Install this package:
emerge -a dev-python/pymoc
If the package is masked, you can unmask it using the autounmask tool or standard emerge options:
autounmask dev-python/pymoc
Or alternatively:
emerge --autounmask-write -a dev-python/pymoc
| Version | EAPI | Keywords | Slot |
|---|---|---|---|
| 0.5.2 | 8 | ~amd64 ~x86 | 0 |
<pkgmetadata> <maintainer type="project"> <email>sci-astronomy@gentoo.org</email> <name>Gentoo Astronomy Project</name> </maintainer> <maintainer type="person"> <email>universebenzene@sina.com</email> <name>Astro Benzene</name> </maintainer> <longdescription lang="en"> Frequently astronomical survey catalogues or images are sparse and cover only a small part of the sky. In a Multi-Order Coverage map the extent of data in a particular dataset is cached as a pre-calculated mask image. The hierarchical nature enables fast boolean operations in image space, without needing to perform complex geometrical calculations. Services such as VizieR generally offer the MOC masks, allowing a faster experience in graphical applications such as Aladin, or for researchers quickly needing to locate which datasets may contain overlapping coverage. The MOC mask image itself is tessellated and stored in NASA HealPix format, encoded inside a FITS image container. Using the HealPix (Hierarchical Equal Area isoLatitude Pixelization) tessellation method ensures that more precision (pixels) in the mask are available when describing complex shapes such as approximating survey or polygon edges, while only needing to store a single big cell/pixel when an coverage is either completely inside, or outside of the mask. Catalogues can be rendered on the mask as circles. </longdescription> <upstream> <remote-id type="pypi">pymoc</remote-id> <remote-id type="github">grahambell/pymoc</remote-id> </upstream> </pkgmetadata>
| Type | File | Size | Versions |
|---|
| Type | File | Size |
|---|---|---|
| DIST | pymoc-0.5.2.tar.gz | 33741 bytes |
| EBUILD | pymoc-0.5.2.ebuild | 636 bytes |
| MISC | metadata.xml | 1681 bytes |