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NCU Lulin Observatory
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Observing Setup
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Telescope
Telescope parameters
Primary Mirror Diameter
m
Secondary Mirror Diameter
m
Focal Length
m
Optical Throughput
%
Camera
Camera parameters
Pixel Pitch
µm
Quantum Efficiency
%
Dark Current Rate
e-/s/pix
Readout Noise
e-/pix
Full Well Capacity
e-
Filter
Filter parameters
Central Wavelength
nm
Filter Bandwidth
nm
Filter Transmission
%
System
Throughput Correction
%
Coordinates (J2000, decimal degrees)
Right Ascension
deg
Declination
deg
Morphology
Morphology
Point Source (e.g., Star)
Extended Source (e.g., Galaxy)
Brightness
Brightness System
Vega Magnitude
AB Magnitude
Jansky Flux (Jy)
Wavelength Flux (erg/s/cm²/Å)
Apparent Magnitude
mag
Zero Point Flux
erg/s/cm²/Å
Flux Density
Jy
Spectral Energy Distribution (SED)
SED Model
Flat Spectrum
Spatial Spreading (FWHM, arcsec)
Seeing
Diffraction
Optical
Tracking
Atmosphere & Background
Add moonlight to sky background
Dark Sky Brightness (mu_dark, baseline)
mag/arcsec²
Extinction Coefficient
mag/airmass
Observatory Location
Latitude
deg
Longitude
deg
Elevation
m
Exposure Strategy
Single Exposure Time
s
Calculation Goal
Solve for SNR (given exposures)
Solve for Exposures (given target SNR)
Number of Exposures
Target SNR
When
Sweep time range
Observation Time (local)
Start Time (local)
End Time (local)
Time Step
min
Photometry — aperture and sky annulus
Aperture Factor (k_ap)
Sky Annulus (k_in – k_out)
Sky Estimator
Median (rejects neighbours, costs π/2)
Mean
Primary Result
—
Waiting for input…
Signal & Noise Budget
Source Rate
—
e-/s
Sky Background
—
e-/s/pix
Peak Pixel Rate
—
e-/s/pix
Single Exp. SNR
—
Physical Diagnostics
Total FWHM
—
arcsec
Pixel Scale
—
"/pix
Effective Area
—
m²
System Throughput
—
%
Enclosed Flux
—
%
Aperture Pixels
—
px
Sky Estimate Cost
—
px
Observation Limits
Saturation Time Limit
—
s
Optimal Exposure Time
—
s
Observing Window
Bug Report
Wang, Tong & Hsu, Po-Chih & Prof. Chen, Ting-Wan