Result for 0C0477D7AEAD4852FEB2697D27270E55453C6DAE

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-1.8.21/hawki_cal_dark.so
FileSize18688
MD5636AB618171FEB6B4E0FCB009E58FCB9
SHA-10C0477D7AEAD4852FEB2697D27270E55453C6DAE
SHA-25606B90C13DD13FB10DD089F2C9F343CF6C0A39682F3B7A7B5EF4F378631F752E1
SSDEEP384:JUUJNhh+hPa8ncTnE4KszfxrIRm+hOz7Ll:FJNhka8WE4Ksb5mIh
TLSHT12582C6CA7256C937C895B5BA34AF9E53119941E8DD68CBC33ACC4C900601B7FCA61F5B
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
FileSize184482
MD52A9ACD5A8E062002F64B214A3B6B00FF
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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.21+dfsg-1build1
SHA-10600C46860A116FB748364715FA18ECAE1EBA0AC
SHA-2562F942E0CDB1F7E91576879FA81FC9A13FD3C56B3C0AFD51DFBAD967AC412F017