|
| Preserve the scientific integrity of ROTSE results | |
| Provide appropriate recognition of all ROTSE collaboration members | |
| Facilitate rapid analysis and publication of as much ROTSE science as possible |
Core Science:
ROTSE core science includes all analyses related to gamma-ray bursts, all triggered responses, special campaigns, and any other studies of astrophysical transience which utilize a substantial fraction (more than 1% of the sky) of the survey data.
Auxiliary Science: Anything else
Core Science Papers:
Publication of core science papers will include three steps:
Conference Presentations of Core Science:
| Early conference presentation of new core science results must be reviewed by the collaboration. This will be done by submitting the results to be presented 9preferably in the form of final slides) to the collaboration 1 week before the conference. All collaboration members are invited to comment. Final approval will be made by consensus of the collaboration. Non-response by the collaboration will constitute approval. | |
| Any collaboration member may request to present ROTSE material at a conference. Decisions will be made by the collaboration council. All collaboration members may present ROTSE material in seminars or colloquia. | |
| The collaboration council is responsible for making public presentation or ROTSE results as broad as possible. it is also charged with equitable distribution of public appearances. A guided principal is that all junior collaboration members must be afforded the opportunity to publicly present ROTSE results. The council is charged with pursuing talks at major conferences, and with seeking colloquium and seminar invitations for junior members. |
Auxiliary Science:
There is a lot of other science to be done with ROTSE sky patrols
which is far removed from the core goals of the project. This includes, for example,
early observation of a (nonGRB) transient discovered by someone else. We can only
benefit by getting these kinds of results published.
|