$B$D$C$F$b!"Hs8x3+$N$rJL$K$D$1$F$$$k$o$1$G$O$J$$!#(B
Copyright 1999- Jun Makino
2004/02 2004/01 2003/12 2003/11 2003/10 2003/09 2003/08 2003/07 2003/06 2003/05 2003/04 2003/03 2003/02 2003/01$BEvLL$NM=Dj(B
$B!V4m$J$$!W!VE>$s$@!W$J$I$N6l>p$d$40U8+$,B?$/4s$;$i$l$F$$$^$9!#(B$B$N$K0BA4$G$"$k$H$$$&$N$O$A$g$C$HL5M}$,$J$$$+$H$$$&5$$b$7$J$/$b$J$$$h$&(B $B$J!#(B
$B$3$N?^$N>e$N$_$?$$$J46$8!#2<$N$,IaDL$N!#$3$N@_7W$@$H!"(B
#diff -C0 extconf.rb extconf.rb~
*** extconf.rb 2004-03-26 16:25:19.000000000 +0900
--- extconf.rb~ 2001-12-01 14:24:58.000000000 +0900
***************
*** 23 ****
- print "Under cygwin\n"
--- 22 ----
***************
*** 47,48 ****
! (have_library(gl_libname) || have_library("Mesa"+gl_libname)) &&
! (have_library(glu_libname) || have_library("Mesa"+glu_libname)) &&
--- 46,47 ----
! (have_library(gl_libname, nil) || have_library("Mesa"+gl_libname, nil)) &&
! (have_library(glu_libname, nil) || have_library("Mesa"+glu_libname, nil)) &&
***************
*** 68 ****
! have_library(glut_libname) &&
--- 67 ----
! have_library(glut_libname, nil) &&
#diff -C0 glut.c glut.c~
*** glut.c 2004-03-26 16:37:28.000000000 +0900
--- glut.c~ 2000-01-07 01:37:43.000000000 +0900
***************
*** 18 ****
! glut_ ## _funcname (obj,arg1) \
--- 18 ----
! glut_ ## _funcname ## (obj,arg1) \
***************
*** 28 ****
! glut ## _funcname (glut_ ## _funcname ## Callback); \
--- 28 ----
! glut ## _funcname ## (glut_ ## _funcname ## Callback); \
glut.c $B$O(B gcc 3.3.1 $B$G$OJ86g$r$$$&!#(BLinux $B>e$N(B 2.95.3 $B$G$O$b$A$m$sJ86g(B
$B$$$o$J$$$7!"(B 3.3.2 $B$d(B 3.2 $B$G$OJ86g$@$1$G%3%s%Q%$%k$9$k$_$?$$$K8+$($k$s(B
$B$@$1$I!"(BCygwin $B$N(B 3.3.1 $B$G$O%U%'%$%k$7$?$h$&$J!#2?8N$@!)(B
$B$"!"(B Ruby/OpenGL $B$N%Z!<%8$rNI$/$_$k$H!"(B RAA $B$N%Z!<%8(B$B$G%@%&%s(B
$B%m!<%I$,;X$7$F$k%U%!%$%k$,$*$b$$$-$j8E$$!"!"!":n
408 2:16 cd rd2latex/doc 412 2:17 cd /usr/local/lib/ruby/site_ruby/1.8/rd/ 425 2:19 copy $old/../lib/rd/* . 427 2:19 sudo cp -rpi $old/../lib/rd/* . 428 2:19 cd- 430 2:19 rd2 -r rd/rd2latex-lib rd2latex.rd$B$H!"$$$-$J$j(B rd2 $B$,(B latex $B%=!<%9$rEG$/!#7k9=AGE(!#(B
206 18:25 tar xvzf glut*z
207 18:25 cd glut-3.7
208 18:25 cd linux
211 18:26 mv ../Glut.cf Glut.cf.orig
212 18:26 copy Glut.cf ..
213 18:26 cd ..
214 18:26 copy Glut.cf Glut.cf.linux.org
218 18:29 chmod +w Glut.cf
219 18:29 locate libGL
$B$3$3$G(B Glut.cf $B$rJT=8(B
diff -C0 Glut.cf.linux.org Glut.cf
*** Glut.cf.linux.org 1998-08-08 09:13:27.000000000 +0900
--- Glut.cf 2004-03-21 18:31:05.000000000 +0900
***************
*** 94,95 ****
! OPENGL = $(TOP)/../lib/libMesaGL.so /* modified per Mesa README PFM 6/31/96 */
! GLU = $(TOP)/../lib/libMesaGLU.so /* modified per Mesa README PFM 6/31/96 */
--- 94,103 ----
!
