Result for 17B4E1BB8AF493BEB9E994D995AE7C363D932FDB

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-1.8.18/hawki_step_basic_calib.so
FileSize14188
MD5CDCD5DE2BA7E2F608D1C69CF30B94602
SHA-117B4E1BB8AF493BEB9E994D995AE7C363D932FDB
SHA-256D00FA4972F20FF176893DED57BA71354AB0793624540F98D5C9AE8080048A68B
SSDEEP192:zeU8poDZFvI/K2WxSX3Qgc2EwjHtltlA9E7m6sX+TOuA+7nhiVbID7OiQSwiAopI:3DPv2FggTjNltlD7mZummiGS652wnIW
TLSHT13D52A68BF7D2CEB1D7C221B40457472EA6304870EA2BCFD3794C2658F0A669C5C6336A
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
FileSize221550
MD57CA8C8F751AC49CD58D14D76DA00B8B5
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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.18+dfsg-4
SHA-1BA8CEACF21DD0E05B10A5C496CD082AD9365547E
SHA-256949029E1EA39C0BBA2A85405157D2B6E9179DF9FAFA1E585C720E7DE40B0B7D9