![]() ![]() In a future suggestion I will encourage the addition of other resources such as: In search by name or position there are three options: Yes, especially when we use the feature to access external data. (1) - There is probably many visualization feature that can be added. ![]() Then if the telescope coordinates are not available I can open a prompt to enter the coordinates or search for an object name (there is already as a function to call skychart to get the coordinates). What I can add to this software is the capability to open non-fits image, like jpg and png. The original idea is to help to center an object before capture, but this can be extended to other images. Then it can send the image to Skychart for display. My CCD capture software CCDciel already do plate solving using a local or other software. So I prefer to split your request in two parts, one to improve the display capability in Skychart and one to extend the plate solving function of CCDciel. In your screenshot I find very interesting to compare a star position from the image and from the catalog.īut I not want to transform Skychart in an image processing software.įor me the plate solving is part of the image processing because it is much more precise if done with the linear image, before stretching.īut if high precision is not require, like to show the image on the map, a stretched or jpeg image is OK. There is probably many visualization feature that can be added. I have in my Groups of Astronomy and Sky Photography encouraging much to use for the resources and possibility of using great catalogs like Gaia DR1, USNO B, NOMAD. I want to make a big public announcement of the Sk圜hart Software in Brazil so that it can be used in teaching Astronomy both for independent astronomers and in schools. Independent Astronomical Observatory Constellations of the South - Brazil. The list of catalogs is also very good and suggestion. We can make the location of the coordinates by the name of the OBJECT which greatly facilitates the process for beginners. The program that has apparently been discontinued X Parallax VIU has a very practical and functional mechanism of astrometry. It is important that the file or files selected for astrometry be able to be adjusted (brightness and contrast) and that the settings apply to the others. The program Astro ImageJ only makes in Mono and saves the result only in Mono it is important that the Sky Chart save in Mono and CUBE RGB. It is important to do astrometry in both FITS mono, FITS Cube, and other formats such as PNG, JPG, and others. ![]() It would be a good option to download reference FITS to use New Astrometry features.Īnother way is to use the site itself as it is done in the program Astro ImageJ in that using the "my API key" Astro Image J makes the process of Astrometry both automatic and with the selection of parameters. The suggested catalog and great catalog is the UCAC4 which is also suggested for Astrometry by MPC.įeatures and codes in Python can be used: In a second moment, you can report to the MPC. The more efficient it is, the more it will be valued. It will be used even more and for various astronomy. The Astrometry Resource in the Sky Charts will make the program take on a large dimension. 0001858: Implementation of Astrometry in images with Sky Chart. ![]()
0 Comments
Leave a Reply. |
AuthorWrite something about yourself. No need to be fancy, just an overview. ArchivesCategories |