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"It is what one does": why people participate and help others in electronic communities of practice

, and . The Journal of Strategic Information Systems, 9 (2-3): 155--173 (September 2000)
DOI: http://dx.doi.org/10.1016/S0963-8687(00)00045-7

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"It is what one does": why people participate and help others in electronic communities of practice, and . The Journal of Strategic Information Systems, 9 (2-3): 155--173 (September 2000)No excess of bright galaxies around the redshift 7.1 quasar ULAS J1120+0641, , , , , , , and . (2014)cite arxiv:1406.0851Comment: Accepted for publication in MNRAS, 8 pages.Constraining Lyman-alpha spatial offsets at $3<z<5.5$ from VANDELS slit spectroscopy, , , , , , , , , and 12 other author(s). (2019)cite arxiv:1905.09467Comment: Submitted to MNRAS.PoolTestR: An R package for estimating prevalence and regression modelling for molecular xenomonitoring and other applications with pooled samples., , , , and . Environ. Model. Softw., (2021)Chasing passive galaxies in the early Universe: a critical analysis in CANDELS GOODS-South, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1709.00429Comment: 28 pages, 13 figures, 2 tables.MOONS: a multi-object optical and near-infrared spectrograph for the VLT, , , , , , , , , and 70 other author(s). Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, volume 8446 of Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, (September 2012)National study of information seeking behavior of academic researchers in the United States., , , , , , , , , and . J. Assoc. Inf. Sci. Technol., 61 (5): 869-890 (2010)Sketch Worksheets in STEM Classrooms: Two Deployments., , , , , and . AI Magazine, 41 (1): 19-32 (2020)The evolution of the galaxy UV luminosity function at redshifts z ~ 8-15 from deep JWST and ground-based near-infrared imaging, , , , , , , , , and 3 other author(s). (2022)cite arxiv:2207.12356Comment: 28 pages, 4 figures in main manuscript, submitted to MNRAS.The evolving far-IR galaxy luminosity function and dust-obscured star-formation rate density out to z~5, , , , , , , and . (2017)cite arxiv:1706.00426Comment: 17 pages, 12 figures, 5 tables, submitted to MNRAS.