Parents (Total: 7)
The searched file hash is included in 7 parent files which include package known and seen by metalookup. A sample is included below:
| Key |
Value |
| FileSize | 451432 |
| MD5 | 806CB6A07D053F721A8E675196114EB6 |
| 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 | 2.4.11+dfsg-1 |
| SHA-1 | D4EE6BE1F295CE3F05E675E4F234B3A20BF3B199 |
| SHA-256 | E2F48D24F4D2E931655F871957B4718228B438460887A47BEAC55B6C6D323744 |
| Key |
Value |
| FileSize | 50548 |
| MD5 | CE97199AC53CBABEEF181222D785FEF0 |
| 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 | 2.4.11+dfsg-1 |
| SHA-1 | 461A7E2E9BA801019D4DFFE40C7BBE11118ABE66 |
| SHA-256 | B3BF246A8E98A1FCF47095371E1C2A680DF034AB25670E2344C7F54B228FC3D9 |
| Key |
Value |
| FileSize | 527876 |
| MD5 | 1EDF8496263A6ADC7FA6A5315429C69F |
| 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 | 2.4.11+dfsg-1 |
| SHA-1 | B819EEA56280AD4ABCC44E5D419874F364EF861F |
| SHA-256 | 591F4DC68AFEC363D198CBB54130A8FFCC76FF7F0F3FEE4034C8C6347C8CD4E0 |
| Key |
Value |
| FileSize | 494108 |
| MD5 | 02A3A726877552855F37063639962D69 |
| 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 | 2.4.11+dfsg-1 |
| SHA-1 | F0C3B24956A696442FCB32E293471A377BAA1960 |
| SHA-256 | B278D9B2C829C63930C1DD03871AC2A331689C9689B54528681565BE256BB13C |
| Key |
Value |
| FileSize | 460432 |
| MD5 | C4C5EBB37D7DBB8298549F3C6954D382 |
| 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 | 2.4.11+dfsg-1 |
| SHA-1 | CD3572D24E59B9C5CC2677F15ACDA24FFDA85C4C |
| SHA-256 | 4ACCFB4EC42FBCD04415B3421FF1F11B47DE7CE1669F475BEC1727F12E938654 |
| 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 | 449624 |
| MD5 | D0F643F072D886E3E40C2CF001467000 |
| 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 | 2.4.11+dfsg-1 |
| SHA-1 | E4B3CF0B72CB879E436EB5436B6A298D1A1E625C |
| SHA-256 | 61D5F2B79EAB5F4A393688ADD1495B2461504B353BE7F9EE0F9DE4C0CB4D4609 |