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M81_and_M82.jpg
Bode's Nebula (M81 and M82)929 viewsMessier 81 (right) and Messier 82 (left) are located in the constellation of Ursa Major. These galaxies are relatively close to each other (about 150,000 light years) and easy to spot with a small telescope or binoculars. The image consist of 55 exposures taken with a Canon 60Da camera, Orion ED80T telescope, and a Celestron CGEM mount. Exposures were stacked with Nebulosity 4 and processed with Pixinsight 1.8Nov 30, 2015
IC5070.jpg
IC5070 (Pelican Nebula)909 viewsIC5070 (Pelican Nebula) located in the constellation of Cygnus is part of a large H-II cloud. The hydrogen gas is excited by the energy originating from nearby stars, and then emits its own light in the red wavelength of hydrogen. The image consist of 4 hours of exposures taken with a Canon 60Da camera, ES 127mm refractor with .8 reducer, mounted on a Celestron CGEM mount. The image was stacked with Nebulosity 4 and processed with Pixinsight 1.8.Nov 23, 2015
M8_and_M20.jpg
Lagoon Nebula (M8) and Trifid Nebula (M20)925 viewsThe Lagoon Nebula (M8) on the left and Trifid Nebula (M20) on the bottom right are located in the constellation of Sagittarius. M8 is an emission nebula about three times the size of the full moon. The nebula’s brightest region is illuminated by two supper giant stars while the rest of the nebula is illuminated by the open star cluster NGC 6530. M8’s smaller neighbor, M20, is a combination of emission nebula (red) and reflection nebula (blue). The image consist of 4 hours of exposure taken with a Canon 60Da camera and Orion ED80T telescope mounted on a Celestron CGEM mount. Exposures were stacked with Nebulosity 4, processed with PixInsight 1.8, and minor cosmetic touches with Photoshop CS6.Nov 23, 2015
2015_11_13_90mmSMII_41AU02_noLR_Ha_small.jpg
Massive Filament on the Sun931 viewsA dark filament of magnetism in the sun's southern hemisphere has curled upon itself to form a circle of gargantuan proportions. The circumference of the ring is almost a million kilometers (600,000 miles)! Magnetic filaments are very often unstable, and have a tendency to collapse. Filaments crashing to the surface of the sun can cause of a type of explosion called a Hyder flare. Any flare from this filament could be extra-energetic as it releases the tension stored in its million-km coil. Image taken from Alamogordo, NM on 11/13/15 at 10:14 AM MST (1714 UTC) using a Meade Instruments Coronado 90mm SolarMax II telescope and Imaging Source 41AU02 camera.
Nov 13, 2015
SHOcombineFinal.jpg
Narrowband image of the Crescent Nebula in Cygnus868 viewsThe Crescent Nebula (NGC 6888) is found in the constellation Cygnus, whose emission is powered by strong stellar winds from a Wolf-Rayet star colliding with previously expelled outer envelopes of the stars atmosphere. This narrow band image is a combination of 5 hrs of H alpha data (Astrodon 5 nm Gen 2 filter) and 5 hrs 20 m of O[III] data (Astrodon 3 nm Gen 2 filter). Taken with a Takahashi CCA-250 f/5 astrograph and QSI683wsg camera on a Paramount ME; August 11th , 13th and Sept 14th - 17th, 2015 in Mayhill, NM (Ha, 15 x 1200 sec lights @ -20o C; O[III], 16 x 1200 sec lights @ -20o C 21 darks; 126 bias; 128 flats) Image acquisition with MaxIm DL 6.08; Calibrated, aligned, integrated, and processed in PixInsight 1.8.4.1185 Ripley (x64); Colors assigned ( Red = Ha, Green = 15% Ha + 85% O[III], Blue = O[III] ) and combined using SHO-AIP script.Oct 31, 2015
The_Crescent_Nebula_Ha5xOIII.jpg
The Crescent Nebula in Ha and O[III]771 viewsThe Crescent Nebula (NGC 6888) is an emission nebula found in the constellation Cygnus. The emission is powered by strong stellar winds from a Wolf-Rayet star colliding with previously expelled outer envelopes of the stars atmosphere. This image is a combination of 5 hrs of H alpha data (Astrodon 5 nm Gen 2 filter) and 5 hrs 20 m of O[III] data (Astrodon 3 nm Gen 2 filter). Taken with a Takahashi CCA-250 f/5 astrograph and QSI683wsg camera on a Paramount ME; August 11th , 13th and Sept 14th - 17th, 2015 in Mayhill, NM (Ha, 15 x 1200 sec lights @ -20o C; O[III], 16 x 1200 sec lights @ -20o C 21 darks; 126 bias; 128 flats) Image acquisition MaxIm DL 6.08; Processed in PixInsight 1.8.4.1185 Ripley (x64). The calibrated, aligned, and integrated Ha and O[III] images were stretched using Masked Stretch, Ha stretch matched to O[III] with Linear Fit, and combined using Pixel Math.Oct 23, 2015
