Parents (Total: 29)
The searched file hash is included in 29 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 | 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 | 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 | 525508 |
MD5 | 02A40EB100388240DB4D5D6169497C90 |
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 | 1DF42B5AAC2B9A9BD2D43985F3D8ABB2D7B93FBB |
SHA-256 | 54DC6921752833B0AD602101C2BD1ADE309304A73249C9EFE3E22121EB856F01 |
Key |
Value |
FileSize | 451824 |
MD5 | 1F48F63051D9F44902CAF24A014F7EA7 |
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 | 1F8850C8DF01377F7D9588E80BA2C9DB502D4044 |
SHA-256 | 0A8C64809D35D4085A35B94D11899977427986C005708D095B5B089F504E52EE |
Key |
Value |
FileSize | 454368 |
MD5 | 60DE75C96E5EEC0B0CB809D3B38C05AD |
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 | 2362C669BEDA660467F4EAF89E0BD6020E351A71 |
SHA-256 | A6CE560A5A7EC6D78F19A88181F56DD7D73263A6DDB72A6C829DD442A9F575A1 |
Key |
Value |
FileSize | 50524 |
MD5 | E6F5B5FB25F0A2CE2EA40DFFB8792A44 |
PackageDescription | ESO data reduction pipeline calibration data downloader for HAWK-I
This package downloads calibration data of 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-calib |
PackageSection | contrib/science |
PackageVersion | 2.4.9+dfsg-1 |
SHA-1 | 25ECA67E4915678719CFD89DA2C2A7C1DEA2D78E |
SHA-256 | CDB604476CB6E65AD0E8F56E42657A129B0DD8A09030EF7F9C55FEDF7379BCED |
Key |
Value |
FileSize | 451748 |
MD5 | 071B9F4695EF80D6D86B48ECB848BDB1 |
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 | 2EFAE4DCB62A49CB19F7510008CFF9C14342BE11 |
SHA-256 | ABAE21EFC2A432D5D37BD2D33604B5CE713A35277F7F34E80A7E278641E8009B |
Key |
Value |
FileSize | 139556 |
MD5 | 5B331B4C29CDEA31ABDABCA2DF77C8C5 |
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 | 2.4.9+dfsg-1 |
SHA-1 | 310344B1A0173F0464ACB0F5ABBEA7B1222D192E |
SHA-256 | 502865AF6FE1F979384E0F443A3EA2979174BE5616BAB38D7022B8B1E527F004 |