Search Publications

The Nearby Neutron Star RX J0720.4-3125 from Radio to X-Rays
DOI: 10.1086/375052 Bibcode: 2003ApJ...590.1008K

Frail, D. A.; Kulkarni, S. R.; van Kerkwijk, M. H. +3 more

We present radio, optical, ultraviolet, and X-ray observations of the isolated, thermally emitting neutron star RX J0720.4-3125 using the Parkes radio telescope, the Very Large Array, the Hubble Space Telescope, and the Chandra X-Ray Observatory. From these data we show that the optical/UV spectrum of RX J0720.4-3125 is not well fitted by a Raylei…

2003 The Astrophysical Journal
eHST 64
Buried Alive in the Coronal Graveyard
DOI: 10.1086/378699 Bibcode: 2003ApJ...598..610A

Ayres, Thomas R.; Harper, Graham M.; Brown, Alexander

We have used the High Resolution Camera (HRC-I) of the Chandra X-Ray Observatory to search for coronal (T~106 K) emission from the archetype ``noncoronal'' red giants Arcturus (α Bootis=HD 124897, K1 III) and Aldebaran (α Tauri=HD 29139, K5 III). Our program follows up previous detections of ultraviolet coronal proxies such as C IV λ154…

2003 The Astrophysical Journal
eHST 64
Cloning Dropouts: Implications for Galaxy Evolution at High Redshift
DOI: 10.1086/376588 Bibcode: 2003ApJ...593..640B

Broadhurst, Tom; Bouwens, Rychard; Illingworth, Garth

The evolution of high-redshift galaxies in the two Hubble Deep Fields, HDF-N and HDF-S, is investigated using a cloning technique that replicates z~2-3 U dropouts to higher redshifts, allowing a comparison with the observed B and V dropouts at higher redshifts (z~4-5). We treat each galaxy selected for replication as a set of pixels that are k-cor…

2003 The Astrophysical Journal
eHST 64
The Evolution of the Galaxy Luminosity Function in the Rest-Frame Blue Band up to z=3.5
DOI: 10.1086/378081 Bibcode: 2003ApJ...593L...1P

Cimatti, A.; Daddi, E.; Fontana, A. +14 more

We present an estimate of the cosmological evolution of the field galaxy luminosity function (LF) in the rest-frame 4400 Å B band up to redshift z=3.5. To this purpose, we use a composite sample of 1541 I-selected galaxies selected down to IAB=27.2 and 138 galaxies selected down to KAB=25 from ground-based and HST multicolor …

2003 The Astrophysical Journal
eHST 63
Space Velocities of Southern Globular Clusters. IV. First Results for Inner Galaxy Clusters
DOI: 10.1086/367801 Bibcode: 2003AJ....125.1373D

Girard, Terrence M.; van Altena, William F.; López, Carlos E. +1 more

We have measured the absolute proper motions of four low-latitude, inner Galaxy globular clusters. These clusters are NGC 6266 (M62), NGC 6304, NGC 6316, and NGC 6723. The proper motions are on the Hipparcos system, since no background extragalactic objects are found in these high-extinction regions. The proper-motion uncertainties range between 0…

2003 The Astronomical Journal
Hipparcos 63
Distances to nearby galaxies around IC 342
DOI: 10.1051/0004-6361:20030912 Bibcode: 2003A&A...408..111K

Dolphin, A. E.; Grebel, E. K.; Sharina, M. E. +1 more

We present an analysis of Hubble Space Telescope/WFPC2 images of six nearby galaxies in the projected vicinity of IC 342: Cas dSph, KK 35, UGCA 86, Cam A, NGC 1560, and Cam B. We derive distances to five of them from the luminosity of the tip of the red giant branch stars with a typical accuracy of ~ 10%. The galaxy distances are 0.79 Mpc (Cas dSp…

2003 Astronomy and Astrophysics
eHST 63
Monte Carlo simulations and generation of the SPI response
DOI: 10.1051/0004-6361:20031171 Bibcode: 2003A&A...411L..81S

von Kienlin, A.; Shrader, C. R.; Schanne, S. +13 more

In this paper we discuss the methods developed for the production of the INTEGRAL/SPI instrument response. The response files were produced using a suite of Monte Carlo simulation software developed at NASA/GSFC based on the GEANT-3 package available from CERN. The production of the INTEGRAL/SPI instrument response also required the development of…

2003 Astronomy and Astrophysics
INTEGRAL 63
How are Emerging Flux, Flares and CMEs Related to Magnetic Polarity Imbalance in Midi Data?
DOI: 10.1023/A:1025678917086 Bibcode: 2003SoPh..215..307G

Mandrini, C. H.; Démoulin, P.; Green, L. M. +1 more

In order to understand whether major flares or coronal mass ejections (CMEs) can be related to changes in the longitudinal photospheric magnetic field, we study 4 young active regions during seven days of their disk passage. This time period precludes any biases which may be introduced in studies that look at the field evolution during the short-t…

2003 Solar Physics
SOHO 63
Ulysses COSPIN observations of cosmic rays and solar energetic particles from the South Pole to the North Pole of the Sun during solar maximum
DOI: 10.5194/angeo-21-1217-2003 Bibcode: 2003AnGeo..21.1217M

Balogh, A.; Kunow, H.; Posner, A. +10 more

In 2000-2001 Ulysses passed from the south to the north polar regions of the Sun in the inner heliosphere, providing a snapshot of the latitudinal structure of cosmic ray modulation and solar energetic particle populations during a period near solar maximum. Observations from the COSPIN suite of energetic charged particle telescopes show that lati…

2003 Annales Geophysicae
SOHO Ulysses 63
Observations with the Visual and Infrared Mapping Spectrometer (VIMS) during Cassini's flyby of Jupiter
DOI: 10.1016/S0019-1035(03)00134-9 Bibcode: 2003Icar..164..461B

Sotin, C.; Brown, R. H.; Baines, K. H. +24 more

The Cassini Visual and Infrared Mapping Spectrometer (VIMS) is an imaging spectrometer covering the wavelength range 0.3-5.2 µm in 352 spectral channels, with a nominal instantaneous field of view of 0.5 mrad. The Cassini flyby of Jupiter represented a unique opportunity to accomplish two important goals: scientific observations of the jovia…

2003 Icarus
Cassini 63