output
20022012
most citedThe Imprint of The Extragalactic Background Light in the Gamma-Ray Spectra of Blazars

273 citations

Showing astro-phShow all

6 papers · 1 filter

astro-ph200822 cited

Search for Cosmic Strings in the GOODS Survey

J. L. Christiansen, E. Albin, K. A. James +3

We search Hubble Space Telescope Treasury Program images collected as part of the Great Observatories Origins Deep Survey for pairs of galaxies consistent with the gravitational le…

astro-ph200882 cited

Precise radial velocities of giant stars. IV. A correlation between surface gravity and radial velocity variation and a statistical investigation of companion properties

S. Hekker, I. A. G. Snellen, C. Aerts +3

Since 1999, we have been conducting a radial velocity survey of 179 K giants using the CAT at UCO/Lick observatory. At present ~20-100 measurements have been collected per star wit…

astro-ph20073 cited

Radial velocities of giant stars: an investigation of line profile variations

S. Hekker, I. A. G. Snellen, C. Aerts +3

Since 1999, a radial velocity survey of 179 red giant stars is ongoing at Lick Observatory with a one month cadence. At present ~20-100 measurements have been collected per star wi…

astro-ph2007101 cited

The spin axes orbital alignment of both stars within the eclipsing binary system V1143Cyg using the Rossiter-McLaughlin effect

S. Albrecht, S. Reffert, I. Snellen +2

Context: The Rossiter-McLaughlin (RM) effect, a rotational effect in eclipsing systems, provides unique insight into the relative orientation of stellar spin axes and orbital axes…

astro-ph200684 cited

Precise radial velocities of giant stars: I. Stable stars

S. Hekker, S. Reffert, A. Quirrenbach +4

Context: Future astrometric missions such as SIM PlanetQuest need very stable reference stars. K giants have large luminosities, which place them at large distances and thus the ji…

astro-ph20063 cited

HI Density Distribution Driven by Supernovae: A Simulation Study

Jacqueline A. Hodge, Avinash A. Deshpande

We model the complex distribution of atomic hydrogen (HI) in the interstellar medium (ISM) assuming that it is driven entirely by supernovae (SN). We develop and assess two differe…