REDUC TUTORIAL

Updates
V3.82-V3.85
Scrollbars for large images
Save RED...
Various optimisations
Visual selection of images (BestOf Vis)

V3.81-V3.82
NaN error fixed
The searchbox is apparent on images saved with Save->BMP ... : fixed

V3.75 - V3.80
AVI -> BMP Conversion Tool
Crop Image
Save an image series
Horizontal and Vertical swap
Binning x2
FITS 8 bits
Italian translation
V3.74, 3.74b
Internal improvements
V3.73
Dark and Bias preprocessing
New BestOf routines
False color optimisation
V3.71
Reads FITS 32 bits real (BITPIX=-32)
Automatic calculation of the sampling when using QuadPx
File list : Checkbox and Inv options
Logarithmic display
Popup tuning of visualization levels

V3.65b
Reads FITS 32 bits integer
Customizable cameras List
False color visualization
Mathematical Surface's image
New formatted EZReport
Last values of Delta, Epsilon & Pre-Orientation automatically reloaded
BestOf optimization
Bugs correction and optimization
Spanish Tutorial

V3.62
QUADPX
SURFACE


CONTENTS :
Presentation and basic features
  Loading
  Main window
  Files selection
  Sorting
  Centroiding !
  Calibrating
  Measuring
  Publishing
Advanced features
  Automated reductions
  Shift and Add features
  Automatic rejection
  Drift calibration (single frame)
  Drift calibration (multiple frames)
  Using QuadPx function
  Adjustment of a tridimensional mathematical surface
  Dark and Bias preprocessing
  Horizontal and Vertical swap
  Binning x2
Others features
  Language
  Visualisation levels
  Saving the images
  Save an image series
  Crop images
Customizing the camera list
Samples from the real life ! (FAQ)
  Useful Shifts and Adds

Presentation and basic features

Loading frames


File/Open


Select the frames you want to measure in the dialog box.
It is a classical multi-selection box.

Reduc can read :
- FITS 8, 16 & 32 bits integer, FITS 32 bits real
- Bitmap
- AVI

Select all files : Ctrl+A
Select consecutive files :click on the first file, keep the shift key pressed and click on the last file you want to select.
Select non consecutive files : click on the files with the control key pressed.

AVI -> BMP Conversion Tool

Select AVI in the File menu

Click Select AVI button in the conversion tool window and select the file to be converted.

 

Click the Convert button
Choose the library where you want the bmp files to be created and give a generic name for the files.
The generic name will be indexed automatically by Reduc.
The conversion tool close automatically after the conversion and you can now select the bmp files as explained in the previous chapter.

Main Window
Most of the work is done on this window, so we take a minute to localize some items


1 Title bar displays the current frame's name
2 The name of the selected frames are displayed in the list box. We will see further this list in details. The number of files selected is shown in grey (Sel : xx)
3 The frame is displayed here in its real size. If you shot a color frame, RVB channels are summed by Reduc and the frame will be displayed as a black and white one
4 Some stats about the frame
5 Bold, coordinates and intensity of the pixel under the mouse cursor
6 Level sliders for display (cf. Visualisation levels)
7 Zoom (4x) of the cursor area.Checkbox Inv inverses video of the zoom window
8 Settings of centroid detection
9 Section views of the last centroid
10 Star model
11 Auto reduction parameters (see Automated reductions)
12 Calibration on a star drift (single frame)
13 Calibration on a star drift (multiple frames)
14 The checkbox allows to check/uncheck all the files. Inv inverts the selection


Files selection

All automated functions except BestOf are applied only to the checked files.
The frames can be selected and deselected with a click in the checkbox.
To select/deselect quickly a set of of frames just hold the left button pressed and move the mouse on the list.


Sorting the frames
It's very easy to obtain many frames in a short time.
At the time of reduction it could be better to select only the best ones. Reduc offers a feature to sort the frames by selecting Processing / BestOf in the menu bar.The file list is sorted from the best to the worse and the best frame is loaded immediatly.
Reduc sorts all the frames in the list, checked or unchecked. However it doesn't change the state of the check marks.

