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-rw-r--r--sci-astronomy/bpz/metadata.xml4
-rw-r--r--sci-astronomy/casapy-bin/metadata.xml8
-rw-r--r--sci-astronomy/eazy/metadata.xml6
-rw-r--r--sci-astronomy/eye/metadata.xml14
-rw-r--r--sci-astronomy/galfit-bin/metadata.xml4
-rw-r--r--sci-astronomy/lephare/metadata.xml4
-rw-r--r--sci-astronomy/missfits/metadata.xml12
-rw-r--r--sci-astronomy/mosstack/metadata.xml14
-rw-r--r--sci-astronomy/psfex/metadata.xml8
-rw-r--r--sci-astronomy/scamp/metadata.xml6
-rw-r--r--sci-astronomy/sextractor/metadata.xml16
-rw-r--r--sci-astronomy/skymaker/metadata.xml10
-rw-r--r--sci-astronomy/starlink-bin/metadata.xml8
-rw-r--r--sci-astronomy/stiff/metadata.xml6
-rw-r--r--sci-astronomy/stilts/metadata.xml14
-rw-r--r--sci-astronomy/stuff/metadata.xml6
-rw-r--r--sci-astronomy/swarp/metadata.xml4
-rw-r--r--sci-astronomy/topcat/metadata.xml14
-rw-r--r--sci-astronomy/weightwatcher/metadata.xml8
-rw-r--r--sci-astronomy/zebra/metadata.xml30
-rw-r--r--sci-astronomy/zpeg/metadata.xml8
21 files changed, 102 insertions, 102 deletions
diff --git a/sci-astronomy/bpz/metadata.xml b/sci-astronomy/bpz/metadata.xml
index b57d8eab6..008ef62b2 100644
--- a/sci-astronomy/bpz/metadata.xml
+++ b/sci-astronomy/bpz/metadata.xml
@@ -6,7 +6,7 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- Bayesian Photometric Redshifts is a method to infere photometric
- redshifts of galaxies.
+Bayesian Photometric Redshifts is a method to infere photometric
+redshifts of galaxies.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/casapy-bin/metadata.xml b/sci-astronomy/casapy-bin/metadata.xml
index fdf3ea3f5..ef1c2d6cc 100644
--- a/sci-astronomy/casapy-bin/metadata.xml
+++ b/sci-astronomy/casapy-bin/metadata.xml
@@ -6,8 +6,8 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription>
- CASA, the Common Astronomy Software Applications package, is being developed
- with the primary goal of supporting the data post-processing needs of the
- next generation of radio astronomical telescopes such as ALMA and VLA.
- </longdescription>
+CASA, the Common Astronomy Software Applications package, is being developed
+with the primary goal of supporting the data post-processing needs of the
+next generation of radio astronomical telescopes such as ALMA and VLA.
+</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/eazy/metadata.xml b/sci-astronomy/eazy/metadata.xml
index 695876072..66032a84a 100644
--- a/sci-astronomy/eazy/metadata.xml
+++ b/sci-astronomy/eazy/metadata.xml
@@ -6,8 +6,8 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- Easy and Accurate Zphot from Yale is a photometric redshift code
- designed to produce high-quality redshifts from 0 to 4 for situations
- where complete spectroscopic calibration samples are not available.
+Easy and Accurate Zphot from Yale is a photometric redshift code
+designed to produce high-quality redshifts from 0 to 4 for situations
+where complete spectroscopic calibration samples are not available.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/eye/metadata.xml b/sci-astronomy/eye/metadata.xml
index 964c66ad9..0bbded1cf 100644
--- a/sci-astronomy/eye/metadata.xml
+++ b/sci-astronomy/eye/metadata.xml
@@ -6,12 +6,12 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- In EyE (Enhance Your Extraction) an artificial neural network
- connected to pixels of a moving window (retina) is trained to
- associate these input stimuli to the corresponding response in one
- or several output image(s). The resulting filter can be loaded in
- SExtractor to operate complex, wildly non-linear filters on
- astronomical images. Typical applications of EyE include adaptive
- filtering, feature detection and cosmetic corrections.
