Package: artist Version: 1.1~beta-1 Architecture: amd64 Maintainer: Michael Olberg Installed-Size: 8381 Depends: libc6 (>= 2.14), libcfitsio3 (>= 3.060), libgcc1 (>= 1:4.1.1), libgsl0ldbl (>= 1.9), libpython2.7 (>= 2.7), libqhull5 (>= 2003.1), libstdc++6 (>= 4.1.1), python (<< 2.8), python (>= 2.7), python-support (>= 0.90.0), paraview, python-matplotlib, python-numpy, python-pyfits, python-qt4, python-scipy Priority: optional Section: science Filename: pool/contrib/a/artist/artist_1.1~beta-1_amd64.deb Size: 3741568 SHA256: cfdfb52cbb3a72508f34ccdb8a66ca50688127dbc8ff0da9b0b2c069dae099fb SHA1: 31c3c315cb33cdd98cbdd5ee397bcff0c1b52e0d MD5sum: 1468c01a0ec09b19b6198d1de25e6992 Description: adaptable radiative transfer innovations for submm telescopes Submillimeter observations are a key for answering many of the big questions in modern-day astrophysics, such as how stars and planets form, how galaxies evolve, and how material cycles through stars and the interstellar medium. With the large submillimeter facilities ALMA and Herschel a new window will open to study these questions. Within the ASTRONET first joint call for proposals, "Common Tools for Future Large Submillimeter Facilities", we have been awarded funding for our program, "Adaptable Radiative Transfer Innovations for Submillimeter Telescopes (ARTIST)", to develop a next generation model suite for comprehensive multi-dimensional radiative transfer calculations of the dust and line emission, as well as their polarization, to help interpret observations with these groundbreaking facilities. . The ARTIST package consists of: o An innovative radiative transfer code (LIME) using adaptive gridding that allows simulations of sources with arbitrary multi-dimensional (1D, 2D, 3D) and time-dependent structures, ensuring rapid convergence. o Unique tools for modeling the polarization of the line and dust emission, information that will come with standard ALMA observations. o A library of commonly used analytic/semi-analytic models as well as a comprehensive graphical user interface. Package: boa Version: 20110825 Architecture: amd64 Depends: boalib Maintainer: Michael Olberg Priority: optional Section: science Filename: pool/contrib/b/boa/boa_20110825_amd64.deb Size: 46176272 SHA256: bf8f1700a0b877fc50f2698d145ffb2d8c8bf7baf25b9a0bbf59d5fd44264f72 SHA1: 2cfcf04ed4c1990411a618e56a2f9bc16e3f92ca MD5sum: 5bbadae382e64028c7c5cad12b2a0d89 Description: boa bolometer array analysis software The Bolometer Array analysis software, is a new data reduction package that has been developed especially to process data acquired with bolometer arrays at the APEX telescope. The primary goal was to handle data observed with LABOCA, the Large APEX Bolometer Camera. BoA can also handle data acquired with other bolometer arrays, such as ASZCa (the APEX SZ Camera), and SABOCA (the Submillimeter APEX Camera). The design of BoA has been done with two major goals in mind: to provide a comprehensive tool for the visualisation, reduction and analysis of data from the new generation of bolometer arrays, and to facilitate the extension and modification of the software by users with no strong programming background. The development of BoA is a collaborative effort from scientists at the MPIfR and AIfA, wich additional contributions from people working at APEX and in various institutes in Europe. Package: boalib Version: 20110825 Architecture: amd64 Depends: libc6 (>= 2.8), libgcc1 (>= 1:4.1.1), libstdc++6 (>= 4.1.1), zlib1g (>= 1:1.1.4), python2.5, python2.5-boapackages Maintainer: Michael Olberg Priority: optional Section: science Filename: pool/contrib/b/boalib/boalib_20110825_amd64.deb Size: 60538232 SHA256: 4480aa9610ccbf6bd1ae248f19239415c21860a49d06c32fce076b8e01bd1c55 SHA1: f5e3093c11ab14daf3d5f08cebd7243f65eaeb34 MD5sum: e19d3b6e196ea3fbd1ad6c2900e9ab51 Description: boa support libraries boalib is a collection of libraries and utilities needed to run BoA. BoA itself is contained in package boa. Package: drp Version: 1.0-2 Architecture: amd64 Maintainer: Michael Olberg Installed-Size: 1691 Depends: libc6 (>= 2.14), libx11-6 Priority: optional Section: science Filename: pool/contrib/d/drp/drp_1.0-2_amd64.deb Size: 268950 