Methods Eye (visible window) Camera – film Camera – CCD (Digital)

1. Collecting Electromagnetic Information Methods Eye (visible window) Camera – film Camera – CCD (Digital)

2. Collecting Electromagnetic Information Eye (visible window) Advantages: Everyone wants to see objects directly Disadvantages: Light gathering capability – can see without telescope down to magnitude 6 Image cannot be stored Cannot do a time exposure

3. Collecting Electromagnetic Information Camera – film Advantages: * Inexpensive * Can do a time exposure Disadvantage: * Resolution * Cannot be conveniently manipulated * Deterioration * Long Exposure Times

4. Collecting Electromagnetic Information Camera – CCD (Digital) Advantages: Resolution Can do a time exposure Can store directly to a computer Can be manipulated Short Exposure Times Disadvantages Expense Pixilated Image

5. Collecting Electromagnetic Information – Digital Processing Raw Image Mask Processed Image of a comet Raw Image Processed Image

6. Comparison – Film vs CCD The Advantages of CCD Imaging Professional astronomers have been using CCDs for nearly two decades and have no thoughts about going back to film.  The advantages are impressive: * CCD cameras are up to 100 times more sensitive than film * CCD images are digital, meaning no film-processing, scanning, scratching, or fading * CCD cameras have a much greater dynamic range than film, meaning they can more easily capture both faint and bright detail in a single exposure * CCDs are capable of resolving finer detail than film (this can, however, be limited by the telescope used and the atmospheric conditions) For the amateur, several other advantages apply as well: * Taking images with a CCD is generally much easier than with film * Learning goes faster due to the ease-of-use and shorter exposure times * Light pollution is less obtrusive and more easily removed from CCD images, meaning imaging from a backyard site is more likely to be possible with CCD

7. Comparison – Film vs CCD Efficiency and Exposure • Efficiency • * A CCD can record as much as 90% of the incident photons • * Film will record less than 5% of the incident photons • CCD will record object 10 to 20 times fainter than film with the same exposure time • Exposure Times • * CCD can record the same image with less than one tenth of the exposure time for film

8. Comparison – Film vs CCD Exposure Above:On the left is a CCD image taken from a suburban location.  The exposure time is about 30 minutes.  On the right is a film image of the same object taken using a similar telescope.  The exposure time is over 2 hours and the level of detail is far less than the CCD image.  At full resolution the difference is even more impressive.

9. Comparison – Film vs CCD Format The Advantages of Film The single biggest advantage of film (at present) is format.  A 35mm film frame is 35mm x 26mm in size.  Amateur CCD chips are typically less than 15mm across.  This means that, on a given telescope, more of the sky can be captured at once with film.  This is an advantage since many deep-sky objects are very large in apparent size.  However, CCD chips as big as (or even bigger than) 35mm film are becoming available to advanced amateurs.  It is only a matter of time before these are available at a price within reach of the average amateur. Above:  A comparison of the size of a 35mm film negative with a relatively large amateur CCD chip (Kodak's KAF-3202 used in the SBIG ST-10 camera).

10. Comparison – Film vs CCD Resolution Figure 1.   Replica (via a high quality microscope) of a test pattern recorded on 35mm Fuji Provia film using prime lens optics at f11.  The highest resolved grid is indicated by the arrow (at column 1, row 3).  It has 75 line pairs per mm, or about 2700 line pairs across the 35mm film.  The contrast is about 10% (vs. 100% for pure black to pure white).  In the row 0 column 2 pattern the contrast is about 50% or 5 times greater.  Figure 3.  Magnification of the central part of the Cool Pix 5000 5.2 megapixel digital camera resolution image.  Item col 0, row 3 (i.e. 0/3) is resolved (IMHO, in the same sense as the film doing 1/3).  However, note the LACK OF GRAIN NOISE in the digital picture (compare with figure 1).  Clean grain-free digital images are an advantage that helps make prints than would normally be associated with film at a given resolution.

11. Comparison – Film vs CCD Price A CCD camera with the format and resolution of a piece of 35mm film costs much more than a film astrophotography setup.  However, most people are willing to sacrifice format for the speed and convenience of a CCD camera.  Unless large prints are going to be made, CCDs can otherwise outperform film in almost every aspect.  These days most people simply view images on a computer monitor, email images to friends, or post pictures on websites; for these purposes, small images are sufficient. For the amateur whose goal is to take pretty pictures of the night sky, a high-quality, entry-level CCD offers many advantages at a cost very comparable to film imaging.  A quick look at the websites of the most prominent astrophotographers in the world will show that they have invested as much in film as most CCD users have invested in their setups.  It will also show that most astrophotographers have begun shooting CCD images as well!

12. Photometry Photometer – An instrument which measure the brightness of an object Will measure the TOTAL brightness of an object, which might be difficult to interpret. However, when combined with filters, can be used to measure the amount of light produced over a narrow range of frequencies. This can be compared with standard Blackbody radiation curves to determine the temperature of the object

13. Photometry Photometer – An instrument which measure the brightness of an object Will measure the TOTAL brightness of an object, which might be difficult to interpret. However, when combined with filters, can be used to measure the amount of light produced over a narrow range of frequencies. This can be compared with standard Blackbody radiation curves to determine the temperature of the object Intensity X Wavelength

14. Photometry Photometer – An instrument which measure the brightness of an object Will measure the TOTAL brightness of an object, which might be difficult to interpret. However, when combined with filters, can be used to measure the amount of light produced over a narrow range of frequencies. This can be compared with standard Blackbody radiation curves to determine the temperature of the object Intensity X Wavelength

15. Photometry Photometer – An instrument which measure the brightness of an object Will measure the TOTAL brightness of an object, which might be difficult to interpret. However, when combined with filters, can be used to measure the amount of light produced over a narrow range of frequencies. This can be compared with standard Blackbody radiation curves to determine the temperature of the object Temperature of object is 7000 K Intensity X Wavelength

16. Spectroscopy Revisited Spectroscopes can be used to analyze the image through the eyepiece. The spectra can then be viewed with the eye, a camera, or a CCE for analysis.