Parents (Total: 66)
The searched file hash is included in 66 parent files which include package known and seen by metalookup. A sample is included below:
Key |
Value |
FileSize | 139804 |
MD5 | 5D5DC8F30BCEB06D8E5109FBFF8D136B |
PackageDescription | ESO data reduction pipeline documentation for HAWK-I
This package contains the HTML documentation and manpages for the data
reduction pipeline for the HAWK-I instrument of the Very Large Telescope
(VLT) from the European Southern Observatory (ESO). |
PackageMaintainer | Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org> |
PackageName | cpl-plugin-hawki-doc |
PackageSection | doc |
PackageVersion | 2.4.11+dfsg-1 |
SHA-1 | 068725FD5D7DA2B884D21D553649487D0CF3428A |
SHA-256 | 0E6E7D65120EA7F396E0C014D4CC9D915FF5A730F7FFBD32890E7A6D131E59D9 |
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 | 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 | 93920 |
MD5 | C4DC7F4FABEF0D5A58459B4558A0FE78 |
PackageDescription | ESO data reduction pipeline documentation for HAWK-I
This package contains the HTML documentation and manpages for the data
reduction pipeline for the HAWK-I instrument of the Very Large Telescope
(VLT) from the European Southern Observatory (ESO). |
PackageMaintainer | Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com> |
PackageName | cpl-plugin-hawki-doc |
PackageSection | doc |
PackageVersion | 2.4.6+dfsg-1build1 |
SHA-1 | 100B3637C7E76C9D71F010D3B0B79967A1F39CEE |
SHA-256 | 3E9CA44E30A795879ED0B5D4A98686E99AA37F93B03DCE259E23D1B94AD242A7 |
Key |
Value |
FileSize | 91756 |
MD5 | A2560745BC4032F5CEA81C83683DFAA3 |
PackageDescription | ESO data reduction pipeline documentation for HAWK-I
This package contains the HTML documentation and manpages for the data
reduction pipeline for the HAWK-I instrument of the Very Large Telescope
(VLT) from the European Southern Observatory (ESO). |
PackageMaintainer | Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com> |
PackageName | cpl-plugin-hawki-doc |
PackageSection | doc |
PackageVersion | 2.4.8+dfsg-2 |
SHA-1 | 1384BCB093F9D00A8BB5B295E6F22853DE0D8B74 |
SHA-256 | FA274B9810C32695E1D5C30846D592F104EE38BAB8DC05804D53FFE57816C75E |
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 | 92036 |
MD5 | DCD32CC007E3FD19FA8255F70ABF725B |
PackageDescription | ESO data reduction pipeline documentation for HAWK-I
This package contains the HTML documentation and manpages for the data
reduction pipeline for the HAWK-I instrument of the Very Large Telescope
(VLT) from the European Southern Observatory (ESO). |
PackageMaintainer | Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com> |
PackageName | cpl-plugin-hawki-doc |
PackageSection | doc |
PackageVersion | 2.4.8+dfsg-4 |
SHA-1 | 188F8638534ED41B1618E6DC0F88C20A73D0458E |
SHA-256 | D33567F6D149BC0306B86ECC522F11BE9071C3DC99436677A8219BA0793AB263 |
Key |
Value |
FileSize | 470896 |
MD5 | 04E6CDD5BC92409B9B8ACCDBDA45598D |
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 | 1AB820B4CF5A53A38486A13C3E51A928A2FE694D |
SHA-256 | F4E93FD2283238717114016AB9CA5CDBD1B98D37FDA6784152CB5222AD3B3867 |
Key |
Value |
FileSize | 515728 |
MD5 | 178BC39B67CCFAC7374837B6783DEFDE |
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 | 1B3779DC0D999F9AA02A89F5F799490440FB4A47 |
SHA-256 | 88F0D4E52748D0A396F071C0EAF70FDD8F9BB0D1A987F7729A2B4E284A95C891 |