Search Publications

The Interplanetary Responses to the Great Solar Activities in Late October 2003
DOI: 10.1007/s11207-005-6877-2 Bibcode: 2005SoPh..226..337W

Wang, Yuming; Wang, Jingxiu; Wang, S. +4 more

Based on the observations of the Sun and the interplanetary medium, a series of solar activities in late October 2003 and their consequences are studied comprehensively. Thirteen X-ray flares with importance greater than M-class, six frontside halo coronal mass ejections (CMEs) with span angle larger than 100 and three associated erupt…

2005 Solar Physics
SOHO 21
The ISO-2MASS AGN survey: on the type-1 sources
DOI: 10.1051/0004-6361:200500152 Bibcode: 2005A&A...440L...5L

Cesarsky, C.; Siebenmorgen, R.; Haas, M. +9 more

We combined the ISOCAM Parallel Mode Survey at 6.7 µm (LW2 filter) with the Two Micron All Sky Survey in order to obtain a powerful tool to search for AGN independent of dust extinction. Using moderate colour criteria H-K>0.5 and K-LW2>2.7 we have selected a sample of 77 AGN candidates in an effective area of ~10 square degrees. By mea…

2005 Astronomy and Astrophysics
ISO 21
A new model of total solar irradiance based on sunspot areas
DOI: 10.1029/2005GL022839 Bibcode: 2005GeoRL..3214109P

Walton, Stephen R.; Preminger, Dora G.

We show that daily sunspot area can be used in a simple model to reconstruct daily variations in the total solar irradiance, S. The model assumes that all fluctuations in S are correlated with the emergence of sunspots on the solar disk. Cotemporal data for S and sunspot area are analysed to extract the finite impulse response function that descri…

2005 Geophysical Research Letters
SOHO 21
The Evolution of Stellar Mass in Galaxies in the NICMOS Ultra Deep Field
DOI: 10.1086/432932 Bibcode: 2005AJ....130.1337G

Gwyn, S. D. J.; Hartwick, F. D. A.

We measure the buildup of the stellar mass of galaxies from z=6 down to z=1. Using 15 band multicolor imaging data in the NICMOS Ultra Deep Field we derive photometric redshifts and masses for 796 galaxies down to HAB=26.5 mag. The derived evolution of the global stellar mass density of galaxies is consistent with previous star formatio…

2005 The Astronomical Journal
eHST 21
Absolute spectrophotometry of northern compact planetary nebulae
DOI: 10.1051/0004-6361:20052666 Bibcode: 2005A&A...436..967W

Corradi, R. L. M.; Wright, S. A.; Perinotto, M.

We present medium-dispersion spectra and narrowband images of six northern compact planetary nebulae (PNe): BoBn 1, DdDm 1, IC 5117, M 1-5, M 1-71, and NGC 6833. From broad-slit spectra, total absolute fluxes and equivalent widths were…

2005 Astronomy and Astrophysics
eHST 21
A Chandra Observation of the Nearby Lenticular Galaxy NGC 5102: Where are the X-Ray Binaries?
DOI: 10.1086/429982 Bibcode: 2005ApJ...625..785K

Ponman, T. J.; Jones, C.; Kraft, R. P. +2 more

We present results from a 34 ks Chandra ACIS-S observation of the low-mass X-ray binary (LMXB) population and the hot interstellar medium (ISM) in the nearby (d=3.1 Mpc) lenticular galaxy NGC 5102, previously shown to have an unusually low X-ray luminosity. We detect 11 X-ray point sources within the D25 optical boundary of the galaxy (…

2005 The Astrophysical Journal
eHST 21
Deep Photometry of the Globular Cluster M5: Distance Estimates from White Dwarf and Main-Sequence Stars
DOI: 10.1086/444407 Bibcode: 2005ApJ...632..266L

Sarajedini, Ata; Layden, Andrew C.; Cool, Adrienne M. +1 more

We present deep VI photometry of stars in the globular cluster M5 (NGC 5904) based on images taken with the Hubble Space Telescope. The resulting color-magnitude diagram reaches below V~27 mag, revealing the upper 2-3 mag of the white dwarf cooling sequence and main-sequence stars 8 mag and more below the turnoff. We fit the main sequence to subdw…

2005 The Astrophysical Journal
eHST 21
A Study of Flare-associated X-Ray Plasma Ejections. III. Kinematic Properties
DOI: 10.1086/497625 Bibcode: 2005ApJ...635.1291K

Cho, K. -S.; Moon, Y. -J.; Park, Y. D. +2 more

In this study, we have investigated the kinematic properties of flare-associated X-ray plasma ejections. First, we obtained the speed profiles of well-observed several events and compared them with the GOES soft X-ray flux profiles as well as the HXT hard X-ray flux profiles of their associated flares. Second, we have estimated the Alfvén speed at…

2005 The Astrophysical Journal
SOHO 21
Early signatures of large-scale field line opening. Multi-wavelength analysis of features connected with a "halo" CME event
DOI: 10.1051/0004-6361:20041378 Bibcode: 2005A&A...434..329P

Vilmer, N.; Pohjolainen, S.; Khan, J. I. +1 more

A fast "halo"-type coronal mass ejection (CME) associated with a two-ribbon flare, GOES class M 1.3, was observed on February 8, 2000. Soft X-ray and EUV images revealed several loop ejections and one wave-like moving front that started from a remote location, away from the flare core region. A radio type-II burst was observed near the trajectory …

2005 Astronomy and Astrophysics
SOHO 21
Toward magnetic field dissipation during the 23 July 2002 solar flare measured with Solar and Heliospheric Observatory/Michelson Doppler Imager (SOHO/MDI) and Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI)
DOI: 10.1029/2004JA010934 Bibcode: 2005JGRA..110.8104Z

Zharkova, Valentina V.; Zharkov, Sergey I.; Ipson, Stanley S. +1 more

We analyze the SOHO/MDI high-cadence magnetic field variations that occurred in a bipolar area around the apparent neutral line (ANL) prior to and during the 2B/X4.8 flare on 23 July 2002 and their association with the hard X-ray (HXR) and Hα emission observed with RHESSI and BBSO. Magnetic field changes started 6 min prior to the hard …

2005 Journal of Geophysical Research (Space Physics)
SOHO 21