Index: /branches/eam_branches/ipp-20120905/dvodist/Makefile.in =================================================================== --- /branches/eam_branches/ipp-20120905/dvodist/Makefile.in (revision 34552) +++ /branches/eam_branches/ipp-20120905/dvodist/Makefile.in (revision 34553) @@ -1,3 +1,3 @@ -default: +default: php help: @echo "USAGE: make php" @@ -25,4 +25,5 @@ $(TGT-UTIL)/blank.html \ $(TGT-UTIL)/ipp.menu.dat \ +$(TGT-UTIL)/ipp.page.php \ $(TGT-UTIL)/ipp.php \ $(TGT-UTIL)/markdown.php \ @@ -31,33 +32,11 @@ ROOT = \ $(TGT-ROOT)/PScolorlogo2.jpg \ -$(TGT-ROOT)/docs.txt \ -$(TGT-ROOT)/help.txt \ -$(TGT-ROOT)/index.txt \ $(TGT-ROOT)/index.php \ +$(TGT-ROOT)/test.php \ +$(TGT-ROOT)/docs.php \ +$(TGT-ROOT)/help.php \ $(TGT-ROOT)/ipp.css -TEST = \ -$(TGT-ROOT)/help.php \ -$(TGT-UTIL)/ipp.page.php - -test: $(TEST) - php: $(ROOT) $(UTIL) $(PROG) - -## # non-generated php code is copied directly -## $(TGT-ROOT)/%: $(SRC-ROOT)/% -## @if [ ! -d $(TGT-ROOT) ]; then mkdir -p $(TGT-ROOT) || exit; fi -## cp $(SRC-ROOT)/$* $(TGT-ROOT)/$* || exit -## chmod +x $(TGT-ROOT)/$* || exit -## -## $(TGT-PROG)/%: $(SRC-PROG)/% -## @if [ ! -d $(TGT-PROG) ]; then mkdir -p $(TGT-PROG) || exit; fi -## cp $(SRC-PROG)/$* $(TGT-PROG)/$* || exit -## chmod +x $(TGT-PROG)/$* || exit -## -## $(TGT-UTIL)/%: $(SRC-UTIL)/% -## @if [ ! -d $(TGT-UTIL) ]; then mkdir -p $(TGT-UTIL) || exit; fi -## cp $(SRC-UTIL)/$* $(TGT-UTIL)/$* || exit -## chmod +x $(TGT-UTIL)/$* || exit # mkd files are used to generate php files @@ -72,4 +51,20 @@ rm -f $(TGT-UTIL)/$*.php || exit $(GENERATE) --htdocs @HTDOCS@ $(SRC-UTIL)/$*.mkd $(TGT-UTIL)/$*.php || exit + +$(TGT-PROG)/%: $(SRC-PROG)/% + @if [ ! -d $(TGT-PROG) ]; then mkdir -p $(TGT-PROG) || exit; fi + cp $(SRC-PROG)/$* $(TGT-PROG)/$* || exit + chmod +x $(TGT-PROG)/$* || exit + +# non-generated php code is copied directly +$(TGT-ROOT)/%: $(SRC-ROOT)/% + @if [ ! -d $(TGT-ROOT) ]; then mkdir -p $(TGT-ROOT) || exit; fi + cp $(SRC-ROOT)/$* $(TGT-ROOT)/$* || exit + chmod +x $(TGT-ROOT)/$* || exit + +$(TGT-UTIL)/%: $(SRC-UTIL)/% + @if [ ! -d $(TGT-UTIL) ]; then mkdir -p $(TGT-UTIL) || exit; fi + cp $(SRC-UTIL)/$* $(TGT-UTIL)/$* || exit + chmod +x $(TGT-UTIL)/$* || exit # utilities ################################################# Index: /branches/eam_branches/ipp-20120905/dvodist/www-root/docs.mkd =================================================================== --- /branches/eam_branches/ipp-20120905/dvodist/www-root/docs.mkd (revision 34553) +++ /branches/eam_branches/ipp-20120905/dvodist/www-root/docs.mkd (revision 34553) @@ -0,0 +1,125 @@ + + +# DVO Documentation + +## Release Notes on 3pi.20120525 + +This database contains PS1 3pi observations through 2012/01/21. The +ubercal zero points have been applied to all exposures included in +that analysis. The remaining exposures have been tied to the ubercal +system via relative photometry. The ubercal measurements are given +10x their poisson weight to ensure they drive the photometric +solution. + +The database has been merged with the PS1 Synthetic photometry +database (based on 2MASS and USNO-B). For objects brighter than the +saturation limit, the Synthetic photometry has been used for the mean +magnitudes (these can be identified by having bit 0x04 raised in the +mean filter flags). Objects which used ubercal photometry have the +bit 0x08 raised in the mean filter flags. + +This database has also been merged with the 2MASS, WISE, and +SuperCOSMOS databases. The following photcodes are used for those +external photometric sources: + + + + + + + + + + + + + + + + + + + + + + + + + +
