# Novel Deep Level Image State Ensemble Enhancement Method for M87 Imaging
## 1 Introduction
The ability of infrared light to penetrate dust makes the test image taken from the SST ideal for multiple reasons. First, the quality of the image is high due to NASA employing some of the best scientists and engineers on the planet. Image analysts have worked their scientific wizardry and have taken this selected image to the very limits of the SST's capability. Second, the infrared (IR) regime of the spectrum has many applications that are of interest to industry and scientific study. IR can be used in fire rescue to see through the thick smoke of a burning building and help save people that are trapped [8], medical applications such as detection of melanomas [9] and breast cancer, remote sensing by [10] satellite for oceanography [11] and meteorology [12], agriculture and food science [13], and autonomous navigation [14], just to name a few. ISED and ISEE need at least two-color bands to be implemented, depending on the sensor scheme or camera involved; however, one could feasibly apply the proposed methods to the aforementioned applications in order to construct a broad range of filters or selective enhancements to optimize the systems. Due to deep Ln ISED and ISEE's unique method of image decomposition and enhancement, we discovered, by observation via image processing the test image, that there is evidence for a past explosive outburst that is tangential to HST-1 and it seems to have originated from HST-1 and a structure resembling a vortex located over the vicinity of M87's black hole and galactic center. HST-1 is a knot structure that was observed to change in luminance in the path of the eastbound superluminal jet [15]. This study also observed that on the west side of the outer dust ring, there is a linear relationship between the vortex and observed channel that is the apparent path of the superluminal counter-jet that forms the C-like shockwave structure to the west of the IR core. This jet is rendered invisible due to its relativistic Doppler shift [16]. The counter-jet channel has a linear relationship to a possible second knot, which I will refer to as HST-2. Furthermore, near the vortex is a blue C-like structure that seems to originate within the vicinity of the vortex structure, and it extends outward to follow the apparent path of the shockwave. The IR outburst is located on the northeastern portion of the IR core, and it seems to be near HST-1. Additionally, with select ISED filters and ISEE reconstruction schemes, we were able to resolve the dusty IR core, outer dust ring, and shockwaves with stunning clarity. The clarity is due to the enhanced contrast from the combination of ISED and ISEE reconstruction. The filter reduces the blue-biased glare and noise, which enhances the contrast and informative structural details of the IR core, and the outer dust ring becomes more pronounced. The ISEE reconstruction restores a portion of the information to the image. Image quality assessments (IQAs) are shown with the corresponding images in the Results and Discussion section. Moreover, located on the southwestern portion of the dusty outer ring, there is a globular mass that appears to be feeding the black hole or perhaps was formed from another outburst from the black hole. The mass is a clump of matter like that of the globular structure that apparently obscures regions of the eastbound visible spectrum superluminal jet, perhaps a globular cluster because so many are prevalent in M87 [17]. As a final point, within M87's dusty IR core, there appears to be a direct disturbance caused by the proximity of the supermassive black hole. In order to further analyze the findings, a Sobel filter was applied to a tighter crop of the galactic core image to produce images of the Sobel gradient magnitude, directional gradients, and gradient direction. Furthermore, image differencing with intensity scaling was used to build an additional set of images to compare the ISEE images to the original image [18]. Several overlays were also constructed from the SST ISED test image and a Hubble Space Telescope (HST) image [19].