TELESCOPE PRESETS
William Optics FLT-110 + SBIG ST-402
William Optics FLT-110 + SBIG ST-i
OGS RC20 + SBIG ST-8 (binned 2x2)
OGS RC20 + SBIG ST-8 (unbinned)
LCO Henrietta Swope (40inch) + SITe#3 Detector
Takahashi FCT-200 + FLI 4710 (binned 2x2)

WEBCCD

WebCCD is used to create FITS images of the sky based on a specific imaging system's parameters. Use it to create finder charts that match your imaging system. The tool uses the Digitized Sky Survey (DSS) for its data source and is restricted to the limitations of the DSS (60 x 60 arc minute max). Click Here for an image comparison created by WebCCD.

 

SIMBAD ID SEARCH
OBJECT ID

 

OBJECT
OBJECT RA
OBJECT DEC
TELESCOPE
CCD WIDTH   (pixels)
CCD HEIGHT  (pixels)
TELESCOPE FOCAL LENGTH
CCD PIXEL SIZE X (microns)
CCD PIXEL SIZE Y (microns)
CCD BINNING X
CCD BINNING Y
PLATE ROTATION (degrees)
LEFT HANDED	false     true
DSS SURVEY	POSS2/UKSTU Red POSS2/UKSTU Blue POSS2/UKSTU IR POSS1 Red POSS1 Blue Quick-V HST Phase 2 (GSC2) HST Phase 2 (GSC1)
RETURN FITS IMAGE
RETURN PNG IMAGE

 

 

Created by Don Carona, Physics Observatory, Texas A&M University