M
Maxim Voronkov
Researcher at Commonwealth Scientific and Industrial Research Organisation
Publications - 142
Citations - 6826
Maxim Voronkov is an academic researcher from Commonwealth Scientific and Industrial Research Organisation. The author has contributed to research in topics: Maser & Galaxy. The author has an hindex of 40, co-authored 139 publications receiving 6036 citations. Previous affiliations of Maxim Voronkov include Australia Telescope National Facility.
Papers
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Journal ArticleDOI
Variability monitoring of the hydroxyl maser emission in G12.889+0.489
TL;DR: In this article, a series of observations with the Australia Telescope Compact Array have monitored the variability of the ground-state hydroxyl maser emission from G12, with the peak flux densities of the 1665- and 1667-MHz emission were observed to vary at a level of ∼20
Journal ArticleDOI
ASKAP commissioning observations of the GAMA 23 field
Denis Leahy,Andrew M. Hopkins,Ray P. Norris,Ray P. Norris,J. Marvil,Jordan D. Collier,Jordan D. Collier,Jordan D. Collier,Edward N. Taylor,James R. Allison,Craig S. Anderson,Martin Bell,Maciej Bilicki,Jonathan Bland-Hawthorn,Sarah Brough,Michael J. I. Brown,Simon P. Driver,G. Gürkan,Lisa Harvey-Smith,Lisa Harvey-Smith,Ian Heywood,Ian Heywood,Benne W. Holwerda,Jochen Liske,Angel R. Lopez-Sanchez,David McConnell,Amanda J. Moffett,Matt S. Owers,Kevin A. Pimbblet,Wasim Raja,Nick Seymour,Maxim Voronkov,Lingyu Wang,Lingyu Wang +33 more
TL;DR: In this paper, the authors have observed the G23 field of the Galaxy AndMass Assembly (GAMA) survey using the Australian Square Kilometre Array Pathfinder (ASKAP) in its commissioning phase to validate the performance of the telescope and to characterise the detected galaxy populations.
Journal ArticleDOI
The evolutionary status of protostellar clumps hosting class II methanol masers
BM Jones,Gary A. Fuller,Shari Breen,Adam Avison,J. A. Green,Alessio Traficante,D. Elia,Simon Ellingsen,Maxim Voronkov,Manuel Merello,Manuel Merello,Sergio Molinari,Eugenio Schisano +12 more
TL;DR: In this article, the authors characterize the properties of 6.7 GHz methanol masers using dust emission detected by the Herschel Infrared Galactic Plane Survey (Hi-GAL) to assess their evolutionary state.
Journal ArticleDOI
The ASKAP Variables and Slow Transients (VAST) Pilot Survey
Tara Murphy,David L. Kaplan,Adam Stewart,Andrew O'Brien,Emil Lenc,Sergio Pintaldi,Joshua Pritchard,Dougal Dobie,Archibald Fox,James K. Leung,Tao An,Martin Bell,J. W. Broderick,Shami Chatterjee,Shi Dai,Daniele d’Antonio,J. Gerry Doyle,Bryan Gaensler,George Heald,Assaf Horesh,Megan L. Jones,David McConnell,Vanessa A. Moss,Wasim Raja,Gavin Ramsay,Stuart D. Ryder,Elaine M. Sadler,Gregory R. Sivakoff,Yuanming Wang,Ziteng Wang,Michael S. Wheatland,Matthew Whiting,James R. Allison,Craig S. Anderson,Lewis Ball,Keith W. Bannister,Douglas C.-J. Bock,R. Bolton,John D. Bunton,R. Chekkala,Aaron Chippendale,F. R. Cooray,Nikhel Gupta,Douglas B. Hayman,K. Jeganathan,Baerbel Koribalski,K. Lee-Waddell,Elizabeth K. Mahony,J. Marvil,Naomi McClure-Griffiths,P. Mirtschin,A. Ng,Sarah Pearce,Chris Phillips,Maxim Voronkov +54 more
TL;DR: The VAST Phase I Pilot Survey as mentioned in this paper consists of 162$ hours of observations conducted at a central frequency of 888~MHz between 2019 August and 2020 August, with a typical rms sensitivity of 0.24~mJy~beam$^{-1}$ and angular resolution of $12-20$ arcseconds.
Journal ArticleDOI
How do methanol masers manage to appear in the youngest star vicinities and isolated molecular clumps
A. M. Sobolev,D. M. Cragg,Simon Ellingsen,Michael J. Gaylard,Sharmila Goedhart,Christian Henkel,Maria S. Kirsanova,A. B. Ostrovskii,N. V. Pankratova,O. V. Shelemei,D. J. van der Walt,T. S. Vasyunina,Maxim Voronkov +12 more
TL;DR: In this article, a multiline analysis of the methanol masers allows us to determine the physical parameters in the regions of maser forma- tion, and it is shown that most of the maser sources from the Perseus arm are associated with embedded stellar clusters and a considable portion is situated close to compact Hii regions.