Parents (Total: 94)

The searched file hash is included in 94 parent files which include package known and seen by metalookup. A sample is included below:

Key	Value
FileSize	363444
MD5	008665630BEAB04AA3E699DF53464A28
PackageDescription	ESO 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).
PackageMaintainer	Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.2.0+dfsg-1build1
SHA-1	016893D9A8DABB8BCACD581CEE5327857904F01D
SHA-256	C671E8C5D435484D7BD2ADE46FC2CAA48D49C8518AE118BED3AB6D604EE5336B

Key	Value
FileSize	184482
MD5	2A9ACD5A8E062002F64B214A3B6B00FF
PackageDescription	ESO 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).
PackageMaintainer	Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	1.8.21+dfsg-1build1
SHA-1	0600C46860A116FB748364715FA18ECAE1EBA0AC
SHA-256	2F942E0CDB1F7E91576879FA81FC9A13FD3C56B3C0AFD51DFBAD967AC412F017

Key	Value
FileSize	182452
MD5	EF08A2321C9439CC934330A4A5C4BF24
PackageDescription	ESO 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).
PackageMaintainer	Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	1.8.21+dfsg-1build1
SHA-1	0719138B7E3D860ECEB47FD703C3FE69D4B2F7AE
SHA-256	892AD0D3BC3DF8545BA7454295F7C457B2BFBD5E913D4537D99838C60A222AEC

Key	Value
FileSize	477952
MD5	3CAA106DD6246DCF218DE138AE022F77
PackageDescription	ESO 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).
PackageMaintainer	Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.4.3+dfsg-1
SHA-1	07D5C627FC555F637353012D04FEE7C6F1E6113C
SHA-256	4B04179EDF606ECC3AE590EC5EB34589B088566F820C6F00530B40016D5D6193

Key	Value
FileSize	195760
MD5	AD2C0CE7BFA6DD0C55A03053260B56BB
PackageDescription	ESO data reduction pipeline for HAWK-I 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).
PackageMaintainer	Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	1.8.14+dfsg-2
SHA-1	086A952CA52A913571A4B157A2FACE4144827EDA
SHA-256	2D7C4EE843C799609FC589F29F835C883F9AA2BE52375FA434E627D2452C14C0

Key	Value
FileSize	453352
MD5	5CFC0CB5C37652E14DA39B16073327E6
PackageDescription	ESO 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).
PackageMaintainer	Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.4.9+dfsg-1
SHA-1	09AD28C108CC2A32C4F9E9E6E17CB27DA90FFD5E
SHA-256	7A78D83C1E6E73EB9D53CA7D68B3C5EB49076AFE08652C402C0E2888B970DE64

Key	Value
FileSize	447632
MD5	33FC2B0C89624E65DA7B1A1A7C293E5D
PackageDescription	ESO 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).
PackageMaintainer	Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.4.8+dfsg-4
SHA-1	0B922EA38B7546D45FD6C7684420AF3A767B96A4
SHA-256	D1FF152F6C9ECAF1CF7282E6A5365DB706C7490C3F8999E902AAA1A8383EECE3

Key	Value
FileSize	426848
MD5	C8FC8B61CFE578FB387193CC0948C4CE
PackageDescription	ESO 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).
PackageMaintainer	Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.2.0+dfsg-1+b1
SHA-1	0D7A9C3BDB5386D1AD3C03E278B8A26A53117B63
SHA-256	E99CF0D36C035AAC0C944D8858B13809B9E0F719118FEA0D5165C368314DEA9E

Key	Value
FileSize	489816
MD5	0DC386B9AA2A31F951B2CAB6994240A4
PackageDescription	ESO 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).
PackageMaintainer	Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.4.9+dfsg-1
SHA-1	174D5C4F5AF18807F53EFF58FA4460491B0A01A0
SHA-256	1A2BE31E56411C85A56DFA78B4D7E21032BB44C3A3A3C03F2A8F1F1DD66465F1

Key	Value
FileSize	166042
MD5	B97749A724F73C32C3325C17663564D8
PackageDescription	ESO 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).
PackageMaintainer	Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	1.8.21+dfsg-1build1
SHA-1	1A54E42B7554DE056107B4700225D916C9932974
SHA-256	0E51D833B4411CD82D6A2A5FE156078517284A85462E8AC7D767EF137DF6136F