Differences

This shows you the differences between two versions of the page.

--- grb:papers [2013/05/09 13:42] – stephen.fairhurst@LIGO.ORG
+++ grb:papers [2013/05/23 16:30] (current) – duncan.macleod@LIGO.ORG
@@ Line 1: / Line 1: @@
-====== GRB technical papers ======
+This page has moved [[lvc:grb:papers|here]].
-Over the past few years, we have worked on a number of aspects of GRB searches and astrophysics, these include:
-  * Estimates of the expected rates
-  * Chances of detection based on the observing scenarios paper
-  * Improved detection chances if distance is known
-  * Face on search
-  * Sky patches
-  * Time shifts (both long and short) for background estimation
-  * Preparation for advanced detectors: longer templates, etc
-  * Search 1 polarization for HL?
-The git repository hosting papers on this subject is available [[https://gravity.astro.cf.ac.uk/cgit/grb-methods/ | at this link]].
-===== GRB pipeline paper =====
-Discuss
-  * face on
-  * sky patch
-  * background estimation
-Suggestion is to use a GRB from the S6D time (June 26 to Oct 20).
-Advanced detector proof of principle
-===== GRB astro paper =====
-GRB motivation/rates
-  * Argue that GRB time is valuable and that this lets you reduce the threshold
-  * Observing scenarios from Hannah's work
-  * Known redshift to improve odds
-Measure redshift and GW amplitude
-  * cosmology
-  * beaming angles
-  * use populations to get beaming angles
-Localizations
-  * triangulation
-  * from snr on sky grid of loudest template
-  * same for face on