aboutsummaryrefslogtreecommitdiff
path: root/gnu/packages/avahi.scm
diff options
context:
space:
mode:
authorSharlatan Hellseher <sharlatanus@gmail.com>2023-05-30 20:58:37 +0100
committerEfraim Flashner <efraim@flashner.co.il>2023-06-14 14:52:22 +0300
commit308bee5f000703f063f5fbccd1c439e8c905a09c (patch)
tree1983217669f9cc0577ac76fe1f620ca9677db1c7 /gnu/packages/avahi.scm
parent95c1e5121a1238c745860d7a7033bdb30c91b7cf (diff)
downloadguix-308bee5f000703f063f5fbccd1c439e8c905a09c.tar.gz
guix-308bee5f000703f063f5fbccd1c439e8c905a09c.zip
gnu: Add python-tweakwcs.
* gnu/packages/astronomy.scm (python-tweakwcs): New variable. Signed-off-by: Efraim Flashner <efraim@flashner.co.il>
Diffstat (limited to 'gnu/packages/avahi.scm')
0 files changed, 0 insertions, 0 deletions
his implies the use new image generation mechanisms. - Raw disk images: images of partitions are created using tools such as mke2fs and mkdosfs depending on the partition file-system type. The partition images are then assembled into a final image using genimage. - ISO9660 images: the ISO root directory is populated within the store. GNU xorriso is then called on that directory, in the exact same way as this is done in (gnu build vm) module. Those mechanisms are built upon the new (gnu image) module. * gnu/image.scm: New file. * gnu/system/image.scm: New file. * gnu/build/image: New file. * gnu/local.mk: Add them. * gnu/system/vm.scm (system-disk-image): Rename to system-disk-image-in-vm. * gnu/ci.scm (qemu-jobs): Adapt to new API. * gnu/tests/install.scm (run-install): Ditto. * guix/scripts/system.scm (system-derivation-for-action): Ditto. Mathieu Othacehe