Latest CCD images

Click on the thumbnails for full size images

Dumbbell nebula revisited with H-alpha and OIII filters. I've copied earlier photographs of the Dumbbell nebula that were taken with RGB-filters (2007) and the FTF1020C colour CCD (2000, now out-of-use).

Dumbbell nebula in HOO august 2023 Dumbbell nebula
DUMBBELL nebula HOO palette
August 21/22, sept. 6/7 2023
25cm Newton f/D=5.7 reduced with
simple coma-corrector to f/D=4.6
FTT1010M CCD with Baader 6.5nm
H-alpha and OIII filters
H-alpha 133*120 sec
OIII 128*120 sec
FoV: 0.34x0.34 degr
Date: 16 september 2007
25cm Newton f/D=5.7
FTT1010-M CCD
RGB-filterweel
Exp. RGB 12x90sec
FoV: 0.3x0.3 gr
Date: 23 august 2000
Scope: 25cm Newton at f/D=5.7
CCD: FT1020 colour CCD
Exp.: Sum of 29 images of 120sec

Coincidentally I photographed M101 on 17 May 2023, two days before supernova SN2023ixf was discovered. On 19 may I could confirm the supernova during a short break in the clouds. The wheather cleared on 24 May and the few astronomically dark hours enabled me to photograph M101 and SN2023ixf in L and RGB.
Below the results shown in different ways.

Image information:
Equipment: 25cm Newton f/D=5.7 with FTT1010M CCD and RGB filterwheel
Sub-image exposures:
	17 May: Luminance 15*120sec
	24 May: Luminance 30*120sec
	25 May: RGB 30*120sec each
FoV: 0.48x0.44 deg
SN2023ixf in M101 17&24 may 2023 M1 HOO as RGB, 25/27 feb 2022 width=330 M101 Pinwheel galaxy
Gif switching between 17 and 24/25 May 2023
17 May and 24 May side by side Sum of 17 and 24/25 May images

M42 imaged with SII, H-alpha and OIII narrow-band filters (Baader Planetarium, 6.5-8.5nm bandwidth), shown in three different ways. To the left H-alpha is shown in Red while the OIII image is distributed over Green (100%) and Blue (100%) to obtain the characteristic teal colour. The middle image has the same colour assignment and is unsharp masked, i.e. the luminance of the image was devided by a smoothed version of itself, lowering the intensity of the central part of the nebula and revealing the (nearly overexposed) trapezium star cluster. The image to the right shows M42 with H-alpha again assigned to Red (150%), S-II to Green (400%) and OIII to Green (80%) and Blue (100%). In order to have a clear effect, the Sulfur contribution had to be increased 4-fold.

Images are obtained on february 8, 2023, with the FTT1010-M CCD camera and the f/D=3.5 Newton configuration described below (and in the equipment section, see here). M42 is a relatively bright object and for H-alpha and OIII short, 60-second exposures were needed to avoid overexposure of the central part: H-alpha 19x60 seconds, OIII 30x60seconds. The Sulfur contribution is much weaker and 16 exposures of 120 seconds were acquired.

The images cover a 0.8x0.8 degree field of view, are sharpened and shown with a gamma of 2.2. The luminance is based on the (photopic) eye sensitivity for the H-alpha wavelength (656nm: sensitivity 0.08) and OIII wavelength (501nm: sensitivity 0.34). Thus L=0.08*H-alpha+0.34*OIII.

Horse nebula HOO
14/27/28 february 2023
H-alpha 155x2min
OIII 95x2min
FoV 0.73x0.73 degrees
Gamma 2.0
Intenser red contributions are shown with increasing whiter appearance
The image is sharpened and rotated 90-degrees (CCW)
M42 in HOO. Gamma 2.2. M42 in HOO, unsharp masked. Gamma 2.2 M42 in HSO, Gamma 2.2 Horse head nebula in HOO.
M42, HOO M42, HOO,
Unsharp masked.
M42, HSO Horsehead nebula
Images obtained with the FTT1010-M CCD camera and my latest Newton telescope. In fact it is a modified Cassegrain telescope with a 25cm, f=1091mm primary. By adding a plane-convex lens close to the CCD the effective focal length is reduced to f=880mm and the f/D is improved from 4.3 to 3.5. Without this lens, coma of the parabolic primary over the 12mmx12mm focal plane of the CCD is substantial. The plano-convex lens reduces coma and increases sensitivity by some 50% (which compensates for the relatively low quantum efficiency of the CCD's I'm (still) using). For more details click here.
The images are cropped to 0.5x0.5 degrees of the 0.8x0.8 degrees field of view. The bandwidth of the H-alpha and OIII filters are 6.5nm and 8.5nm (Baader-Planetarium).

