All Astronomy Calculators Related Post

Doppler Boosting Calculator Calculate Relativistic Doppler Boosting & Beaming Velocity of Source (as fraction of c): Observer Angle θ (degrees from line of motion): Rest-Frame Luminosity (arbitrary units): Calculate Doppler Boosting About the Doppler Boosting Calculator The Doppler Boosting Calculator is a precise scientific tool that computes the relativistic enhancement of brightness due to the […]

Jet Opening Angle Calculator Bulk Lorentz Factor Γ (γ): Jet Velocity β (fraction of c): Calculate Jet Opening Angle About the Jet Opening Angle Calculator The Jet Opening Angle Calculator is a scientifically accurate, peer-reviewed tool that computes the relativistic Jet Opening Angle (θj) in active galactic nuclei (AGN), gamma-ray bursts (GRBs), and blazars using

Relativistic Beaming Calculator Calculate Relativistic Beaming Effects Velocity v (as fraction of c): Observer Angle θ (degrees): Calculate Beaming About the Relativistic Beaming Calculator The Relativistic Beaming Calculator is a precision scientific tool that computes the dramatic effects of Relativistic Beaming (also known as Doppler boosting or headlight effect) in special relativity. This phenomenon occurs

Fast Radio Burst Calculator Redshift (z) Fluence (Jy ms) Observing Frequency (MHz) Dispersion Measure (pc cm⁻³) What do you want to calculate? All ParametersIsotropic Radiated Energy & LuminosityComoving & Luminosity DistanceTotal Isotropic Energy Calculate FRB Parameters About the Fast Radio Burst Calculator The Fast Radio Burst Calculator is a scientifically rigorous, peer-reviewed tool that instantly

SKA Sensitivity Calculator Calculate SKA Sensitivity & Integration Time Observing Frequency (MHz): Bandwidth (MHz): Source Flux Density (mJy): Desired Signal-to-Noise Ratio (SNR): SKA Configuration: SKA-Low (50–350 MHz)SKA-Mid (350–15000 MHz) Calculate Sensitivity About the SKA Sensitivity Calculator The SKA Sensitivity Calculator is a scientifically accurate tool designed to estimate the sensitivity and required integration time of

VLA Sensitivity Calculator Array Configuration: A (Most Extended – Highest Resolution)BCD (Most Compact – Highest Sensitivity) Observing Frequency (GHz): Bandwidth (MHz): Integration Time (hours): Number of Antennas (typically 27): Calculate Sensitivity About the VLA Sensitivity Calculator The VLA Sensitivity Calculator is an astronomically accurate, peer-reviewed tool that predicts the exact RMS noise and sensitivity achievable

ALMA Sensitivity Calculator Calculate ALMA Observation Sensitivity Observing Frequency (GHz): Bandwidth (GHz): Integration Time (hours): Number of Antennas: 50 (Typical 12-m Array)66 (Full 12-m Array)43 (ACA 7-m Array) Array Configuration: Compact (C43-1 to C43-4)Intermediate (C43-5 to C43-7)Extended (C43-8 to C43-10) Precipitable Water Vapor (mm): Excellent (Quintile 1)Good (Quintile 2)Average (Quintile 3)Poor (Quintile 4) Calculate Sensitivity

Beam Size Calculator Wavelength λ (nm): Propagation Distance z (m): Beam Waist w₀ (μm): Calculation Method: 1/e² Intensity (Standard)D4σ (Second Moment)FWHM Calculate Beam Size About the Beam Size Calculator The Beam Size Calculator is a scientifically accurate, peer-reviewed tool that instantly computes Gaussian beam propagation parameters using the exact ABCD matrix formalism and ISO 11146

Radio Telescope FOV Calculator Calculate Field of View (FOV) for Your Radio Telescope Dish Diameter (meters): Observing Frequency (MHz): Or Enter Wavelength Directly (meters): Calculate FOV About the Radio Telescope FOV Calculator The Radio Telescope FOV Calculator is a precision scientific tool that computes the angular Field of View (FOV) of parabolic radio telescopes using

Visibility Function Calculator Calculate Interferometric Visibility Maximum Intensity (I_max): Minimum Intensity (I_min): Source Type (Optional): General SourcePoint Source (Visibility = 1)Uniform DiskBinary Star System Calculate Visibility Function About the Visibility Function Calculator The Visibility Function Calculator is a precision scientific tool that computes the interferometric visibility (also known as fringe visibility or coherence degree) using