Result for 1D81B6B7E20F887EF4E167C6E954F44996457AA9

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.4.9/hawki_twilight_flat_combine.so
FileSize23268
MD58A8AFE491C6569BC7F630C5921DAF796
SHA-11D81B6B7E20F887EF4E167C6E954F44996457AA9
SHA-256E1716F5F90098BF619B6F38178A4BB86CC05BD9B7444AAD79AB9D1E03AB36B9A
SSDEEP384:6uq0M6PL7UmbQdtZuphscJjk3D2l6wwiB+:6t0M6hQPwEcJk3Kl6wQ
TLSHT103A2B6DBAA3A6D57C895A13C540F8F02463081D5E24E4B2335DC48605E91B9D8FBFFEA
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
FileSize448916
MD515510D708B30FD3447AB413D215ADBF9
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
PackageVersion2.4.9+dfsg-1
SHA-1617C0F0EC2D7EA25558AFB56BCCB07552925D079
SHA-2569202A8FDCCDB13C2F3ACC2DC6A1BDFA123AD464F752FF6FE14DB8FC365CA9AE6