In order to adapt to the various configurations of Reduc users, two options are available according to the type of pictures acquired:

BestOf (Max) grants the priority to the central concentration, the central pixel has a large influence, it is recommended for low noise frames and small stars images. Generally obtained with short focal length and/or short integration time.
Bestof (S/N) gives privileges the S/N ratio and the density of the star. It is generally recommended when the stars show a noticeable disk or with noisy frames. Generally obtained with long focal length and/or long exposure time.

The results between the two routines can be very different. Try and choose the one that gives the best results with your own images.


Centroiding !
Two clicks for a centroid :
Click on a star. Reduc draws a detection box (green square)
around the star and estimates its centroid. If this deduction
is ok for you, a right click will memorize it.
Do the same thing with a second star.
   

Many things happen with these two clicks. Let's see :
- First the detection box is showed as a green box. Its size can be modified from 3x3 to 61x61 pixels with the horizontal trackbar. 13x13 is a convenient setting for most of my images so I put it as default.
Reduc estimates a new centroid each time you change the size of the detection box.
- If Automatic is checked, you can click very approximately (in a range about one time the box size), Reduc will find the star centroid correctly.
- Checking Manual forces Reduc to search the centroid in a range of only the box size (and forces you to click on the star). Automatic is the default value but Manual can be useful for tight double stars, it avoids Reduc searching the brightest centroid when you want to measure the secondary component.




- The Yellow Window shows a section view of the star. The colors match the two axis colors of the zoom window. Max, Moy, Min are the maximum, average and minimum pixels value inside the detection box. Seuil is a threshold value from which pixels are considered as significant for Reduc's centroid algorithms. This value is imaged by an horizontal dotted line which can be dragged to change Seuil value. Moving the line forces Reduc to re-model the star and reestimate the centroid.
Vertical dotted lines are the limit of the detection box.
When the modl is ok for you you can right click in the yllow area and Reduc will save this centroid instead of its own estimation.
At each new star Reduc reestimates its own value. Automatic estimation by Reduc is almost always the best one for webcams images.
Vertical dotted lines reprsents the limits of the detection box.

- Ctl Adj forces Reduc to consider only adjacent pixels when modelling. It is very useful (necessary !) with low signal/noise images. Checked is the default value.
It can be unchecked if your stars are very spreaded.

- The Green Window is the modelling window. The star is as Reduc "sees" it.

The first right click opened a window named Reduction. It has some specific features and we'll see them before all.

1 Camera selection list. The last camera used is recalled at the next start of Reduc.
2 Pixels size. Pixel size is automatically selected when changing camera. The camera list can be customized at your needs by clicking the [...] button.
3 Quadrants orientation. Default quadrants orientation is North up and East left. Switch from one to others orientations by clicking the buttons labelled N,S,E,W in Pre-orientation section . Give here a rough image orientation. The important thing is the succession of the quadrants.
4 Centroid coordinates and an indication of the star intensity.
5 Actual mode (Calibration mode or Measurement mode)
6 D = image inclination regarding the celestial equator. Automatic calculation in Calibration mode.
7 E = pixel sampling. Automatically calculation in Calibration mode.
8 q= position angle of the double star. Automatic calculation in Measurement mode.
9 r = double star separation in arcsec. Automatic calculation in Measurement mode.
10 dM is a difference of magnitude estimation. I say estimation, this value is not fairly reliable with webcams (maybe cause some problems of linearity ?). Seems fairly good with CCD.
11 s= standard deviation for theta and rho (these values aren't significative in Calibration mode)
12 Tabs of the reduction sheets.
13 Menu options :
- Add to log = save the reductions into a log file (see Publishing)
- Clear = clear both reduction sheet (a message box will prevent accidental click !). Must be used each time you change of couple. Constant value (camera, pre-orientation, D, E) are preserved.
- Sort = Many sorting options of the reduction sheet and an automatic rejection option are available.






Reduction sheets :

The first tab (Raw) activates the sheet of raw data. (xA,yA,intA) are coordinates and intensity estimation of the first component, (xB,yB,intB) of the secondary component. Last column is the name of the frame.
The second tab (Reduced) activates the sheet of reduced data. Here are individual reductions for each frame with theta, rho, estimated mag difference and theta and rho residues (individual measurement minus mean).
In the both sheets a click on a row recalls the corresponding frame in the main window.
A color code give some information about the measurements dispersion in the second sheet :
Green residues <= 0.674 s
Blue residues are >=0.674 s and < 2 s
Fuchsia >= 2 s
Take a look at right. Obviously, the last frame has a (hmmm) problem with theta and rho residues far greater than others frames in the set. Maybe a very bad frame, maybe an awkward click when measuring, who knows ? Click on the row, you can now suppress this measurement with the 'Delete' option on right click. When selecting the row, the frame has been recalled in the main window, you can now re-measure it if you want.

