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Skynet Algorithm for Single-dish Radio Mapping. I. Contaminant-cleaning, Mapping, and Photometering Small-scale Structures

  • Authors: J. R. Martin, D. E. Reichart, D. A. Dutton, M. P. Maples, T. A. Berger, F. D. Ghigo, J. B. Haislip, O. H. Shaban, A. S. Trotter, L. M. Barnes, M. L. Paggen, R. L. Gao, C. P. Salemi, G. I. Langston, S. Bussa, J. A. Duncan, S. White, S. A. Heatherly, J. B. Karlik, E. M. Johnson, J. E. Reichart, A. C. Foster, V. V. Kouprianov, S. Mazlin, and J. Harvey

2019 The Astrophysical Journal Supplement Series 240 12.

  • Provider: AAS Journals

Caption: Figure 15.

Gaussian random noise background-subtracted (top) and residuals (bottom) vs. W, the sum of the weights of the non-rejected local background models that determine the global background model at each point, for 1/10 and 1/5 beamwidth rasters, and for 1, 3, 6, 12, and 24 beamwidth background-subtraction scales (background-subtraction scale times the sampling density of the data sets increases from left to right). The rms of the data varies with W, but not with background-subtraction scale or sampling density independently. Curves are 1, 2, and 3σ model noise envelopes that have been fitted to all of these data simultaneously (Equations (6) and (7)).

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