+In EyE (Enhance Your Extraction) an artificial neural network
+connected to pixels of a moving window (retina) is trained to
+associate these input stimuli to the corresponding response in one
+or several output image(s). The resulting filter can be loaded in
+SExtractor to operate complex, wildly non-linear filters on
+astronomical images. Typical applications of EyE include adaptive
+filtering, feature detection and cosmetic corrections.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/galfit-bin/metadata.xml b/sci-astronomy/galfit-bin/metadata.xml
index 6b4fa6b4a..90190836d 100644
--- a/sci-astronomy/galfit-bin/metadata.xml
+++ b/sci-astronomy/galfit-bin/metadata.xml
@@ -6,7 +6,7 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- GALFIT is a data analysis algorithm that fits 2-D analytic functions
- to galaxies and point sources directly to digital images.
+GALFIT is a data analysis algorithm that fits 2-D analytic functions
+to galaxies and point sources directly to digital images.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/lephare/metadata.xml b/sci-astronomy/lephare/metadata.xml
index 508212313..0c2cbc460 100644
--- a/sci-astronomy/lephare/metadata.xml
+++ b/sci-astronomy/lephare/metadata.xml
@@ -6,7 +6,7 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- Le Photometric Analysis for Redshift Estimate is a set of commands
- to compute photometric redshifts and to perform SED fitting.
+Le Photometric Analysis for Redshift Estimate is a set of commands
+to compute photometric redshifts and to perform SED fitting.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/missfits/metadata.xml b/sci-astronomy/missfits/metadata.xml
index 3115c8d55..136e880c2 100644
--- a/sci-astronomy/missfits/metadata.xml
+++ b/sci-astronomy/missfits/metadata.xml
@@ -6,11 +6,11 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- MissFITS is a program that performs basic maintenance and packaging
- tasks on FITS files using an optimised FITS library. MissFITS can:
- * add/edit/remove FITS header keywords
- * split/join Multi-Extension-FITS (MEF) files
- * unpile/pile FITS data-cubes
- * create/check/update FITS checksums, using R. Seaman’s protocol.
+MissFITS is a program that performs basic maintenance and packaging
+tasks on FITS files using an optimised FITS library. MissFITS can:
+* add/edit/remove FITS header keywords
+* split/join Multi-Extension-FITS (MEF) files
+* unpile/pile FITS data-cubes
+* create/check/update FITS checksums, using R. Seaman’s protocol.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/mosstack/metadata.xml b/sci-astronomy/mosstack/metadata.xml
index 570109a05..2cc9b1528 100644
--- a/sci-astronomy/mosstack/metadata.xml
+++ b/sci-astronomy/mosstack/metadata.xml
@@ -6,16 +6,16 @@
<name>Mikko Laine</name>
</maintainer>
<longdescription>
- An open source stacking software for astronomical images taken with a DSLR
- camera. Mosstack can calibrate, debayer, register, align and stack photos
- taken with modern DSLR's from Canon. It has a command line user interface
- inspired by AstroSurf IRIS and a graphical user interface written with PyQt4
- </longdescription>
+An open source stacking software for astronomical images taken with a DSLR
+camera. Mosstack can calibrate, debayer, register, align and stack photos
+taken with modern DSLR's from Canon. It has a command line user interface
+inspired by AstroSurf IRIS and a graphical user interface written with PyQt4
+</longdescription>
<use>
<flag name="opencl">Enables OpenCL support and pulls in pyopencl. This makes
- some operations much faster but requires specific hardware and drivers.</flag>
+some operations much faster but requires specific hardware and drivers.</flag>
<flag name="qt4">Pulls in PyQt4. Program works on command line interface
- without it but for GUI the library is required.</flag>
+without it but for GUI the library is required.</flag>
</use>
<upstream>
<remote-id type="bitbucket">mikko_laine/mosstack</remote-id>
diff --git a/sci-astronomy/psfex/metadata.xml b/sci-astronomy/psfex/metadata.xml
index 5121f0c8d..e1b68e8d9 100644
--- a/sci-astronomy/psfex/metadata.xml
+++ b/sci-astronomy/psfex/metadata.xml
@@ -6,10 +6,10 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- PSFEx (“PSF Extractor”) extracts models of the Point Spread
- Function (PSF) from FITS images processed with <pkg>sci-libs/sextractor</pkg>, and
- measures the quality of images. The generated PSF models can be used
- for model-fitting photometry or morphological analyses.
