[211] | 1 | Duchamp version 1.0.7 (2006/11/22) |
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| 2 | ---------------------------------- |
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| 3 | |
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| 4 | One new feature, and some improvements and bug-fixes. |
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| 5 | |
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| 6 | * The user can now elect to Hanning-smooth the spectral direction of the cube |
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| 7 | before the searching is done. This can be done instead of the wavelet |
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| 8 | reconstruction (although if both are selected, the reconstruction takes |
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[215] | 9 | precendence). This functionality is switched on and off by the flagSmooth |
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| 10 | parameter, and the width of the Hanning kernel is governed by the |
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| 11 | hanningWidth parameter. |
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[211] | 12 | |
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| 13 | * The smoothed array can also be written to a FITS file and read in at the |
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| 14 | start in the same manner as the reconstructed array. |
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| 15 | |
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| 16 | * Several improvements have been made to the memory management. Several |
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| 17 | memory leaks were fixed, and the memory usage of Duchamp is considerably |
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| 18 | less, which will be a help for running it on large cubes. The speed of |
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| 19 | some routines has also been improved, by removing unnecessarily repetitive |
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| 20 | loops. |
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| 21 | |
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[215] | 22 | * The sorting routines have been changed, and should now be slightly quicker |
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| 23 | (and a bit more robust). |
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| 24 | |
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[211] | 25 | * Enabled the scale bar (plotted on the 0th moment map in the spectral output |
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| 26 | file) to be able to deal with much finer spatial scales (as may be expected |
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| 27 | from VLBI data). |
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| 28 | |
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[215] | 29 | * Other minor changes to code and presentation. |
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[211] | 30 | |
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| 31 | |
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[194] | 32 | Duchamp version 1.0.6 (2006/11/01) |
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| 33 | ---------------------------------- |
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| 34 | |
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| 35 | Some incremental improvements and changes to the code: |
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| 36 | |
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| 37 | * The statistics used for the detection are now calculated once for |
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| 38 | the entire cube, rather than being calculated separately for each |
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| 39 | channel map and spectrum. This results in a uniform threshold value |
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| 40 | across the entire cube. The way the statistics calculations are |
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| 41 | implemented in the code was changed, using a new statistics class. |
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| 42 | |
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| 43 | * This means we can report a peak signal-to-noise value for each |
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| 44 | detection. This is given in the text-based output, as well as in the |
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| 45 | summary information above the spectral output for each source. |
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| 46 | |
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[195] | 47 | * The user can now elect not to have the moment map displayed in a |
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| 48 | PGPlot window, through the use of the new flagXOutput |
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| 49 | parameter. This should help in cases of running Duchamp on a dumb |
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| 50 | terminal (with no X-display capabilities), or as part of a batch |
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| 51 | script where the continual popping-up of the PGPlot window might |
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| 52 | become annoying. |
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| 53 | |
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[194] | 54 | * There a different Flags reported for the case of an object lying on |
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| 55 | the spatial edge and spectral edge of the cube (E and S respectively). |
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| 56 | |
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| 57 | * A few minor bug fixes: |
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| 58 | - When providing a subsection, any axes with the range given by * |
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| 59 | had the pixel values offset incorrectly. This has been fixed. |
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| 60 | - Negative searches now correctly invert the reconstructed array |
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| 61 | when it is read in from a file. |
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| 62 | |
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| 63 | * Other minor changes to the code, to improve memory handling and |
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| 64 | remove redundant arrays and variables. |
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| 65 | |
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| 66 | |
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[146] | 67 | Duchamp version 1.0.5 (2006/09/06) |
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[142] | 68 | ---------------------------------- |
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| 69 | |
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[146] | 70 | Since version 1.0, there have been a range of mostly minor |
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| 71 | changes. These are generally bug-fixes, thanks to feedback from a |
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[157] | 72 | number of users, as well as a few extra features. |
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[146] | 73 | |
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[157] | 74 | Here is a summary of the changes since version 1.0: |
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[142] | 75 | |
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[157] | 76 | USER INTERFACE: |
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[146] | 77 | |
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[142] | 78 | * The user is now able to enter the value of flag parameters in the |
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| 79 | parameter file as strings, as well as integers (so one can enter |
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| 80 | true or 1 to give the same result). |
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| 81 | |
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[157] | 82 | GRAPHICAL OUTPUT: |
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| 83 | |
