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Observations of standard stars with NICMOS grism (G096), when compared with the same standards taken by STIS (G750L), show a disagreement over the wavelength range 0.8 to 1 micron. Further comparison with ACS F850LP data confirms thisnon-linearity to be due to NICMOS in the sense that fainter stars in NICMOS appear too faint relative to a brighter normalisation. We investigate this over a wide ...
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ژورنال
عنوان ژورنال: Diabetologia
سال: 1986
ISSN: 0012-186X,1432-0428
DOI: 10.1007/bf00870148