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Sky Quality Meter - FAQ

General SQM Questions

What kind of sensor is used in the Sky Quality Meter?
A TAOS TSL237S sensor is used, you can view the specs here. The sensor is covered with a HOYA CM-500 filter, you can view the spectral response curves here, PDF spec sheet here including response data points.

Should the meter be recalibrated?
Normally there is no recalibration required. However, in some cases we have seen that the IR filter becomes frosted due to moisture. Take a look into the lens and you should see a clear blue area (the IR filter) and a small black dot (the sensor). If there is a white frosting on the blue glass, then the unit will require recalibration. Contact here for recalibration.

Do you provide a calibration certificate?
There is no calibration certificate available. The NIST meter that we use to calibrate against is the EXTECH Instruments Model 401027. You can read more about Extech meters here

Do you have any benchmarks for linking magnitudes per square arc sec with the Bortle scale?
We believe that if you check this Wikipedia Bortle Dark-Sky Scale link, the descriptions associated with each mag/sq arcsec are sufficiently detailed that you could draw up a pretty decent correspondence.

Have you measured the spectral response of the detector with the IR rejection filter, and how closely does it match the response of the human eye?
We haven't measured the spectral response curve ourselves, but the sensor manufacturer has. It is very close to that of the human eye. The Hoya CM-500 filter cuts off the entire infrared part of the spectrum. The response is that of the "clear" line in Figure 2 of the TCS230 datasheet (which is for a different sensor in the TAOS line).

The combined spectral response compared to other standards is shown in this Night Sky Photometry with Sky Quality Meter report in Fig 12, on page 6.

Do you know the contribution from the Milky Way with the wide-angle of acceptance of your photometer? I would like to subtract the Milky Way if possible.

The northern Milky Way contributes about 0.10 mpsas under 21.5 mpsas (moonless) skies.

The southern Milky Way might be as big an effect as 0.85 mpsas where it goes near-overhead.

For more information, see Surface Photometries of the Milky Way (Schlosser+ 1997)

How does transparency affect the SQM readings?

The SQM's readings are assuming 'best transparency'.

You can get an updated definition of the transparency in your area from:

Also, frequently local weather stations can provide "visibility" and "relative humidity" numbers which could potentially be used as surrogates for actual transparency measurements (which aren't possible with a handheld meter).

How does zodiacal light affect the SQM readings?
It is likely to be less than a 1 or 2 percent effect. The primary reason is that the brightest and widest part of the zodiacal light is nearest the horizon where the SQM has almost no sensitivity (due to it being a zenith-looking device). The portions at higher altitude are the narrowest and faintest and they would barely creep into the sensitivity cone of the SQM.

What are "Magnitudes per Square Arc Second"?

Magnitudes are a measurement of an objects brightness, for example a star that is 6th magnitude is brighter than a star that is 11th magnitude.

The term arcsecond comes from an arc being divided up into seconds. There are 360 degrees in an circle, and each degree is divided into 60 minutes, and each minute is divided into 60 seconds. A square arc second has an angular area of one second by one second.

The term magnitudes per square arc second means that the brightness in magnitudes is spread out over an square arcsecond of the sky. If the SQM provides a reading of 20.00, that would be like saying that a light of a 20th magnitude star brightness was spread over one square arcsecond of the sky.

Quite often astronomers will refer to a sky being a "6th magnitude sky", in that case you can see 6th magnitude stars and nothing dimmer like 11th magnitude stars. The term "6th magnitude skies" is very subjective to a persons ability to see in the night, for example I might say "6th magnitude skies" but a young child with better night vision might say "7th magnitude skies". You can use this nifty calculator created by SQM user K. Fisher to do that conversion, or this chart.

The "magnitudes per square arcsecond" numbers are commonly used in astronomy to measure sky brightness, below is a link to such a comparison. See the third table in section 10 for a good chart showing how these numbers in magnitudes per square arcsecond relate to natural situations:


Each magnitude lower (numerically) means just over 2.5 times as much more light is coming from a given patch of sky. A change of 5 mags/sq arcsec means the sky is 100x brighter.

Also, a reading of greater than 22.0 is unlikely to be recorded and the darkest we've personally experienced is 21.80.

Reading accuracy

The value produced by the sensor in the SQM is affected by temperature. There is a temperature sensor in the SQM that compensates for this effect. However, when the SQM is first powered up, the light sensor is colder than when the power has been on for a few seconds. Depending on the ambient temperature this will result in the first reading being slightly higher than subsequent readings.

