Astronomical image and data analysis
With information and scale as central themes, this comprehensive survey explains how to
handle real problems in astronomical data analysis using a modern arsenal of powerful …
handle real problems in astronomical data analysis using a modern arsenal of powerful …
ISO spectroscopy of gas and dust: from molecular clouds to protoplanetary disks
EF van Dishoeck - Annu. Rev. Astron. Astrophys., 2004 - annualreviews.org
▪ Abstract Observations of interstellar gas-phase and solid-state species in the 2.4–200 μm
range obtained with the spectrometers on board the Infrared Space Observatory (ISO) are …
range obtained with the spectrometers on board the Infrared Space Observatory (ISO) are …
SINGS: the SIRTF nearby galaxies survey
ABSTRACT The SIRTF Nearby Galaxy Survey is a comprehensive infrared imaging and
spectroscopic survey of 75 nearby galaxies. Its primary goal is to characterize the infrared …
spectroscopic survey of 75 nearby galaxies. Its primary goal is to characterize the infrared …
The Infrared Camera (IRC) for AKARI–Design and imaging performance
T Onaka, H Matsuhara, T Wada… - Publications of the …, 2007 - academic.oup.com
Abstract The Infrared Camera (IRC) is one of two focal-plane instruments on the AKARI
satellite. It is designed for wide-field deep imaging and low-resolution spectroscopy in the …
satellite. It is designed for wide-field deep imaging and low-resolution spectroscopy in the …
The CH out-of-plane bending modes of PAH molecules in astrophysical environments
We present 10-15 μm spectra of a sample of H ii regions, YSOs and evolved stars that show
strong unidentified infrared emission features, obtained with the ISO/SWS spectrograph on …
strong unidentified infrared emission features, obtained with the ISO/SWS spectrograph on …
A hyperluminous galaxy at z = 2.8 found in a deep submillimetre survey
We present a detailed study of SMM 02399-0136, a hyperluminous, active galaxy selected
from a submm survey of the distant Universe. This galaxy is the brightest source in the fields …
from a submm survey of the distant Universe. This galaxy is the brightest source in the fields …
Variations of the mid-IR aromatic features inside and among galaxies
We present the results of a systematic study of mid-IR spectra of Galactic regions,
Magellanic H ii regions, and galaxies of various types (dwarf, spiral, starburst), observed by …
Magellanic H ii regions, and galaxies of various types (dwarf, spiral, starburst), observed by …
Mid-infrared diagnostics to distinguish AGNs from starbursts
We present new mid-infrared (MIR) diagnostics to distinguish emission of active galactic
nuclei (AGN) from that originating in starburst regions. Our method uses empirical …
nuclei (AGN) from that originating in starburst regions. Our method uses empirical …
ISM properties in low-metallicity environments-I. Mid-infrared spectra of dwarf galaxies
We present new ISOCAM mid-infrared spectra of three starbursting nearby dwarf galaxies,
NGC1569, NGC1140 and IIZw40 and the 30Dor region of the LMC and explore the …
NGC1569, NGC1140 and IIZw40 and the 30Dor region of the LMC and explore the …
The bulk of the cosmic infrared background resolved by ISOCAM
Deep extragalactic surveys with ISOCAM revealed the presence of a large density of faint
mid-infrared (MIR) sources. We have computed the 15 μm integrated galaxy light produced …
mid-infrared (MIR) sources. We have computed the 15 μm integrated galaxy light produced …