Messier_27_in_the_constellation_Vulpecula_sRGB.jpg
Messier 27 in Vulpecula782 viewsMessier 27, which was discovered in 1764 by Charles Messier, is a bright planetary nebula in the constellation Vulpecula. The nebulosity is due to the expulsion of a star's outer layers in the later stages of its life and is illuminated by the stars intense radiation (blue star in the center of the nebula). Image was taken in Mayhill, NM on the nights of 14, 15, 16, 17 September 2015; total of 5 hrs 40 min exposure through an Astro-Physics 178 mm f/9 refractor with field flattener and an SBIG STF8300c camera with OAG (ST-i) on an Astro-Physics 1200 mount (17 x 20 min lights dithered @ -15o C; 33 darks; 128 bias; 128 flats); image acquisition with MaxIm DL 6.10 and processed with PixInsight 1.8.4.1170. Processing included Bayer drizzle, a Synthetic Luminance, and Multiscale Processing. Oct 07, 2015
LunarEclipse2015.jpg
Lunar Eclipse of Sept 2015790 viewsThe 9/27/15 Lunar Eclipse in Mayhill, New Mexico (9/28/15 02:59:14 UT) taken with an Astro-Physics 178mm f/9 refractor with field flattener and SBIG STF8300c camera on an Astro-Physics 1200 mount; processed in PixInsight 1.8.4.1170.Sep 28, 2015
M17_Hubble_post.jpg
M17 in narrowband (Hubble palette)907 viewsMessier 17 also known as the Swan Nebula or Omega nebula is located in the constellation of Sagittarius. The Nebula is composed mainly of ionized hydrogen. It is around 5,000 light years away from Earth and is one of the most massive star forming regions in the Milky Way galaxy. This false color image utilizes the Hubble palette that maps Ha to green, OIII to blue, and SII to red. Once the images from each filter are combined it creates an interesting photo. This was my first serious attempt at narrowband imaging and hopefully it will improve. The image consist of around 180 minutes of data from each filter.Sep 21, 2015
Cygnus_Loop.jpg
Cygnus Loop886 viewsThe Cygnus Loop, located in the constellation of Cygnus the Swan, is a supernova remnant that occurred after a massive star exploded between 5,000 to 10,000 years ago. The loop is about 3 degrees in size and continues to expand. The data for this image was obtained on the 17th and 19th of Jul 2015. It consist of 67 X 5min exposures obtained with a Canon 60Da camera, Orion ED80T telescope, and a Celestron CGEM mount.Sep 11, 2015
IC_1318_2014_09_26_100ed_F7_2_XS_60min_Carboni_2.jpg
The Sadr Region in Cygnus1177 viewsThe Sadr Region is a region around Gamma Cygni in the constellation of Cygnus the Swan. This area hangs high overhead in the northern hemisphere during the summer. Contained within this region is defuse nebula IC 1318, an emission nebula with several dark nebulas intermixed. Image was taken with a 100mm f7.2 refractor and Hap Griffin modified Canon 1000D with an Astrodon filter from Alamogordo, NM on 9/26/2014. Stack of 15 ea 4 min exposures processed using Nebulosity 2.5 and PS V7.01 using Carboni tools.Sep 07, 2015
CrescentNebula.jpg
The Crescent Nebula in Cygnus728 viewsThe Crescent Nebula (NGC 6888) is an emission nebula found in the constellation Cygnus. A leading hypothesis suggests that the strong stellar winds from the central Wolf-Rayet star collides with the stars outer atmospheric envelope ejected in a previous evolutionary phase, which energizes the nebula and leads to the observed structure. This H alpha image is a total of 5 hours of exposure taken with a Takahashi CCA-250 f/5 astrograph and QSI683wsg camera (Astrodon 5 nm Ha filter) on a Paramount ME; August 11th , 13th 2015 in Mayhill, NM (15 x 1200 sec lights @ -20o C; 21 darks; 126 bias; 128 flats) Image acquisition MaxIm DL 6.08; Calibration, alignment, integration, and processing in PixInsight 1.8.4.1107 Ripley (x64).Sep 01, 2015
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