Result for 0F050FA28CCE10F9C7D56E4309E19E4132F85331

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-1.8.14/hawki_step_detect_obj.so
FileSize18592
MD56C2A3B0212051689893864BC27A569DC
SHA-10F050FA28CCE10F9C7D56E4309E19E4132F85331
SHA-2568C6A937DB27569368561BD52F166E5F3B604B9B11D7AD3EE50D0442C78B2CC39
SSDEEP192:hB8prvxJgZg9lvA1MnLRmdeFwUekKORQAII+qffD7wSG7sOjHDmxLrsQy:hYxJ39RLOe95tXPzG7mg
TLSHT15E82F7CA66279957D4D4233BC47F0E158B19C6E9B3588F0B21CE54646D82BECC232EE7
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
FileSize220538
MD531D6CCA4666BB9CF91D70F85DF43457A
PackageDescriptionESO data reduction pipeline for HAWK-I 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
PackageVersion1.8.14+dfsg-2
SHA-1260CAF94A6F4CE159F52A9364FA6A81610CC3619
SHA-256A2E741FAF01616FAD42B2B5AE51B4AB0CAF93A19207EB47B6D178189F6DF71C3