Source Photcode
2MASS_J 2011
2MASS_H 2012
2MASS_K 2013
WISE_W1 2014
WISE_W2 2015
WISE_W3 2016
WISE_W4 2017
SYNTH.g 3001
SYNTH.r 3002
SYNTH.i 3003
SYNTH.z 3004
SYNTH.y 3005
SCOS.103a.E 1150
SCOS.4414.OG590 1151
SCOS.4415.OG590 1152
SCOS.IIIaF.OG590 1153
SCOS.IIIaF.RG610 1154
SCOS.IIIaF.RG630 1155
SCOS.IIIaJ.GG385 1156
SCOS.IIIaJ.GG395 1157
SCOS.IVN.RG715 1158
SCOS.IVN.RG9 1159
+ +
+Map of the mean per-star residual (inst mag brighter than -10) for +i-band (ubercal data only). +
+ +
+Map of the mean per-star residual (inst mag brighter than -10) for +g-band (ubercal data only). +
+ +

Comparison with 2MASS

+ +The plots below compare the PS1 grizy photometry with 2MASS photometry +by examining the location of the color-color locus for early (< K0) +main sequence stars. + +For each pixel (0.5 degree on a side), I select all objects with PS1 r +< 20 and detected JHK magnitudes, keeping only those with S/N in +the mean > 50 and standard deviations less than 0.05 magnitudes. I +then fit the stellar locus in g-r,r-i for the g-r range 0.2 to 1.0, +and keep only objects that fall within 0.05 of that (linear) stellar +locus fit.
+ +I then fit the stellar locus with a line in each of the color-color diagrams +g-i,i-J; g-i,i-H; g-i,i-K. I measure the mean i-J color expected from +the fit for stars with g-i = 0.5. The figures below show the maps of +the i-J, i-H, and i-K offsets as well as the J-H and H-K offsets at +g-i = 0.5. The center of these maps is RA,DEC = 0,0, (east is left, +north is up). The pixels are 0.5 degrees on a side.
+ +These maps show three main features. The Galactic Plane is quite +clear, and not surprising: this test is particularly sensitive to +reddening.
+ +Several large scale patches are also visible (eg, the black patch near +RA ~ 150 deg). Disappointingly, these correspond to areas without +good ubercal ties -- in other words, these are regions in which the +data were obtained in non-photometric conditions. This shows the +limitation of using relative photometry to tie across individual +exposures. If the exposures have an extinction gradient, the +correction far from the photometrically tied region can drift from the +correct value. The largest region at RA ~ 150 matches a section with +poor i-band photometry and has a depth of roughly 0.1 magnitudes in +i-J. Assuming this is completely due to i-band errors, this +corresponds to about 0.06 magnitudes of drift to the center of this +region.
+ +The third pattern is at a lower level of intensity: N-S strips with +roughly E-W bands. They are most noticable in K and H-K. These +appear to correspond well to the 2MASS scanning pattern, and have an +amplitude corresponding to about 0.02 - 0.04 magnitudes of offset in +K.