+PSFEx (“PSF Extractor”) extracts models of the Point Spread
+Function (PSF) from FITS images processed with <pkg>sci-libs/sextractor</pkg>, and
+measures the quality of images. The generated PSF models can be used
+for model-fitting photometry or morphological analyses.
</longdescription>
<use>
<flag name="plplot">Build with <pkg>sci-libs/plplot</pkg> to allow diagnostic plots during processing</flag>
diff --git a/sci-astronomy/scamp/metadata.xml b/sci-astronomy/scamp/metadata.xml
index 5b8a3c398..d4357bf76 100644
--- a/sci-astronomy/scamp/metadata.xml
+++ b/sci-astronomy/scamp/metadata.xml
@@ -6,9 +6,9 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- SCAMP computes astrometric and photometric solutions from SExtractor catalogs
- and stores them in header files. These headers files can be read by SWarp to
- coadd images.
+SCAMP computes astrometric and photometric solutions from SExtractor catalogs
+and stores them in header files. These headers files can be read by SWarp to
+coadd images.
</longdescription>
<use>
<flag name="plplot">Build with <pkg>sci-libs/plplot</pkg> to allow diagnostic plots during processing</flag>
diff --git a/sci-astronomy/sextractor/metadata.xml b/sci-astronomy/sextractor/metadata.xml
index 651b20e47..9564e71e6 100644
--- a/sci-astronomy/sextractor/metadata.xml
+++ b/sci-astronomy/sextractor/metadata.xml
@@ -6,17 +6,17 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- SExtractor (Source Extractor) is a program that builds a catalogue of
- objects from an astronomical image. Although it is particularly
- oriented towards reduction of large scale galaxy-survey data, it
- performs rather well on moderately crowded star fields. It has the
- ability to automatically separate stars and galaxy using neural
- networks.
+SExtractor (Source Extractor) is a program that builds a catalogue of
+objects from an astronomical image. Although it is particularly
+oriented towards reduction of large scale galaxy-survey data, it
+performs rather well on moderately crowded star fields. It has the
+ability to automatically separate stars and galaxy using neural
+networks.
</longdescription>
<use>
<flag name="modelfit">
- Enable profile model fitting, needs <pkg>sci-libs/atlas</pkg>
- and <pkg>sci-libs/fftw</pkg>
+Enable profile model fitting, needs <pkg>sci-libs/atlas</pkg>
+and <pkg>sci-libs/fftw</pkg>
</flag>
</use>
</pkgmetadata>
diff --git a/sci-astronomy/skymaker/metadata.xml b/sci-astronomy/skymaker/metadata.xml
index 18cb8766d..268814ffc 100644
--- a/sci-astronomy/skymaker/metadata.xml
+++ b/sci-astronomy/skymaker/metadata.xml
@@ -6,10 +6,10 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- SkyMaker is a program that simulates astronomical images. It accepts
- object lists in ASCII generated by the Stuff program to produce
- realistic astronomical fields. There are various options for the user:
- build a realistic Point Spread Function, generate a list of stars and
- galaxies. Galaxies are modeled analytically.
+SkyMaker is a program that simulates astronomical images. It accepts
+object lists in ASCII generated by the Stuff program to produce
+realistic astronomical fields. There are various options for the user:
+build a realistic Point Spread Function, generate a list of stars and
+galaxies. Galaxies are modeled analytically.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/starlink-bin/metadata.xml b/sci-astronomy/starlink-bin/metadata.xml
index 111f0287a..ef0e61480 100644
--- a/sci-astronomy/starlink-bin/metadata.xml
+++ b/sci-astronomy/starlink-bin/metadata.xml
@@ -6,9 +6,9 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- The Starlink Project, referred to by users as Starlink and by
- developers as simply The Project, was a UK astronomical computing
- project which supplied general-purpose data reduction
- software.