For the most accurate results, it is best to take many readings and disregard the very first reading.

The temperature sensor and light sensor are separated on the circuit board. Waiting for a while will allow a changing temperature to migrate so that both sensors are at the same temperature.

This issue is due to the transient response of the TSL237 which briefly changes its light-to-frequency characteristic when it is warmed by applied power. Ironically, the normally very sensible practice of leaving it out at the environmental temperature probably makes it more significant.

What is the range of the Sky Quality Meters

There is no specific limit on the range of the SQM because the calibration step fixes the maximum and minimum frequencies to intermediate values. For normal night-time viewing, the meter should accurately read from about 16 to 23 mpsas, but is it has a range from about 7 (brightest) to 23 (darkest).

Each sensor is slightly different. The calibration uses the dark period of the sensor compared to a frequency at a specified light level.

The meter sets a bright limit of 400kHz which is the specification for light saturation of the TSL237S sensor. When the sensor frequency reaches this value, the output is set to 0 mpsas. The only thing that will extend sensitivity in bright settings is to limit the amount of light received with an optical filter. Filters can be fitted over the meter manually or with the help of an adaptor like these.

The internal limit for the dark period is 60 seconds which works out to about 26mpsas for most sensors.

Some testing can be done using the UDM software with simulation mode on a connected meter.

Can the mpsas readings be converted to Lux or Foot Candles

No. Lux (lx) and foot candles (fc) are a measure of "Illumination" (light hitting a surface). Meters that measure this usually have a white surface were light hits and is measured by a sensor inside which is calibrated to Lux or fc.

The SQM measures "Luminance", the light given off by a surface. In the case of night sky viewing for astronomy, it is the light given from the night sky that you would see with your eye. Luminance meters see the light as your eye would (from a point outwards in a cone) and only a small sensor area is used. The SQM produces a reading of magnitudes per square arcsecond which can be converted to other Luminance values like "candela per square meter". We have such a converter on our website here.

When determining brightness differences with the SQM, you can convert the reading to cd/m^2 then get the ratio between your various readings by division. Using this method, you should be able to say that "light fixture A is X times brighter than light fixture B".

For the Sky Quality Meters, the un-diffused value of light is received in a cone shape with the response shown here.

Temperature reading

For purposes of light sensor compensation, there is a temperature sensor located inside the meter.

This internal temperature reading is available to the user. The value is not the ambient or outdoor temperature.

How to point the meter

The meter is calibrated to be pointed upwards (Zenith) when taking readings.

Pointing in directions that see obstructions or the ground will result in inaccurate readings.

Can the field of view be narrowed

Adding a shroud is possible, but it will likely cover the field of view, then the reading will become darker by a fixed amount. You can determine that darkening amount by taking readings with/without the shroud in an evenly lit dark open sky. Then you would subtract your shrouded readings by that measured difference.

See FOV comparison chart for as reference of what the field view is for your meter.

SQM & SQM-L Questions

What is the difference between the SQM and SQM-L?

Here is a chart showing the differences at a glance.

The main difference is the field of view. The SQM-L (with lens) is an improvement over the SQM. The lens collects more light from a smaller cone so that the meter is not affected from lights or shading on the horizon.

The SQM spec for field of view is located in this technical report. A comparison of the angular response for both meters is here. Generally speaking, the SQM-L 'Half Width Half Maximum' is ~10 degrees as opposed to ~42 degrees for the SQM.

The SQM-L is better suited for astronomy and dark sky enthusiasts. It has a lens to narrow the field of view so that street lights and buildings or trees do not affect the reading very much.

If you expect to always take readings at dark sky sites in an open field then the regular SQM will do fine for that task.

Note: The SQM-LE has the same optics as the SQM-L.

Does the SQM or SQM-L have an external port that can be connected to a PC?

No, the SQM and SQM-L do not have an external port. These models have a minimum of components to reduce costs, and they cannot communicate with a PC.

The SQM-LE has the same optics as the SQM-L as well as a computer interface via an Ethernet connection. If you intend on just connecting the unit to a laptop rather than a network, an Ethernet crossover cable can be used.

Meter makes a quiet clicking noise instead of providing a reading.

Try replacing the battery with a fresh one.

How can I get the model and serial number from the SQM or SQM-L?
The temperature in degrees Celsius then degrees Fahrenheit are displayed when you press and hold the button a second time. Also, the model and serial number are displayed after the temperature.