Bubble nebula, NGC7635 in HOO Bubble nebula
NGC7635
19 nov, 12/14 dec 2022
25cm Newton f/D=3.5
Exposure:
H-alpha 76x120sec
OIII 93x120sec
Cropped FoV: 0.50 x 0.50 degr
Crescent nebula, NGC6888 in HOO Crescent nevel
NGC6888
20/23 aug, 1/21 sep 2022
25cm Newton f/D=3.5
Exposure:
H-alpha 94x120sec
OIII 149x120sec
Cropped FoV: 0.52 x 0.52 degr

Hickson44 star motion 2012/2022 M1 SHO as RGB, 25/27 feb 2022 M1 HOO as RGB, 25/27 feb 2022 PK205 H-alpha 4, 5 and 7 mar 2022
Proper motion of 2 stars
in Hickson44 galaxy field.
2012 / 2022
25cm Newton f/D=5.7
FTT1010M CCD with
RGB-filter wheel
FoV: 0.28x0.28degr
M1, SHO as RGB
H-a: Febr. 25..27, 2022
SII,OIII: Jan 28, 2011
25cm Newton f/D=5.7
FTT1010M CCD with
SHO-filter wheel
H-alpha: 151x120sec
SII,OIII: 26x120sec
FoV: 0.37x0.28 degr
M1, HOO as RGB
H-a: Febr. 25..27, 2022
OIII: Jan 28, 2011
25cm Newton f/D=5.7
FTT1010M CCD with
SHO-filter wheel
H-alpha: 151x120sec
OIII: 26x120sec
FoV: 0.37x0.28 degr
PK205 planetary neb.
4, 5 and 7 March 2022
25cm Newton f/D=5.7
FTT1010M CCD with
Baader H-alpha filter.
203x2 minute exposures
FoV: 0.43x0.43 degr
NGC2903 26 and 28 feb 2022 M90 and IC3583, 7 and 8 march 2022 M105, NGC3384, NGC3389 M31 Andromeda
NGC2903
February 26&28, 2022
25cm Newton f/D=5.7
FTT1010M CCD with
RGB-filter wheel
Lum.: 83x120sec
RGB: 24x120sec
FoV: 0.38x0.38degr
M90 and IC3583
March 7&8, 2022
25cm Newton f/D=5.7
FTT1010M CCD with
RGB-filter wheel
Lum.: 94x120sec
RGB: 30x120sec
FoV: 0.38x0.38 degr
M105, NGC3384,3389
Feb. 28 (RGB) and
March 4&7, 2022
25cm Newton f/D=5.7
FTT1010M CCD with
RGB-filter wheel
Lum.: 111x120sec
RGB: 30x120sec
FoV: 0.38x0.38 degr
M31 Andromeda nebula
December 2&25, 2021
FTF2020M CCD with
RGB-filter wheel
300mm Tele-objective
F#4.0, on fork-mount
Lum.: 48x2 min
RGB: 18x3 min
FoV, cropped: 0.48 degr

Eclipse of Moon, 28 September 2015 ECLIPSED MOON IN PISCES STAR FIELD
September 28, 2015
300mm Tele-objective F#4.0
FTF2020-M CCD
RGB-filter wheel
Eclipsed Moon: 2 sec RGB
Star field: 30 sec RGB
FoV: 4.7x3.5 degrees

