V1647 ORIONIS: Keck/Nirspec 2 MICRON Echelle ObservationsWe present new Keck II NIRSPEC high-spectral resolution 2 um echelle observations of the young eruptive variable star V1647 Orionis. This star went into outburst in late 2003 and faded to its…Colin Aspin, Tom P. Greene, Bo Reipurth·Oct 21, 2008SaveLearn
NEAR-IR Spectroscopy of Young Stars in the Braid Nebula Star Formation Region in Cygnus Ob7We present 1.4 to 2.5 um integral field spectroscopy of 16 stars in the Braid Nebula star formation region in Cygnus OB7. These data forms one aspect of a large-scale multi-wavelength survey aimed at…Colin Aspin, Tracy L. Beck, Tae-Soo Pyo et al.·Oct 21, 2008SaveLearn
Direct Distance Measurement to the Dusty White Dwarf GD 362We present trigonometric parallax observations of GD 362 obtained over seven epochs using the MDM 2.4m Hiltner Telescope. The existence of a dust disk around this possibly massive white dwarf makes…Mukremin Kilic, John R. Thorstensen, Detlev Koester·Oct 21, 2008SaveLearn
Enhanced lensing rate by clustering of massive galaxies: newly discovered systems in the SLACS fields[Abridged] We exploit the clustering of massive galaxies to perform a high efficiency imaging search for gravitational lenses. Our dataset comprises 44 fields imaged by the Hubble Space Telescope…Elisabeth R. Newton, Philip J. Marshall, Tommaso Treu·Oct 21, 2008SaveLearn
Measuring Distance Ratios with CMB-Galaxy Lensing Cross-correlationsWe propose a method for cosmographic measurements by combining gravitational lensing of the cosmic microwave background (CMB) with cosmic shear surveys. We cross-correlate the galaxy counts in the…Sudeep Das, David N. Spergel·Oct 21, 2008SaveLearn
Is there a standard measuring rod in the Universe?The Caltech-Jodrell Bank very long baseline interferometry (VLBI) Surveys give detailed 5 GHz VLBI images of several hundred milliarcsecond (mas) radio sources, and the full width at half-maximum…J. C. Jackson·Oct 21, 2008SaveLearn
Highlights of multi-wavelengths surveys in the Zone of AvoidanceRather than giving a complete overview on extragalactic Zone of Avoidance research, this paper will highlight some recent discoveries in the ZOA, such as new NIR to FIR observations (IRSF, Spitzer)…R. C. Kraan-Korteweg, K. J. van der Heyden, M. E. Cluver et al.·Oct 21, 2008SaveLearn
The cosmological consequence of an obscured AGN population on the radiation efficiencyIn light of recent indications for a large population of obscured active galactic nuclei (AGNs), we revisit the mean radiation efficiency from accretion onto supermassive black holes (SMBHs),…Alejo Martinez-Sansigre, Andrew M. Taylor·Oct 21, 2008SaveLearn
Evaluating and Improving Semi-analytic modelling of Dust in Galaxies based on Radiative Transfer CalculationsThe treatment of dust attenuation is crucial in order to compare the predictions of galaxy formation models with multiwavelength observations. Most past studies have either used simple analytic…Fabio Fontanot, Rachel S. Somerville, Laura Silva et al.·Oct 21, 2008SaveLearn
Planetary microlensing signals from the orbital motion of the source star around the common barycentreWith several detections, the technique of gravitational microlensing has proven useful for studying planets that orbit stars at Galactic distances, and it can even be applied to detect planets in…S. Rahvar, M. Dominik·Oct 21, 2008SaveLearn
A structure and energy dissipation efficiency of relativistic reconfinement shocksWe present a semi-analytical hydrodynamical model for the structure of reconfinement shocks formed in astrophysical relativistic jets interacting with external medium. We take into account exact…Krzysztof Nalewajko, Marek Sikora·Oct 21, 2008SaveLearn
The Discovery of a Very Faint X-ray Transient in the Globular Cluster M15We have identified an X-ray transient (hereafter M15 X-3) in the globular cluster M15 from an archival Chandra grating observation. M15 X-3 appears at an X-ray luminosity of 6*1033 ergs/s with a…Craig O. Heinke, Haldan N. Cohn, Phyllis M. Lugger·Oct 21, 2008SaveLearn