SHA256: 76ff157d9d3ba504650e3428d61ffda05b5ecf3ab45b5b8ec4e7c0c38bf16209 SHA1: ed68e7b72114a5776d5117caeb1fa577461ae0e7 MD5sum: 9482a1d62d5e75270b1dbef9b6ba6b25 Description: data reduction of radioastronomical spectral line data A program to reduce radio-astronomical spectral line data. Support for various input formats, e.g. FITS. . The program uses plain X11 as the graphical user interface toolkit. Package: gildas Version: 201503c-precise1 Architecture: amd64 Maintainer: Michael Olberg Installed-Size: 100785 Depends: libblas3gf, libc6 (>= 2.14), libcfitsio3 (>= 3.060), libgcc1 (>= 1:4.1.1), libgfortran3 (>= 4.3), libglib2.0-0 (>= 2.16.0), libgtk2.0-0 (>= 2.18.0), liblapack3gf | liblapack.so.3gf | libatlas3gf-base, libpng12-0 (>= 1.2.13-4), libpython2.7 (>= 2.7), libstdc++6 (>= 4.4.0), libmotif4, libforms2 Homepage: http://www.iram.fr/IRAMFR/GILDAS Priority: extra Section: contrib/science Filename: pool/contrib/g/gildas/gildas_201503c-precise1_amd64.deb Size: 21185216 SHA256: 09f95a152ec37a810d1370ce961768e3553f3b8b56dfbf2e8285f83e3c345ae5 SHA1: e4ffbd2d4aab2452e81f9007e6206c67f9907ee1 MD5sum: 6724b5fce8290dfb50f4b5ec06d5e078 Description: Grenoble Image and Line Data Analysis System GILDAS is a collection of state-of-the-art software oriented toward (sub-)millimeter radioastronomical applications (either single-dish or interferometer). It is daily used to reduce all data acquired with the IRAM 30M telescope and Plateau de Bure Interferometer PDBI (except VLBI observations). GILDAS is easily extensible. GILDAS is written in Fortran-90, with a few parts in C/C++ (mainly keyboard interaction, plotting, widgets). Package: gildas-doc Version: 201503c-1 Architecture: all Maintainer: Michael Olberg Installed-Size: 46775 Homepage: http://www.iram.fr/IRAMFR/GILDAS Priority: extra Section: contrib/doc Filename: pool/contrib/g/gildas-doc/gildas-doc_201503c-1_all.deb Size: 17703544 SHA256: 28c3dc44918b30e265e92d653a6e18387cbc2eb0060bf161f624735c131cc3a5 SHA1: c89d678fc1ad8bdcd1c8b2983b4a27f26bb19f74 MD5sum: 119e4f39d11b795b617cab6240c91b43 Description: Grenoble Image and Line Data Analysis System GILDAS is a collection of state-of-the-art software oriented toward (sub-)millimeter radioastronomical applications (either single-dish or interferometer). It is daily used to reduce all data acquired with the IRAM 30M telescope and Plateau de Bure Interferometer PDBI (except VLBI observations). GILDAS is easily extensible. GILDAS is written in Fortran-90, with a few parts in C/C++ (mainly keyboard interaction, plotting, widgets). This is the documentation package. Package: pgplot5 Version: 5.2.2-19+xs1 Architecture: amd64 Maintainer: Carlo Segre Installed-Size: 2194 Depends: libc6 (>= 2.14), libgcc1 (>= 1:4.1.1), libgfortran3 (>= 4.6), libpng12-0 (>= 1.2.13-4), libquadmath0 (>= 4.6), libx11-6, zlib1g Suggests: gfortran, libpng-dev, zlib1g-dev, libx11-dev, libxaw7-dev, libxt-dev, x11proto-core-dev, libgif-dev, libmotif-dev Conflicts: pgplot Replaces: pgplot Homepage: http://www.astro.caltech.edu/~tjp/pgplot/ Priority: optional Section: non-free/math Filename: pool/contrib/p/pgplot5/pgplot5_5.2.2-19+xs1_amd64.deb Size: 559588 SHA256: 879d926a301f432bb73b32f20c2c1bba16d6734c3bf728a4562e463ae06b761e SHA1: 4baeeadbc15a1230907c40ed98c141f947aeda9f MD5sum: 2d6843f1540b9550821e2e62374a80a4 Description: large subroutine library for plotting scientific data This package contains both runtime and development libraries. Many routines are included in pgplot for viewing scientific data. Many (about 70) output devices are supported. 2-D , 3-D , contour, image manipulation, etc. are well supported. Interactive routines are included. Both a C and a FORTRAN library are present. See http://astro.caltech.edu/~tjp/pgplot/ for documentation. Package: python-odin Source: odinpy Version: 1.0 Architecture: amd64 Maintainer: Michael Olberg Installed-Size: 563 Depends: python2.7, python (>= 2.7), python (<< 2.8), libc6 (>= 2.3.4) Priority: optional Section: python Filename: pool/contrib/o/odinpy/python-odin_1.0_amd64.deb Size: 159296 SHA256: 1a5d24d2c497e4f1965e050116bdada1e7f69458ba92db09698da2c8645f8aa7 SHA1: f82affcea4cfdef7d17f911cbb1ad5fe4f9a6a9d MD5sum: ab1ef6b17de5bb6968da47f550ff0912 