Result for 1FF2FDC0B3FA9ADDCD57F2F8D1BB8BB31E3FBCD0

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.4.9/hawki_step_subtract_bkg.la
FileSize1048
MD51147E98CE5B1E009972CFE657A2EB02E
SHA-11FF2FDC0B3FA9ADDCD57F2F8D1BB8BB31E3FBCD0
SHA-2566C93AFE48BA6AB7637F0E1305C7AF753E3CD4FC38B22E433E61C5CF0926A0869
SSDEEP24:1eSG5WJEOiw5xIY+Ahmfvi4HvD2NGDe5/Aj7:3G5WJc2xIY1hmfKQLcA3
TLSHT15411F03A839A9125BBD4065D8ADF703E429948790B2A5F5053C798DF128B42B1557E23
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
FileSize448916
MD515510D708B30FD3447AB413D215ADBF9
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
PackageVersion2.4.9+dfsg-1
SHA-1617C0F0EC2D7EA25558AFB56BCCB07552925D079
SHA-2569202A8FDCCDB13C2F3ACC2DC6A1BDFA123AD464F752FF6FE14DB8FC365CA9AE6