Fingers of GodVery long wavelength universal gravitational waves cannot now produce in clusters of galaxies velocity dispersions greater than that which these systems would possess if they were expanding with the…J. C. Jackson·Oct 21, 2008SaveLearn
Evidence for Blue Straggler Stars Rejuvenating the Integrated Spectra of Globular ClustersIntegrated spectroscopy is the method of choice for deriving the ages of unresolved stellar systems. However, hot stellar evolutionary stages, such as hot horizontal branch stars and blue straggler…A. Javier Cenarro, J. L. Cervantes, Michael A. Beasley et al.·Oct 21, 2008SaveLearn
VHE Gamma-ray Afterglow Emission from Nearby GRBsGamma-ray Bursts (GRBs) are among the potential extragalactic sources of very-high-energy (VHE) gamma-rays. We discuss the prospects of detecting VHE gamma-rays with current ground-based Cherenkov…P. H. Tam, R. R. Xue, S. J. Wagner et al.·Oct 21, 2008SaveLearn
The INTEGRAL-OMC Scientific ArchiveThe Optical Monitoring Camera (OMC) on-board the INTEGRAL satellite has, as one of its scientific goals, the observation of a large number of variable sources previously selected. After almost 6…A. Domingo, R. Gutierrez-Sanchez, D. Risquez et al.·Oct 21, 2008SaveLearn
The UKIRT Infrared Deep Sky Survey and the search for the most distant quasarsThe UKIRT Infrared Deep Sky Survey (UKIDSS) Large Area Survey (LAS) has the necessary combination of filters (Y, J, H and K), depth (Y <~ 20.2) and area coverage (~4000 deg2) to detect several…Daniel J. Mortlock, Mitesh Patel, Stephen J. Warren et al.·Oct 21, 2008SaveLearn
The inhomogeneous response across the solar disc of unresolved Doppler velocity observationsUnresolved Doppler velocity measurements are not homogenous across the solar disc (Brookes et al. 1978). We consider one cause of the inhomogeneity that originates from the BiSON instrumentation…A. M. Broomhall, W. J. Chaplin, Y. Elsworth et al.·Oct 21, 2008SaveLearn
Molecular Tracers of Embedded Star Formation in OphiuchusIn this paper we analyze nine SCUBA cores in Ophiuchus using the second-lowest rotational transitions of four molecular species (12CO, 13CO, C18O, and C17O) to search for clues to the evolutionary…Melissa Gurney, Rene Plume, Doug Johnstone·Oct 21, 2008SaveLearn
Astronomical imaging: The theory of everythingWe are developing automated systems to provide homogeneous calibration meta-data for heterogeneous imaging data, using the pixel content of the image alone where necessary. Standardized and complete…David W. Hogg, Dustin Lang·Oct 21, 2008SaveLearn
Ejection of hypervelocity binary stars by a black hole of intermediate mass orbiting Sgr A*The discovery of hypervelocity binary stars (HVBs) in the Galactic halo would provide definite evidence of the existence of a massive black hole companion to Sgr A*. Here we use an hybrid approach to…A. Sesana, P. Madau, F. Haardt·Oct 21, 2008SaveLearn
An enigmatic HI cloudThe discovery of an HI cloud with peculiar properties at equatorial coordinates (J2000) ra=07h49m, dec=04d30m is presented. The HI object was detected at 21cm using the 300-m NAIC Arecibo telescope.…L. Dedes, C. Dedes, P. W. M Kalberla·Oct 21, 2008SaveLearn
Asteroseismology of Red Giant starsSun-like oscillations, that is p-modes excited stochastically by convective noise, have now been observed in a number of Red Giant stars. Compared to those seen in the Sun, these modes are of large…N. J. Tarrant, W. J. Chaplin, Y. P. Elsworth et al.·Oct 21, 2008SaveLearn
Capability of the PAMELA Time-Of-Flight to identify light nuclei: results from a beam test calibrationPAMELA is a space telescope orbiting around the Earth since June 2006. The scientific objectives addressed by the mission are the measurement of the antiprotons and positrons spectra in cosmic rays,…D. Campana, R. Carbone, G. De Rosa et al.·Oct 21, 2008SaveLearn
Temperature and Metallicity in the Intra-cluster Medium of ABELL 262 observed with SuzakuWe studied the temperature and abundance distributions of intra-cluster medium (ICM) in the Abell 262 cluster of galaxies observed with Suzaku. Abell 262 is a bright, nearby poor cluster with ICM…Kosuke Sato, Kyoko Matsushita, Fabio Gastaldello·Oct 21, 2008SaveLearn