Result for 03D080ECF7F8F76D491C06F48E3E53A8D7B49E1E

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.4.9/hawki_step_refine_offsets.so
FileSize14688
MD5EB92B0D2871CA90B4E4A6C85ED2F47A0
SHA-103D080ECF7F8F76D491C06F48E3E53A8D7B49E1E
SHA-2563F7D9FF727ADF2BEAEBD1B10953286CF6EF3D738450A95807296B797474DA279
SSDEEP192:oiBq78jnXAl6hfFz6/CXr35ntl1Kh/Eosv+BUbxHeexW9xjfLxyR3L8QL:oiU4XAl6hdzQCXFtPB7+BWfW3DL0Rb
TLSHT1B26282DBADF74977C9D06B3D501B0E60412485DAF20B4B13669E51E01F026ECEE6AECB
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