Hickson44 group in Leo M95 with SN2012aw M95 and M96 April 2007 reprocessed
Hickson 44 group
April 16, 2012 and April 4, 2011
25cm Newton f/D=5.7
FTT1010-M CCD with
RGB-filterwheel
Lum.: 87x100sec (2011)
RGB: 15x120sec binned (2012)
FoV: 0.4x0.3degr
M95 with SN2012aw
March 28, 2012
25cm Newton f/D=5.7
FTT1010-M CCD
Lum.: 37x120sec
RGB (2007):14x100sec binned
FoV: 0.13x0.13degr
M95 and M96
March 11 and April 7, 2007
Reprocessed
25cm Newton, f/D=5.7
FTF2020-M CCD
RGB-filterwheel
L: 55x90sec RGB: 14x100sec binned
FoV: 0.87x0.67degr

M58, NGC4567/68 M106 and NGC4217 Crab nebula SHO NGC2683 Lynx
M58 and Siamese twins
NGC4567 and NGC4568
May 3, 2011
25cm Newton f/D=5.7
FTF2020-M CCD with
RGB-filter wheel
Lum.: 58x120sec
RGB: 25x120sec binned
FoV: 0.85x0.61degr
North=Left
M106 and NGC4217
May 1, 2011
25cm Newton f/D=5.7
FTF2020-M CCD with
RGB-filter wheel
Lum.: 114x100sec
RGB: 19x100sec binned
FoV: 0.90x0.64 degr
M1 Crab nebula
January 28, 2011
25cm Newton f/D=5.7
FTT1010-M CCD with
SHO-filter wheel
Lum.: H+O
SHO: 25x120sec
FoV: 0.26x0.26 degr
NGC2683
8,11 en 17 april 2010
25cm Newton f/D=5.7
FTT1010-M CCD with
RGB-filter wheel
Lum.: 59x2 min
RGB: 12x2 min
FoV: 0.28x0.28 degr

NGC3198 Ursa Major NGC4490 and NGC4485 NGC3184 Ursa Major Comet Lulin 2 march 2009
NGC3198
6 and 9 april 2010
25cm Newton f/D=5.7
FTT1010-M CCD with
RGB filter wheel
Lum.: 79x90 sec
RGB: 16x120sec
FoV: 0.28x0.28degr
NGC4490 and 4485
20 apr/22 may 2009
25cm Newton f/D=5.7
FTT1010-M CCD with
RGB filter wheel
Lum.: 72x90 sec
RGB: 18x120sec
FoV: 0.28x0.28degr
NGC3184
20/22 april 2009
25cm Newton f/D=5.7
FTT1010-M CCD with
RGB filter wheel
Lum.: 75x90 sec
RGB: 12x120sec
FoV: 0.28x0.28degr
Comet Lulin
March 2, 2009
25cm Newton f/D=5.7
FTF2020-M CCD with
RGB filter wheel
Lum.: 1x60 sec
RGB: 4x60sec
FoV: 0.9x0.9degr

Images made with the FTF2020-M CCD camera equipped with a Baader H-alpha filter (7nm bandwidth) and with either the 25cm Newton using a simple coma-corrector, resulting in f/D=4.7, or a Leica f=300mm teleobjective at F#4.
IC1848 Detail East in H-alpha IC1848 Eastern part
2 jan 2009
25cm Newton f/D=4.7
Exposure: 84x150 sec
Field of View: 1.1 x 1.0 degr.
IC1805 and IC1848 in H-alpha IC1805 and 1848
27/28 dec 2008
f=300mm Leica teleobj.
Exposure: 66x3 min
Field of View: 4.6 x 3.5 degr.
IC410 in H-alpha IC405 in H-alpha Auriga nevel complex in H-alpha IC59 and IC63 near Gamma Cass.
IC410
30 dec 2008
25cm Newton f/D=4.7
Exposure: 55x150sec
FoV: 0.9 x 0.9 degr.
IC405
29 dec 2008
25cm Newton f/D=4.7
Exposure: 59x150sec
FoV: 1.1 x 0.8 degr.
Auriga nevels
IC405, IC410 en IC417
27/28 dec 2008
f=300mm Leica teleobj.
Exposure: 112x3 min
FoV: 4.6 x 4.4 degr.
IC59&IC63
7 december 2008
25cm Newton f/D=4.7
Exposure: 31x3 min
FoV: 1.1x0.9 degr.