
Free Background Remover: Remove BG from Image Online - Pixelcut
Download your image as a PNG with no background or keep editing with Pixelcut until your image is ready to be shared or used on your next project. Our BG Remover automatically removes …
batcelldetect HEADAS help file - NASA
Users can increase the significance of a detection and reduce false detections by requiring more than one adjacent pixel exceed the threshold, using the "nadjpix" parameter. The "nullborder" …
bkg x out Background region center X sky coord 0.05 arcsec pixel bkg y out Background region center Y sky coord 0.05 arcsec pixel bkg rad1 phys out Background region: circle or inner …
NovaPro UHD Jr - NovaStar
Customized BKG settings Supports pure color and image BKGs. Personalized image scaling Supports 3 kinds of image scaling modes: full screen, pixel to pixel, custom. Capture function …
Kepler Data Products Overview - California Institute of Technology
Jun 24, 2024 · Location: Go to Kepler Full Frame Image (FFI) & Engineering Data Search (MAST) and specify an Archive Class of “Background Pixel (BKG)”. Format: FITS (see KAM Table 2-1 …
Description - heasarc.gsfc.nasa.gov
The task ebkgreg searchs for the most suitable position of a region to get the background estimation of any source in an EPIC image (PN or MOS). This task has two processing …
MAST K2 Search and Retrieve
Jul 16, 2020 · Available ancillary data files including CBVs, FFIs (and engineering data), thruster firing listings, and the latest Spice kernels for the Kepler spacecraft. This page lists the K2 …
Bleach: Urahara Pixel w-bkg by ShiningamiMaxwell on DeviantArt
Aug 22, 2006 · a commisioned pic of Urahara from the anime/manga Bleach. This one is in PNG format with a background, because sometimes saving as a Gif screws up my colors. i think the …
photutils.background.local_background — photutils 2.2.0 - Read …
[docs] class LocalBackground: """ Class to compute a local background using a circular annulus aperture.
| notebook.community
We assumed that the image had a typical value of 1.5" per pixel. But we can make a more accurate estimation by fitting the pixels to a moffat profile around a detected star.
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