Issue |
A&A
Volume 581, September 2015
|
|
---|---|---|
Article Number | A80 | |
Number of page(s) | 16 | |
Section | Astronomical instrumentation | |
DOI | https://doi.org/10.1051/0004-6361/201525879 | |
Published online | 08 September 2015 |
Online material
Appendix A: Properties of young substellar objects
We report in Table A.1 the properties of the young substellar objects used in Fig. 1.
Physical and atmospheric parameters of the young planetary-mass objects and companions used to investigate the depth of the 1.62 μm methane absorption band.
Appendix B: ASDI patterns using other ADI algorithms
We display in Fig. B.1 the ADI-reduced version of Fig. 3 with the sADI, rADI, PCA, and LOCI algorithms.
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Fig. B.1
Same as Fig. 11 with sADI (top left panel), rADI (top right panel), LOCI (bottom left panel), and PCA (bottom right panel) processing. The same parameters were used as in Fig. 12. The scaling made use of the bytscl IDL function and is identical in the panels. |
Open with DEXTER |
© ESO, 2015
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