Astronomy - USA (2022-06)

(Maropa) #1

WWW.ASTRONOMY.COM 57


to fill in the small gap. Several are avail-


able online and work well.


The IMX 455 CMOS chip is the first


to capture data in true 16 bits. Most cam-


eras use chips that capture data in 14 bits


and interpolate up to 16 bits. True 16-bit


data has an incredible number of tonal


values so stretching can be performed


without the image falling apart. By cap-


turing in 16 bits, you have the full range


of 65535 density levels, which allows you


to pull out more detail during process-


ing. If you’re simply stretching 8-bit data,


it doesn’t look good because of the lim-


ited number of tonal values.


The QHY 600 is available in both


mono and color versions, and in a variety


of configurations depending on how you


plan to use the camera. I spoke at length


about shooting color versus mono in my


review of the QHY 410C color camera,


which appeared in the February issue.


To sum it up, traditionalists like myself


prefer shooting mono with separate fil-


ters for the RGB and narrow bands.


It does get a bit more complicated,


however. A color camera records all


colors simultaneously utilizing a Bayer


matrix. This makes creating colored


images a lot easier and can be an advan-


tage for imaging certain objects, like


comets. If you are used to working with


a mono CCD camera, the switch to a


CMOS mono camera should not be


difficult.


The one difference that I have found


between the two is that because CMOS


has such low noise, you only need RGB


exposures to create an image, with no


luminance exposure required. If you feel


you do need a luminance, you can fabri-


cate one by averaging all the color data.


Due to the large size of the files and


the fast download


speeds, QHYCCD built


in a 2-gigabyte DDR3


image buffer to smooth


data transfer to the host


computer. The data


from the QHY 600, in


addition to its real 16-bit depth, are also


true raw data, meaning the recorded


data have undergone no adjustments,


such as noise suppression or hot pixel


removal. It is the original signal, which


can be processed and manipulated as the


situation necessitates. The camera has


one other great feature: There’s zero


amplifier glow even with extended expo-
sure times.
Dew, condensation, and ref lections
have always been problems with digital
cameras. The QHY 600 addresses them
with a desiccant plug for the hermetically
sealed CMOS chamber, high-end anti-
ref lective coatings on all glass surfaces,
and a heater to keep external windows
moisture-free. The sensor is cooled by a
regulated two-stage thermocouple device
to maintain a constant temperature.

Creating images
I try to keep my processing as simple
as possible, yet I sacrifice nothing in

producing the final results. I use MaxIm
DL for my initial processing: the creation
of master darks, f lats, and bias frames. I
also use it to reduce and combine all my
data files. I find that the sigma combine
function works great to maintain as
much information as possible and still
remove outliers like hot pixels. Be careful
with these. Some hot pixels change value
so that the dark frame does not remove
them completely. You need outlier rejec-
tion and at least five frames to affect
their removal.
After creating the master files, I save
them as a 16-bit TIFF file. I then import
it into Photoshop, stretching it with
curves or levels to bring out all the detail.
CMOS data have such low noise that cer-
tain plug-ins work wonders. These typi-
cally are Luminar, Topaz II, and the real
secret weapon, the sharplet filter in the
Redfield suite. There are numerous star
reduction methods, which include Russ
Croman’s Star Shrink and the minimum
filter in Photoshop. In all cases, I use
these powerful tools with the stars
selected and feathered.
Large stars can be reduced using the
liquefy filter and choosing the pucker
tool. If it sounds like there are a lot of
tricks to make striking images, you’re
right. But the challenge can be part of
the fun.
If noise does show up in your image,
it’s usually in the shadows. Make a dupli-
cate layer, generously apply the noise

The optional filter
holder is seen here,
attached to the
QHY 600. QHYCCD

PRODUCT


INFORMATION


QHY600PH


Sensor: Sony IMX455 back-illuminated
Sensor size: 36mm x 24mm (full frame)
Image buffer: 2 gigabytes
Pixel size: 3.76x3.76 micrometers
Effective pixel area: 9576x6388
Output: 16-bit with 65535 levels
Exposure range: 40ms to 3600s
Computer interface: USB 3.0
Weight: 30 ounces (850 grams)
Dimensions: 5.2 x 3.5 inches
(131.8mm x 90mm)
Price: $4,599
Free download pdf