Samal, Manash R.; Fich, Michel; Parsons, Harriet; Yuan, Jinghua; Zhang, Chuan-Peng; Malinen, Johanna; Bendo, George J.; Rivera-Ingraham, A.; Liu, Hong-Li; Wouterloot, Jan; Li, Pak Shing; Qian, Lei; Rawlings, Jonathan; Rawlings, Mark G.; Feng, Siyi; Aikawa, Yuri; Akhter, S.; Alina, Dana; Bell, Graham; Bernard, J. -P; Blain, Andrew; Bogner, Rebeka; Bronfman, L.; Byun, D. -Y; Chapman, Scott; Chen, Huei-Ru; Chen, M.; Chen, Wen-Ping; Chen, X.; Chen, Xuepeng; Chrysostomou, A.; Cosentino, Giuliana; Cunningham, M. R.; Demyk, K.; Drabek-Maunder, Emily; Doi, Yasuo; Eswaraiah, C.; Falgarone, Edith; Fehér, O.; Fraser, Helen; Friberg, Per; Garay, G.; Ge, J. X.; Gear, W. K.; Greaves, Jane; Guan, X.; Harvey-Smith, Lisa; HASEGAWA, Tetsuo; Hatchell, J.; He, Yuxin; Henkel, C.; Hirota, T.; Holland, W.; Hughes, A.; Jarken, E.; Ji, Tae-Geun; Jimenez-Serra, Izaskun; Kang, Miju; Kawabata, Koji S.; Kim, Gwanjeong; Kim, Jungha; Kim, Jongsoo; Kim, Shinyoung; Koo, B. -C; Kwon, Woojin; Kuan, Yi-Jehng; Lacaille, K. M.; Lai, Shih-Ping; Lee, C. F.; Lee, J. -E; Lee, Y. -U; Li, Dalei; Li, Hua-bai; Lo, N.; Lopez, John A. P.; Lu, Xing; Lyo, A. -Ran; Mardones, D.; Marston, A.; McGehee, P.; Meng, F.; Montier, L.; Montillaud, Julien; Moore, T.; Morata, O.; Moriarty-Schieven, Gerald H.; Ohashi, S.; Pak, Soojong; Park, Geumsook; Paladini, R.; Pattle, Kate M.; Pech, Gerardo; Pelkonen, V. -M; Qiu, K.; Ren, Zhi-Yuan; Richer, John; Saito, M.; Sakai, Takeshi; Shang, H.; Shinnaga, Hiroko; Stamatellos, Dimitris; Tang, Y. -W; Traficante, Alessio; Vastel, Charlotte; Viti, S.; Walsh, Andrew; Wang, Bingru; Wang, Hongchi; Wang, Junzhi; Ward-Thompson, D.; Whitworth, Anthony; Xu, Ye; Yang, J.; Yang, Yao-Lun; Yuan, Lixia; Zavagno, A.; Zhang, Guoyin; Zhang, H. -W; Zhou, Chenlin; Zhou, Jianjun; Zhu, Lei; Zuo, Pei; Zhang, Chao (2018)
    The low dust temperatures (<SUB>?</SUB>, ~12 pc, and ~500 M <SUB>?</SUB> pc<SUP>-1</SUP>, respectively. Ten massive clumps, including eight starless ones, are found along the filament. The most massive clump as a whole may ...

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