! # Change to remove Mesa references --- JM
! #OPENGL = $(TOP)/../lib/libMesaGL.so /* modified per Mesa README PFM 6/31/96 */
! #GLU = $(TOP)/../lib/libMesaGLU.so /* modified per Mesa README PFM 6/31/96 */
!
! #OPENGL = /usr/X11R6/lib/libGL.so /* modified per Mesa README PFM 6/31/96 */
! #GLU = /usr/X11R6/lib/libGLU.so /* modified per Mesa README PFM 6/31/96 */
! OPENGL = -lGL
! GLU = -lGLU
!
220 18:31 ./mkmkfiles.imake
221 18:32 cd lib/glut
223 18:32 copy ../../linux/Makefile .
224 18:32 mv Makefile Makefile.old
225 18:32 copy ../../linux/Makefile .
228 18:33 chmod +w Makefile
Makefile $B$rJT=8(B
diff -C0 Makefile~ Makefile
*** Makefile~ 1998-08-08 09:13:27.000000000 +0900
--- Makefile 2004-03-21 18:34:03.000000000 +0900
***************
*** 486,487 ****
! OPENGL = $(TOP)/../lib/libMesaGL.so
! GLU = $(TOP)/../lib/libMesaGLU.so
--- 486,489 ----
! #OPENGL = $(TOP)/../lib/libMesaGL.so
! #GLU = $(TOP)/../lib/libMesaGLU.so
! OPENGL = -lGL
! GLU = -lGLU
229 18:34 make
233 18:35 ln -s libglut.so.3.7 libglut.so
234 18:35 ln -s libglut.so.3.7 libglut.so.3
235 18:35 sudo cp -d libglut.* /usr/local/lib
236 18:35 ls /usr/local/lib/*gl*
237 18:35 cd ../gle
238 18:35 make
239 18:36 gcc -shared -o libgle.so.3.7 *.o
240 18:36 ln -s libgle.so.3.7 libgle.so
241 18:36 ln -s libgle.so.3.7 libgle.so.3
242 18:36 sudo cp -d libgle.* /usr/local/lib
243 18:36 cd ..
244 18:36 cd mui
246 18:36 make
247 18:36 gcc -shared -o libmui.so.3.7 *.o
248 18:36 ln -s libmui.so.3.7 libmui.so
249 18:36 ln -s libmui.so.3.7 libmui.so.3
250 18:36 sudo cp -d libmui.* /usr/local/lib
251 18:37 ldconfig
252 18:37 /sbin/ldconfig
253 18:37 cd ../../progs/demos/ideas
257 18:39 make
258 18:39 ./ideas
$B:G8e$O%G%b%W%m%0%i%`$NPlanets To Cosmology: Essential Science In Hubble's Final Years 3 - 6 May, 2004 Space Telescope Science Institute 3700 San Martin Drive Baltimore, Maryland 21218Dear Colleague,The upcoming STScI May Symposium will take place May 3-6, 2004, with registration and a reception on May 2, 2004. The Symposium will concentrate on the most recent science accomplished by HST and other observatories and potential future advances. A broad range of topics will be covered, with sessions devoted to: Planets (both in the solar system and extrasolar); Star Formation (in the Local Group, in clusters); Black Holes (at galaxy centers, potential existence in globular clusters); the ISM and the IGM (the baryon content, feedback); Galaxy Formation and Evolution (mass assembly, morphological evolution); Cosmology (the nature of dark energy, high-z supernovae, cosmological parameters). In addition, a Panel will discuss suggestions for the selection process for future HST observations.
The program is composed primarily of invited talks, with a small number of contributed talks, and a panel discussion. If you intend to present a poster, please indicate so on the registration form. Please take note of the requirements for the poster session.
The Provisional PROGRAM is enclosed below. We strongly encourage you to register as soon as possible.
Http://webst.stsci.edu/sd/Planets_to_Cosmology/index.html
Hoping to see you on Baltimore,
The Organizing Committee.
