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작성자 : 한국천문학회 | 등록일시 : 2019-05-24 13:27 | |||||||||
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e-MERLIN/VLBI National Facility - Call for e-MERLIN proposals cycle-9 *********** e-MERLIN/VLBI National Facility **************** ******* CALL FOR e-MERLIN PROPOSALS - Cycle-9 ***** ***********http://www.e-merlin.ac.uk/observe.html ******** ************** DEADLINE : 26th June 2019 ****************** e-MERLIN requests proposals from the international astronomical community for observations to be made during Cycle-9. Proposals are competitively peer-reviewed under standard STFC rules by the PATT e-MERLIN Time Allocation Committee. Allocation will be made on the basis of scientific merit and technical feasibility alone. During e-MERLIN operations ~50% of observing time has been allocated to large legacy projects and the remaining formal time will be allocated via PATT to standard proposals solicited prior to each observing semester. e-MERLIN Science: e-MERLIN observations address a broad range of http://www.e-merlin.ac.uk/science.html and its unique combination of angular resolution (mas) and sensitivity (microJy) provide crucial insights in multiple science areas including: • star-formation and black hole growth in galaxies; • the physical processes which govern the formation of stars; • the modes of activity in nearby galaxies; • transient radio sources; • Radio spectral lines (masers and in absorption); • The energetic processes in relativistic outflows from jets generated by black holes and compact objects; • Along with multiple other applications. e-MERLIN provides high resolution (12-150mas) and high sensitivity (microJy) imaging at cm wavelengths as well as polarimetry, spectroscopy and astrometry. e-MERLIN is an SKA-pathfinder instrument providing observations with resolutions and frequencies comparable to those that will be provided by SKA1-mid. *** Cycle-8 e-MERLIN Observations: Quarters 3 & 4 2019 *** Deadline for Receipt of Proposals - 23:59:59 UT on 26th June 2019 Ang. res. Sensitivity L-band (1.23-1.74GHz) - ~150mas ~12uJy/bm* C-band (4.5 - 7.5GHz) - ~40mas ~10uJybm* K-band (19 - 25GHz) - ~12mas ~20uJy/bm * Assumes inclusion of Lovell Telescope at L/C-band and a full imaging track (~12hrs including calibration). The full call for proposals, including technical specifications is available at: e-MERLIN is partially supported via theRadioNet Transnational Access activity via the EU Horizon 2020 programme RadioNet. This activity provides travel support for eligible e-MERLIN users. For further information or contact e-MERLIN staff (emerlin@jb.man.ac.uk). EVN+e-MERLIN Observations: The full integration of e-MERLIN telescopes within the EVN is also available for proposals. This mode of observations provides 'short-spacing' (10-200km spacing) component to VLBI. This allows imaging of wider range of spatial scales. Proposals for EVN+e-MERLIN observations should be made via the EVN-PC. The current Call for EVN Proposals (including combined e-MERLIN+EVN observations is detailed at https://www.evlbi.org. The deadline for EVN proposals is 1st June 2019 ************************************************************************* e-MERLIN/VLBI National Facility, The University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, United Kingdom Email:emerlin@jb.man.ac.uk |
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