Search Publications

Deuterium Abundance toward WD 0621-376: Results from the FUSE Mission
DOI: 10.1086/339129 Bibcode: 2002ApJS..140...81L

Sembach, K. R.; Moos, H. W.; Chayer, P. +5 more

Far Ultraviolet Spectroscopic Explorer observations are presented for WD 0621-376, a DA white dwarf star in the local interstellar medium (LISM) at a distance of about 78 pc. The data have a signal-to-noise ratio of ~20-40 per 20 km s-1 resolution element and cover the wavelength range 905-1187 Å. LISM absorption is detected in the line…

2002 The Astrophysical Journal Supplement Series
IUE 33
Space Telescope Imaging Spectrograph Observations of High-Velocity Interstellar Absorption-Line Profiles in the Carina Nebula
DOI: 10.1086/339373 Bibcode: 2002ApJS..140..407W

Walborn, Nolan R.; Danks, Anthony C.; Landsman, Wayne B. +1 more

An atlas of ultraviolet interstellar absorption-line profiles toward four stars in the Carina Nebula is presented. The observations have been made with the Space Telescope Imaging Spectrograph on the Hubble Space Telescope, with a resolving power of 114,000. Low-ionization, high-ionization, and excited-state lines from a wide array of chemical spe…

2002 The Astrophysical Journal Supplement Series
eHST 29
X-Ray Light Curves of Gamma-Ray Bursts Detected with the All-Sky Monitor on RXTE
DOI: 10.1086/340328 Bibcode: 2002ApJS..141..415S

Hurley, K.; Smith, D. A.; Levine, A. +6 more

We present X-ray light curves (1.5-12 keV) for 15 gamma-ray bursts (GRBs) detected by the All-Sky Monitor (ASM) on the Rossi X-Ray Timing Explorer. We compare these soft X-ray light curves with count rate histories obtained by the high-energy (>12 keV) experiments BATSE, Konus-Wind, the BeppoSAX Gamma-Ray Burst Monitor, and the burst monitor on…

2002 The Astrophysical Journal Supplement Series
Ulysses 15
Speckle Observations of Composite Spectrum Stars with PISCO in 1993-1998
DOI: 10.1086/341094 Bibcode: 2002ApJS..142...95P

Festou, M. C.; Arnold, L.; Scardia, M. +8 more

We present speckle interferometry observations of 47 composite spectrum stars obtained between 1993 and 1998 at the Pic du Midi Observatory with the PISCO speckle camera. 76% of over 150 independent 10 minute sequences of observations led to a companion detection. Binary component angular separations ranged from 0.05" to 1.2". We also obtained a s…

2002 The Astrophysical Journal Supplement Series
Hipparcos 11
A New Database of Observed Spectral Energy Distributions of Nearby Starburst Galaxies from the Ultraviolet to the Far-Infrared
DOI: 10.1086/342834 Bibcode: 2002ApJS..143..377W

Gordon, Karl D.; Calzetti, Daniela; Clayton, Geoffrey C. +3 more

We present a database of UV-to-FIR data of 83 nearby starburst galaxies. The galaxies are selected based upon the availability of IUE data. We have recalibrated the IUE UV spectra for these galaxies by incorporating the most recent improvements. For 45 of these galaxies we use observations by Storchi-Bergmann et al. and McQuade et al. for the spec…

2002 The Astrophysical Journal Supplement Series
IUE eHST 8
An Empirical Ultraviolet Template for Iron Emission in Quasars as Derived from I Zwicky 1
DOI: 10.1086/320357 Bibcode: 2001ApJS..134....1V

Vestergaard, M.; Wilkes, B. J.

We present an empirical template spectrum suitable for fitting and subtracting/studying the Fe II and Fe III emission lines in the rest frame ultraviolet spectra of quasars and active galactic nuclei, the first empirical ultraviolet iron template to cover the full range of 1250-3090 Å. Iron emission is often a severe contaminant in optical-ultravi…

2001 The Astrophysical Journal Supplement Series
eHST 502
The Distribution of Thermal Pressures in the Interstellar Medium from a Survey of C I Fine-Structure Excitation
DOI: 10.1086/323326 Bibcode: 2001ApJS..137..297J

Tripp, Todd M.; Jenkins, Edward B.

We used the Space Telescope Imaging Spectrograph (STIS) with its smallest entrance aperture (0.03" wide slit) and highest resolution echelle gratings (E140H and E230H) to record the interstellar absorption features for 10 different multiplets of neutral carbon at a resolving power of λ/Δλ=200,000 in the UV spectra of 21 early-type stars. Our objec…

2001 The Astrophysical Journal Supplement Series
IUE eHST 206
CHIANTI-An Atomic Database for Emission Lines. IV. Extension to X-Ray Wavelengths
DOI: 10.1086/320854 Bibcode: 2001ApJS..134..331D

Young, P. R.; Del Zanna, G.; Dere, K. P. +1 more

CHIANTI provides a database of atomic energy levels, wavelengths, radiative transition probabilities, and electron excitation data for a large number of ions of astrophysical interest. It also includes a suite of Interactive Data Language programs to calculate optically thin synthetic spectra and to perform spectral analysis and plasma diagnostics…

2001 The Astrophysical Journal Supplement Series
SOHO 180
NICMOS Observations of High-Redshift Radio Galaxies: Witnessing the Formation of Bright Elliptical Galaxies?
DOI: 10.1086/321781 Bibcode: 2001ApJS..135...63P

Pentericci, L.; Fosbury, R.; Röttgering, H. J. A. +3 more

We present the results of a near-infrared imaging program of a sample of 19 radio galaxies with redshift between 1.7 and 3.2, using the NICMOS Camera 2 on the Hubble Space Telescope (HST). The galaxies were observed in H band, which, for 18 of the 19 targets, samples the rest-frame optical emission longward of the 4000 Å break. For many sources th…

2001 The Astrophysical Journal Supplement Series
eHST 108
The MACHO Project: Microlensing Detection Efficiency
DOI: 10.1086/322529 Bibcode: 2001ApJS..136..439A

Alcock, C.; Allsman, R. A.; Alves, D. R. +21 more

The MACHO project is a search for dark matter in the form of massive compact halo objects (MACHOs). The project has photometrically monitored over forty million stars in the Large Magellanic Cloud (LMC), Small Magellanic Cloud (SMC), and Galactic bulge in search of rare gravitational microlensing events caused by these otherwise invisible objects.…

2001 The Astrophysical Journal Supplement Series
eHST 71