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|Abstract:||Due to an indexing error, the M- and N-band columns of Table 1 were in error (what was labeled M-band was actually the L-band part of the spectrum, but using the M-band filter zero-point; what was labeled N-band was actually the M-band part of the spectrum, but using the N-band filter zero-point). This error was only in the code that produced the table in the paper and the electronic tables available online. Everything else was unaffected (all figures—including plots of M- and N-band magnitudes—were computed correctly, as were all spectra—both in figures and in electronic tables available online).3 Table 1 in its complete and correct form appears below, and similar (corrected) tables for the other three atmosphere types are available in electronic form online, in addition to corrected versions of the magnitude-evolution files previously published.|
|Electronic Publication Date:||7-Oct-2013|
|Citation:||Spiegel, David S, Burrows, Adam. (2013). Erratum: ”Spectral and Photometric Diagnostics of Giant Planet Formation Scenarios” <A href=”/abs/2012ApJ...745..174S”>(2012, ApJ, 745, 174)</A>. \apj, 776 (138 - 138. doi:10.1088/0004-637X/776/2/138|
|Type of Material:||Journal Article|
|Journal/Proceeding Title:||Astrophysical Journal|
|Version:||Final published version. This is an open access article.|
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