 




Calibrating
Before reducing we need some informations :
- Quadrants orientation
- Relative pixel size (l x h)
- Precise image orientation
- Sampling (number of arcsec/pixel)

From a standard star :
- Reduc will compute image orientation
- Reduc will compute the sampling

You must give :
- Characteristics of the calibration star

HOW TO PROVIDE CALIBRATION PARAMETERS


Select Calibration to switch Reduc in Calibration mode
Provide Theta and Rho of the calibration star (Reduc recomputes on the fly the new parameters as soon as you introduce new values).

When using several standard stars for an imaging session (recommended), repeat the entire procedure of calibration for each star and compute (manually) the means of D,E. These means will be reintroduced when switching to Measurement mode.

Calibration with a calibration star

It is the same procedure than a simple reduction.
- Load the set of images
- Reduce it manually or automatically

When the reduction is finished :
- Select Calibration is the reduction sheet
- Type the theta and rho values of the calibration star

The parameters are computed and introduced in D and E.

Reduc recomputes all that is necessary immediately when you type new values.

Don't forget to click on Measure before measuring !

NOTE : The second reduction sheet (Reduced tab) can't be displayed when in Calibration mode


Instrumental constants already known

You can type D,E at any time when you are in measurement mode.

Reduc recomputes all that is necessary immediately when you type new values.

Others calibrations

On the demand of some of us I have implemented two methods to calibrate the orientation on drift images. You will find in the advanced functions section.


 

Measuring

After calibration we know the precise image orientation and the pixel sampling. So we can switch to Measurement mode.
If you know D,E by other means than by Reduc calibration, you can provide them at any time in the corresponding zones.

 

Measurement session is the easiest phase of Reduc's learning !!!
- Load the set of images
- Sort it
- Click on the main component of the first frame to obtain its centroid, if detection is ok, right click to memorize.
NOTE that usually Reduc detects automatically the first component when loading, so if detection is ok you can right click directly.
- Repeat the same for the secondary component
- Select the next frame in the list and so on ... you stop when you want.

Each frame processed causes a complete refresh of the reduction. Both reduction sheet can be displayed in Measurement mode. Results are displayed in the Reduction window.


Remeber to press Clear before reducing a new double star :


Publishing !

OK, our frames are reduced. What now ? Ready for publication !

Reduc can create three logs in text format. One is a complete report of the reduction session (Log Texte), the other is an ASCII delimited file (Log Data) which can be imported in either database or spreadsheet programs and the last is a formatted report as asked by some users.

A form can help to fill in the report (AutoInfo tab).
Do this at each star reduced and you will obtain a complete session logs.

The window can be called from the main window by the menu Window/Log or from Reduction window menu Add to log.
You can see and edit the content of the logs by selecting either the Text Log, Data Log or EZReport tabs.

NOTE : the content of the tabs can be edited in Reduc.

Save the logs by clicking Save in the menu. When saving, the two logs are saved, their default names are ReducLog.txt, ReducDat.txt and ReducEZReport.txt and can be changed.



Automated Reductions
Reducing manually a great number of frames isn't very funny ;o) Reduc can make it easier.

Select a good frame in the file list
- Click on the primary component and adjust if necessary the size of the search box like in manual reduction BUT DON'T right click
- Instead Click on 'comp A'


- In the same way, select the secondary component and adjust if necessary the size of the search box.
- Then click on 'comp B'
- Finally press AutoReduc button and voila ! After a while all the frames are reduced


Obviously only the selected frames of the list are reduced.

TAKE CARE : AutoReduc works perfectly when the stars are clearly separated and have a good difference of magnitude. However AutoReduc can make mistakes when the stars are too tight or the search box is too large or when the stars are too near in magnitude. Take always a look in the Reduced tab to validate. The sort options are very useful to check. Flagrant errors will give lines with 0 or about 0 for separation and in the other case the mag difference will be enormous and angle and distance residus will be important.