+ +
+Map of the i-J color at g-i = 0.5. +
+ +
+Map of the i-H color at g-i = 0.5. +
+ +
+Map of the i-K color at g-i = 0.5. +
+ +Combinations of the above maps can highlight any problems in 2MASS +which are driven by the color rather than the mean magnitudes. + +
+Map of the J-H color at g-i = 0.5. +
+ +
+Map of the H-K color at g-i = 0.5. +
Index: anches/eam_branches/ipp-20120905/dvodist/www-root/docs.txt =================================================================== --- /branches/eam_branches/ipp-20120905/dvodist/www-root/docs.txt (revision 34552) +++ (revision ) @@ -1,123 +1,0 @@ -

DVO Documentation

- -

Release Notes on 3pi.20120525

- -This database contains PS1 3pi observations through 2012/01/21. The -ubercal zero points have been applied to all exposures included in -that analysis. The remaining exposures have been tied to the ubercal -system via relative photometry. The ubercal measurements are given -10x their poisson weight to ensure they drive the photometric -solution. - -The database has been merged with the PS1 Synthetic photometry -database (based on 2MASS and USNO-B). For objects brighter than the -saturation limit, the Synthetic photometry has been used for the mean -magnitudes (these can be identified by having bit 0x04 raised in the -mean filter flags). Objects which used ubercal photometry have the -bit 0x08 raised in the mean filter flags. - -This database has also been merged with the 2MASS, WISE, and -SuperCOSMOS databases. The following photcodes are used for those -external photometric sources: - - - - - - - - - - - - - - - - - - - - - - - - - -
Source Photcode
2MASS_J 2011
2MASS_H 2012
2MASS_K 2013
WISE_W1 2014
WISE_W2 2015
WISE_W3 2016
WISE_W4 2017
SYNTH.g 3001
SYNTH.r 3002
SYNTH.i 3003
SYNTH.z 3004
SYNTH.y 3005
SCOS.103a.E 1150
SCOS.4414.OG590 1151
SCOS.4415.OG590 1152
SCOS.IIIaF.OG590 1153
SCOS.IIIaF.RG610 1154
SCOS.IIIaF.RG630 1155
SCOS.IIIaJ.GG385 1156
SCOS.IIIaJ.GG395 1157
SCOS.IVN.RG715 1158
SCOS.IVN.RG9 1159
- -
-Map of the mean per-star residual (inst mag brighter than -10) for -i-band (ubercal data only). -
- -
-Map of the mean per-star residual (inst mag brighter than -10) for -g-band (ubercal data only). -
- -

Comparison with 2MASS

- -The plots below compare the PS1 grizy photometry with 2MASS photometry -by examining the location of the color-color locus for early (< K0) -main sequence stars. - -For each pixel (0.5 degree on a side), I select all objects with PS1 r -< 20 and detected JHK magnitudes, keeping only those with S/N in -the mean > 50 and standard deviations less than 0.05 magnitudes. I -then fit the stellar locus in g-r,r-i for the g-r range 0.2 to 1.0, -and keep only objects that fall within 0.05 of that (linear) stellar -locus fit.
- -I then fit the stellar locus with a line in each of the color-color diagrams -g-i,i-J; g-i,i-H; g-i,i-K. I measure the mean i-J color expected from -the fit for stars with g-i = 0.5. The figures below show the maps of -the i-J, i-H, and i-K offsets as well as the J-H and H-K offsets at -g-i = 0.5. The center of these maps is RA,DEC = 0,0, (east is left, -north is up). The pixels are 0.5 degrees on a side.
- -These maps show three main features. The Galactic Plane is quite -clear, and not surprising: this test is particularly sensitive to -reddening.
- -Several large scale patches are also visible (eg, the black patch near -RA ~ 150 deg). Disappointingly, these correspond to areas without -good ubercal ties -- in other words, these are regions in which the -data were obtained in non-photometric conditions. This shows the -limitation of using relative photometry to tie across individual -exposures. If the exposures have an extinction gradient, the -correction far from the photometrically tied region can drift from the -correct value. The largest region at RA ~ 150 matches a section with -poor i-band photometry and has a depth of roughly 0.1 magnitudes in -i-J. Assuming this is completely due to i-band errors, this -corresponds to about 0.06 magnitudes of drift to the center of this -region.
