凯克对160个伽马射线爆发宿主星系的观测

D. Perley, J. S. Bloom, J. Prochaska
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引用次数: 4

摘要

我们在凯克天文台进行了多年的研究,通过多色地面光学成像和光谱学,研究了斯威夫特时代伽玛射线爆发大样本的宿主星系,并发布了初步数据。迄今为止观测到的目标超过160个(以及近100个宿主检测,其中大多数以前没有在文献中报道过),我们的努力代表了迄今为止最广泛的GRB宿主调查。虽然目标是不均匀的,但我们的观测跨越了已知的grb多样性,包括短爆发、长爆发、光谱软grb (xrf)、超高能量grb、x射线微弱grb、暗grb、sn - grb和其他子类。我们还提供了我们数据库的预览(目前可通过方便的网络界面在线获得),包括多色测光,红移和线ID的目录。最终的光度测定和简化的成像和光谱将在不久的将来可用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
KECK OBSERVATIONS OF 160 GAMMA-RAY BURST HOST GALAXIES
We present a preliminary data release from our multi-year campaign at Keck Observatory to study the host galaxies of a large sample of Swift-era gamma-ray bursts via multi-color ground-based optical imaging and spectroscopy. With over 160 targets observed to date (and almost 100 host detections, most of which have not previously been reported in the literature) our effort represents the broadest GRB host survey to date. While targeting was heterogeneous, our observations span the known diversity of GRBs including short bursts, long bursts, spectrally soft GRBs (XRFs), ultra-energetic GRBs, X-ray faint GRBs, dark GRBs, SN-GRBs, and other sub-classes. We also present a preview of our database (currently available online via a convenient web interface) including a catalog of multi-color photometry, redshifts and line ID’s. Final photometry and reduced imaging and spectra will be available in the near future.
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