Astrophysics (Index)About

STMAG system

(Space Telescope magnitude system, ST system, ST magnitude system)
(absolute monochromatic magnitude calibration used for HST)

The STMAG system of magnitudes sets the zero point for monochromatic magnitudes, specifically setting it to Fλ 3.63×10-9 erg cm-2 s-1 Å-1. The STMAG system is analogous to the AB system, but adopts a zero point for each wavelength based upon a wavelength-differential rather than a frequency-differential. Though the system is explained as monochromatic, this merely means it is calculated for a band by dividing by the EMR energy received by the wavelength-interval (bandwidth). Such a measure can only be determined from data over a non-zero bandwidth since a zero-width wavelength-interval must have zero energy. The ST magnitude is:

mST = - 5/2 log Fλ - 21.1.

Magnitudes require some adopted zero point as a consequence of their being logarithmic: "zero flux" cannot be used since zero has no logarithm (or its logarithm might be referred to as "minus infinity"). A brightness must be chosen to be represented by "zero magnitude", part of the definition of the magnitude's scale.

The ST stands space telescope: some Hubble Space Telescope instrument procedures make use of the system.


(measure,brightness,logarithmic,EMR,magnitude)
Further reading:
https://www.astronomy.ohio-state.edu/martini.10/usefuldata.html
https://hst-docs.stsci.edu/acsdhb/chapter-5-acs-data-analysis/5-1-photometry
https://www.stsci.edu/hst/instrumentation/acs/data-analysis/zeropoints
https://www.stsci.edu/hst/wfpc2/Wfpc2_dhb/wfpc2_ch52.html
https://hst-docs.stsci.edu/stisdhb/chapter-5-stis-data-analysis/5-3-working-with-imaging-data
https://hst-docs.stsci.edu/wfc3dhb/chapter-9-wfc3-data-analysis/9-1-photometry
https://pysynphot.readthedocs.io/en/stable/units.html
https://www.eso.org/sci/observing/tools/standards/spectra/hststandards.html
http://pleiadi.pd.astro.it/isoc_photsys.00/isoc_nicmosst/index.html
https://ui.adsabs.harvard.edu/abs/1986HiA.....7..833K/abstract
https://ui.adsabs.harvard.edu/abs/1996ApJS..107..423S/abstract
https://ui.adsabs.harvard.edu/abs/1996MNRAS.283..666M/abstract
https://ui.adsabs.harvard.edu/abs/2000ApJ...532..308B/abstract
https://ui.adsabs.harvard.edu/abs/2005MNRAS.359..874D/abstract

Referenced by pages:
AB system
photometric system
Vega system

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