Result for 0248EC92557D5D81BFA795B4E8FC52760F611EE1

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-1.8.21/hawki_cal_dark.so
FileSize18692
MD5C9104ACB94D275D16EA429BF6F5472FA
SHA-10248EC92557D5D81BFA795B4E8FC52760F611EE1
SHA-256186425FC692054E7C723D74D5B75A5571A379CD55043C6F42AAA7461BD761FB1
SSDEEP192:46vu8p4HtlwuUZ5Ln5vvM0XuZSTz0MED4WZE6xTj6aIwOrI9gURnYM/mNda3w4yh:4BNlwuUXxE6uZZD4CdIxrIRm+h4GdL
TLSHT16A82B5CB7216C927C890B43A346B4E57319897D6DD194BB33A8C04900A21BFFDE69F5B
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
FileSize223236
MD5250B250B503BC1BE132F283F2DE01047
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
PackageVersion1.8.21+dfsg-1
SHA-1745F2CE42DE269179A9D006DAA409DDB5E4373D2
SHA-25697E966AABBC439DB1190D4805629759BA2314151762DE45E9E685D8179ACF04A