- -The third pattern is at a lower level of intensity: N-S strips with -roughly E-W bands. They are most noticable in K and H-K. These -appear to correspond well to the 2MASS scanning pattern, and have an -amplitude corresponding to about 0.02 - 0.04 magnitudes of offset in -K.
- -
-Map of the i-J color at g-i = 0.5. -
- -
-Map of the i-H color at g-i = 0.5. -
- -
-Map of the i-K color at g-i = 0.5. -
- -Combinations of the above maps can highlight any problems in 2MASS -which are driven by the color rather than the mean magnitudes. - -
-Map of the J-H color at g-i = 0.5. -
- -
-Map of the H-K color at g-i = 0.5. -
Index: /branches/eam_branches/ipp-20120905/dvodist/www-root/help.mkd =================================================================== --- /branches/eam_branches/ipp-20120905/dvodist/www-root/help.mkd (revision 34553) +++ /branches/eam_branches/ipp-20120905/dvodist/www-root/help.mkd (revision 34553) @@ -0,0 +1,14 @@ + + +# DVO Distribution Help + +These web pages contain the PS1 DVO databases, making it easy to +download entire databases with the 'wget' command. It is necessary to +include an authorized user and the password. + +Use a wget command on the directory of interest, eg: + + wget --user=ps1sc --password=(PASS) -r -np -nH http://dvodist.ipp.ifa.hawaii.edu/3pi.20120509 + +Ask your DRAVG representative if you need the password. + Index: anches/eam_branches/ipp-20120905/dvodist/www-root/help.php =================================================================== --- /branches/eam_branches/ipp-20120905/dvodist/www-root/help.php (revision 34552) +++ (revision ) @@ -1,107 +1,0 @@ - - -# DVO Distribution Help - -These web pages contain the PS1 DVO databases, making it easy to -download entire databases with the 'wget' command. It is necessary to -include an authorized user and the password. - -Use a wget command on the directory of interest, eg: - - wget --user=ps1sc --password=(PASS) -r -np -nH http://dvodist.ipp.ifa.hawaii.edu/3pi.20120509 - -Ask your DRAVG representative if you need the password. - -### Header 3 - -> This is a blockquote Lorem ipsum dolor sit amet, - consectetuer adipiscing elit. Aliquam hendrerit mi posuere lectus. - Vestibulum enim wisi, viverra nec, fringilla in, laoreet - -> more blockquote - -# Download - -* files - * indent list - * more indent - - indent 3 - - indent 4 - * indent 5 - code block -* more indent 2 -* three indent -* other things - -* This is a blockquote Lorem ipsum dolor sit amet, - consectetuer adipiscing elit. Aliquam hendrerit mi posuere lectus. - Vestibulum enim wisi, viverra nec, fringilla in, laoreet - - This is a blockquote Lorem ipsum dolor sit amet, - consectetuer adipiscing elit. Aliquam hendrerit mi posuere lectus. - Vestibulum enim wisi, viverra nec, fringilla in, laoreet - -* more blockquote - - - -[Markdown 1.0.1][dl] (18 KB) -- 17 Dec 2004 - -[dl]: http://daringfireball.net/projects/downloads/Markdown_1.0.1.zip - - -Introduction ------------- - -Markdown is a text-to-HTML conversion tool for web writers. Markdown -allows you to write using an easy-to-read, easy-to-write plain text -format, then convert it to structurally valid XHTML (or HTML). - -Thus, "Markdown" is two things: (1) a plain text formatting syntax; -and (2) a software tool, written in Perl, that converts the plain text -formatting to HTML. See the [Syntax][] page for details pertaining to -Markdown's formatting syntax. You can try it out, right now, using the -online [Dingus][]. - - [syntax]: /projects/markdown/syntax - [dingus]: /projects/markdown/dingus - -The overriding design goal for Markdown's formatting syntax is to make -it as readable as possible. The idea is that a Markdown-formatted -document should be publishable as-is, as