|
Class Summary |
| AduHorizontalFit |
Takes a (multi-extension) fits file and reads it horizontal line per
horizontal line. |
| Aperture |
This class uses an recursive algorithm to determine the area of intersection
of a quadratic pixel with an arbitrary aperture. |
| Aperture.Circular |
Test the aperture class on a criculare aperture at center zero, zero and
with radius 1. |
| Aperture.Circular100 |
Test the aperture class on a circulare aperture at center 100, 100 and
with radius 10, for x,y = 0->200 |
| AptSite |
A Site implementation describing the location of Stella. |
| AsciiCatalog |
This class reads an ascii-file and parses it to a list of star description. |
| AsciiCatalog.BJG2004 |
Reads the stromgren catalog of NGC 1807 and 1817. |
| AsciiCatalog.FieldBy |
Reads the stromgren catalog of NGC 1807 and 1817. |
| AsciiCatalog.FieldC1 |
Reads the stromgren catalog of NGC 1807 and 1817. |
| AsciiCatalog.FieldM1 |
Reads the stromgren catalog of NGC 1807 and 1817. |
| Astro |
Class Astro contains certain routines, that are everyday's need in an
astronomer's life. |
| Astro.Distance |
Prints out the distance between two points. |
| Astro.HeliacalRise |
Prints the date when the sun rises with the target in Germany. |
| Astro.Jd |
Prints out current jd or, if a parameter is given, the jd of the date
given in the first argument. |
| Astro.Mjd |
Prints out current jd or, if a parameter is given, the jd of the date
given in the first argument. |
| BrightestStars |
Reads in the brightest star catalog (Ochsenbein 1988). |
| BrightStarCatalog |
Reads in the brightest star catalog (Ochsenbein 1988). |
| Broker |
A stand-alone code excerpt for static telescope brokerage. |
| Broker.Height |
Test the height of an astronomical object. |
| Broker.Sol |
Test the solar height. |
| ConstellationFactory |
A class to provide outlines of constellations as shapes. |
| ConstellationFactory.Hip |
A class to convert constellation input files that use HIP-numbers to
parsable SkyPath objects. |
| ConstellationShape |
A helper class that allows drawing the classical star constellations. |
| Convert |
Class containing several conversion routines often used in astronomical
context. |
| FindMultiplets |
A small class that reads a serialized catalog, roams through all entries
and checks for neighbours within a given distance and magnitude range. |
| GridShape |
A class that comprises a grid-line. |
| HauckCatalog |
Class to serialize Hauck 1997 Stromgren standards Hauck & Mermilliod,
A&AS 129, 431 (1998) into an object stream containing a list of
Stardescriptions. |
| HeaderCardDescriptor |
A helper class that bundles FITS-header cards into descriptors that can
then be resolved at run-time to provide true header cards. |
| HeliocentricJulianDate |
Command line tool to calculate a heliocentric julian date from FITS header
keywords or from command line options. |
| HipparchosCatalog |
Reads in the Hipparchos Star Catalog |
| HipparchosCatalog.SubSample |
Creates a sub-sample. |
| HtmIndex |
Simple class that allows working with the Hierarchical Triangular mesh index. |
| JulianDate |
The julian date converts java time stamps into jd and vice versa via its
inverse function. |
| Landolt92Catalog |
Class to serialize Landolt Johnson standards from AJ 104, 340 (1992)
into an object stream
containing a list of
Stardescriptions. |
| LightCurveSimulator |
Very simple program to simulate light curves. |
| LightCurveSimulator.Series |
Parses the command line and prints out a simluated light curve. |
| Location |
Class to represent observing sites. |
| ModifiedJulianDate |
The julian date converts java time stamps into jd and vice versa via its
inverse function. |
| MoonPosition |
A class calculating the position of the moon. |
| MoonPosition.Test |
Testing purpose mainly. |
| OrbitFit |
An orbit analyser takes radial velocity data and fits an orbit to it. |
| OrbitFit.File |
Reads the rv from a file. |
| OrbitModel |
The orbit model is the differentiable model that fits to a radial velocity
of an SB1 orbit. |
| OrbitModel.Calculate |
Supply the orbit parameters t0, P, e, omega, K1 and vB to the command
line to get the orbit solution for the specified time. |
| OrbitModel.Quadrature |
Calculates the phases of quadrature, defined as ν=±90, or, if
a second argument is given, which is then the argument of periastron,
as the times of maximum rv, which follows
from the defintion of rv to |
| OrbitModel.Test |
For testing. |
| PastelStar |
Uses the Pastel catalog to resolve a given name on the command line. |
| Position |
A class defining a position in the sky via right ascension and declination. |
| Precesser |
Class to do a simple precession. |
| RaDeParser |
A class that allows parsing of different formats of right ascension
and declination. |
| Resolver |
A class used to resolve targets by names, get their postions and field of
view. |
| Resolver.CatalogServlet |
Tries the servlet catalog method. |
| Resolver.NameServlet |
Tries the servlet resolve method. |
| Resolver.Print |
A simple test class. |
| Seeing |
A class providing some essential seeing properties. |
| Seeing.Motion |
Test the image motion part. |
| SextractorRead |
Class that reads sextractor files into a list of Sextractor stars. |
| SextractorRead.Wcs |
We convert a ICAT output sextractor file to a WCS input file, filtering
all non-stars out of the list. |
| SightInfo |
A small class that allows calculation of fundamental astronomical properties
of an object at a given location. |
| SightInfo.Print |
A class to test the main astronomical info. |
| SimpleSid |
Class to calculate the sidereal time for a given location and Date. |
| SimpleSite |
A helper class that implements the Site interface. |
| SimpleSol |