Description: Python interface to the Odin C-library Package: python2.5-boapackages Version: 20110825 Architecture: amd64 Depends: libc6 (>= 2.8), libgcc1 (>= 1:4.1.1), libstdc++6 (>= 4.1.1), zlib1g (>= 1:1.1.4), python2.5 Maintainer: Michael Olberg Priority: optional Section: science Filename: pool/contrib/p/python2.5-boapackages/python2.5-boapackages_20110825_amd64.deb Size: 2234952 SHA256: 53a056821bd73b1d7b27535293cd10a7c155edf42b7ceb445d2ace2c9dacfaed SHA1: fd8d3528eb3b723fe5b09e392d2db3fee580b3a6 MD5sum: d4b4bd56ebec424b4124bae2496e0875 Description: boa support python packages these are the python2.5 packages needed by boalib. boalib is a collection of libraries and utilities needed to run BoA. BoA itself is contained in package boa. Package: qtrainer Version: 1.2-2 Architecture: amd64 Maintainer: Michael Olberg Installed-Size: 247 Depends: libc6 (>= 2.2.5), libgcc1 (>= 1:4.1.1), libqmapcontrol0, libqt4-network (>= 4:4.5.3), libqt4-sql (>= 4:4.5.3), libqt4-xml (>= 4:4.5.3), libqtcore4 (>= 4:4.7.0~beta1), libqtgui4 (>= 4:4.5.3), libqwt5-qt4, libstdc++6 (>= 4.1.1) Recommends: garmin-forerunner-tools, sqlite3 Priority: optional Section: contrib/utils Filename: pool/contrib/q/qtrainer/qtrainer_1.2-2_amd64.deb Size: 111460 SHA256: dfe067e2efd684c6f1f95c7bb8e4da53f51747d3df3742b0db59ba0668043630 SHA1: eee735bffe68749b6b12a8512a53a58b923d489d MD5sum: e235b09d6ab8f7b148ab4d19ab4446fd Description: Qt application to log and view data from Garmin Forerunner devices. It is geared towards running, using a sqlite database to store track data. Qtrainer is written in C++ using the Qt4 gui framework. Package: radex Version: 20111130-1 Architecture: amd64 Maintainer: Michael Olberg Installed-Size: 13208 Depends: libc6 (>= 2.2.5), libgcc1 (>= 1:4.1.1), libgfortran3 (>= 4.3) Homepage: http://home.strw.leidenuniv.nl/~moldata/radex.html Priority: optional Section: science Filename: pool/contrib/r/radex/radex_20111130-1_amd64.deb Size: 2181428 SHA256: 187ac1de4d53a5ed35e0aacc974e05bf248b754a65f744c3db9c3019d41265c3 SHA1: 8c37e30498db419da01d44fcbd4d92d14617e6d7 MD5sum: e421f86693bd66be2d2c62bb19df9a4c Description: perform statistical equilibrium calculations A statistical equilibrium radiative transfer code, RADEX, is made available for public use as part of the Leiden Atomic and Molecular Database (LAMDA). RADEX is a one-dimensional non-LTE radiative transfer code, that uses the escape probability formulation assuming an isothermal and homogeneous medium without large-scale velocity fields. RADEX is comparable to the LVG method and provides a useful tool in rapidly analyzing a large set of observational data providing constraints on physical conditions, such as density and kinetic temperature. . RADEX provides an alternative to the widely used rotation diagram method which relies upon the availability of many optically thin emission lines and is useful only in roughly constraining the excitation temperature in addition to the column density. RADEX makes no extrapolation of collisional rate coefficients outside the temperature range specified in the molecular data file used as input. Instead they are kept constant. . RADEX is offered both as a on-line version for quick estimations of physical conditions, and as source code for extensive grids of calculations. . The formalism adopted in RADEX is summarized in Van der Tak, F.F.S., Black, J.H., Schöier, F.L., Jansen, D.J., van Dishoeck, E.F. 2007, A&A 468, 627 (arXiv:0704.0155v1). Package: xs Version: 1.2.23-oso1 Architecture: amd64 Maintainer: Michael Olberg Installed-Size: 1270 Depends: libc6 (>= 2.14), libpng12-0 (>= 1.2.13-4), libx11-6, libxm4 (>= 2.3.4), libxt6, pgplot5 (>= 5.2.2-19+xs1), libmotif4 Priority: optional Section: science Filename: pool/contrib/x/xs/xs_1.2.23-oso1_amd64.deb Size: 406960 SHA256: 6041e4966f895c3bbbd2d924f01d92b014960ba9f5d095bc0dfdc38a647296bb SHA1: ebf615776124a09c4dfe42fd4251657e8e28ff4f MD5sum: 4b1b119205266ff247bdd89dd7e3759c Description: data reduction of radioastronomical spectral line data A program to reduce radio-astronomical spectral line data. Support for various input formats, e.g. FITS. . The program uses Open Motif as the graphical user interface toolkit.