Jul 182015
 
M8 - The Lagoon Atlas EQ-G Stellarvue SVQ100, Apogee Ascent A694 8x20min through a Baader Ha 7nm filter.

M8 – The Lagoon
Atlas EQ-G
Stellarvue SVQ100, Apogee Ascent A694
8x20min through a Baader Ha 7nm filter.

The Lagoon Nebula (catalogued as Messier 8 or M8, and as NGC 6523) is a giant interstellar cloud in the constellation Sagittarius. It is classified as an emission nebula and as a H II region.

The Lagoon Nebula was discovered by Giovanni Hodierna before 1654[4] and is one of only two star-forming nebulae faintly visible to the naked eye from mid-northern latitudes. Seen with binoculars, it appears as a distinct oval cloudlike patch with a definite core. In the foreground is the open cluster NGC 6530.

From Wikipedia, the free encyclopedia

Home Observatory Site looking South.  The faint open cluster appearing on the left is M7 in Scorpius.

Future home observatory site looking south. The faint open cluster appearing on the left is M7 in Scorpius. Taken with a Canon 6D and 24-70mm f/2.8 at 24mm and f/4 for 20 sec at 1600 ISO.

 Conditions were decent up until some clouds rolled in around 3:00am.  There was a lot of lightning flashing to the north so I packed up a little early and headed back to the house.  SQM measurements started around 20.2 but improved to 20.4 with a max of 20.5 around 1:00am.

The light pollution domes seen in the image are Oak Ridge to the south west (right side) and Clinton to the east/south east (left side).

May 312015
 

Last year (2014) I was conducting some mosaic tests for future projects.  I attempted a widefield 9 panel mosaic in Cygnus and processed the hydrogen alpha data but never got around to completing the tri-color Hubble Pallet image until now due to some difficult to process issues in the O[III] and S[II] channels.  Those difficulties, combined with the fact that I only gathered about one frame of each channel per panel in the mosaic (very thin data!), meant that I wasn’t exactly thrilled to process this one to completion.  Time away from the hobby due to the out of state relocation though has made me a little anxious to get back to imaging so I decided to revisit some of this forgotten data.

Cygnus Mosaic Cropped & Reduced to 50% Size. 9 Panels, 1x20min per Ha, O[III], S[II] Channel per panel. Total Time 9 hours. Taken with an Apogee U16M and Tak FSQ-106ED.

Cygnus Mosaic Cropped & Reduced to 50% Size. 9 Panels, 1x20min per Ha, O[III], S[II] Channel per panel. Total Time 9 hours. Taken with an Apogee U16M and Tak FSQ-106ED.

Jan 252015
 
IMG_0196_ABE_Annotated

Comet Lovejoy C/2014 Q2 Annotated 1/24/2015 from Norris Lake, TN. Canon 6D, 70mm f/2.8, 6 seconds @ ISO 3200

 

IMG_0196_ABE

Comet Lovejoy C/2014 Q2, 1/24/2015 from Norris Lake, TN Canon 6D, 70mm f/2.8, 6 seconds @ ISO 3200

 

IMG_0193

Star Party with Knox Observers, ORION, and SMAS members. 1/24/2015, from Norris Lake, TN.  Looking towards Orion rising in the East.

 

Jan 112015
 

I’ve temporarily pulled the portable (read small) rig out onto my back patio by the pool which has a narrow window allowing imaging of the southern sky.  Since the move to TN I haven’t had a lot of time to do any astronomical imaging but the bug to get out do some imaging finally got to me.

20150110-Rosette-Ha-6x20min

Rosette Nebula, Atlas EQ-G Mount, Stellarvue SVQ100 APO, Apogee U8300, 6x20min exposure with 3nm Astrodon Ha Filter.

Jan 102015
 
Comet-LovejoyIMG_9899_r

Animation of Comet Lovejoy over a span of about 60 minutes. Canon 6D, 70-200mm @ 200mm, 30sec exposures.

 

Luminance Animation of Comet Lovejoy C/2014 Q2

Luminance Animation of Comet Lovejoy C/2014 Q2

 

Comet Lovejoy 2014 Q2 – January 10th 2015, Atlas EQ-G Mount, Stellavue SVQ100 (100mm f/5.8 APO), Apogee U8300 CCD, 5x3min each L,R,G,B filters. (Clinton, TN)

 

 

Jan 032015
 
Double-Cluster_25P

The Double Cluster – Caldwell 14 Open Clusters NGC 869 & 884 Canon 6D, ISO 1600, 60 seconds Canon 70-200 f/2.8 @ f/2.8 Tracking on Atlas EQ-G Cherry Springs Dark Sky Park, PA

 

A widefield shot of the famous Double Cluster from Sept 17th 2014 at Cherry Springs State Park.  The Double Cluster is in Perseus but is in close proximity to Cassiopeia.

 

Double_Cluster_25P_Annotated

Annotated Double Cluster

Dec 262014
 

Apogee A694 Evaluation – Before Repair

I purchased one of the first Apogee Ascent A694 Cameras (Sony ICX694 Chip) before the acquisition by Andor and had some random horizontal banding across the top of the frame that was not possible to calibrate out:

Random Horizontal Banding: Pre-Repair

Andor issued an RMA and took care of the costs under warranty.  They stated that they repaired the camera by replacing the whole electronics board.

Apogee A694 Evaluation – Post Repair

 

I was hoping to not see the random horizontal bands again but upon firing up the camera and cooling down to -15C there were still there although they are now contained in a smaller region closer to the top of the frame.  It still moves around so calibration is difficult if not impossible.  When using a small number of frames it is hard to statistically reject the band.  You can see below in M42, reproduced at 50% size, that a bright band stands out across the top of the bias and dark calibrated image even after calibration.  This is especially obvious in narrowband images where the background pixel count isn’t much higher than the bias floor.  The band is also visible across the bottom of the Horse Head shot (I flipped the image) although it doesn’t stand out quite as much.

For a low bias noise camera geared towards narrowband imaging that I plan to use for portable imaging (lower frame count) I don’t think that my options are too great:

  1. Cropping out the top part of the frame (It’s a small chip to begin with)
  2. Trying to fix it in post processing (Different for every image)

 

I am also including 100% size images of the bias, master bias, dark, and master darks used to calibration the two trial images.

 

M42-Stacked

Apogee Ascent A694 – 6x10min Ha Evaluation after Repair.

 

Stacked-Horse-Head

Apogee Ascent A694 6x20min Post Repair Evaluation

 

 

 

Here is what several bias frames look like animated to give you an idea how the horizontal banding moves around and therefore is not well calibrated:

A694-Bias-animation

This is certainly better than what it was before but I am still left with these bands appearing faintly in my images.

All images were captured with the CCD cooled to -15C.  They were captured with MaximDL 5 and calibrated / processed in Pixinsight.

Oct 262014
 

I began work on a tri-color Hubble Pallet image during the summer of 2014 but due to weather and other obligations did not capture much in the way of Oxygen [O III] and Sulfur [S II] emission data for the mosaic project so am leaving it as a monochrome image using only the Hydrogen Alpha emission line data.

Cygnus Mosaic in Hydrogen Alpha Emission Line FSQ-106ED Apogee U16 CCD Baader 7nm Ha Filter AP900GTO Mount 6x20min Exposure Campmeeting Observatory, Sewickley, PA

Cygnus Mosaic in Hydrogen Alpha Emission Line
FSQ-106ED
Apogee U16 CCD
Baader 7nm Ha Filter
AP900GTO Mount
6x20min Exposure
Campmeeting Observatory, Sewickley, PA

Cygnus Mosaic – Annotated