WFC3 At a Glance

This page gives a high-level overview of WFC3's characteristics. Click on a given plot or figure to enlarge. For more detailed descriptions of WFC3's components and behaviors, see the WFC3 Handbook. Another good source of high level information is the WFC3 Summary handout.

Two Channels

Observations with WFC3 can make use of the UVIS or IR Channels. A channel select mechanism directs incoming light to the desired channel. The light path within WFC3 for both channels. The IR light path is drawn in red, and the UVIS light path is drawn in pink.

WFC3 detectors are capable of observing at all wavelengths between 200 - 1700nm. The QE curves for the UVIS and IR detectors are shown below. These curves do not include the effects of HST's OTA, nor WFC3's optics and filters.

Detector characteristics

See the Detectors page for more information.

IR Channel

Components: Teledyne 1Kx1K HgCdTe detector. MBE-grown, substrate removed.
Total Field of View: 123 x 136 arcsec
Pixel Size: 0.13 arcsec
Nominal Operating Temperature: 145 K
Median Dark Current: 0.015 e-/sec/pix
Dark Current Tail (% of pixels with Dark Current >0.4 e-/sec/pix): 0.7%
Readnoise (CDS): 15.5 e- (16 read linear fit)
Full Well: 93,000 e- (95% linearity)

UVIS Channel

Components: 2 e2V thinned, backside illuminated, UV optimized 2Kx4K CCDs
Total Field of View: 162 x 162 arcsec
Pixel Size: 0.04 arcsec
Nominal Operating Temperature: -83C
Dark Current: 0.16-0.41 e-/hour/pixel
Readnoise: 3.1 e-
Full Well: 75,000 - 80,000 e-

Filters

WFC3's complement of filters cover the entire useful wavelength range dictated by the detectors. Individual plots of filter throughputs are available in the WFC3 Handbook. Plots and tables of raw filter throughputs are available on the filter page.

The plots below show the total system throughput for all of WFC3's filters.