Jul 7, 2015 - 1 National Radio Astronomy Observatory, PO Box 2, Green Bank, WV 24944, USA. 2 Eleanor Roosevelt HS, 7447 Cleveland Ave, Coronoa, CA ...
The Astronomical Journal, 150:39 (1pp), 2015 July
doi:10.1088/0004-6256/150/1/39
© 2015. The American Astronomical Society. All rights reserved.
ERRATUM: “THE GBT 67–93.6 GHz SPECTRAL LINE SURVEY OF ORION-KL” (2015, AJ, 149, 162) D. T. Frayer1, Ronald J. Maddalena1, M. Meijer1,2, L. Hough1,3, S. White1, R. Norrod1, G. Watts1, M. Stennes1, R. Simon1, D. Woody1, S. Srikanth4, M. Pospieszalski4, E. Bryerton4, M. Whitehead1, P. Ford1, M. Mello1, and M. Bloss1 1
National Radio Astronomy Observatory, PO Box 2, Green Bank, WV 24944, USA 2 Eleanor Roosevelt HS, 7447 Cleveland Ave, Coronoa, CA, 92880, USA Department of Physics, West Virginia University, P.O. Box 6315, Morgantown, WV 26506, USA 4 National Radio Astronomy Observatory Central Development Lab, 1180 Boxwood Estate Road, Charlottesville, VA 22903, USA Received 2015 May 26; accepted 2015 June 3; published 2015 July 7 3
Due to an error at the publisher, the wrong image was used in Figure 4. The correct Figure 4 is shown below. None of the extended figure panels are affected. IOP Publishing sincerely regrets this error.
Figure 4. Example portion of the survey that includes the strong HCN(1–0) emission line. The top panel shows the full data range, while the bottom panel shows the same data zoomed-in along the y-axis to highlight the visibility of weak features. Spectral features are marked by the dotted-lines and labeled by species. The dottedlines of neighboring transitions from the same species are connected by a solid line below the spectrum for clarity. The feature labeled with a “U” is unidentified. The full survey plotted with overlapping spectra separated by 0.5 GHz is provided as supplemental online material in the published article.
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