search for: luminosity

...ude of rotational velocity (2) 49- 52 F4.2 mag AB ? Internal B band extinction (3) 54- 58 F5.1 mag BMag ? Absolute B band magnitude (4) 60- 63 F4.1 mag/arcsec2 SBB ? Average B band surface brightness (5) 65- 69 F5.2 [solLum] logKLum ? Log K_S_ band luminosity (6) 71- 75 F5.2 [solMass] logM26 ? Log mass within Holmberg radius (7) 77 A1 --- l_logMHI Limit flag on logMHI 78- 82 F5.2 [solMass] logMHI ? Log hydrogen mass (8) 84- 87 I4 km/s VLG ? Radial velocity (9) 89- 92 F4.1 --- Theta1 ? Tid...

...l velocity (2) > 49- 52 F4.2 mag AB ? Internal B band extinction (3) > 54- 58 F5.1 mag BMag ? Absolute B band magnitude (4) > 60- 63 F4.1 mag/arcsec2 SBB ? Average B band surface brightness (5) > 65- 69 F5.2 [solLum] logKLum ? Log K_S_ band luminosity (6) > 71- 75 F5.2 [solMass] logM26 ? Log mass within Holmberg radius (7) > 77 A1 --- l_logMHI Limit flag on logMHI > 78- 82 F5.2 [solMass] logMHI ? Log hydrogen mass (8) > 84- 87 I4 km/s VLG ? Radial velocity (9) > 89- 92 F4.1 ---...

...;t help to communicate information at all. In fact, it actually hinders proper reading of the graph, The issue is that "Platinum", "Silver", and to a lesser extent, "Garbage" are almost the same color. Platinum and Silver are the worst offenders, being almost the same luminosity and a very light change in hue. (Platinum is a little more "blue"). The idea is that graphs should make it easier to read, not more of a challenge. Graphs often use a gradient of color to indicate "better-ness" and which colors are culturally dependent. Generically, A spectrum...

...gative residuals with the hue/. Varying the chroma and the luminance only affect the distinctions between large and small and significant and non significant. But my positive and negative residuals are both large (absolutely) and significant, meaning that they will have the same chroma and luminosity, but different hues. I guess the key here is to find two separate hue values that appear substantially different *on a grayscale printer* at the same chroma and luminance. I have read through Zeileis et al. (2007, 2008) but can't quite find the answer there. I have also tried the Friend...

...gt; 49- 52 F4.2 mag AB ? Internal B band extinction (3) >> 54- 58 F5.1 mag BMag ? Absolute B band magnitude (4) >> 60- 63 F4.1 mag/arcsec2 SBB ? Average B band surface brightness (5) >> 65- 69 F5.2 [solLum] logKLum ? Log K_S_ band luminosity (6) >> 71- 75 F5.2 [solMass] logM26 ? Log mass within Holmberg radius (7) >> 77 A1 --- l_logMHI Limit flag on logMHI >> 78- 82 F5.2 [solMass] logMHI ? Log hydrogen mass (8) >> 84- 87 I4 km/s VLG ? Radial velocity (9) >&g...

It looks like fixed width. I just used the last position of each field to get the size and used the 'readr' package; > input <- "And XVIII 000214.5+450520 0.69 17 9 0.00 -8.7 26.8 6.44 6.78 < 6.65 -44 0.5 MESSIER031 0.6 1.54 + PAndAS-03 000356.4+405319 0.10 17 0.00 -3.6 27.8 4.38 2.8 MESSIER031

dear R-users, I am facing a quite regular and basic problem when it comes to dealing with datasets, but I cannot find any satisfying answer so far. I have a messy dataset of galaxies like that : And XVIII 000214.5+450520 0.69 17 9 0.00 -8.7 26.8 6.44 6.78 < 6.65 -44 0.5 MESSIER031 0.6 1.54 PAndAS-03 000356.4+405319 0.10 17 0.00 -3.6 27.8 4.38

dear R experts---I am struggling with the requirements to prepare my files for my printers. I am printing in 2/2 format, which means cyan and black for me, which they take from my color-separated pdf files. R comes into play, because it produces all the figures that are embedded in my book (pdflatex). now, TeX has no problems producing CMYK files. However, R produces RGB files (for

On Fri, 25 May 2012 14:00:01 -0500, <theora-request at xiph.org> wrote: > Message: 1 > Date: Fri, 25 May 2012 19:26:18 +0200 > From: Raphael Canut <nhwcodec at gmail.com> > Subject: [theora] NHW codec - improvement of precision > To: theora at xiph.org > Message-ID: > <CAKE58qHqSsrgJP4OX++eetMmT2WTv=8ZvfXoou7bWjOnbUSrAQ at mail.gmail.com> > Content-Type:

Dear r-helpers, I wonder whether, given the "#rrggbb" representation of a colour, there is a simple way to select the complementary colour, also expressed as a "#rrggbb" string. Any suggestions would be appreciated. John -------------------------------- John Fox, Professor Department of Sociology McMaster University Hamilton, Ontario Canada L8S 4M4 905-525-9140x23604

https://bugs.freedesktop.org/show_bug.cgi?id=47965 Bug #: 47965 Summary: I can't modify brightness with nVidia 1000m Quadro Classification: Unclassified Product: xorg Version: unspecified Platform: All OS/Version: All Status: NEW Severity: normal Priority: medium Component: