Mid-infrared sources in the ELAIS Deep X-ray Survey
We present a cross-correlation of the European Large Area Infrared Space Observatory (ISO) survey (ELAIS) with the ELAIS Deep X-ray Survey of the N1 and N2...
Mid-infrared Spectral Variability Atlas of Young Stellar Objects
Optical and near-infrared variability is a well-known property of young stellar objects. However, a growing number of recent studies claim that a considerable...
Mid-infrared spectroscopy of infrared-luminous galaxies at z ~ 0.5-3
We present results on low-resolution mid-infrared (MIR) spectra of 70 IR-luminous galaxies obtained with the infrared spectrograph (IRS) onboard Spitzer. We...
Mid-infrared spectrum of the zodiacal light observed with ISOPHOT
We present 29 mid-infrared spectra of the zodiacal light distributed over the sky. The observed 5.9-11.7 mu m spectral shapes are well represented by blackbody...
Mid-IR cosmological spectrophotometric surveys from space: Measuring AGN and star formation at the cosmic noon with a SPICA-like mission
We use the SPace Infrared telescope for Cosmology and Astrophysics (SPICA) project as a template to demonstrate how deep spectrophotometric surveys covering...
Mid-IR Spectra of Type Ia SN 2014J in M82 Spanning the First 4 Months
We present a time series of 8-13 μm spectra and photometry for SN 2014J obtained 57, 81, 108, and 137 days after the explosion using CanariCam on the Gran...
MIGHTEE-H I: H I galaxy properties in the large-scale structure environment at z 0.37 from a stacking experiment
We present the first measurement of H I mass of star-forming galaxies in different large scale structure environments from a blind survey at z ~ 0.37. In...
MIGHTEE-H I: possible interactions with the galaxy NGC 895
The transformation and evolution of a galaxy is strongly influenced by interactions with its environment. Neutral hydrogen (H I) is an excellent way to trace...
MIGHTEE-HI: Evolution of HI Scaling Relations of Star-forming Galaxies at z < 0.5
We present the first measurements of H I galaxy scaling relations from a blind survey at z > 0.15. We perform spectral stacking of 9023 spectra of star-forming...