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JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies - I. Survey overview and first results

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 481:3 (2018) 3497-3519

Authors:

Amelie Saintonge, Christine D Wilson, Ting Xiao, Lihwai Lin, Ho Seong Hwang, Tomoka Tosaki, Martin Bureau, Phillip J Cigan, Christopher JR Clark, David L Clements, Ilse De Looze, Thavisha Dharmawardena, Yang Gao, Walter K Gear, Joshua Greenslade, Isabella Lamperti, Jong Chul Lee, Cheng Li, Michal J Michalowski, Angus Mok, Hsi-An Pan, Anne E Sansom, Mark Sargent, Matthew WL Smith, Thomas Williams, Chentao Yang, Ming Zhu, Gioacchino Accurso, Pauline Barmby, Elias Brinks, Nathan Bourne, Toby Brown, Aeree Chung, Eun Jung Chung, Anna Cibinel, Kristen Coppin, Jonathan Davies, Timothy A Davis, Steve Eales, Lapo Fanciullo, Taotao Fang, Yu Gao, David HW Glass, Haley L Gomez, Thomas Greve, Jinhua He, Luis C Ho, Feng Huang, Hyunjin Jeong, Xuejian Jiang, Qian Jiao, Francisca Kemper, Ji Hoon Kim, Minjin Kim, Taehyun Kim, Jongwan Ko, Xu Kong, Kevin Lacaille, Cedric G Lacey, Bumhyun Lee, Joon Hyeop Lee, Wing-Kit Lee, Karen Masters, Se-Heon Oh, Padelis Papadopoulos, Changbom Park, Sung-Joon Park, Harriet Parsons, Kate Rowlands, Peter Scicluna, Jillian M Scudder, Ramya Sethuram, Stephen Serjeant, Yali Shao, Yun-Kyeong Sheen, Yong Shi, Hyunjin Shim, Connor MA Smith, Kristine Spekkens, An-Li Tsai, Aprajita Verma, Sheona Urquhart, Giulio Violino, Serena Viti, David Wake, Junfeng Wang, Jan Wouterloot, Yujin Yang, Kijeong Yim, Fangting Yuan, Zheng Zheng
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SPIRITS 16tn in NGC 3556: A Heavily Obscured and Low-luminosity Supernova at 8.8 Mpc

ASTROPHYSICAL JOURNAL 863:1 (2018) ARTN 20

Authors:

Jacob E Jencson, Mansi M Kasliwal, Scott M Adams, Howard E Bond, Ryan M Lau, Joel Johansson, Assaf Horesh, Kunal P Mooley, Robert Fender, Kishalay De, Donal O'Sullivan, Frank J Masci, Ann Marie Cody, Nadia Blagorodnova, Ori D Fox, Robert D Gehrz, Peter A Milne, Daniel A Perley, Nathan Smith, Schuyler D Van Dyk
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The KMOS Redshift One Spectroscopic Survey (KROSS): the origin of disc turbulence in z ≈ 1 star-forming galaxies

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 474:4 (2018) 5076-5104

Authors:

HL Johnson, CM Harrison, AM Swinbank, AL Tiley, JP Stott, RG Bower, Ian Smail, AJ Bunker, D Sobral, OJ Turner, P Best, M Bureau, M Cirasuolo, MJ Jarvis, G Magdis, RM Sharples, J Bland-Hawthorn, B Catinella, L Cortese, SM Croom, C Federrath, K Glazebrook, SM Sweet, JJ Bryant, M Goodwin, IS Konstantopoulos, JS Lawrence, AM Medling, MS Owers, S Richards
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The very-faint X-ray binary IGR J17062-6143: a truncated disk, no pulsations and a possible outflow

ArXiv 1712.03949 (2017)

Authors:

J van den Eijnden, N Degenaar, C Pinto, A Patruno, K Wette, C Messenger, JV Hernandez Santisteban, R Wijnands, JM Miller, D Altamirano, F Paerels, D Chakrabarty, AC Fabian
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A precise measurement of the magnetic field in the corona of the black hole binary V404 Cygni

Science American Association for the Advancement of Science 358:6368 (2017)

Authors:

Y Dallilar, SS Eikenberry, A Garner, RD Stelter, A Gottlieb, P Gandhi, P Casella, VS Dhillon, TR Marsh, SP Littlefair, L Hardy, Robert Fender, Kunal Mooley, DJ Walton, F Fuerst, M Bachetti, AJ Castro-Tirado, M Charcos, ML Edwards, NM Lasso-Cabrera, A Marin-Franch, K Ackley, JG Bennett, AJ Cenarro, B Chinn, HV Donoso, R Frommeyer, K Hanna, J Julian, P Miller, S Mullin, CH Murphey, C Packham, F Varosi, C Vega, C Warner, AN Ramaprakash, M Burse, S Punnadi, P Chordia, A Gerarts, H De Paz Martín, MM Calero, R Scarpa, SF Acosta, B Siegel, FF Pérez

Abstract:

Observations of binary stars containing an accreting black hole or neutron star often show x-ray emission extending to high energies (>10 kilo--electron volts), which is ascribed to an accretion disk corona of energetic particles akin to those seen in the solar corona. Despite their ubiquity, the physical conditions in accretion disk coronae remain poorly constrained. Using simultaneous infrared, optical, x-ray, and radio observations of the Galactic black hole system V404 Cygni, showing a rapid synchrotron cooling event in its 2015 outburst, we present a precise 461 ± 12 gauss magnetic field measurement in the corona. This measurement is substantially lower than previous estimates for such systems, providing constraints on physical models of accretion physics in black hole and neutron star binary systems.
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