STScI Logo
STScI Logo
HST
Banner
FAQ

Space Telescope Science Institute
STIS Instrument Handbook
help@stsci.edu
Table of Contents Previous Next Index Print



The F25LYA filter with the FUV-MAMA provides narrowband imaging of the HI 1216 Å Lyman-α line.
Lyman-α imaging. Differencing two images taken with 25MAMA and F25SRF2 is another option.
Sensitivity is limited by geocoronal Lyman-α. Observers can limit the background (with some cost to the total amount of observing time per orbit) by using the DARKTIME special requirement.
Users may also want to consider whether the ACS SBC detector with the F122M filter might be a better choice for their observing program.
Pivot λ (Å)
FWHM (Å)
AB mag zero point
Speak
Bλ
R80 (arcsec)
Table 14.8: F25LYA FUV-MAMA Sensitivity & Throughput
Figure 14.95: Extended Source S/N vs. flux for the F25LYA FUV-MAMA mode. Top curves are for an area of 0.2 arcsec2; bottom curves are for 1 arcsec2. Average sky assumed. Curves are labeled by required exposure time (seconds).
Fraction of Energy Encircled
Figure 14.96: Point Source PSF for F25LYA FUV-MAMA, 7."5 square (at pixel 739, 368, log scaled, B-V=-0.04)

Table of Contents Previous Next Index Print

Copyright  | Help  | Printable Page