A class implementing SolarPosition. |
| SimpleSol.Test |
Test purpose. |
| SkyPath |
A sky path uses a Morphing object to convert a ra-dec path on
the sky to a pixel path. |
| SolarPosition.Plato |
Calculates the overlap between night time and target-above-horizon
for a full year. |
| SolarPosition.Test |
Test purpose. |
| SpectralFits |
This class deals with FITS file received as output from the SES spectrograph. |
| StarCatalog |
The object representing a resource-based catalog, like VizieR catalogs or
database catalogs. |
| StarCatalog.Distance |
For sorting star lists to distance of center. |
| StarCatalog.Test |
A test class. |
| StarDescription |
A helper class containing general information on a star. |
| StarDescription.StarComparator<T extends StarDescription> |
Gets a star definition comparator linked to the named property of the
star. |
| StarSextractor |
Star description derived out of sextractor output. |
| StarSextractor.PixelPosition |
Returns a comparator that sorts sextractor stars depending on pixel
distance from a certain central pixel, stated at construct. |
| StromgrenIndices |
This small class allows calculation of expected RMS in T_eff, Fe/H, and
log(g) determination from Stromgren indices (no H_beta necessary). |
| StromgrenIndices.FeH |
We use the provided uncertainties in Fe/H and b-y to calculate
uncertainties in T_eff from the Olsen list. |
| StromgrenIndices.LogG |
We use the provided uncertainties in Fe/H and b-y to calculate
uncertainties in T_eff from the Olsen list. |
| StromgrenIndices.Teff |
We use the provided uncertainties in Fe/H and b-y to calculate
uncertainties in T_eff from the Olsen list. |
| SunPosition |
A class calculating the position of the moon. |
| SunPosition.Test |
Testing purpose mainly. |
| TenerifeSite |
A Site implementation describing the location of Stella. |
| TruncatedJulianDate |
The julian date converts java time stamps into jd and vice versa via its
inverse function. |
| TychoCatalog |
Reads in the Tycho2 Star Catalog (Hog et al, A&A 355, L27). |
| TychoCatalog.SubSample |
Creates a sub-sample. |
| VizierStar |
This class converts a net.cds.Vizier.Table into a list of
StarDescriptions. |
| VizierStar.HipparchosUcac2 |
This class compares the hipparchos main catalogue with the UCAC2
catalogue. |
| VizierStar.Retrieve |
Mainly for testing the class. |
| WcsFit |
Tries to fit pixels pairs in a fits image to a WcsProjection that
minimizes the differences from the projected pixel pairs to the catalog
pairs. |
| WcsFit.Linear |
We solve for a wcs, reading the pixel pairs and the matched catalog
from an ascii file. |
| WcsFit.Parser |
|
| WcsFit.Polynomial |
We solve for a wcs, reading the pixel pairs and the matched catalog
from an ascii file. |
| WcsFit.PositionExchange |
To check if the uncertainty in the WCS determination is from the
sextractor positions, we take the IRAF positions as input for the wcs
fitter. |
| WcsFit.Residual |
This class tries to fit the residuals on command the command line |
| WcsFit.SigmaMaps |
Takes a valid WCS from a file plus a matched file and outputs the
sigma maps. |
| WcsFit.Stepper |
We solve for a wcs, reading the pixel pairs and the matched catalog
from an ascii file. |
| WcsFit.Variable |
We solve for a wcs, reading the pixel pairs and the matched catalog
from an ascii file. |
| WcsMatch |
We match the brightest stars found in an image at given x/y
coordinates to given catalog entries. |
| WcsMatch.Coarse |
Simple matcher class that takes an input catalog and matches it to a
(sextractor) output of positions. |
| WcsMatch.Test |
Test the method on a very simple system. |
| WcsModel |
A mapping of pixel coordinates to WCS coordinates, ICRS 2000 right
ascension and declination in almost any possible case. |
| WcsProjection |
A wcs projection normally converts pixel on the CCD to ra/de. |
| WcsProjection.EulerRotation |
A Euler rotation, defined by the coordinates of the native pole. |
| WcsProjection.Gnomonic |
The gnomic projection is the oldest known azimuthal projection. |
| WcsProjection.LinearGnomonicRaDe |
A combination from a full-linear projection from pixel space to
intermediate world coordinates, followed by a gnomic projection and
a euler rotation to get to ra and dec. |
| WcsProjection.LinearPixelProjection |
The linear transformation from pixel space to intermediate world
coordinates. |
| WcsProjection.PolynomialGnomonicRaDe |
A combination from a full-polynomial projection from pixel space to
intermediate world coordinates . |
| WcsProjection.PolynomialPixelProjection |
This now fits intermediate world coordinates from pixel coordinates
with Legendre polynomials such that the pixel coordinates are
slightly distorted
before calculating the intermediate coordinates. |
| WcsProjection.ReadWcs |
A test for reading and interpreting header cards that describe a pure
linear pixel-to-intermediate transformation, a gnomic projection
and finally a rotation to yield ra and dec. |
| WcsProjection.ThreeStepWcs |
A combination put together from three individual WcsProjections,
a pixel projection that transfers CCD-pixel into intermediate
world coordinates, a true geometric projection (like Gnomonic) and
a final rotation to yield coordinates in a known space. |
| WcsProjection.VariableGnomonicRaDe |
A combination from a full-linear projection from pixel space to
intermediate world coordinates with varying projection center. |
| WcsProjection.VariablePixelProjection |
It turned out, that the quality of the WCS solution is highly dependant
on the correct position of the native pole, rj. |
| WcsShift |
A class that deals with fits files having a valid WCS defined in their
header. |
| WcsShift.Shift |
Class to print out the fits-file name followed by pixel shift for
a central ra/de. |