Search Publications

PDRs4All: A JWST Early Release Science Program on Radiative Feedback from Massive Stars
DOI: 10.1088/1538-3873/ac604c Bibcode: 2022PASP..134e4301B

Hartigan, Patrick; Zhang, Yong; Gordon, Karl D. +134 more

Massive stars disrupt their natal molecular cloud material through radiative and mechanical feedback processes. These processes have profound effects on the evolution of interstellar matter in our Galaxy and throughout the universe, from the era of vigorous star formation at redshifts of 1-3 to the present day. The dominant feedback processes can …

2022 Publications of the Astronomical Society of the Pacific
ISO 59
Consistent Dust and Gas Models for Protoplanetary Disks. III. Models for Selected Objects from the FP7 DIANA Project
DOI: 10.1088/1538-3873/aaf4e5 Bibcode: 2019PASP..131f4301W

Waters, L. B. F. M.; Pinte, C.; Woitke, P. +17 more

The European FP7 project DIANA has performed a coherent analysis of a large set of observational data of protoplanetary disks by means of thermo-chemical disk models. The collected data include extinction-corrected stellar UV and X-ray input spectra (as seen by the disk), photometric fluxes, low and high resolution spectra, interferometric data, e…

2019 Publications of the Astronomical Society of the Pacific
ISO IUE eHST 72
Data Reduction and Early Science Calibration for FORCAST, A Mid-Infrared Camera for SOFIA
DOI: 10.1086/674144 Bibcode: 2013PASP..125.1393H

Schoenwald, J.; Wang, J.; Vacca, W. D. +7 more

FORCAST is a mid-infrared (5-40 µm) facility instrument for the Stratospheric Observatory for Infrared Astronomy (SOFIA). After achieving first light flight in 2010 May, FORCAST has completed two observatory characterization flights and thirteen science flights on SOFIA. In this paper we describe the photometric calibration of FORCAST which …

2013 Publications of the Astronomical Society of the Pacific
ISO 51
Multiwavelength Analyses of Faint Infrared Galaxies
DOI: 10.1086/504116 Bibcode: 2006PASP..118..754B

Berta, Stefano

The present work follows a chronological outline covering the development of infrared space facilities in recent decades. The Infrared Astronomical Satellite (launched in 1984), Infrared Space Observatory (1995), and Spitzer Space Telescope (2003 August) constitute a logical sequence in the study of galactic infrared properties, with a well-modula…

2006 Publications of the Astronomical Society of the Pacific
ISO 3
Infrared Space Observatory Observations of the 53W002 Group at 6.7 Microns: In Search of the Oldest Stellar Populations at z = 2.4
DOI: 10.1086/423432 Bibcode: 2004PASP..116..712K

Keel, William C.; Windhorst, Rogier A.; Eales, Stephen A. +5 more

We present a deep Infrared Space Observatory (ISO) observation at 6.7 µm of the 53W002 group of galaxies and active galactic nuclei (AGNs) at z=2.4. This approximately samples the emitted K band. Faint, blue star-forming objects are not detected, as expected from their very blue color across the emitted optical and UV spectrum. However, 53W0…

2004 Publications of the Astronomical Society of the Pacific
ISO eHST 0
SINGS: The SIRTF Nearby Galaxies Survey
DOI: 10.1086/376941 Bibcode: 2003PASP..115..928K

Kewley, Lisa J.; Gordon, Karl D.; Calzetti, Daniela +20 more

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 emission of galaxies and their principal infrared-emitting components, across a broad range of galaxy properties and star formation environments. SINGS will provide new insights into th…

2003 Publications of the Astronomical Society of the Pacific
ISO IUE 1183
The Nuclear Spectral Energy Distribution of NGC 4395, the Least Luminous Type 1 Seyfert Galaxy
DOI: 10.1086/316394 Bibcode: 1999PASP..111..801M

Moran, Edward C.; Filippenko, Alexei V.; Ho, Luis C. +5 more

We present X-ray (ROSAT), infrared, and radio observations of NGC 4395, which harbors the optically least luminous type 1 Seyfert nucleus discovered thus far. In combination with published optical and ultraviolet spectra, we have used these data to assemble the broadband spectral energy distribution (SED) of the galaxy's nucleus. Interestingly, th…

1999 Publications of the Astronomical Society of the Pacific
ISO 64
Automatic Noise Estimation from the Multiresolution Support
DOI: 10.1086/316124 Bibcode: 1998PASP..110..193S

Starck, Jean-Luc; Murtagh, Fionn

We describe an automated approach for determining the noise associated with astronomical images. Detector noise is ever present and must be determined for high-quality image filtering or compression. We also show that the method can be used for very high quality cosmic-ray hit removal. Our method is based on a multiresolution transform of the imag…

1998 Publications of the Astronomical Society of the Pacific
ISO 54
Asteroids as Far-Infrared Photometric Standards
DOI: 10.1086/316213 Bibcode: 1998PASP..110.1001M

Müller, Thomas G.

1998 Publications of the Astronomical Society of the Pacific
ISO 0