Advanced features

Shift and Add Features

Sometimes the stars don't have enough signal and the frames can't be reduced individually. The most current case is when a double star has a visible main component and a weak secondary . Reduc offers two functions allowing you to combine the set of frames in an unique image that will be measurable:
- Auto Align and Stack : Reduc shifts and adds automatically the set of images in the list.In the same way as at the time of a reduction, it will be necessary to adjust the size of the search box in order to include the main component before launching the operation.
- Stack Reductions: Reduc adds the frames from the Reduction Window. Shift is done according to the coordinates of the main component, you don't need to adjust the search box of detection. Since you can eliminate frames in the Reduction Window, this option permits to select the frames to be added.
- Align List : aligns without adding
- Stack List : adds without alignment (useful on an already aligned list)

When clicking Align or Stack, you can adjust the size of the final image as well as its centering. The effects of the adjustements are materialized by the red/white dotted cross.
NOTES:
- Reduc can combine pictures of different sizes.
- The reference component for the alignement is not necessarily in the final image.

 

Just after an alignment, the list of files is blue.
To optimize the calculations, Reduc uses a special format and create a list of 'virtual' frames which are the result of the last alignment. These frames can be used use as if they were normal image, ie. you can reduce them or to add them (Stack List menu).
The only difference is that this list is managed entirely by Reduc and that these files will be erased according to its needs.
Many possibilities are open with these options. Look at 'Samples of the real life' section.

Automatic Rejection
You can suppress the image having not enough quality. It's useful when you reduce automatically a great number of frames.
In the Reduction Window select Sort>Rejection.
The analysis is instantaneous and the pictures are suppressed from the reduction tabs.
The criterions are very large and concern only a small amount of the frames.
Less than three meaningful pixels to estimate the centroïd of one of the components 3 pixels are indeed the strict minimum to be able to do a reduction!
Insufficient light peak The peak of light is near the background noise. Reduc tried to find a centroïd but the quality is very doubtful.
Rho < sampling No miracle, Reduc cannot measure two stars that would be contained in a same pixel
Theta Residue > 3 s
Rho Residue > 3 s
This case is very exceptional. The maxi residues are usually just above 2 s and reach 3 s very rarely. The picture is probably unexploitable (or has been exploited very badly by Reduc!)

Drift Calibration
Some of us think that a star trail is the best way to evaluate the Esat/West axis. In the absolute it appears applicable. The trail is however very sensitive to the turbulence, if one wishes to get an information of quality it is necessary to apply some rules at the time of the capture and of the exploitation of the picture:

- Aim at a brilliant star that doesn't saturate the sensor
- Bring it on the east side of the sensor (just outside if possible)
- Start the exposure
- Stop the RA motor
- Stop the exposure when the star has crossed the sensor.

Three factors are important, the length of the trail, its duration in time and the intrinsic quality of the picture.
The length must be the greater possible, a complete crossing of the sensor is the best but you can deal with a few less if you are afraid about losing the star.
The duration : a trail of two seconds doesn't bring any valid information, it is necessary to be the longest possible, about ten seconds can be sufficient. In case of uncertaintyyou can to make several and use the mean of the results.
The quality of the frame :the star must be bright enough in order to let a straightforward trail on the sensor. Avoid the weak stars and the double stars oriented to 90° or 270°!
The time of exposure is long enough to spoil the frame with noise. It is imperative to preprocess the frame, the hot pixels will distort heavily the reduction. Subtraction of the offset and dark are imperative (Flat field application can be useful if the optic path is very dirty).

CALIBRATION :

- Load the correctly preprocessed frame and adjust the levels in order to see easily the trail.

- Click a point close to an extremity of the trail. Choose a place where the trace is well established (fig. 1)

- Adjust the size of the detection box to a value a little superior to the width of the trail. (fig. 2)

- Click on the 'comp A' button (fig. 3)



(1)
(2) (3)
- Click a point at the other extremity of the trail. Again choose a place where the trace is well established (fig. 4)

- Click now the 'B comp' button (fig. 5)

(4) (5)

- Finally click on the 'Drift Analysis' button to launch the analysis (fig.6)

- The points of calculation are marked with green crosses and the curve of regression is in red. It is time to give to Reduc the orientation of the quadrants. Click the corresponding button of the dialogue box. (fig.7)

- The calculated value are propagated automatically in the reduction sheet. (fig. 8)

- The pre-orientation is put up to date too. (fig.9)

It's highly recommended to capture several drift images and to keep the mean value of their reductions as the final calibration value.