+The Starlink Project, referred to by users as Starlink and by
+developers as simply The Project, was a UK astronomical computing
+project which supplied general-purpose data reduction
+software.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/stiff/metadata.xml b/sci-astronomy/stiff/metadata.xml
index 1ab3a27af..c100b1037 100644
--- a/sci-astronomy/stiff/metadata.xml
+++ b/sci-astronomy/stiff/metadata.xml
@@ -6,8 +6,8 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- STIFF is a program that convert scientific FITS images to the
- more popular TIFF, in 8 (grayscale) or 24 (true colour: 3 times 8) bits per
- pixel.
+STIFF is a program that convert scientific FITS images to the
+more popular TIFF, in 8 (grayscale) or 24 (true colour: 3 times 8) bits per
+pixel.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/stilts/metadata.xml b/sci-astronomy/stilts/metadata.xml
index 46b14de5c..f2c84722f 100644
--- a/sci-astronomy/stilts/metadata.xml
+++ b/sci-astronomy/stilts/metadata.xml
@@ -6,12 +6,12 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- The Starlink Tables Infrastructure Library Tool Set is a set of
- command-line tools based on STIL, the Starlink Tables Infrastructure
- Library. It deals with the processing of tabular data; the package
- has been designed for, but is not restricted to, astronomical tables
- such as object catalogues. Some of the tools are generic and can
- work with multiple formats (including FITS, VOTable, CSV, SQL and
- ASCII), and others are specific to the VOTable format.
+The Starlink Tables Infrastructure Library Tool Set is a set of
+command-line tools based on STIL, the Starlink Tables Infrastructure
+Library. It deals with the processing of tabular data; the package
+has been designed for, but is not restricted to, astronomical tables
+such as object catalogues. Some of the tools are generic and can
+work with multiple formats (including FITS, VOTable, CSV, SQL and
+ASCII), and others are specific to the VOTable format.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/stuff/metadata.xml b/sci-astronomy/stuff/metadata.xml
index 5970575e9..ade4c41c5 100644
--- a/sci-astronomy/stuff/metadata.xml
+++ b/sci-astronomy/stuff/metadata.xml
@@ -6,8 +6,8 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- Stuff is a program that simulates “perfect” astronomical
- catalogues. It generate object lists in ASCII which can read by the
- SkyMaker program to produce realistic astronomical fields.
+Stuff is a program that simulates “perfect” astronomical
+catalogues. It generate object lists in ASCII which can read by the
+SkyMaker program to produce realistic astronomical fields.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/swarp/metadata.xml b/sci-astronomy/swarp/metadata.xml
index 110a1fe70..209ee5d8f 100644
--- a/sci-astronomy/swarp/metadata.xml
+++ b/sci-astronomy/swarp/metadata.xml
@@ -6,7 +6,7 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- SWarp takes astronomical FITS images with a WCS-like projection,
- resample and stack them all.
+SWarp takes astronomical FITS images with a WCS-like projection,
+resample and stack them all.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/topcat/metadata.xml b/sci-astronomy/topcat/metadata.xml
index 4cf0383c9..65b998b7d 100644
--- a/sci-astronomy/topcat/metadata.xml
+++ b/sci-astronomy/topcat/metadata.xml
@@ -6,12 +6,12 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- Tool for OPerations on Catalogues And Tables is an interactive
- graphical viewer and editor for tabular data. Its aim is to provide
- most of the facilities that astronomers need for analysis and
- manipulation of source catalogues and other tables, though it can be
- used for non-astronomical data as well. It understands a number of
- different astronomically important formats (including FITS and
- VOTable) and more formats can be added.