Announcement: Making Waves with Intermediate-Mass Black Holes Center for Gravitational Wave Physics Penn State University 20-22 May, 2004 To register and for more details: http://cgwp.gravity.psu.edu/events/IMBH/imbh.shtml .AN Overview: Over the last few years, X-ray and optical observations have hinted at the existence of black holes in a new mass range: hundreds to thousands of solar masses, the so-called intermediate-mass black holes. Many of the best candidates appear associated with dense stellar clusters, where there are many interactions that could generate detectable gravitational radiation. Indeed, these are one of the rare classes of sources for which rigorous proof of their existence may require detection of gravitational waves. This focus session's goal is to explore the interplay between the astrophysics and the gravitational wave physics of intermediate-mass black holes, from cosmology and cluster dynamics to probes of the Kerr spacetime. The framing questions are: What is the current evidence for the existence of intermediate-mass black holes and their environments, and what are the scenarios in which they emit gravitational radiation? What are the proposed mechanisms for the formation of intermediate-mass black holes, and what implications do these have for gravitational wave observations? What information about astrophysics or fundamental physics could be derived from observations of gravitational radiation from intermediate-mass black holes? What realistic additions or modifications to detectors would optimize the search for gravitational waves from intermediate-mass black holes? Scientific Organizing Committee: Monica Colpi (University of Milano Bicocca) Lee Samuel Finn (Penn State) Karl Gebhardt (University of Texas) Avi Loeb (Harvard University) Cole Miller (University of Maryland) Fred Rasio (Northwestern University)$B$3$N%[%F%k$O%M%C%H%o!<%/$,Mh$F$J$$$+$i(B2$BEY$H$$$-$?$/$J$$!#(B
$B%+%a%i(B $B$,$J$+$J$+5$0c$$$8$_$F$$$FAGE(!#$=$3$^$G$7$F(B drift scan $B$9$k$N$+!)(B $B$H$$$&5$$b$9$k$1$I!#(B
252 20:26 tar tvzf subversion-1.0.1.tar.gz
253 20:26 tar xvzf subversion-1.0.1.tar.gz
254 20:26 cd subversion-1.0.1
255 20:26 dir
256 20:26 cat README
257 20:27 perl -v
258 20:28 ./configure --enable-maintainer-mode
259 20:29 make
$B$H$9$k$H(B Python $B$,$I$&$3$&$H$$$&%(%i!<$,$G$k$N$G!"(B INSTALL $B$r8+$k$H(B
Python 2.0 $B0J>e$,$$$k$H$N$3$H!#$G!"(B Python 2.3.3 $B$rMn$H$7$F(B
configure; make $B$9$k$H(B ld $B$,Ff$J%(%i!<$r=P$9!#(B ld $B$r(Brpm $B$G(B 2.14 $B$K(B
$B$"$2$F$_$h$&$H$9$k$H!"!"!"(B glibc2.3 $B$,$$$k$H8@$o$l$k!#(B libc2.3.2
$B$r%3%s%Q%$%k$9$k$K$O?7$7$$(B binutils $B$,$$$k$i$7$$!#$"$l(B?
578 0:07 tar xvzf binutils-2.11.2.tar.gz
579 0:08 cd binutils-2.11.2
580 0:08 configure ; make
581 0:10 setenv CC /usr/bin/gcc
582 0:10 configure
583 0:11 make
584 0:12 make clean
585 0:12 make
586 0:14 cd ../binutils-2.12.1
587 0:14 cd ../binutils-2.12.