(6)
(7)
(8) (9)

Drift Calibration on multiple frames
This method is dedicated to the users of commercial webcams without a long exposure mod. The remarks about the drift method remains valid. It is essential here to choose a brilliant star to have a good S/N ratio during the movement of the star. Obviously it must not saturate the sensor.
The method of capture is identical to the one exposed in the previous chapter.

- Select only the frames showing the movement of the star (fig. 1)


(1)
- Adjust the size of the detection box so that it includes largely the star (fig. 2) (2)
- Click on the 'Synthetic Drift' button (fig. 3) (3)
- The pictures are displayed on the screen as Reduc analys them. It is an opportunity to control that there are not any bad plots.

- At the end the analysis a synthetic picture of the movement of the star is displayed and a dialog box of dialogue asks for the orientation of the picture. It is time to give to Reduc the orientation of the quadrants. Click the corresponding button (fig.4)
(4)
- The calculated value are propagated automatically in the reduction sheet. (fig. 5)

- The pre-orientation is put up to date too. (fig.6)
(5) (6)
If the curve of regression appears disjointed that is that there are probably incorrect pictures. You can modify to leisure the selection of pictures and can launch again the analysis while clicking the 'Synthetic Drift' button again.
It's highly recommended to capture several drift images and to keep the mean value of their reductions as the final calibration value.

Using QuadPx Function



Original size


After QuadPx

It is difficult to measure tight stars. QuadPx resamples the displayed image and enlarges it by a factor two while keeping constant the distribution of the light by unit of area. This method of enlarging is perfectly adapted to the measurement by Reduc because it works on this distribution. If needed QuadPx can be applied twice on the same image.

Since V3.71, Reduc takes into account the scale change and adjusts the reduction automatically with Quaded images.

Après un deuxième QuadPx

SURFACE : Adjustment of a tridimensionnal surface

This feature uses the Surface algorithm especially designed to measure the very tight stars. Developed by Guy Morlet and Pierre Bacchus to measure the images acquired on the 50cm refractor of the observatory of Nice, it was until now reserved to private usage of the members of the French Astronomical Society. It is integrated in Reduc with the authorization and the courtesy of the authors.

Surface is at full power on images with a high signal to noise ratio. Therefore it is not usable in the automatic reductions. After having shift-and-added the image, the measure is made in four stages:
1 - click on the most brilliant pixel of the main star and click 'comp A' button
2 - click then on the most brilliant pixel of the secondary star and click the button 'comp B' button.
If the secondary star doesn't show a visible peak, click on what seems you to be the center of the star.
3 - select Special/Surface menu
4 - At the end of the calculations, a window with the internal elements of Surface's reduction appears. Click on OK button and the measurements will be taken automatically in account in the window Reduction of Reduc.

We are going to study a practical case somewhat complicated in order to show all the possibilities of Surface combined with the other functions of Reduc:


This picture (1) is beyond the Reduc's capacities. The centers of the stars are separated by a merely four pixels and the secondary component doesn't present a peak.
(1)
We have said that it is necessary to click the most brilliant pixel of the main star.
Reduc is going to help us to find it quickly.
Adjust the research box to draw a large window first (the centering is switched to Automatic)(2a)
(2a)

Then reduce it to a 3x3 dimension, Reduc goes itself on the most brilliant pixel of the main component (2b).
(2b)
Click on 'comp A' button to identify the component (3) (3)
The secondary component doesn't present a peak, it is impossible to reproduce this operation on it. First check the Manual option while keeping the size of the box to 3x3. Then, looking at the shape of the stars, click on the center of the secondary star. (4) (4)
Click on 'comp B' button to identify the secondary component (5)
Launch the Surface analysis (6). (6)

Most of the time Surface does the reduction and we will that just after. Here we get an error message (7). Surface can't calculate the positions of the components.
The probable reason can be:
- the stars are too tight and don't offer enough surface (under-sampling)
- the signal is too weak
- it is simply impossible to measure

(7)

Here the stars are too 'small' to allow Surface to work.
Never mind, we have a very useful feature in Reduc and we will resample the image with QuadPx (8).

