Result for 01C2B78B38085BED3F99A5DA3EDC445665B8C8E0

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.2.0/hawki_sci_jitter.so
FileSize39992
MD5068F2FD80A56C6A0CB1D85CF45EC8E1A
SHA-101C2B78B38085BED3F99A5DA3EDC445665B8C8E0
SHA-2568F9026B89884056692AE72B877F0150BEA7005DC16F2CF5B935742DE7B6E2B54
SSDEEP768:G5Vi4wQl9oYU1Ti989tltW/5ac7TxIDRkMe2efkEZ9uIqP:G5jwQfoRb8/ZIFk0n3
TLSHT16F0319CA6A525977C1D02736319F0BD9A22052E1C2CDA707518C87142D47F9F8AFEFAE
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
FileSize426848
MD5C8FC8B61CFE578FB387193CC0948C4CE
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
PackageVersion2.2.0+dfsg-1+b1
SHA-10D7A9C3BDB5386D1AD3C03E278B8A26A53117B63
SHA-256E99CF0D36C035AAC0C944D8858B13809B9E0F719118FEA0D5165C368314DEA9E