Changes between Version 20 and Version 21 of glga_manual
- Timestamp:
- Aug 19, 2016, 9:13:00 PM (10 years ago)
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glga_manual
v20 v21 89 89 90 90 * Line-Styles and Colors: 91 * dotted [[span(style=color: #FF0000, red )]]ellipse: Photometry Aperture91 * dotted red ellipse: Photometry Aperture 92 92 * dotted sky blue ellipses: Photometry Annulus (used to estimate the background level/statistics) 93 93 * dotted yellow ellipses: The annulus that is not used for background estimations (when background regions are in use) … … 116 116 For all the buttons, you have a counterpart on the menu bar, but the opposite is not true. The letter in the parenthesis shows the short key to the same action, once you click on the image. A full set of all actions is also available on the terminal. 117 117 118 1. Change Mask: Generally, when drawing a new region to mask the image, it would be applied on all band, and its easier to look at the composite image (however you can still choose to look at other band and edit the common mask file). If a band is selected (and not a composite image), then you will have an opportunity to generate masks for the chosen band. The file that contains each band mask is sto [[span(style=color: #FF0000, red )]]separately. Under this button, you will see the status of the masking.118 1. Change Mask: Generally, when drawing a new region to mask the image, it would be applied on all band, and its easier to look at the composite image (however you can still choose to look at other band and edit the common mask file). If a band is selected (and not a composite image), then you will have an opportunity to generate masks for the chosen band. The file that contains each band mask is stored separately. Under this button, you will see the status of the masking. 119 119 {{{ 120 120 Current: All Bands: the generated mask would be used for all bands and it is displayed with Green color. … … 126 126 3. Undo Region: Removing the last added region. Currently this only works for common regions, i.e. green masks. 127 127 128 4. Remove a region: After clicking on this button you need to lick inside a region to remove it. This works for both band-masks and common-mask (i.e. Green and Pink regions). If the regions does not exist (in case of any mistake), the action would be igno [[span(style=color: #FF0000, red )]].128 4. Remove a region: After clicking on this button you need to lick inside a region to remove it. This works for both band-masks and common-mask (i.e. Green and Pink regions). If the regions does not exist (in case of any mistake), the action would be ignored. 129 129 130 130 5. Clean all regions: After user verification, it removes all the region. This works for both band-masks and common-mask (i.e. Green and Pink regions). 131 131 132 6. Save region: Normally all common-regions (Green reg.) would be saved after doing the measurement. However, once can save any change before doing the measurement. This is helpful when working with big galaxies. One should note that all band-masks are sto [[span(style=color: #FF0000, red )]]instantly and users should not be worried about saving their pink masks. This is because, we don not expect to have a lot of masking for each individual mask.132 6. Save region: Normally all common-regions (Green reg.) would be saved after doing the measurement. However, once can save any change before doing the measurement. This is helpful when working with big galaxies. One should note that all band-masks are stored instantly and users should not be worried about saving their pink masks. This is because, we don not expect to have a lot of masking for each individual mask. 133 133 134 7. Find Star: This helps to find stars and point sources by defining the proper PSF and limiting magnitude. the inputs must be ente [[span(style=color: #FF0000, red )]]in the terminal.134 7. Find Star: This helps to find stars and point sources by defining the proper PSF and limiting magnitude. the inputs must be entered in the terminal. 135 135 136 136 8. Delete Centeroid: Removing all the previously masked point sources inside a specified region. … … 142 142 143 143 144 10: ds9: Opens the fits file of the displayed image in the TV. If not band has been specified (in case of using the composite image), the use-file ('r' band for /sdss and /panstarrs) would be opened. In ds9, one can play around with the '[[span(style=color: #FF0000, red )]]' elliptical aperture, (e.g. re-center it, or resize it). The parameter of this '[[span(style=color: #FF0000, red )]]' aperture can be later on captu[[span(style=color: #FF0000, red )]]by GLGA TV and update the ellipse144 10: ds9: Opens the fits file of the displayed image in the TV. If not band has been specified (in case of using the composite image), the use-file ('r' band for /sdss and /panstarrs) would be opened. In ds9, one can play around with the [[span(style=color: #FF0000, red )]] elliptical aperture, (e.g. re-center it, or resize it). The parameter of this [[span(style=color: #FF0000, red )]] aperture can be later on captured by GLGA TV and update the ellipse 145 145 146 11: Contours On/Off: If ds9 is open, then isophots can be displayed. This helps to locate a proper border around the galaxy. To rotate the '[[span(style=color: #FF0000, red )]]'aperture, first select it by clicking inside it on ds9. You see four selection points around it. Press Shift-key on keyboard and choose one of the four point to rotate the ellipse by dragging the mouse. To move the ellipse, click and drag ...146 11: Contours On/Off: If ds9 is open, then isophots can be displayed. This helps to locate a proper border around the galaxy. To rotate the [[span(style=color: #FF0000, red )]] aperture, first select it by clicking inside it on ds9. You see four selection points around it. Press Shift-key on keyboard and choose one of the four point to rotate the ellipse by dragging the mouse. To move the ellipse, click and drag ... 147 147 148 148 [[Image(ds9_demo.jpeg, 30%)]] 149 149 150 12: Import Ellipse: To import the '[[span(style=color: #FF0000, red )]]'aperture from ds9 to the TV (when ds9 is open). All ellipse information would be updated and be used for the measurement. Note: ds9 can also be used a bridge between Pylipes (i.e. the python code to modify the ellipse) and GLGA TV. However, Saving (in Pylipse) and loading (in TV: Menu > Pyliupse > Load Ellipse) is a way to import from Pylipse to GLGA TV.150 12: Import Ellipse: To import the [[span(style=color: #FF0000, red )]] aperture from ds9 to the TV (when ds9 is open). All ellipse information would be updated and be used for the measurement. Note: ds9 can also be used a bridge between Pylipes (i.e. the python code to modify the ellipse) and GLGA TV. However, Saving (in Pylipse) and loading (in TV: Menu > Pyliupse > Load Ellipse) is a way to import from Pylipse to GLGA TV. 151 151 152 152 … … 155 155 14: Run SExtractor: Running SExtractor to update the ellipse information. If SExtractor has been already run and the information exists in the data-base, the GUI asks whether to use the previous results, or run SExtractor again. Note: one can run SExtractor automatically for the entire data-base, and if there is any adjustment needed, it is possible to re-run it in the TV. In this case, TV first creates a temporary masked image (applying both band-mask and common-mask files) and then runs SExtractor. This way one can take care of any foreground/background problems that could have been already resolved. Also there are other masking options just to run SExtractor (see: menu > SExtractor) 156 156 157 15: Edit Ellipse: Editing the ellipse parameter in the TV. To see all the options, look at the terminal and follow the right commands. Note: if in the middle of the editing, user clicks on any button on the control-panel, the ellipse editing action would be igno [[span(style=color: #FF0000, red )]]and the new command would be run.157 15: Edit Ellipse: Editing the ellipse parameter in the TV. To see all the options, look at the terminal and follow the right commands. Note: if in the middle of the editing, user clicks on any button on the control-panel, the ellipse editing action would be ignored and the new command would be run. 158 158 159 159 16: Original Ellipse: Use the original ellipse paramter and update the TV
