Hello, I am trying something new with my website. I mostly tend to my Flickr gallery at this point, so to reduce the upkeep and redundancy, I am using the Flickr API to pull my latest images straight from my gallery over there. Clicking on any image will simply take you to its page within my Flickr gallery (external link).
A categorical listing of work, separated into albums, is located here (external link).
A color composite of JWST commissioning data and some earlier, coincidentally imaged HST data. The nucleus of the galaxy is blatantly active when viewed in infrared with JWST.
Red-orange: JWST/MIRI F560W
Blue-cyan: HST/ACS/WFC F814W
North is 123.96° clockwise from up.
The thing about NIRCam and wideband infrared filters in general is that you get stars. Lots of stars. Even though this nebula is a pretty bright nebula, it has a hard time competing with all the stars. I’ve done the best I could do to show the nebula despite this fact. I think it’s worth zooming in to see the details better, because in the full view, stars are competing too hard with the nebula.
In particular, there are these interesting red "cometary" blobs that seem contained within little hollowed out parts of the bluer part of the nebula. These are very interesting, and difficult to see in any previous views of this nebula, from HST all the way up to JWST’s other camera, the MIRI. I know the nebula is formed by dust created by the star and sculped by winds from the star, but I’m not sure how these red blobs and their hollowed bubbles work out. I might guess that the red blobs are themselves producing some kind of wind force that is hollowing out their own little parts of the nebula. Or perhaps they are collapsing? Anyway, not knowing everything is the fun part about astronomy.
There was a very bright diffraction spike from a star off the lower left of the detector which I spent a long time trying to get rid of. It’s not a perfect solution, and some artifacts may be visible from this. I think it helped a lot to reduce the distraction from this rather annoying line that crossed the whole image.
I made a Behance project showing some of the steps I used to process this image.
Grayscale "screen" for overall brightness: NIRCam F444W
Red: NIRCam F335M
Green: NIRCam F210M
Teal: NIRCam F150W
Blue: NIRCam F090W
North is 40.56° clockwise from up.
This version of WR 124 is a combination of Hubble and JWST MIRI data. A press release recently featured the same data, and since this is one of my favorite objects, of course I had to have a go at it. The official release from the ERO team was a little bit dark. I also went ahead and used the same G’MIC processing to remove much of the banding noise from the dark parts of the image, allowing me to make it even brighter.
Red: JWST/MIRI F1800W
Yellow: JWST/MIRI F1280W
Yellow-Green: JWST/MIRI F1130W
Cyan: JWST/MIRI F770W
Blue: HST WF/PC2 F656N
North is 40° clockwise from up.
A combination of JWST and HST data showing a new view of ultraluminous infrared galaxy Arp 220. Here, I’ve tried to cut down on the redness because if I were to simply take all the data and throw it together, much of the galaxy would be lost in a red glare. Instead, the central details are actually visible. This is important because the imagery reveals what I presume to be the cores of the two galaxies that merged to create this single disturbed galaxy, not yet fully merged themselves. Prior to JWST observations two cores were already detected, but these new data reveal them in more detail than before.
Surrounding the center are some splotchy red and orange areas representing the MIRI (Mid-Infrared) data. This is essentially glowing dust. That is, the dust emits light in certain mid-infrared wavelengths, revealing it in much greater detail. In visible light, dust requires background illumination to see it or it is otherwise invisible. The eight faint, fuzzy red lines/bars emanating from the center are diffraction spikes caused by support structures of JWST.
Other interesting features include the blue clusters of younger stars resulting from recent star formation brought about when dust and gas collided as the galaxies orbited and merged with one another. Colorful background galaxies were also revealed in JWST data that were previously invisible or below the signal to noise ratio for HST observations. Note that many individual stars and star clusters are visible within the galaxy, thanks to the resolving power of JWST. What may look like noise in this galaxy is actually resolved stars!
Regarding the processing of this image: It took a long time to smooth this out to an aesthetically pleasing image. The shortwave NIRCam imagery is muddled by fine and coarse banding, which makes for a rather unsightly image if not taken care of. I’d like to thank the makers of the open source project G’MIC and specifically Simeon Schmauß for assisting me in greatly reducing and nearly eliminating the banding problems.
