Result for 122602FFD3A32C98CC257FB5220C2F415F158BDD

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.4.11/hawki_step_detect_obj.so
FileSize67972
MD5B24A1E975E2C236CEBC312895B03878B
SHA-1122602FFD3A32C98CC257FB5220C2F415F158BDD
SHA-256EF814ABC50166C23043CA08F2C4204B8044033376D7AF7EDA49B3DFD6ABD8303
SSDEEP192:AS3q8lZxNPjzKBA5XnRxnnR47uA9e7x6mIgIh0gBcOjHDaUoG75hj2rLrsQX:ASlxNPKBAlRlR4j9qNIh0gE1G7DCf
TLSHT11A6373CB73775BD7C0D4AAB9D4CB0F249716C5D993278F932D8C4A701E816E88A21B87
hashlookup:parent-total1
hashlookup:trust55

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Parents (Total: 1)

The searched file hash is included in 1 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize451432
MD5806CB6A07D053F721A8E675196114EB6
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.4.11+dfsg-1
SHA-1D4EE6BE1F295CE3F05E675E4F234B3A20BF3B199
SHA-256E2F48D24F4D2E931655F871957B4718228B438460887A47BEAC55B6C6D323744