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

Oct 132014
 

I am starting to pack up Campmeeting Observatory in preparation for a move to Knoxville, TN.  It has only been a short 3 years that Campmeeting Observatory has been in operation but I am sure it will find a new home.  For the time being, updates will be seldom as other priorities will take center stage and extensive observatory site preparation may be required.

Aug 272014
 
Cherry Springs panorama from the northern side of the overnight astronomy field

Cherry Springs panorama from the northern side of the overnight astronomy field

 

Cherry Springs

Cherry Springs

Monday night was my first visit to a dark site; or at least my first visit since catching the astronomy bug.  Upon arriving at Cherry Springs after the 4 hour drive I noticed there were quite a few people  still hanging around after the Black Forest Star Party which was held over the weekend.  According to some of the other amateur astronomers, the weekend star party was a bust.

We found a vacant spot to setup our tents right next to one of the RV style power outlet posts scattered throughout the observing fields.  I can’t stress how wonderful it is to have power provided  on the field for the astrophotographically inclined!

The grounds were well kept and the main bathrooms much nicer than expected.  The surrounding area is gorgeous for anyone who enjoys the outdoors.

 

Untracked 30 Second Exposure

Untracked 30 Second Exposure

As nice as the park was, the show obviously didn’t start until the sun went down.  The Milky Way was more prominent before astronomical twilight than I’m used to seeing here in the PGH region after astronomical twilight; even at the Greene County site.  By 10:00pm it was gorgeous and I snapped a quick 3o second shot on a tripod and marveled that the dark lanes extending out from the Rho Ophiuchi / Antares region were clearly visible in a short exposure so close to the horizon.

Seeing the sky like this puts everything in a different perspective.

Yes, it’s depressing being back in light polluted Pittsburgh but I’m really glad I finally made it out to Cherry Springs after all this time.

I had plans to shoot some other objects but due to poor planning and setup of my tent I couldn’t take some of the deep southern objects I was hoping for.  I settled for 5.5 hours of exposure time on NGC 7023:  The Iris Nebula.  I have shot the Iris before but was never totally happy.  I’m still not quite satisfied but it’s certainly better than what I’ve gotten around here.

4 minute Exposure Canon 6D 200mm f/2.8 Tracking, Unguided

4 minute Exposure
Canon 6D
200mm f/2.8
Tracking, Unguided

NGC-7023-LRGB-Combine-V2

NGC 7023 Atlas EQ-G Mount Stellarvue SVQ100 – 100mm f/5.8 Quadruplet Apogee Ascent A694 CCD 5.5 Hours Total LRGB Exposure

 

The Iris Nebula, also NGC 7023 and Caldwell 4, is a bright reflection nebula and Caldwell object in the constellation Cepheus. NGC 7023 is actually the cluster within the nebula, LBN 487, and the nebula is lit by a magnitude +7 star, SAO 19158.[1] It shines at magnitude +6.8. It is located near the Mira-type variable star T Cephei, and near the bright magnitude +3.23 variable star Beta Cephei (Alphirk). It lies 1,300 light-years away and is six light-years across.[2]

Courtesy of Wikipedia.

Aug 202014
 

Thursday night at Wagman was one of the most transparent nights I’ve ever seen at Wagman.  The MW was easily visible and dipping further into the south than usual.  I took a few pictures around the observatory to try and show how nice the view was.

 

Aug 112014
 

8/10/2014 – During a full moon night at Wagman Observatory I decided to play with the Brashear Refractor and determine requirements for extension tubes and other adapters to reach focus with a small chip high speed, webcam like, imaging camera for lunar and planetary imaging.  As luck would have it, very little was needed outside of the ordinary adapters, focus was easy to reach, and the Brashear performed well considering the lousy seeing and the “flatness” or lack of contrast we normally have during a full moon.  Hunting around on the eastern limb of the moon took us to Crater Neper whose central peak just catches the light and whose shadow can be seen against the rear crater wall.

 

Crater Neper

Crater Neper taken through the Amateur Astronomers Association of Pittsburghs 11 inch Brashear Refractor at Wagman Observatory

Aug 012014
 

Another decent night at the AAAP Greene County Dark Sky Site.

NGC 6914 is a reflection nebula nestled amongst the diffuse emission nebula in Cygnus.

NGC 6914 SVQ-100 Apogee Ascent A694 Atlas EQ-G w/eqmod 5x10min Lum 6x10min Red 6x10min Green 6x10min Blue Total:  3.8 Hours Greene County, PA

NGC 6914
SVQ-100
Apogee Ascent A694
Atlas EQ-G w/eqmod
5x10min Lum
6x10min Red
6x10min Green
6x10min Blue
Total: 3.8 Hours
Greene County, PA

Playing around with an 8mm circular fisheye lens as well for an all sky timelapse.

[youtube:http://youtu.be/l92QPyDS_GQ]

Jul 302014
 

Development of our rural countryside is rapidly increasing due to emergent industries like oil and gas.  A single industrial site is often lit up like a little town on the map making one wonder if residential, commercial, or industrial development is the true light pollution problem?

Click on the Images below for an animation comparing Light Pollution levels in 2003 to 2012.

Greene County LP 2003 vs 2012

AAAP Greene County Site with Light Pollution growth from 2003 to 2012

 

Pittsburgh Area Light pollution growth from 2003 to 2012.

Pittsburgh Area Light pollution growth from 2003 to 2012.