Result for 054072D878386C090756FD7DB9A7EE6D9C15F4DB

Query result

Key Value
FileName./usr/lib/mips-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_cal_distortion.so
FileSize27372
MD59CF299C5E0A404207E230952A5811388
SHA-1054072D878386C090756FD7DB9A7EE6D9C15F4DB
SHA-25632E394E686A869FADD3E0729AB225ABD0082DBF94D3F3E4D6B641BB94CFB1E42
SSDEEP384:kBU08zJ8swQ74q6zms84mHX6Y0eJ3W3pXHkQ+noM0YPaHQXDdaeY+KSUe5hsc6D:kqzJ8swQ7z7H6eOonAiawXkIUr
TLSHT193C2535F1350CF5DF0E3C3BCB817C9A110B0A0626ACC4663D87DF545AA8CA59E93BA66
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
FileSize226012
MD54C289725D3042772C3CC4229546F32DC
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
PackageVersion1.8.21+dfsg-1
SHA-1889A99B4EFD1D9875279122129BC03E6D652C846
SHA-2563E3320066BBF6E79776FAB1ECD889581BBED37D5A340ABF0247820338B9C6E8C