Data from the following proposals were used to create this image:
Proposal 2739 (no info as of this post)
An ACS Survey of a Complete Sample of Luminous Infrared Galaxies in the Local Universe
Reddish orange "screen": JWST MIRI F1130W
Red: JWST NIRCam F444W+F356W+F277W
Green: JWST NIRCam F200W+F150W+F090W
Blue: HST F814W+F435W
North is up.
Now here’s a dramatically long, straight bar of dust. There were other barred spirals that were expected to look something more like this, but the bar as viewed by JWST’s MIRI (Mid-Infrared Instrument) showed something less organized than expected. In NGC 1300, however, the bar is about as plain to see as bars get.
Curiously, to me, anyway, the dust seems to be softer and less sharp than this view of NGC 1566. They were observed using the same filters (hence, resolution should not be the cause). I’m not sure what it means, if anything.
Red (screen layer mode): MIRI F2100W
Orange: MIRI F1130W
Cyan: MIRI F770W
Extra overall brightness in grayscale: MIRI F1000W
North is 15.53° counter-clockwise from up.
As seen by JWST.
Grayscale "Screen": F210M
Red: F200W
Green: F150W
Blue: 140M
Titan’s north pole is up.
NASA / ESA / CSA / Judy Schmidt
The latest view of another dusty spiral galaxy from JWST’s MIRI. Took a bit of doing this time because the pipeline images available from the archive had a lot of alignment issues. I had to manually mosaic this. Luckily it wasn’t too difficult, or at least my human brain handled it fine. Not sure what is so confounding to a computer brain.
Red (screen layer mode): MIRI F2100W
Orange: MIRI F1130W
Cyan: MIRI F770W
Extra overall brightness in grayscale: MIRI F1000W
North is 1.5° counter-clockwise from up.
Update: Simeon Schmauß over on Twitter (@stim3on) recommended G’MIC for taking care of the horizontal noise / banding. It worked pretty great. There’s a Photoshop plugin for it, too.
Wanted to process my own version of this one, since nebular landscapes are some of my favorite views. Having a hard time with the linear noise pattern, especially near the top of the image.
In the center of this view is a newly forming star crossed by a dark disk of dust (say that three times fast!) which is casting shadows to the left and right, and allowing cones of light out the top and bottom. Think of it like a light bulb inside of a donut with a bunch of fog. Though the infrared light can penetrate much of the dust, there are clues in the image that show some of the dust is still too thick to see through. At the lower right especially are a lot of background galaxies. On the left, the background galaxies are fewer, and what we see are dimmer, so we can tell there is more dust there.
You can see the official release here. They’ve got a much better description than I could ever write.
Orange "screen": NIRCam/F444W-F470N (not arithmetic)
Red: NIRCam/F444W
Green: NIRCam/F335M
Blue: NIRCam/F200W, F187N, F115W
North is 100° counter-clockwise from up.
NASA / ESA / CSA / Jupiter ERS Team / Ricardo Hueso Alonso / Judy Schmidt
A 2-color collaboration with Ricardo Hueso. He came up with the color mapping and overall look of the image, and I reprocessed the data with a lot of inspiration from his work to fix a few cosmetic issues.
The diffraction spikes seen extending at regular angles from the brighter parts of the image were purposefully left in to highlight some of the difficulties working with data.
Orange: F212N
Cyan: F335M
Background is grayscale containing F335M data only.
Jupiter’s north pole is at the top.
NASA / ESA / CSA / Jupiter ERS Team / Judy Schmidt
A view of Jupiter seen in infrared by JWST on July 27, 2022.
A lot of work went into creating three congruent images to allow for the use of 3 color channels. Jupiter’s rapid rotation and not fitting within a single detector field makes things challenging.
Red-orange: NIRCam F360M
Yellow-green: NIRCam F212N
Cyan: NIRCam F150W2
Jupiter’s north pole is at the top.