On this page a 21°×40° wide-field view which covers most of the constellations Andromeda and Lacerta is presented.
The center of the photographed region lies about 20° south of the galactic plane and is rich of high galactic latitude nebulae.
Most famous objects are M33 (Triangulum galaxy), M31 (Andromeda Galaxy) and SH2-126, a large HII region in Lacerta.
Click on the images to load a full resolution version with more than 100 megapixels using a JavaScript viewer.
The triangulum Galaxy M33 is depicted in the top right corner, the Andromeda galaxy M31 is in the center and SH2-126 is the red nebula at bottom.
This image is a false color composite in which H-alpha (including red continuum) is mapped to red, blue continuum (including [OIII] and H-beta emissions) is mapped to green, and red continuum (without H-alpha) is mapped to blue.
Reflection nebulae appear green to blue, while HII regions are red.
Stars in the continuum channels are partially subtracted to make the faint nebulae visible.
Selected details
Here are two details that also can be seen using the JavaScript viewer.
M31 accreting its companions M32 (the smaller one) and M110. The irregular shape of the halo is caused by remnants of of previously accreted galaxies.
SH2-126 (red) surrounded by high galactic latitude nebulae (mostly gray).
Discoveries
The views above show many nebulae that cannot be found in catalogs. (The JavaScript Viewer allows identifying objects using catalogs or SIMBAD and defining new objects.)
Some (probably not all) of these unexplored nebulae have been collected in the list below. Click on the following link for a presentation.
In the JavaScript viewer, the object outlines can be toggled on and off by pressing the '2' key. This can be helpful to make certain structures (namely the strange ellipses B9 and B10) visible.
SIMBAD queries for certain object types can be made easily in the JavaScript Viewer by drawing a circle and pressing a shortcut key or via the menu
A repository with the discoveries can also be found on GitHub
Image data
Images where captured with a camera array which is described on the instruments page.
Image data are:
Projection type:
Stereographic
Center position:
RA: 0h04, DEC: 41°
Orientation:
Above:
North is right
JavaScript viewer:
North is up
Scale:
10 arcsec/pixel (in center at maximum resolution)
FOV:
40°×21° (RA×DEC, through center)
Exposure times:
Sum of exposure times of all frames used to calculate the image.
H-alpha:
6.8 d
Continuum channels:
5.0 d
Image processing
All image processing steps are deterministic, i.e. there was no manual retouching or any other kind of non-reproducible adjustment. The software which was used can be downloaded here.
Image processing steps where:
H-alpha only: bias correction, photon counting
Dark current subtraction, flatfield correction, noise estimation
Alignment and brightness calibration using stars from PPMXL catalog
Stacking with masking unlikely values and background correction
Extracting stars
Denoising and deconvolution both components (stars and residual)
RGB-composition
Dynamic range compression using non-linear high-pass filter
Tonal curve correction
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Media on this page can be used under Creative Commons Attribution-
Noncommercial-Share Alike 4.0 license or other licenses.