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[142] | 84 | * Added a new function that draws the edge of the blank region on the |
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[146] | 85 | maps and image cutouts. There is a new flag parameter -- |
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| 86 | drawBlankEdges -- that controls the use of this function (the |
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| 87 | default is true). |
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| 88 | Also, the edge of the field is plotted on the image cutouts as a |
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| 89 | yellow line. This distinguishes it from the purple blank pixel |
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| 90 | dividing line. |
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[142] | 91 | |
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[146] | 92 | * The size of the tick mark in the image cutout (indicating the |
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| 93 | spatial scale of the image) is now adaptable, so that it shows the |
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| 94 | scale that best fits the image (ranging from 1 arcsec to 15 |
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| 95 | degrees). (This is a change from the previous standard length of 15 |
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| 96 | arcmin.) |
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[142] | 97 | |
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[113] | 98 | * The zoomed spectrum had its flux scale determined by all points in |
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[146] | 99 | the zoom box,including those flagged by the Milky Way (MW) |
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| 100 | range. This has been fixed so that any MW channels will not affect |
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| 101 | the flux scaling, potentially improving the appearance of objects |
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| 102 | detected close in velocity to strong MW emission or absorption. |
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[112] | 103 | |
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[157] | 104 | * Improved Karma Annotation file output, so that files without good |
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| 105 | WCS are dealt with appropriately. |
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| 106 | |
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| 107 | TEXT-BASED OUTPUT: |
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| 108 | |
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[113] | 109 | * The position resolution in the IAU-format names has been increased, |
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| 110 | so that distinct objects close to one another are more readily |
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| 111 | distinguished. Overlapping sources at different velocities may |
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| 112 | still have the same name, but this is a more general problem. |
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[112] | 113 | |
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[146] | 114 | * The presentation of the results in tabular format has been improved, |
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| 115 | so that the precision of faint sources is sufficient to show their |
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| 116 | flux, for instance, is not 0. This also applies to the information |
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| 117 | presented above the spectral plots. |
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[112] | 118 | |
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[146] | 119 | * Improved error and warning reporting, so that the formatting and |
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| 120 | presentation of information is clearer. |
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| 121 | |
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[157] | 122 | FITS I/O RELATED: |
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| 123 | |
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[172] | 124 | * The previous version was did not deal well with 4 (or greater) |
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| 125 | dimensions in the FITS file -- the memory allocation was badly done, |
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| 126 | and the axes needed to be in a particular order. This has been |
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| 127 | fixed, so that the FITS I/O routines can now handle any sized FITS |
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| 128 | file, with axes in any order (as long as there are two spatial and one |
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| 129 | spectral axes). |
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[157] | 130 | |
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| 131 | * When the FITS file does not have a rest frequency defined, there is |
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| 132 | no way to transform the frequency axis into velocity. In this case, |
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| 133 | the spectral axis is left as frequency, and put into units of MHz. |
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| 134 | |
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[172] | 135 | * If the beam size is not indicated by the FITS header (through the |
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| 136 | BMAJ and BMIN keywords), the user can manually specify the size |
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| 137 | through the parameter file (using parameter beamSize). |
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| 138 | |
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| 139 | * The FITS I/O routines make use of the command fits_file_exists. This |
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| 140 | was introduced into the CFITSIO package from version 2.5, so Duchamp |
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| 141 | will only work with this version or higher. Version 3+ is preferred. |
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| 142 | |
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[157] | 143 | OTHER BUG-FIXING: |
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| 144 | |
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| 145 | * Several bugs related to the blank-pixels were dealt with. |
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| 146 | The correct values were not propagating through correctly, meaning |
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| 147 | that the default values were being used. Also, there was the |
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| 148 | potential for blank pixels to be detected when the FDR method was |
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| 149 | used. Finally, the image cutout displays occasionally did not |
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| 150 | obscure the blank pixels. All these problems should be fixed now. |
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| 151 | |
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| 152 | * The FDR setup routine was occasionally failing with a segmentation |
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| 153 | fault, due to it accessing unallocated memory. This has been fixed. |
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| 154 | |
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| 155 | * Fixed bugs that affected the way 2D images (rather than 3D cubes) |
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| 156 | were dealt with. The minChannels test failed when minChannels=0. |
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| 157 | |
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[165] | 158 | * If there is no beam information in the FITS header, the user can now |
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| 159 | enter a beam size as a parameter. |
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| 160 | |
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[146] | 161 | * Other minor fixes to the code, to improve its structure and |
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| 162 | robustness. |
