Result for 16E6EAE9579A592669F36DDBA9EDE86341E80C17

Query result

Key Value
FileName./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_dark_combine.so
FileSize27648
MD50479524FC911E4EF4484AFE01A72FAA3
SHA-116E6EAE9579A592669F36DDBA9EDE86341E80C17
SHA-256E17AA388AA5AAB27BA657C125D1E676DE9A5191F05DFC55DC05781EFADC99AD8
SSDEEP768:FCYX9owgA0gSNfCYuijEBkQ2xXb/2QHMiPkktuiRE+9L26gpiHy3vDrf4jXVoXKv:k29owgA0gSNfCYuijEBkQ2xLZHMiPkkM
TLSHT1A8C29497BF141E06C0C2DC701C5F961281BF4E5CB198BA53F59CED881B06A8C2DBBA9D
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
FileSize451748
MD5071B9F4695EF80D6D86B48ECB848BDB1
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-12EFAE4DCB62A49CB19F7510008CFF9C14342BE11
SHA-256ABAE21EFC2A432D5D37BD2D33604B5CE713A35277F7F34E80A7E278641E8009B