StellarWindow „ Users' Guide „ Nebula display and setting


Click the eToolf icon located on the toolbar to open the setting dialog. Select gNebulash in the left column to open the nebula setting pane.

Nebula display

By default, gMessiersh are selected to be displayed and all of the celestial body groups are ticked.
As for the information overlay display feature, the box gOverlay namesh is not ticked.


Nebula display setting screen
Click the eToolf icon on the toolbar and select eNebulasf in the left column to open the setting screen.

Applicable celestial body groups
The desired celestial body type can be selected among the celestial body groups (i.e. nebulas, star clusters and galaxies) recorded in the Revised New General Catalog*1No celestial bodies are displayed if the box gNoneh is ticked.When selecting Messiers, what is able to be displayed is limited to Messier celestial bodies *2and celestial bodies with their photo recorded in StellarWindow*3 When selecting gAll,h all of those recorded in the Revised New General Catalog are displayed whether or not their photo is recorded in StellarWindow.

Celestial body group setting
Based on the Revised New General Catalog, celestial bodies are divided into small groups allowing you to determine which group is to be displayed and which is not.

Information display

The name of the desired nebula can be overlaid on the image appearing on the screen. A different display color can be selected for each display item. The box below is not ticked by default.


Information display setting screen
A different information display color can be selected for each celestial body group. A dark shade of purple is selected for all of the groups by default.


A different information display color can be selected for each celestial body group. A dark shade of purple is selected for all of the groups by default.
The information of the individual celestial body is displayed in the following order: common name, Messier number and NGC number. @

High-resolution photo delay load

Delay load of high-resolution photos allows you to determine whether or not to load high-resolution photos when the image of the desired nebula is enlarged. By default, this feature is disenabled in the Light Mode while it is enabled in the Standard Mode.
Delay load enables the use of high-resolution photos with the level of visual quality appropriate for observation when the image of the nebula is enlarged. Without performing delay load, low-resolution photos are used. This however does not use up extra memory therefore enabling StellarWindow to perform faster and lighter operations.
When using a small-size laptop with a small screen (i.e. net books), adequate resolutions may be obtained without performing delay load. Delay load is unlikely to be able to be performed in the case of an inadequate amount of remaining memory. It is not possible to perform delay load if the minimum installation (setup option) has been carried out or if no photos of nebulas and star clusters were installed during the customized installation *4 procedure as there is no applicable photo existing in these cases.


High-resolution photo delay load
Tick the box shown above if prioritizing the photofs visual quality over the operation speed (the box is ticked in the Standard Mode by default). If not, do not tick the box (the box is not ticked in the Light Mode by default).

Precautions concerning information display

In the case of a celestial body that has no photo recorded in StellarWindow and that is located according to the right ascension, celestial declination, azimuthal angle and elevation angle shown in the information display located in the upper left of the screen, the coordinates of such a celestial body correspond to those recorded in the Revised New General Catalog. In the case of a celestial body with its photo recorded in StellarWindow, however, the coordinates of the photofs center point, obtained after aligning the star chart and the photo, are displayed.
Please be aware that, depending upon the photofs trimming condition, the coordinates recorded in the catalog and the right ascension and celestial declination displayed on the screen may be misaligned for approximately one minute.
Please also note that the right ascension and celestial declination displayed on the screen refer to the coordinates of the crossover point obtained by connecting the individual selection markers*5and that the photo and the star chart have been aligned.


The right ascension and celestial declination of a celestial body with its photo recorded in StellarWindow
In the case of a celestial body with its photo recorded in StellarWindow, the right ascension and celestial declination displayed on the screen may differ from those recorded in the catalog.
*1 Revised New General Catalog
Covers a large number of deep space celestial bodies apart from stars.
ŠO•”ƒŠƒ“ƒN[ ADC ]
Expository writing [ wikipedia ]

*2 Photos
A number of photos of nebulas, star clusters and galaxies have been provided by Jim Misti of the Misti Mountain Observatory, United States.
I would like to take advantage of this opportunity to express our gratitude to Jim.

*3 Applicable celestial body groups
Please be aware that NGC celestial bodies with their photo recorded in StellarWindow are also displayed in addition to Messier celestial bodies.

*4 Setup options
Please refer to the gInstallation Guideh that comes with the product or thegAdditional information: Customized installationhfor further details concerning the setup options.
Please be aware that the high-resolution photos of nebulas and star clusters do not exist if the minimum installation has been carried out. It is optional not to install the high-resolution photos of nebulas and star clusters by using the customized setup procedure.
The high-resolution photos of nebulas and star clusters can be additionally installed later on.

*5 Crossover point of the selection markers

Refers to the crossover point of the direct lines that connect the individual red selection markers.
In the case of M90 shown above, the selection marker crossover point and the photofs rough center point are almost identical.

 
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