(e.g. D. Arzoumanian, V. K ̈onyves, A. Men’shchikov, Y. Shimajiri, T. Csengeri, G. Fuller, Ph. Andr ́e, N. Schneider)
This group will focus on comparing the proper- ties (e.g. widths) of the filamentary structures identified with ArTéMiS/Herschel in the target clouds (d ∼< 3 kpc) with those measured with Herschel in the nearby clouds of the Gould Belt (cf. Arzoumanian et al. 2011, 2018).
(e.g. N. Peretto, A. Rigby, A. Zavagno, D. Russeil, S. Bontemps, T. Csengeri, G. Fuller, J. Di Francesco, N. Schneider, A. Duarte-Cabral)
This group will focus on studying where and how the transition from a “core-fed” to a “clump-fed” regime of protostellar mass growth occurs in dense cluster-forming clumps.
(e.g. F. Schuller, H. Roussel, A. Rigby, Y. Shimajiri, S. Pezzuto, P. Gallais, Ph. André)
This group, which includes the main developers of the ArTéMiS IDL pipeline (“APIS”) and Scanamorphos software (both made publicly available – www.apex- telescope.org/instruments/pi/artemis/data reduction/ and demonstrated at ESO workshop SD2018, will be in charge of data reduction. AWG1 will also be responsible for the optimum combination of ArTéMiS 350/450 μm & Herschel/SPIRE 350/500 μm data and for the delivery of reliable map/data products. APIS calibrated maps and Scanamorphos-processed maps to be delivered 1 and 2 year(s) after the end of the observations, respectively.
(e.g. A. Men’shchikov, P. Didelon, C. Pichon)
AWG2 will be in charge of the systematic production of catalogs of both compact sources and filamentary structures from the combined ArTéMiS/Herschel maps, using the getimages (Men’shchikov 2017), getsources (Men’shchikov et al. 2012), getfilaments (Men’shchikov 2013), and DisPerSE algorithms (Sousbie 2011).