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A Snapshot Survey for Gravitational Lenses among z>=4.0 Quasars. I. The z>5.7 Sample
DOI: 10.1086/381906 Bibcode: 2004AJ....127.1305R

Strauss, Michael A.; Brinkmann, J.; Fan, Xiaohui +7 more

Over the last few years, the Sloan Digital Sky Survey (SDSS) has discovered several hundred quasars with redshift between 4.0 and 6.4. Including the effects of magnification bias, one expects a priori that an appreciable fraction of these objects are gravitationally lensed. We have used the Advanced Camera for Surveys on the Hubble Space Telescope…

2004 The Astronomical Journal
eHST 58
Long-term variability in the X-ray emission of RX J0720.4-3125
DOI: 10.1051/0004-6361:20040009 Bibcode: 2004A&A...415L..31D

de Vries, C. P.; Vink, J.; Verbunt, F. +1 more

We detect a gradual, long-term change in the shape of the X-ray spectrum of the isolated neutron star RX J0720.4-3125, such that the spectrum of the source can no longer be described as a blackbody spectrum. The change is accompanied by an energy-dependent change in the pulse profile. If the X-ray emission is influenced by the magnetic field of th…

2004 Astronomy and Astrophysics
XMM-Newton 58
Evidence of Magnetic Reconnection along Coronal Hole Boundaries
DOI: 10.1086/383030 Bibcode: 2004ApJ...603L..57M

Doyle, J. G.; Madjarska, M. S.; van Driel-Gesztelyi, L.

The present study reveals for the first time the existence of bidirectional jets, which are a signature of magnetic reconnection, occurring along coronal hole boundaries. The Solar Ultraviolet Measurement of Emitted Radiation spectrometer observations obtained in the N IV 765.15 Å (1.3×105 K) and Ne VIII 770.42 Å (6×105 K) em…

2004 The Astrophysical Journal
SOHO 58
Properties of the background of EPIC-pn onboard XMM-Newton
DOI: 10.1051/0004-6361:20031687 Bibcode: 2004A&A...414..767K

Freyberg, M. J.; Matsushita, K.; Takahashi, I. +2 more

We have investigated the background properties of EPIC-pn onboard XMM-Newton to establish the background subtraction method. Count rates of the background vary violently by two orders of magnitude at the maximum, while during the most quiet period, these are stable within 8% at a 1σ level. The overall spectrum is dominated by particle events above…

2004 Astronomy and Astrophysics
XMM-Newton 58
The dust environment of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361:20035806 Bibcode: 2004A&A...422..357F

Rauer, H.; Fulle, M.; Barbieri, C. +4 more

The new target of the ESA Rosetta Mission is comet 67P/Churyumov-Gerasimenko, which passed its last perihelion on 18 August 2002 and was well observed from fall 2002 to spring 2003. Its most prominent feature was a thin dust tail, which is best fitted by the Neck-Line model. Fits of the whole tail provide the dust environment of 67P during a year …

2004 Astronomy and Astrophysics
Rosetta 58
Chandra Observations of the Three Most Metal Deficient Blue Compact Dwarf Galaxies Known in the Local Universe, SBS 0335-052, SBS 0335-052W, and I Zw 18
DOI: 10.1086/382949 Bibcode: 2004ApJ...606..213T

Bauer, Franz E.; Thuan, Trinh X.; Izotov, Yuri I. +1 more

We present an X-ray study of the three most metal deficient blue compact dwarf (BCD) galaxies known in the local universe, based on deep Chandra observations of SBS 0335-052 (0.025 Zsolar), SBS 0335-052W (0.02 Zsolar), and I Zw 18 (0.02 Zsolar). All three are detected, with more than 90% of their X-ray emission ari…

2004 The Astrophysical Journal
eHST 58
On the light echo in V838 Mon
DOI: 10.1051/0004-6361:20034015 Bibcode: 2004A&A...414..223T

Tylenda, R.

We present a theoretical outline of the light echo phenomenon and results of simple numerical simulations and we study the available images of the light echo in V838 Mon obtained with HST. An investigation of the observed expansion of the light echo leads us to conclude that the distance to V838 Mon is ⪆5 kpc. From an analysis of the inner bright …

2004 Astronomy and Astrophysics
eHST 57
The Iron Unresolved Transition Array in Active Galactic Nuclei
DOI: 10.1086/382038 Bibcode: 2004ApJ...604..551N

Netzer, Hagai

The unresolved transition array (UTA) of iron M-shell ions is a prominent absorption feature in the X-ray spectrum of many active galactic nuclei (AGNs). Modeling photoionized plasmas in an attempt to match the observed silicon and oxygen lines fails to predict the level of ionization of iron as inferred by this feature. It is suggested that the d…

2004 The Astrophysical Journal
XMM-Newton 57
Jupiter's Atmospheric Composition from the Cassini Thermal Infrared Spectroscopy Experiment
DOI: 10.1126/science.1100240 Bibcode: 2004Sci...305.1582K

Smith, M. D.; Strobel, D. F.; Lellouch, E. +39 more

The Composite Infrared Spectrometer observed Jupiter in the thermal infrared during the swing-by of the Cassini spacecraft. Results include the detection of two new stratospheric species, the methyl radical and diacetylene, gaseous species present in the north and south auroral infrared hot spots; determination of the variations with latitude of a…

2004 Science
Cassini 57
Hubble Space Telescope Observations of the Main Sequence of M4
DOI: 10.1086/383543 Bibcode: 2004AJ....127.2771R

Stetson, P. B.; Rich, R. M.; Shara, M. +8 more

We present new results from a photometric study of the main-sequence stars in M4 (NGC 6121=C1620-264), the closest globular cluster to the Sun. Multifield, multiepoch observations at approximately 1, 2, and 6 core radii were obtained with WFPC2 on the Hubble Space Telescope through either the F606W filter or the F555W (V) and F814W (I) filters. Th…

2004 The Astronomical Journal
eHST 57