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Advanced Camera for Surveys Photometry of the Cluster RDCS 1252.9-2927: The Color-Magnitude Relation at z = 1.24
DOI: 10.1086/379234 Bibcode: 2003ApJ...596L.143B

Ford, H. C.; Demarco, R.; Infante, L. +20 more

We investigate the color-magnitude (CM) relation of galaxies in the distant X-ray-selected cluster RDCS 1252.9-2927 at z=1.24 using images obtained with the Advanced Camera for Surveys on the Hubble Space Telescope in the F775W and F850LP bandpasses. We select galaxies based on morphological classifications extending about 3.5 mag down the galaxy …

2003 The Astrophysical Journal
eHST 208
Identification of Solar Sources of Major Geomagnetic Storms between 1996 and 2000
DOI: 10.1086/344611 Bibcode: 2003ApJ...582..520Z

Zhang, J.; Bothmer, V.; Howard, R. A. +1 more

This paper presents identification of solar coronal mass ejection (CME) sources for 27 major geomagnetic storms (defined by disturbance storm timeindex<=-100 nT) occurring between 1996 and 2000. Observations of CMEs and their solar surface origins are obtained from the Large Angle and Spectrometric Coronagraph (LASCO) and the EUV Imaging Telesc…

2003 The Astrophysical Journal
SOHO 207
XMM-Newton observation of the brightest X-ray flare detected so far from Sgr A*
DOI: 10.1051/0004-6361:20030983 Bibcode: 2003A&A...407L..17P

Goldoni, P.; Grosso, N.; Decourchelle, A. +5 more

We report the high S/N observation on October 3, 2002 with XMM-Newton of the brightest X-ray flare detected so far from Sgr A* with a duration shorter than one hour ( ~ 2.7 ks). The light curve is almost symmetrical with respect to the peak flare, and no significant difference between the soft and hard X-ray range is detected. T…

2003 Astronomy and Astrophysics
XMM-Newton 201
The [C II] 158 Micron Line Deficit in Ultraluminous Infrared Galaxies Revisited
DOI: 10.1086/376965 Bibcode: 2003ApJ...594..758L

Lutz, D.; Genzel, R.; Sturm, E. +5 more

We present a study of the [C II] 157.74 µm fine-structure line in a sample of 15 ultraluminous infrared (IR) galaxies (IR luminosity LIR>=1012Lsolar ULIRGs) using the Long Wavelength Spectrometer (LWS) on the Infrared Space Observatory (ISO). We confirm the observed order of magnitude deficit (compared to …

2003 The Astrophysical Journal
ISO 200
Microlensing Optical Depth toward the Galactic Bulge from Microlensing Observations in Astrophysics Group Observations during 2000 with Difference Image Analysis
DOI: 10.1086/375212 Bibcode: 2003ApJ...591..204S

Sumi, T.; Honda, M.; Saito, Y. +27 more

We analyze the data of the gravitational microlensing survey carried out by the Microlensing Observations in Astrophysics (MOA) group during 2000 toward the Galactic bulge (GB). Our observations are designed to detect efficient high-magnification events with faint source stars and short-timescale events, by increasing the sampling rate up to ~6 ti…

2003 The Astrophysical Journal
eHST 197
The Properties of Small Magnetic Regions on the Solar Surface and the Implications for the Solar Dynamo(s)
DOI: 10.1086/345792 Bibcode: 2003ApJ...584.1107H

Title, Alan M.; Schrijver, Carolus J.; Hagenaar, Hermance J.

We find that bipolar active regions that emerge onto the Sun's surface are part of a smoothly decreasing frequency distribution that spans almost 4 orders of magnitude in flux and 8 orders of magnitude in frequency. Distributions of emergence latitude and dipole orientation narrow from nearly uniform for the smallest observed ephemeral regions (~5…

2003 The Astrophysical Journal
SOHO 196
Current sheet flapping motion and structure observed by Cluster
DOI: 10.1029/2002GL016500 Bibcode: 2003GeoRL..30.1327S

Balogh, A.; Zhang, T. L.; André, M. +8 more

Fast vertical flapping oscillations of the plasma sheet have been observed by Cluster on September 26, 2001. The flapping motion had vertical speeds exceeding 100 km/s, an amplitude in excess of 1 RE and a quasiperiod of ~3 min. The current sheet was mostly tilted in the Y-Z plane (with the tilt sometimes exceeding 45°). The waves had t…

2003 Geophysical Research Letters
Cluster 196
ISM properties in low-metallicity environments. II. The dust spectral energy distribution of NGC 1569
DOI: 10.1051/0004-6361:20030814 Bibcode: 2003A&A...407..159G

Bernard, J. -P.; Madden, S. C.; Galliano, F. +3 more

We present new 450 and 850 mu m SCUBA data of the dwarf galaxy NGC 1569. We construct the mid-infrared to millimeter SED of NGC 1569, using ISOCAM, ISOPHOT, IRAS, KAO, SCUBA and MAMBO data, and model the SED in order to explore the nature of the dust in low metallicity environments. The detailed modeling is performed in a self-consistent way, synt…

2003 Astronomy and Astrophysics
ISO 196
XMM-Newton Reveals the Quasar Outflow in PG 1115+080
DOI: 10.1086/377299 Bibcode: 2003ApJ...595...85C

Brandt, W. N.; Chartas, G.; Gallagher, S. C.

We report on an observation of the broad absorption line (BAL) quasar PG 1115+080 performed with the XMM-Newton observatory. Spectral analysis reveals the second case of a relativistic X-ray-absorbing outflow in a BAL quasar. The first case was revealed in a recent observation of APM 08279+5255 with the Chandra X-Ray Observatory. As in the case of…

2003 The Astrophysical Journal
XMM-Newton 195
A Tale of Two Stars: The Extreme O7 Iaf+ Supergiant AV 83 and the OC7.5 III((f)) star AV 69
DOI: 10.1086/374329 Bibcode: 2003ApJ...588.1039H

Hillier, D. John; Lennon, D. J.; Smith, L. J. +5 more

We present a detailed study of AV 83, an O7 Iaf+ supergiant, and AV 69 [OC7.5 III((f))] in the SMC. The stars have similar effective temperatures and luminosities but show very different wind signatures. For our study we have used the non-LTE line-blanketed atmosphere code developed by Hillier and Miller, which explicitly allows for line blanketin…

2003 The Astrophysical Journal
eHST 194