plain text, without looking -like it's been marked up with tags or formatting instructions. While -Markdown's syntax has been influenced by several existing text-to-HTML -filters, the single biggest source of inspiration for Markdown's -syntax is the format of plain text email. - -The best way to get a feel for Markdown's formatting syntax is simply -to look at a Markdown-formatted document. For example, you can view -the Markdown source for the article text on this page here: - - -(You can use this '.text' suffix trick to view the Markdown source for -the content of each of the pages in this section, e.g. the -[Syntax][s_src] and [License][l_src] pages.) - - [s_src]: /projects/markdown/syntax.text - [l_src]: /projects/markdown/license.text - -Markdown is free software, available under a BSD-style open source -license. See the [License] [pl] page for more information. - - [pl]: /projects/markdown/license - - -Discussion List ---------------- - -I've set up a public [mailing list for discussion about Markdown] [ml]. -Any topic related to Markdown -- both its formatting syntax and -its software -- is fair game for discussion. Anyone who is interested -is welcome to join. - -It's my hope that the mailing list will lead to good ideas for future -improvements to Markdown. - - [ml]: http://six.pairlist.net/mailman/listinfo/markdown-discuss - Index: anches/eam_branches/ipp-20120905/dvodist/www-root/help.txt =================================================================== --- /branches/eam_branches/ipp-20120905/dvodist/www-root/help.txt (revision 34552) +++ (revision ) @@ -1,57 +1,0 @@ - - -

DVO Distribution Help

- -

These web pages contain the PS1 DVO databases, making it easy to -download entire databases with the 'wget' command. It is necessary to -include an authorized user and the password.

- -Use a wget command on the directory of interest, eg: - - wget --user=ps1sc --password=(PASS) -r -np -nH http://dvodist.ipp.ifa.hawaii.edu/3pi.20120509 - -Ask your DRAVG representative if you need the password. - -### Header 3 -> This is a blockquote -> more blockquote - -The overriding design goal for Markdown's formatting syntax is to make -it as readable as possible. The idea is that a Markdown-formatted -document should be publishable as-is, as plain text, without looking -like it's been marked up with tags or formatting instructions. While -Markdown's syntax has been influenced by several existing text-to-HTML -filters, the single biggest source of inspiration for Markdown's -syntax is the format of plain text email. - -The best way to get a feel for Markdown's formatting syntax is simply -to look at a Markdown-formatted document. For example, you can view -the Markdown source for the article text on this page here: - - -(You can use this '.text' suffix trick to view the Markdown source for -the content of each of the pages in this section, e.g. the -[Syntax][s_src] and [License][l_src] pages.) - - [s_src]: /projects/markdown/syntax.text - [l_src]: /projects/markdown/license.text - -Markdown is free software, available under a BSD-style open source -license. See the [License] [pl] page for more information. - - [pl]: /projects/markdown/license - - -Discussion List ---------------- - -I've set up a public [mailing list for discussion about Markdown] [ml]. -Any topic related to Markdown -- both its formatting syntax and -its software -- is fair game for discussion. Anyone who is interested -is welcome to join. - -It's my hope that the mailing list will lead to good ideas for future -improvements to Markdown. - - [ml]: http://six.pairlist.net/mailman/listinfo/markdown-discuss - Index: /branches/eam_branches/ipp-20120905/dvodist/www-root/index.mkd =================================================================== --- /branches/eam_branches/ipp-20120905/dvodist/www-root/index.mkd (revision 34553) +++ /branches/eam_branches/ipp-20120905/dvodist/www-root/index.mkd (revision 34553) @@ -0,0 +1,7 @@ + + +@ DVO Database : plain : title : Comment +@ 3pi.20120525 : dir : dir1 : DVO Database Released 2012.05.25, ubercal + relphot + relastro (pm + par) +@ # allsky.tables.20120513 : dir : dir2 : Summary Tables for allsky (FITS & CSV formats) +@ allsky.tables.20120602 : dir : dir2 : Summary Tables for allsky (FITS & CSV formats) +@ catdir.syn.test : dir : dir1 : Test DVO Database Index: anches/eam_branches/ipp-20120905/dvodist/www-root/index.php =================================================================== --- /branches/eam_branches/ipp-20120905/dvodist/www-root/index.php (revision 34552) +++ (revision ) @@ -1,63 +1,0 @@ - - -// generic proxy detection -// if ( $_SERVER['HTTP_X_FORWARDED_FOR'] -// || $_SERVER['HTTP_X_FORWARDED'] -// || $_SERVER['HTTP_FORWARDED_FOR'] -// || $_SERVER['HTTP_CLIENT_IP'] -// || $_SERVER['HTTP_VIA'] -// || in_array($_SERVER['REMOTE_PORT'], array(8080,80,6588,8000,3128,553,554)) -// || @fsockopen($_SERVER['REMOTE_ADDR'], 80, $errno, $errstr, 30)) -// { -// exit('Proxy detected'); -// } - -// list server info: -// $varlist = array ('SCRIPT_NAME', 'HTTP_X_FORWARDED_FOR', 'HTTP_X_FORWARDED', 'HTTP_FORWARDED_FOR', 'HTTP_CLIENT_IP', 'HTTP_VIA', 'REMOTE_ADDR'); -// -// foreach ($varlist as $name) { -// echo "$name : $_SERVER[$name]
\n"; -// } -// -// echo "get list
\n"; -// foreach ($_GET as $key => $value) { -// echo "$key : $value
\n"; -// } - Index: anches/eam_branches/ipp-20120905/dvodist/www-root/index.txt =================================================================== --- /branches/eam_branches/ipp-20120905/dvodist/www-root/index.txt (revision 34552) +++ (revision ) @@ -1,5 +1,0 @@ -DVO Database : plain : title : Comment -3pi.20120525 : dir : dir1 : DVO Database Released 2012.05.25, ubercal + relphot + relastro (pm + par) -# allsky.tables.20120513 : dir : dir2 : Summary Tables for allsky (FITS & CSV formats) -allsky.tables.20120602 : dir : dir2 : Summary Tables for allsky (FITS & CSV formats) -catdir.syn.test : dir : dir1 : Test DVO Database Index: /branches/eam_branches/ipp-20120905/dvodist/www-root/test.mkd =================================================================== --- /branches/eam_branches/ipp-20120905/dvodist/www-root/test.mkd (revision 34553) +++ /branches/eam_branches/ipp-20120905/dvodist/www-root/test.mkd (revision 34553) @@ -0,0 +1,106 @@ + + +# DVO Distribution Help + +These web pages contain the PS1 DVO databases, making it easy to +download entire databases with the 'wget' command. It is necessary to +include an authorized user and the password. + +@ DVO Database : plain : title : Comment +@ 3pi.20120525 : dir : dir1 : DVO Database Released 2012.05.25, ubercal + relphot + relastro (pm + par) +@ allsky.tables.20120602 : dir : dir2 : Summary Tables for allsky (FITS & CSV formats) +@ catdir.syn.test : dir : dir1 : Test DVO Database + +### Header 3 + +> This is a blockquote Lorem ipsum dolor sit amet, + consectetuer adipiscing elit. Aliquam hendrerit mi posuere lectus. + Vestibulum enim wisi, viverra nec, fringilla in, laoreet + +> more blockquote + +# Download + +* files + * indent list + * more indent + - indent 3 + - indent 4 + * indent 5 + code block +* more indent 2 +* three indent +* other things + +* This is a blockquote Lorem ipsum dolor sit amet, + consectetuer adipiscing elit. Aliquam hendrerit mi posuere lectus. + Vestibulum enim wisi, viverra nec, fringilla in, laoreet + + This is a blockquote Lorem ipsum dolor sit amet, + consectetuer adipiscing elit. Aliquam hendrerit mi posuere lectus. + Vestibulum