Result for 077B7E75955A08AB873901C55220AE46561A88FD

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_util_gendist.la
FileSize1017
MD5D913A20B183E06598A3D565F09738CC8
SHA-1077B7E75955A08AB873901C55220AE46561A88FD
SHA-2563F946E85C0EF2A5846307A5AC51E38B84BCD35AFD7370FC26536C70FF5FF09B6
SSDEEP24:KXeSGsWJYZiirr2xIY+Ahmfvi48d1vD2NGDe5/v0:K9GsWJYAirr2xIY1hmfKvdpLcv0
TLSHT18C11053E839E612DABD809C5968E353F438D4038072D0E5952F6E5DB154F46D1157F32
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
FileSize470896
MD504E6CDD5BC92409B9B8ACCDBDA45598D
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
PackageVersion2.4.3+dfsg-1
SHA-11AB820B4CF5A53A38486A13C3E51A928A2FE694D
SHA-256F4E93FD2283238717114016AB9CA5CDBD1B98D37FDA6784152CB5222AD3B3867