Result for 19A9C6D12786FAB7E8FAC978E799818917D9536B

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-1.8.14/hawki_step_detect_obj.la
FileSize1037
MD524BD5D25DF9E6885ABE9A3D26A229D27
SHA-119A9C6D12786FAB7E8FAC978E799818917D9536B
SHA-256CF54672226BE5FBF090E9415C6012C8FD078AC4D63055ED9DA12A856F4A3506F
SSDEEP24:PeShuWJU2icBxIK+Ahmfvi45vD2NGDe5/Aj8:l8WJUzcBxIK1hmfKqLcA4
TLSHT1EB112C3FD3DE313AAFD416558ACF303E42C9883A07322E4063C785DB224B80911A7E2B
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
FileSize225126
MD5CF9FA4C7CE9F844C3D7E55B9BA5844E5
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-1568F0F9D3C91E620D966913560B7CBEA3960D69E
SHA-256B4D26EE3EA7C0A8629B579288D4950615ED647084080BEA567F7948A39315B0B