Result for 02A8FA772B36EB4E76F7255A9E92A9BF8B4AED0E

Query result

Key Value
FileName./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-2.4.8/hawki_dark_combine.so
FileSize27648
MD5F9B23A3F2D05B0FDE21F7475316EDC7B
SHA-102A8FA772B36EB4E76F7255A9E92A9BF8B4AED0E
SHA-2567CA981BAE5E9E1B84324CD8F404EEBC8BE724E8615356ADD17C0218C638D4CBC
SSDEEP768:Wwu4AdoAgw0wSNTyYuiTEBEQ2xrOQHMi/kktuiBE+9L26g4CHy3vDrf4jXVz+fqI:UdoAgw0wSNTyYuiTEBEQ2xrZHMi/kktM
TLSHT1E4C2A49BAF150E06C0C2DC700C9FD52291BE4E5DA1A8BB43F5ADED841602E4C2DBBA5D
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
FileSize451824
MD51F48F63051D9F44902CAF24A014F7EA7
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
PackageVersion2.4.8+dfsg-4
SHA-11F8850C8DF01377F7D9588E80BA2C9DB502D4044
SHA-2560A8C64809D35D4085A35B94D11899977427986C005708D095B5B089F504E52EE