For example, press and release the button once. While the display is still showing something, press and hold the button and watch the following results:

  1. Temperature in degrees Celsius. This is the temperature inside the unit, not the outside temperature.
  2. Temperature in degrees Fahrenheit. This is the temperature inside the unit, not the outside temperature.
  3. Model number, like _2.17. Model 1.xx is the SQM, Model 2.xx is the SQM-L. The last two digits are the firmware revision.
  4. Serial number, like 3647. Model _2.19/_1.19 and greater use hexadecimal numbers, for example serial number 001C hex = 0028 decimal. See character set below
    character set

SQM Questions

What is the field of view for your device?
See FOV comparison chart.

The "effective solid angle" is 1.532 steradians. The angular response if effectively that in the TSL237S datasheet.

It is worth pointing out that this is not a "spot" meter - it accepts light from a wide cone - roughly 80 degrees diameter on the sky (we measured the effective solid angle to be 1.532 steradians). To produce a spot meter, a fast lens and mounting hardware would have been required and this would have dramatically increased the price. In practice, we believe the reading is representative of the range of altitudes over which observers would typically observe.

How was the solid angle of the detected light chosen?

We picked the large solid angle of the detector partly for greatest sensitivity and partly to be representative of the sky conditions over the part of the sky where people would normally be observing and imaging. It is straightforward to reduce this solid angle with a mask, but different observers have different preferences for beam size and so our design offers the maximum flexibility and customizability. The adoption of a different solid angle would require a fixed zeropoint correction to the meter reading.

For equivalent sensitivity at a smaller solid angle, a lens and mounting hardware would be necessary, significantly increasing the cost of the unit for little added functionality.

What if the SQM is reading too dark (reading 23 or 24)?

Ensure that the sensor is aimed at the sky. The SQM sensor is on the same side as the display, so you will aim the display at the sky and press and release the button, when the beeping stops, then you can turn the unit towards you to see the reading.

How should the SQM be held when taking readings?

  1. Hold the meter above your head to prevent shading of your body on the sensor.
  2. The SQM sensor is on the same side as the display, so aim the display at the sky.
  3. Press and release the button.
  4. When the beeping stops, then you can turn the unit towards you to see the reading.

SQM-LE Questions

Is the SQM-LE waterproof?

No, the SQM-LE is not weatherproof. For permanent mounting outside, it should be mounted in a weatherproof housing.

We sell such a housing here.

For people using the unit only during telescope observations, the meter can be stowed away with the telescope.

Here are some sources for plastic domes:
Some considerations for preparing a high end weatherproof enclosure:

Does the SQM-LE stay dew-free and frost-free?

Yes, the heat generated inside the SQM-LE by the internal web server is high enough get rid of dew. When used with this housing, no dew was ever seen inside the unit. In fact, drops of rain on the glass cover evaporated after a few hours.

It may be important to allow moisture to escape, that is why we have an air hole on the bottom of our housing.

As far as frost goes, the unit is too warm to allow that. If the unit is un-powered then moisture will likely build up. It is probably best to always keep the unit powered.

How can I reduce the wiring to the SQM-LE?

A PoE system can be used to transmit "Power Over the Ethernet" cable to the SQM-LE. A PoE system consists of two units:

  1. The PoE Injector puts power into an Ethernet cable.
  2. The PoE Splitter gets the power from the Ethernet cable.

The PoE Injector would be located near the router, and the PoE splitter is located near the SQM-LE.

The PoE soution is very handy if you do not have an electrical outlet near the SQM-LE. You can just run the Ethernet cable to the PoE Splitter then short wires come from the splitter to the SQM-LE.

We have tested these models successfully with the SQM-LE:

If you already have a PoE system (with injector), then you just need a PoE splitter that puts out 5V for the SQM-LE.

How can the SQM-LE be made wireless?
The SQM-LE can be connected to a wireless router that communicates with another wireless router at a base station. We have successfully tested the LinkSys WRT54GL.
The power requirements of the SQM-LE does not make it a candidate for a small solar cell or batteries.

What is the upper operating temperatuire of the SQM-LE?
The maximum operating temperature of all the components inside the SQM-LE is 85C.
We have been operating the unit inside a housing and the unit temperature has reached 65C on many occasions without affecting operation. Here is the housing that we are using: housing.pdf
The light sensor readings are compensated for temperature fluctuations. The temperature sensor located very close to the light sensor.

Cannot find the device IP address on the network.
Use the red crossover cable and connect the SQM-LE directly to the Ethernet port of the computer then use the Lantronix Device Installer to detect the unit.

Can find the device IP address but the unit does not respond.
Use the UDM facility ->Firmware tab -> XPort defaults