English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

We present an upper limit on the brightness of the afterglow of the long GRB030115 measured from Infrared (IR) images taken with the Magellan Classic Caminstrument of Ks > 22 at 6.2 days after the burst. We also present measurmentsof the host galaxy of GRB 030115 from archival optical and IR HST images takenwith the Advanced Camera for Surveys and the Near Infrared Camera and MultiObject Spectrometer 25+ days after the burst. GRB 030115 is classified as anOptically Dark Burst, as its afterglow was found in the J, H, and K IR bandsafter a null result was reported in the optical. This is the first HETE GRB tohave its afterglow found initially in the IR.Comment: 4 pages, 3 figures, to appear in the Santa Fe GRB Conference  Proceedings, 200

IR and Optical Observations of GRB 030115