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| 163 | |
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| 164 | |
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[112] | 165 | Duchamp version 1.0 (2006/06/30) |
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| 166 | -------------------------------- |
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| 167 | |
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[113] | 168 | The first full release version. |
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| 169 | |
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| 170 | Several major changes compared to previous version: |
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| 171 | |
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| 172 | * Incorporated a FitsHeader class, to keep track of header information |
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| 173 | (including WCS) from the FITS file. All units-related calculations |
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| 174 | are done with this class, such as conversion to velocity, and |
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| 175 | pixel-to-WCS conversion. The main advantage of this is improved |
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| 176 | speed of execution, more adaptable to different units, and improved |
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| 177 | code (easier for me!). |
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| 178 | |
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| 179 | * Able to select the dimensionality of the reconstruction, rather than |
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| 180 | just doing it in 3-D. |
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| 181 | |
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| 182 | * Robust text output, so that the columns are sized correctly given |
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| 183 | the data being written, and the relevant units (derived from the |
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| 184 | FITS header) are included in the output table. |
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| 185 | |
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| 186 | * Improved the way the reconstructed image is saved and read back in, |
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| 187 | with a better naming scheme and a better set of new FITS header |
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| 188 | keywords. The MW headers are now not written. |
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| 189 | |
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| 190 | Other, more minor changes include: |
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| 191 | |
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| 192 | * MW channels now not set to 0, but just ignored for searching |
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| 193 | purposes (and for the scaling of the spectral output -- they are |
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| 194 | plotted though and highlighted with a hashed box). |
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| 195 | |
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| 196 | * The scale bar in the moment map in the spectral output file has its |
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| 197 | length indicated. |
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| 198 | |
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| 199 | * Improved VOTable output, with more information about the way Duchamp |
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| 200 | was run. |
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| 201 | |
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| 202 | * Made sure all statistics calculations in the reconstruction are |
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| 203 | based on robust (ie. median) methods. |
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| 204 | |
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| 205 | Also moved to an autoconf based configure/make compilation, for ease of use. |
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| 206 | |
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| 207 | |
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| 208 | Duchamp version 0.9.2 (2006/06/27) |
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| 209 | -------------------------------- |
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| 210 | |
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| 211 | * Added the use of warning flags for detections: for either edge |
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| 212 | location or negative enclosed flux. |
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| 213 | |
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| 214 | * A new command line option added so that the user can specify a FITS |
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| 215 | file to be searched with the default parameters, rather than giving |
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| 216 | a full parameter file. |
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| 217 | |
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| 218 | * The scale bar on the moment cutout now works in general case, using |
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| 219 | an iterative process to get to the correct length. |
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| 220 | |
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| 221 | * RA axes are now done correctly on the full-scale maps. |
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| 222 | |
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| 223 | * Various coding fixes, improving the readability of the code, |
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| 224 | particularly regarding the declaration of temporary variables. |
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| 225 | |
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| 226 | * Changed the way the time of execution is called : now using time.h |
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| 227 | functions, rather than a system call. |
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| 228 | |
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| 229 | * Changed output in Detection/outputDetection.cc for the pixel |
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| 230 | information of detected objects (the info printed above the spectral |
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| 231 | plots) -- now print out number of voxels in object, and have |
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| 232 | improved the formatting a little. |
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| 233 | |
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| 234 | * Improved the functionality of saving the FITS file containing the |
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| 235 | reconstructed array. Added ability to save and read back in the MW |
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| 236 | parameters when saving a reconstructed cube (if a reconstructed cube |
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| 237 | has different MW range to that being considered, it would cause |
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| 238 | problems). ReadRecon now just returns a FAILURE and will reconstruct |
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| 239 | the cube anew. |
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| 240 | |
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| 241 | * Changed default value of flagGrowth to 0. |
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| 242 | |
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| 243 | |
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| 244 | |
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| 245 | Duchamp version 0.9 (2006/05/05) |
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| 246 | -------------------------------- |
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| 247 | |
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| 248 | First public release version. |
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