+Tool for OPerations on Catalogues And Tables is an interactive
+graphical viewer and editor for tabular data. Its aim is to provide
+most of the facilities that astronomers need for analysis and
+manipulation of source catalogues and other tables, though it can be
+used for non-astronomical data as well. It understands a number of
+different astronomically important formats (including FITS and
+VOTable) and more formats can be added.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/weightwatcher/metadata.xml b/sci-astronomy/weightwatcher/metadata.xml
index 26af98c3c..8af502859 100644
--- a/sci-astronomy/weightwatcher/metadata.xml
+++ b/sci-astronomy/weightwatcher/metadata.xml
@@ -6,9 +6,9 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- WeightWatcher is a program that combines weight-maps, flag-maps and
- polygon data in order to produce control maps which can directly be
- used in astronomical image-processing packages like Drizzle,
- <pkg>sci-astronomy/sextractor</pkg> or <pkg>sci-astronomy/swarp</pkg>.
+WeightWatcher is a program that combines weight-maps, flag-maps and
+polygon data in order to produce control maps which can directly be
+used in astronomical image-processing packages like Drizzle,
+<pkg>sci-astronomy/sextractor</pkg> or <pkg>sci-astronomy/swarp</pkg>.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/zebra/metadata.xml b/sci-astronomy/zebra/metadata.xml
index ba10176c2..b9760ac17 100644
--- a/sci-astronomy/zebra/metadata.xml
+++ b/sci-astronomy/zebra/metadata.xml
@@ -6,20 +6,20 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- The Zurich Extragalactic Bayesian Redshift Analyzer is a software to
- compute and analyze photometric redshifts of galaxies.
- ZEBRA combines and extends several of the classical approaches to
- produce accurate photometric redshifts down to faint magnitudes. In
- particular, ZEBRA uses the template-fitting approach to produce
- Maximum Likelihood and Bayesian redshift estimates based on:
- * An automatic iterative technique to correct the original set of
- galaxy templates to best represent the SEDs of real galaxies at
- different redshifts;
- * A training set of spectroscopic redshifts for a small fraction of
- the photometric sample, to improve the robustness of the
- photometric redshift estimates; and
- * An iterative technique for Bayesian redshift estimates, which
- extracts the full two-dimensional redshift and template likelihood
- function for each galaxy.
+The Zurich Extragalactic Bayesian Redshift Analyzer is a software to
+compute and analyze photometric redshifts of galaxies.
+ZEBRA combines and extends several of the classical approaches to
+produce accurate photometric redshifts down to faint magnitudes. In
+particular, ZEBRA uses the template-fitting approach to produce
+Maximum Likelihood and Bayesian redshift estimates based on:
+* An automatic iterative technique to correct the original set of
+galaxy templates to best represent the SEDs of real galaxies at
+different redshifts;
+* A training set of spectroscopic redshifts for a small fraction of
+the photometric sample, to improve the robustness of the
+photometric redshift estimates; and
+* An iterative technique for Bayesian redshift estimates, which
+extracts the full two-dimensional redshift and template likelihood
+function for each galaxy.
</longdescription>
</pkgmetadata>
diff --git a/sci-astronomy/zpeg/metadata.xml b/sci-astronomy/zpeg/metadata.xml
index 921c2c050..fbf281467 100644
--- a/sci-astronomy/zpeg/metadata.xml
+++ b/sci-astronomy/zpeg/metadata.xml
@@ -6,10 +6,10 @@
<name>Gentoo Astronomy Project</name>
</maintainer>
<longdescription lang="en">
- Z-PEG is a software anybody can use to compute photometric
- redshifts. In short, Z-PEG performs a chi square minimization of the
- distance between observed photometric bands and synthetic photometry
- from galaxies simulated by the evolutionary code PEGASE.
+Z-PEG is a software anybody can use to compute photometric
+redshifts. In short, Z-PEG performs a chi square minimization of the
+distance between observed photometric bands and synthetic photometry
+from galaxies simulated by the evolutionary code PEGASE.
</longdescription>
<use>
<flag name="gdl">Install GDL/IDL plotting routines</flag>