(8)

Our stars now are of reasonable size.
It only remains to restart with the operations already described to identify the main and secondary components and to launch Surface again.

Before After QuadPx

This time Surface finds a solution to its equations. Our stars are measured.
The numbers in the window are the calculated elements as Surface adjusts its equations. We find:
xA,yA,xB,yB,luminosity of A and B, the parameters of surfaces fitting , theta, separation in pixels and the gap between the mathematical surface and the picture.
There is a line per iteration of the algorithm, generally greater this number, smaller the reliability of the measure. The program stops automatically when it reaches 25 iterations.

Theta is calculated with an internal orientation, it is automatically recomputed by Reduc according to the calibration of the orientation.
Click OK, the results are send to the Reduction sheet (9). Here the couple is separated by 2"62 but we must remeber that we 'QuadPxed' the image , the real distance is therefore half this value (1"31).
This has been changed since V3.71 and Reduc automatically the distance.
(9)
We can verify the Surface's work by clicking on the measurement line.The big cross shows the center of A and the small cross the center of B (10). Don't be surprised if you see a light shift (1 or 2 pixels at most) between the crosses and the picture. It is a 'secondary effect' when measuring the mathematical model. It is sometimes shifted to better calculation.
Obviously a shift as the one of the picture (11) shows that something is wrong !!!

(10) Image
measured correctly

(11) Someting is wrong !!!
Another quality of Surface is its stability. It can reduce correctly even though the composing B is not perfectly designated. In case of doubt you can verify that the proposed solution is reproducible while changing slightly the position designated for B.
- Recall the picture by a click on the measurement line (12)
- Click slightly on a position slightly different of the center of B (13) and to memorize its position (14). It is useless to do re-designate A, Reduc remembers its position as long as the same image is displayed.
- Launch Surface again and control the result
(12)
(13) (14)
In this example we clicked voluntarily on a position very distant of the center calculated for B. However Surface provides a result equal to the later (15). (15)

Math Image

The Math Image option allows you to see how Surface has modelized the stars.

Look at this example at right with an image of STF 644.

- 16 the original image
- 17 the mathematical model after by Surface's computation

 

(16)

(17)

 


Dark and Bias preprocessing

Recall and basic principles:
Raw image = Science image + Bias + Thermal Noise
When acquiring the images, take care to acquire also some dark frames. 7 to 9 are a good number. These frames are acquired with a closed obturator and an exposure time equal to exposure time of the raw frames.They contain the bias and the thermal noise. Reduc can synthesize a median frame of the set and subtract it to the frame when measuring so you don't need an external software in order to prepare your images. All is done in Reduc's workspace and your original frames aren't modified.

 

Preprocessing activation :
1/ Clic on the Dark button
2/ Select the dark frames

3/ Dark appears at the right of button
Since that all frame loaded is automatically preprocessed.

If the size of the loaded image is incompatible with the one of the dark, Reduc doesn't preprocessed it.
It is useless to disactivate the preprocessed if the list of files is in blue because Reduc can recognize the frames that it already preprocessed.

Stop preprocessing :
1/ Clic on the Dark button
2/ Choose Cancel in the dialog box

3/ Preprocessing is stopped

 


Horizontal and Vertical Swap
You can change the orientation of FITS files when they are loaded by Reduc. Since it is checked the option remains active for all files loaded .


Binning 2x
Some of us used cameras which can image using binning 2x mode. In a same night we can make images using binning 1 and images using binning 2 (eg. on fainter couples). We must take into account the change of calibration between the two modes when reducing. Checking the 2x option alerts Reduc that we change temporarily of image scale.
Obviously this is ok only if the basic value of sampling (E ) is the binning 1 sampling !

Basic sampling in binning 1 mode

Temporary processing of binning 2 images
Reduc recompute automatically all reduction elements


Others features

Langage
Reduc interface is available in French, English and Spanish.
You can switch by the menu ?/Langage/... in the main window.

I thank very much Edgardo Ruben Masa Martin for the spanish translation.


Visualisation levels
The visualisation levels are computed automatically by Reduc when it loads each frame. When unchecking Auto you keep the same tuning from one image to another. You can otherwise change them at any moment by moving the trackbars.


