▪ Abstract Standard star photometry dominated the latter half of the twentieth century
reaching its zenith in the 1980s. It was introduced to take advantage of the high sensitivity …

During the commissioning of JWST, the medium-resolution spectrometer (MRS) on the mid-
infrared instrument (MIRI) observed the planetary nebula SMP LMC 058 in the Large …

We describe the data reduction algorithms for the Multiband Imaging Photometer for Spitzer
(MIPS). These algorithms were based on extensive preflight testing and modeling of the Si …

We present a study of the [C II] 157.74 μ m fine-structure line in a sample of 15 ultraluminous
infrared (IR) galaxies (IR luminosity L IR⩾ 10 12 L⊙; ULIRGs) using the Long Wavelength …

Infrared astronomy is a dynamic area of current research. It has been revolutionized in the
past few years by the advent of large, sensitive, infrared arrays, and the success of several …

We report measurements of the [C II] 157.74 μ m fine-structure line in a sample of seven
ultraluminous infrared galaxies (ULIGs)(L $\mathstrut {_ {{\rm IR}}} $> 10$\mathstrut {^{12}} …

This is the first paper in a series of three where we present the first comprehensive inventory
of solid state emission bands observed in a sample of 17 oxygen-rich circumstellar dust …

We report on the detection of nine lines of the ν 2 bending mode of triatomic carbon, C 3, in
the direction of Sagittarius B2. The R (4) and R (2) lines of C 3 have been also detected in …

Infrared spectra of a number of evolved O-rich stars have been obtained with the Short-and
Long-Wavelength spectrometers on board the Infrared Space Observatory. The very broad …

We have investigated with the Long Wavelength Spectrometer (LWS) of the Infrared Space
Observatory (ISO) the far-infrared spectra (43–197 μ m) of a sample of 17 class 0 sources …