Commit graph

6 commits

Author SHA1 Message Date
Joe Marcus Clarke
4acc6fb2a4 Presenting GNOME 2.20.1 and all related works for FreeBSD. The official
GNOME 2.20 release notes can be found at
http://www.gnome.org/start/2.20/notes/en/ .  Beyond that, this update
includes the new GIMP 2.4 (courtesy of ahze).

The GNOME 2.20 update also includes a huge change in the FreeBSD GNOME
hierarchy.  We are now using the more standard DATADIR of ${PREFIX}/share
rather than ${PREFIX}/share/gnome. The result is that fewer patches and
hacks are needed to port GNOME components to FreeBSD.  This will mean some
user changes may be required, so be sure to read /usr/ports/UPDATING for
more details.

This release and the things we accomplished in it would not have been
possible without mezz's crazy idea to collapse DATADIR, and his persistence
to make it happen successfully.  Ahze and pav also deserve thanks for
their work on porting modules and testing the whole ball of wax on
pointyhat (respectively).

The FreeBSD GNOME team would also like to thank our various testers and
contributors:

Yasuda Keisuke
Frank Jahnke
Pawel Worach
Brian Gruber
Franz Klammer
Yuri Pankov
Nick Barkas
Cristian KLEIN
Tony Maher
Scot Hetzel
Martin Matuska (mm)
Benoit Dejean
Martin Wilke (miwi)
(And anyone else I may have missed)

PRs fixed in this release:

111272, 113470, 115995, 116338
2007-10-24 23:37:25 +00:00
Andrew Pantyukhin
ad3572428a - Update to 1.61
- Minor fixes
2007-06-12 17:00:56 +00:00
Pav Lucistnik
ef906a1401 - Update to 1.44
PR:		ports/90189
Submitted by:	KATO Tsuguru <tkato432@yahoo.com>
2005-12-11 15:15:14 +00:00
Kirill Ponomarev
a2bf054052 - Update to version 1.34
PR:		59327
Submitted by:	Ports Fury
2003-11-16 14:17:23 +00:00
Daichi GOTO
9a914ceab4 update astro/nightfall: 1.1 --> 1.32
PR:		53336
Submitted by:	KATO Tsuguru <tkato@prontomail.com>
2003-07-01 11:47:08 +00:00
Kris Kennaway
91aae0c977 Add nightfall-1.1
Nghtfall can produce animated views of eclipsing binary stars,
calculate synthetic lightcurves and radial velocity curves.
Eventually it can determine the best-fit model for a given set
of observational data of an eclipsing binary star system.

Submitted by:	Christian Brueffer <chris@unixpages.org>
PR:		ports/35193
2002-05-25 10:48:46 +00:00