588 0:14 cd ../binutils-2.12
589 0:14 make clean
590 0:14 configure
591 0:15 make
592 0:16 sudo make install
2.12 $B$K$O>e$,$C$?!#(B
2.14 $B$K!#$3$l$O(B gcc-3.3.2 $B$G!#(B
608 0:18 cd binutils-2.14
609 0:18 make
610 0:18 make clean
611 0:18 make
612 0:21 sudo make install
$B7k6I(B glibc $B$O$=$N$^$^!#(B
Python-2.3.3 $B$r$b$&0lEY(B
623 0:22 cd Python-2.3.3
624 0:22 unsetenv CC
625 0:22 configure
626 0:23 make
627 0:25 make install
628 0:25 sudo make install
$B$3$l$O<:GT(B
640 0:27 sudo csh
$B$3$N$"$H(B make install $B$O@.8y(B
subversion 1.0.1 $B$KLa$C$F(B configure $B$9$k$H!"(B
Berkeley DB 4.0.x$B0J>e$,$$$k(B
$B$H$+8@$o$l$k$N$G$3$l$O(B 4.1.25 $B$r$R$m$C$F$-$F(B setenv CC /usr/bin/gcc
(2.95.3) $B$G(B configure ; make ; sudo make install
$B$5$i$K(B 4.2.52 $B$K$7$?$1$I$3$l$OB?J,JL$K0UL#$O$J$$!#!"LdBj$O!"(B configure
$B$,2?8N$+(Bdb2 $B$r;H$*$&$H$9$k$3$H$G!"$H$j$"$($:(B
diff -C0 configure~ configure
*** configure~ 1970-03-04 15:27:45.000000000 +0900
--- configure 2004-03-16 02:05:39.000000000 +0900
***************
*** 9124 ****
--- 9125,9126 ----
+ echo svn_apu_bdb_lib is $svn_apu_bdb_lib > aho
+ svn_apu_bdb_lib=-ldb
***************
$B$D$^$j!"(B configure $B$N$[$&$r$$$8$C$F2sHr!#$5$i$K(B python2 $B$,(B vine $B$G$O4{(B
$B$K$"$C$F0c$&$H$3$m$r$5$7$F$$$F!"%X%C%@%U%!%$%k$,$J$$$H$+$"$C$?$N$G(B
ln -s /usr/local/bin/python python2
$B$H$+$9$k!#$3$l$G(B
./configure --enable-maintainer-mode --with-berkeley-db=/usr/local/BerkeleyDB.4.2
857 2:25 make
$B$,DL$k$h$&$K$J$k!#$U$&!#$"$H!"(B autoconf $B$H$+(B libtools $B$H$+$$$l$?$1$I!"(B
$BB?J,4X78$J$$$s$8$c$J$$$+$J!#(B
$B$d$O$jE7J83X@l96$NF~;n$N%7%9%F%`$O$o$+$j$K$/$$$H$$$&OC!#(B
$B$=$b$=$bLdBj$NH/C<$,(B $B!V$X%?%l$J%&%'%V!&%G%6%$%J!<$O8D?ML>!"4k6HL>$r=P$7$F%&%'%VH/?.$9$k$J!W(B $B$H$$$&$B$H$$$&$N$OKM$O$"$s$^$j;?@.$G$O$J$/$F!"FAJ];a$NB?J,$b$C$H$b4pK\E*$JpJsH/?.$9$k$J!W(B $B$H0l5$$K0lHL2=$r$7$?$H$3$m$K$"$k!#(B
$B$G!"KM$O$=$N@N$H$"$k$H$3$m$G!"@lLg2H$,<+J,$N@lLgJ,Ln$K$D$$$FHs@lLg2H$K(B
$BBP$7$FH/8@$9$k;~$K$O!"8@$&$[$&$K$O<+3P$,$J$/$F$bHs@lLg2H$NB&$G$O!V@lLg(B
$B2H$NH/8@!W$H$7$F8+$k$s$@$+$i$"$s$^$j$$$$2C8:$J$3$H$O$$$&$J!"$_$?$$$J
$BE7J83X@l96$NF~;n$N%7%9%F%`$O$o$+$j$K$/$$$H$$$&OC!#$J$s$+$b$&$A$g$C$H0c(B
$B$&OC$b$7$?$+$J!#(B
$B?'!9Fq$7$$OC!#(B
4$B7n$+$i$OM}8&$G$*$D$H$a!#(B
Subject: PostDoc Position Available From: Walter DehnenWalter $B$O(B Lecturer $B$K$J$C$?$N$+!#$[$*!#(BDate: Wed, 3 Mar 2004 12:45:55 +0000 (GMT) Dear Colleague, A PostDoctoral position (for up to 3 years) is available for working with me on Galactic structure and dynamics, see (also posted at AAS) http://www.le.ac.uk/personnel/jobs/r0643.html for details. I would be grateful if you could bring this to the attention of suitable candidates, including PhD students working in their final year on galactic dynamics. The closing date for applications is 31st March 2004. Those interested should contact me informally. A permanent faculty position (lectureship) is available as well (same closing date), for details see http://www.le.ac.uk/personnel/jobs/a0671.html With best wishes, Walter Dehnen.
$B$^$"!"$I$&$;$=$&$$$&2q
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$B7k6I%9%T%s7O$N?6$kIq$$$C$F(B 2D $B$H(B 3D $B$GA4A30c$&$H$$$&$3$H$_$?$$$@$+$i!"(B
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2004/3/1-5
IAU Symposium No. 222 - The Interplay among Black Holes, Stars and ISM
in Galactic Nuclei
$B$$$+$J$+$C$?!#$4$a$s$J$5$$!#(B
th visit since Apr 1st, 1999.