activity
20062026
most citedExtreme Properties Of GRB061007: A Highly Energetic OR Highly Collimated Burst?

53 citations · 59 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026★ 2 cited

oMEGACat. IX. Chemical Tagging of Omega Centauri Populations with Machine-Learning-Inferred Abundances from the MUSE Spectrograph

Z. Wang, A. C. Seth, C. Clontz +14

We present chemical abundance measurements for 7,302 red giant branch stars within the half-light radius (~5') of Centauri ( Cen), derived from MUSE spectra using the neural…

astro-ph.GA2025★ 1 cited

oMEGACat. VIII. A Subpopulation Census of ω Centauri

C. Clontz, A. C. Seth, Z. Wang +8

An understanding of the assembly history of the complex star cluster Omega Centauri has long been sought after, with many studies separating the stars on the color-magnitude diagra…

astro-ph.GA2025

oMEGACat. VII. Tracing Interstellar and Intracluster Medium of Centauri using Sodium Absorptions

Z. Wang, A. C. Seth, M. Latour +14

We investigate the foreground interstellar medium along the line of sight and intracluster medium of Centauri ( Cen) by measuring the equivalent width of Na I D absorptions…

astro-ph2006★ 53 cited

Extreme Properties Of GRB061007: A Highly Energetic OR Highly Collimated Burst?

P. Schady, M. De Pasquale, J. Cummings +20

%auto-ignore This paper has been withdrawn by the authors due to dublicate submission. To download the paper please go to astro-ph/0611081

astro-ph2006★ 3 cited

Extreme Properties Of GRB061007: A Highly Energetic Or A Highly Collimated Burst?

P. Schady, M. De Pasquale, M. J. Page +20

GRB061007 is the brightest gamma-ray burst (GRB) to be detected by Swift and is accompanied by an exceptionally luminous afterglow that had a V-band magnitude <11.1 at 80s after th…