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XMM-Newton and Optical Follow-up Observations of Three New Polars from the Sloan Digital Sky Survey
DOI: 10.1086/427260 Bibcode: 2005ApJ...620..929H

Brinkmann, J.; Szkody, Paula; Schmidt, Gary D. +7 more

We report follow-up XMM-Newton and optical observations of three new polars found in the Sloan Digital Sky Survey. Simple modeling of the X-ray spectra, and consideration of the details of the X-ray and optical light curves corroborate the polar nature of these three systems and provide further insights into their accretion characteristics. During…

2005 The Astrophysical Journal
XMM-Newton 12
Energetic particle observations from the Ulysses COSPIN instruments obtained during the October-November 2003 events
DOI: 10.1029/2005JA011049 Bibcode: 2005JGRA..110.9S19M

Dalla, S.; Kunow, H.; Heber, B. +7 more

We report comprehensive observations of solar energetic particle intensities at energies from 0.3 to >100 MeV made by the suite of six Ulysses COSPIN energetic charged particle instruments on the Ulysses spacecraft during the period of intense solar activity in October/November 2003. We also discuss observations of particle anisotropies in sele…

2005 Journal of Geophysical Research (Space Physics)
Ulysses 12
INTEGRAL and XMM-Newton observations of the low-luminosity and X-ray-rich burst GRB 040223
DOI: 10.1393/ncc/i2005-10089-1 Bibcode: 2005NCimC..28..481M

McGlynn, S.; McBreen, S.; Foley, S. +6 more

GRB 040223 was observed by INTEGRAL and XMM-Newton. GRB 040223 has a peak flux of (1.6 ±0.13)×10-8 ergs cm-2 s-1, a fluence of (4.4±0.4)×10-7 ergs cm-2 and a steep photon power law index of -2.3±0.2, in the energy range 20-200 keV. The steep spectrum implies it is an X-ray-rich GRB with emissi…

2005 Nuovo Cimento C Geophysics Space Physics C
XMM-Newton 12
XMM-Newton Observations of Optically Selected Sloan Digital Sky Survey Clusters
DOI: 10.1086/429561 Bibcode: 2005ApJ...622L..17P

Georgakakis, A.; Georgantopoulos, I.; Plionis, M. +1 more

We explore the X-ray properties of a subset of the optically selected Sloan Digital Sky Survey (SDSS) cluster sample of Goto et al. by analyzing seven public XMM-Newton pointings, with exposure times ranging from ~4 to 46 ks. There are in total 17 SDSS clusters out of which only eight are detected at X-ray wavelengths with f0.5-2keV>…

2005 The Astrophysical Journal
XMM-Newton 12
Whistlers observed by the Cluster spacecraft outside the plasmasphere
DOI: 10.1029/2004JA010730 Bibcode: 2005JGRA..110.3212P

Gurnett, D. A.; Pickett, J. S.; Inan, U. S. +4 more

Lightning generated whistlers are ubiquitous within the plasmasphere at both high and low altitudes, and these waves propagate efficiently in both ducted and nonducted modes. On the other hand, in the magnetospheric region outside the plasmasphere, lightning-generated whistlers are commonly observed at low altitudes (up to ∼6000 km) but only rarel…

2005 Journal of Geophysical Research (Space Physics)
Cluster 12
Colors of Luminous Bulges in Cluster MS 1054-03 and Field Galaxies at Redshifts z~0.83
DOI: 10.1086/498707 Bibcode: 2005ApJ...634L...5K

Tran, Kim-Vy; Willmer, Christopher N. A.; Im, Myungshin +3 more

Using Hubble Space Telescope images, we separate the bulgelike (dubbed ``pbulge'') and disklike (``pdisk'') components of 71 galaxies in the rich cluster MS 1054-03 and of 21 in the field. Our key finding is that luminous pbulges are very red, with rest-frame U-B~0.45, while predicted colors are bluer by 0.20 mag. Moreover, these very red colors a…

2005 The Astrophysical Journal
eHST 12
Multiple Outbursts of a Cataclysmic Variable in the Globular Cluster M22
DOI: 10.1086/428836 Bibcode: 2005ApJ...620L.103B

Sumi, T.; MOA Collaboration; Bond, I. A. +19 more

We present a 4 yr light curve of a cataclysmic variable in M22, based on an analysis of accumulated data from the Microlensing Observations in Astrophysics (MOA) microlensing survey. The position of the star coincides with that of a transient event observed by the Hubble Space Telescope (HST) in 1999, originally attributed to microlensing but late…

2005 The Astrophysical Journal
XMM-Newton eHST 12
A serendipitous XMM-Newton observation of the intermediate polar WX Pyx
DOI: 10.1051/0004-6361:20042314 Bibcode: 2005A&A...433..635S

Schlegel, E. M.

We briefly describe a serendipitous observation of the little-studied intermediate polar WX Pyx using XMM-Newton. The X-ray spin period is 1557.3 s, confirming the optical period published in 1996. An orbital period of ~5.54 h is inferred from the separation of the spin-orbit sidelobe components. The soft and hard band spin-folded light curves are…

2005 Astronomy and Astrophysics
XMM-Newton 12
Poisson Recoding Of Solar Images For Enhanced Compression
DOI: 10.1007/s11207-005-4998-2 Bibcode: 2005SoPh..228..253N

Berghmans, David; Nicula, Bogdan; Hochedez, Jean-François

The amount of useful scientific data that a space-borne telescope produces is often limited by the available telemetry of the platform. General purpose image compression schemes are usually used to compress the image either lossy or losslessly. These schemes do not take into account the fact that pixel values of typical solar images are only known…

2005 Solar Physics
SOHO 12
Auroral kilometric radiation and magnetosphere-ionosphere coupling process during magnetic storms
DOI: 10.1029/2004JA010961 Bibcode: 2005JGRA..110.5206S

Misawa, H.; Tsuchiya, F.; Morioka, A. +8 more

This paper presents an investigation of a magnetosphere-ionosphere (M-I) coupling process during magnetic storms, using observations of auroral kilometric radiation (AKR) in the field-aligned acceleration region and plasma density variation in the plasma sheet. The main phase electron precipitation, which AKR does not accompany, was confirmed as n…

2005 Journal of Geophysical Research (Space Physics)
SOHO 11