Changeset 40311
- Timestamp:
- Jan 3, 2018, 11:48:57 AM (9 years ago)
- File:
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- 1 edited
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trunk/doc/release.2015/systematics.20140411/diffusion.tex
r40307 r40311 12 12 \RequirePackage{graphicx} 13 13 \RequirePackage{color} 14 \RequirePackage{code}14 % \RequirePackage{code} 15 15 % \RequirePackage{pbox} 16 \input{ astro.sty}16 \input{magnier.tex} 17 17 18 18 %\newcommand\oldtext[1]{\color{red}#1} … … 32 32 %\def\plotmode{bw} 33 33 34 \def\plotext{pdf}35 %\def\plotext{ps}34 %\def\plotext{pdf} 35 \def\plotext{eps} 36 36 37 37 %\def\picdir{/home/eugene/chipresid.20140404} 38 38 %\def\picdir{/data/kukui.2/eugene/chipresid.20140404} 39 \def\picdir{pics} 39 %\def\picdir{pics} %%% need to set this for local processing 40 \def\picdir{.} %%% need to set this for the zip archive 40 41 41 42 % Pick a terse version of the title here; … … 441 442 high density of stars, but avoids the Galactic Plane where confusion 442 443 may potentially contaminate the measurement. We limit the analysis to 443 good measurements (\ ippmisc{PSF_QF} $>$ 0.85, see444 good measurements (\textsf{PSF\_QF} $>$ 0.85, see 444 445 \citealt{magnier2017.analysis}) of likely stars ($|m_{psf} - 445 446 m_{aper}| < 0.2$). Only measurements with instrumental magnitude $< … … 1288 1289 \bibliographystyle{apj} 1289 1290 %\bibliography{lib}{} 1290 \input{diffusion.bbl} 1291 %\input{diffusion.bbl} 1292 \input{magnier_bib.tex} 1291 1293 1292 1294 \end{document}
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