Collection of Emission, Planetary, and Diffuse Nebulae, Galaxies, and Comets
About Filters: Hydrogen alpha (Ha), doubly ionized oxygen (OIII) and ionized sulfur (SII) filters are used to record gas emission line nebulae from particular regions of our galaxy. Visible light from a narrow bandwidth (corresponding to a particular gas) is color mapped onto red (sulfur), green (hydrogen) and blue (oxygen) channels using the standard Hubble palette. In some cases, I used only the Ha filter (no color mapping). Narrowband filters effectively block the urban glow (street lamps, shopping malls, homes) and light reflected from the moon, significantly increasing S/N. Other images were obtained using conventional LRGB filters, with an Ha filter often used to enhance the hydrogen emission.
About the Images: Unlike planets, comets, and other solar system objects, deep sky objects are quite distant and faint. The closest nebulae are approximately 300-500 light years away, while the most distant object shown in this collection is 25 million light years away. Such distances require very extended camera exposure times - on the order of hours. Total exposure times for some objects are in excess of 7 hrs with 3-4 hrs being typical.
About the Equipment: These images were taken using a CCD camera from SBIG. The camera has two photosensitive chips (CCDs): a larger one to image the target object and a smaller one to lock on a nearby guide star for fine telescope position control to compensate for earth's rotation (over several hours). The camera body and filter wheel are attached a telescope and mounted on a sturdy German equatorial mount. All aspects of the imaging process (aiming, focus, guiding, filter selection, exposure time) are automatically controlled by a notebook computer.
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