Search Publications

MOIRCS Deep Survey. I: DRG Number Counts
DOI: 10.1093/pasj/58.6.951 Bibcode: 2006PASJ...58..951K

Ouchi, Masami; Tanaka, Ichi; Yamada, Toru +11 more

We use very deep near-infrared imaging data taken with Multi-Object InfraRed Camera and Spectrograph (MOIRCS) on the Subaru Telescope to investigate the number counts of Distant Red Galaxies (DRGs). We have observed a 4x7 arcmin^2 field in the Great Observatories Origins Deep Survey North (GOODS-N), and our data reach J=24.6 and K=23.2 (5sigma, Ve…

2006 Publications of the Astronomical Society of Japan
eHST 44
Hubble Space Telescope STIS Spectroscopy and Modeling of the Long-Term Cooling of WZ Sagittae following the 2001 July Outburst
DOI: 10.1086/501039 Bibcode: 2006ApJ...642.1018G

Szkody, Paula; Sion, Edward M.; Godon, Patrick +3 more

We present the latest Hubble Space Telescope Space Telescope Imaging Spectrograph (HST STIS) E140M far-ultraviolet (FUV) spectrum of the dwarf nova WZ Sge, obtained in 2004 July, 3 yr following the early superoutburst of 2001 July. With a temperature T~15,000 K, the white dwarf (WD) is still ~1500 K above its quiescent temperature, it has a FUV fl…

2006 The Astrophysical Journal
IUE eHST 44
Microlensing of the Lensed Quasar SDSS 0924+0219
DOI: 10.1086/505569 Bibcode: 2006ApJ...647..874M

Kochanek, C. S.; Morgan, Nicholas D.; Morgan, Christopher W. +1 more

We analyze V-, I-, and H-band HST images and two seasons of R-band monitoring data for the gravitationally lensed quasar SDSS 0924+0219. We clearly see that image D is a point-source image of the quasar at the center of its host galaxy. We can easily track the host galaxy of the quasar close to image D because microlensing has provided a natural c…

2006 The Astrophysical Journal
eHST 44
Astrophysical constraints from gamma-ray spectroscopy
DOI: 10.1016/j.nuclphysa.2005.02.155 Bibcode: 2006NuPhA.777...70D

Diehl, Roland; von Ballmoos, Peter; Prantzos, Nikos

Gamma-ray lines from cosmic sources provide unique isotopic information, since they originate from energy level transitions in the atomic nucleus. Gamma-ray telescopes explored this astronomical window in the past three decades, detecting radioactive isotopes that have been ejected in interstellar space by cosmic nucleosynthesis events and nuclei …

2006 Nuclear Physics A
INTEGRAL 43
Spectral Modeling of SNe Ia Near Maximum Light: Probing the Characteristics of Hydrodynamical Models
DOI: 10.1086/504101 Bibcode: 2006ApJ...645..480B

Baron, E.; Branch, David; Hauschildt, Peter H. +1 more

We have performed detailed non-local thermodynamic equilibrium (NLTE) spectral synthesis modeling of two types of one-dimensional hydrodynamical models: the very highly parameterized deflagration model W7, and two delayed-detonation models. We find that, overall, both models do about equally well at fitting well-observed SNe Ia near maximum light.…

2006 The Astrophysical Journal
eHST 43
Physical Conditions in Orion's Veil. II. A Multicomponent Study of the Line of Sight toward the Trapezium
DOI: 10.1086/500819 Bibcode: 2006ApJ...644..344A

Abel, N. P.; O'Dell, C. R.; Ferland, G. J. +2 more

Orion's Veil is an absorbing screen that lies along the line of sight to the Orion H II region. It consists of two or more layers of gas that must lie within a few parsecs of the Trapezium cluster. Our previous work considered the Veil as a whole and found that the magnetic field dominates the energetics of the gas in at least one component. Here …

2006 The Astrophysical Journal
eHST 43
In situ dust measurements in the inner Saturnian system
DOI: 10.1016/j.pss.2006.05.021 Bibcode: 2006P&SS...54..967S

Grande, M.; Beckmann, U.; Kempf, S. +38 more

In July 2004 the Cassini-Huygens mission reached the Saturnian system and started its orbital tour. A total of 75 orbits will be carried out during the primary mission until August 2008. In these four years Cassini crosses the ring plane 150 times and spends approx. 400 h within Titan's orbit. The Cosmic Dust Analyser (CDA) onboard Cassini charact…

2006 Planetary and Space Science
Cassini 43
Clustering of i775 Dropout Galaxies at z ~ 6 in GOODS and the UDF
DOI: 10.1086/507678 Bibcode: 2006ApJ...648L...5O

Franx, Marijn; Illingworth, Garth D.; Bouwens, Rychard J. +1 more

We measured the angular clustering at z~6 from a large sample of i775 dropout galaxies (293 with z850<=27.5 from GOODS and 95 with z850<=29.0 from the UDF). Our largest and most complete subsample (having L>~0.5L*z=6) shows the presence of clustering at 94% significance. For this samp…

2006 The Astrophysical Journal
eHST 43
Dependence of flux transfer events on solar wind conditions from 3 years of Cluster observations
DOI: 10.1029/2005JA011342 Bibcode: 2006JGRA..111.4224W

Russell, C. T.; Lavraud, B.; Raeder, J. +6 more

We investigate the dependence of Cluster high-latitude magnetopause and low-latitude flank flux transfer events (FTEs) on solar wind conditions using measurements from Cluster FGM and CIS and ACE MFI and SWEPAM between February 2001 and June 2003. We find that there are strong dependences of Cluster FTE occurrence on the IMF Bxgsm, B

2006 Journal of Geophysical Research (Space Physics)
Cluster 43
The Connection between Bar Strength and Circumnuclear Dust Structure
DOI: 10.1086/508153 Bibcode: 2006ApJ...652.1097P

Martini, Paul; Peeples, Molly S.

We present a comparison of bar strength Qb and circumnuclear dust morphology for 75 galaxies in order to investigate how bars affect the centers of galaxies. We trace the circumnuclear dust morphology and amount of dust structure with structure maps generated from visible-wavelength HST data, finding that tightly wound nuclear dust spir…

2006 The Astrophysical Journal
eHST 43