You can adjust very precisely using the keyboard left/right keys

A right click on the trackbars show a tuning popup. It allows to change the range of the bars :
Max:, Min:
Actual max et min values available
|<-- Max
Max is set to the highest value of the thumbs
Min -->|
Min is set to the lower value of the thumbs
Max >>
Increase Max
<< Max
Decrease Max
Min >>
Increase Min
<< Min
Decrease Min

A false color visualisation can be obtained with the colored checkbox.

Saving the images


Reduc is not an image treatment software but it can be useful to record an image.
Two formats are possible: Bitmap and FITS ( BITPIX=16).

When saving a BMP file, the image is saved as it is seen on the screen. That is to say that the visualization settings influence the recorded picture. Therefore it won't be possible to make future measurements on this picture since the information of origin is definitively lost.

WARNING : if the colored checkbox is checked, saving the image to FITS format loses the astrometric information. The image is saved proportionally to the levels indicated by the bars.
In this example, the pixels of level > 28265 will be brought back to 32767, those < 839 will be brought back to 0. Between these two levels they will take a proportional value in the 0-32767 range.
It doesn't have anything to see with double stars but I also use Reduc for deep sky registration of deep sky pictures :)

Save an image series

You can save all the images selected in the list. Simply use the features :
Save FITS ...
or
Save BMP...


Align and Crop Images  

This features allows you to easily crop images :
- because you want to save only the intersting part of a series of frames
- to decrease the time of treatment of large frames

The procedure is identical to shift and align procedure.
The main difference is that alignment is a simple crop instead of a subpixel alignment.

Remember :
Align and Crop => pixel alignment, simple crop
Align List => sub pixel alignment
Auto Align and Stack => sub pixel alignment


 



Customizing the camera List  

Click on [...] button to customize the list.

Add a camera : type its name and the pixel size.

Delete a camera : blank all information about it.

ABOUT THE PIXEL SIZE
the important thing is the relative size on the final image. Generally with square pixels there is not any problem. With rectagular pixels, two cases must be taken into account :
- the final image is a strict raw image of the sensor (1 pixel on the sensor -> 1 pixel on the image)
- the final image is interpolated by the camera or the capture software in order to simulate square pixels.
In the first case you enter the values corresponding to the features of the camera, in the second it will be necessary to enter an identical value in Horiz and Vert.




Samples from the real life ! (FAQ)

Useful Shifts and Adds
When the signal of each components is sufficient for an individual reduction, I recommend to use it. Unfortunately the frames don't have always the required qualities for an individual reduction: not enough signal, too much noise ... Here are some cases where 'shift and add' can bring a solution.
The most classic case, the main component is well readable but the secondary is nearly drowned in the noise.
Several hot pixels are also present. The second component is just below the main. A third is on the upper left.

After having done a BestOf and selected one of the best pictures, I adjust the search box on the main component. Then I select 'Auto Align and Stack'. Here, I adjust the parameters of alignment in order to be able to measure the third component also on the final picture.

Et voila, the three components will be measured comfortably. Reduc ignored the hot pixels.

The two components are tight, of same magnitude, the frame is noisy and the signal is rather weak! However the pictures seem to carry a little information.

I adjust the search box so that it includes the two components

and launch 'Auto Align and Stack'


According to the pictures it can be interesting to check or uncheck CtlAdj. There is not a general rule, it is necessary to try the two solutions and to keep the one that gives the best final picture.

I have images of a triple system and I am interested in the BC couple. Reduc goes always on the A star at the time of an automatic reduction.
.

First I align the pictures ...

... while isolating the interesting couple. Here the component A is used to align the frames but won't be part of the final picture thanks to the parameters given in the dialog box.

Et voilà !

it remains only to reduce the 'virtual' list as if there was the original images.
I have a couple with two components of same magnitudes. When I ask to Reduc to do an automatic reduction, it can't decide and it takes either one or the other as the main.

   

Two solutions : I reduce manually or I try a Shift and Add
while creating a sufficiently big search box big to include the two components


quand unchecking Ctl Adj, si les DEUX composants paraissent dans la fenêtre modèle, alors Reduc sera capable de continuer sans erreurs.

Et voilà :

  

I don't forget to check Ctl Adj before measurng the final image.