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Burdge Research Group
Lightspeed Exposure Time Calculator
Sensor Properties
Select Sensor
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Pixel Size (μm)
Read Noise (e⁻/pix)
Dark Current (e⁻/pix/s)
Quantum Efficiency
Nonlinearity Scale Factor
Full Well Capacity
Telescope Properties
Select Telescope
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Diameter (cm)
F/number
Telescope Throughput
Altitude (m)
Observing Properties
Exposure Time (s)
Exposures in Stack
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Instrument Throughput
Limiting SNR
Seeing (arcsec)
Object Zenith Angle (deg)
Lunar Phase (deg)
Object-Moon Separation (deg)
Aperture Radius (pix)
Plot Transmission
Plot Magnitude vs. Precision
General Results
RUN
Pixel Scale (arcsec/pix)
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Pivot Wavelength (Å)
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PSF FWHM (arcsec)
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Central Pixel Ensquared Energy (%)
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A_eff at Pivot Wavelength (cm²)
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Limiting AB magnitude
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Saturating AB magnitude
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Airmass
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Zero Point AB Magnitude (1 e⁻/s)
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t_exp where bkg noise = read noise (s)
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Spectrum Observation
RUN
Flat spectrum at AB magnitude:
Blackbody Spectrum
Temperature (K)
Distance (Mpc)
Bolometric Luminosity (erg/s)
Custom spectrum name from spectra.py:
Spectrum Results
Signal (e⁻)
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Total Noise (e⁻)
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SNR
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Photometric Precision (ppm)
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Aperture Size (pix)
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Noise Breakdown
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System Transmission
Photometric Precision vs. Magnitude