• No se han encontrado resultados

CCD image processing of messier objects caught from astronomical observatory of the UTP

N/A
N/A
Protected

Academic year: 2020

Share "CCD image processing of messier objects caught from astronomical observatory of the UTP"

Copied!
6
0
0

Texto completo

Loading

Figure

Figura  1.  Telescopio  del  Observatorio  Astronómico  de  la  Universidad Tecnológica de Pereira
Figura 4. Montaje realizado para la captura de las imágenes.
Figura 6. Fotografía de la Nebulosa Anular de la Lira en color  azul, después de la sustracción de Darks, Flats y Bias
Figura  10.  Nebulosa  Dumbell  M27  en  la  constelación  de  Vulpécula.  Fotografía  RGB  con  50s  de  exposición
+2

Referencias

Documento similar

From an image processing point of view there are four main problems involved in 3D reconstruction using electron microscopy data:.. r Biological material is very sensitive

Due to the very small plate scale of the CCD cameras (1 pixel corresponds to about 50 arcseconds), any effects onto the seeing from turbulence due to the large temper- ature

This will open a the same window as to load an image from catalogs, but with the objects catalogs list.. Once the catalog choosen, the image properties will be displayed in the

 CAMELOT: Optical CCD offering a 10.4 arcmin field with a 0.3 arcsec pixel scale.  TCP: Tromsoe high-speed

[r]

This work describes the design and implementation of a new software framework, Scipion, that models image processing in electron microscopy allowing the integration of several

To do that, we have introduced, for both the case of trivial and non-trivial ’t Hooft non-abelian flux, the back- ground symmetric gauge: the gauge in which the stable SU (N )

Frontal and profile images and voice recordings collected from a clinical population of 285 males were used to estimate the AHI using image and speech processing