enim wisi, viverra nec, fringilla in, laoreet + +* more blockquote + + + +[Markdown 1.0.1][dl] (18 KB) -- 17 Dec 2004 + +[dl]: http://daringfireball.net/projects/downloads/Markdown_1.0.1.zip + + +Introduction +------------ + +Markdown is a text-to-HTML conversion tool for web writers. Markdown +allows you to write using an easy-to-read, easy-to-write plain text +format, then convert it to structurally valid XHTML (or HTML). + +Thus, "Markdown" is two things: (1) a plain text formatting syntax; +and (2) a software tool, written in Perl, that converts the plain text +formatting to HTML. See the [Syntax][] page for details pertaining to +Markdown's formatting syntax. You can try it out, right now, using the +online [Dingus][]. + + [syntax]: /projects/markdown/syntax + [dingus]: /projects/markdown/dingus + +The overriding design goal for Markdown's formatting syntax is to make +it as readable as possible. The idea is that a Markdown-formatted +document should be publishable as-is, as plain text, without looking +like it's been marked up with tags or formatting instructions. While +Markdown's syntax has been influenced by several existing text-to-HTML +filters, the single biggest source of inspiration for Markdown's +syntax is the format of plain text email. + +The best way to get a feel for Markdown's formatting syntax is simply +to look at a Markdown-formatted document. For example, you can view +the Markdown source for the article text on this page here: + + +(You can use this '.text' suffix trick to view the Markdown source for +the content of each of the pages in this section, e.g. the +[Syntax][s_src] and [License][l_src] pages.) + + [s_src]: /projects/markdown/syntax.text + [l_src]: /projects/markdown/license.text + +Markdown is free software, available under a BSD-style open source +license. See the [License] [pl] page for more information. + + [pl]: /projects/markdown/license + + +Discussion List +--------------- + +I've set up a public [mailing list for discussion about Markdown] [ml]. +Any topic related to Markdown -- both its formatting syntax and +its software -- is fair game for discussion. Anyone who is interested +is welcome to join. + +It's my hope that the mailing list will lead to good ideas for future +improvements to Markdown. + + [ml]: http://six.pairlist.net/mailman/listinfo/markdown-discuss + Index: anches/eam_branches/ipp-20120905/dvodist/www-root/test.php =================================================================== --- /branches/eam_branches/ipp-20120905/dvodist/www-root/test.php (revision 34552) +++ (revision ) @@ -1,4 +1,0 @@ - - -non-php, non-html line - Index: anches/eam_branches/ipp-20120905/dvodist/www-root/test2.php =================================================================== --- /branches/eam_branches/ipp-20120905/dvodist/www-root/test2.php (revision 34552) +++ (revision ) @@ -1,54 +1,0 @@ - script: $script
\n"; - -do_markdown ($script); -echo " done script
\n"; - -menu_end(); -?> - -// generic proxy detection -// if ( $_SERVER['HTTP_X_FORWARDED_FOR'] -// || $_SERVER['HTTP_X_FORWARDED'] -// || $_SERVER['HTTP_FORWARDED_FOR'] -// || $_SERVER['HTTP_CLIENT_IP'] -// || $_SERVER['HTTP_VIA'] -// || in_array($_SERVER['REMOTE_PORT'], array(8080,80,6588,8000,3128,553,554)) -// || @fsockopen($_SERVER['REMOTE_ADDR'], 80, $errno, $errstr, 30)) -// { -// exit('Proxy detected'); -// } - -// list server info: -// $varlist = array ('SCRIPT_NAME', 'HTTP_X_FORWARDED_FOR', 'HTTP_X_FORWARDED', 'HTTP_FORWARDED_FOR', 'HTTP_CLIENT_IP', 'HTTP_VIA', 'REMOTE_ADDR'); -// -// foreach ($varlist as $name) { -// echo "$name : $_SERVER[$name]
\n"; -// } -// -// echo "get list
\n"; -// foreach ($_GET as $key => $value) { -// echo "$key : $value
\n"; -// } -