Result for 3CFE07CD4E91800337DEA6A02923A5F8FB609B4C

Query result

Key Value
FileName./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_step_photom_2mass.so
FileSize23064
MD539EAC9A742CD97215B4ED5F558E4A9C4
SHA-13CFE07CD4E91800337DEA6A02923A5F8FB609B4C
SHA-25649E26EB7A1044716A704D4772C3283A4C1B4A2894BA51891A7D55D0033519065
SSDEEP384:RXkUK8+Ol8fqw8MKYnPDme5GSTungRQ7UnuXDEvi9u9+qQOEXC2evnrkvCvRxEGl:R1d+Ol8fqwBKEPDme5GSTungRQUnuXDq
TLSHT1B4A2A4A3AF141E17D5C1CC301C2FC55260FF9E2C61ECBA13B46DD8D52A4566C2EBB94A
hashlookup:parent-total1
hashlookup:trust55

Network graph view

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
FileSize477952
MD53CAA106DD6246DCF218DE138AE022F77
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
PackageVersion2.4.3+dfsg-1
SHA-107D5C627FC555F637353012D04FEE7C6F1E6113C
SHA-2564B04179EDF606ECC3AE590EC5EB34589B088566F820C6F00530B40016D5D6193