Skip banner and navigation tools.

 |  site map

Skip sidebars of related page links.

Guest Investigator Program

The Swift Guest Investigator Program is an annual announcement of opportunity soliciting proposals from the community for research relevant to the Swift mission. The GI programs begin at the start of each April and last for approximately 12 months (Cycle 15 runs from 1st April 2019 until 31st March 2020). Observing time is available for scientists at both US and non-US institutions, although only those Principal Investigators at US institutions will be eligible for funding from NASA. No funding is provided for the fill-in category.

GI Cycle 15: Deadline Thursday 27th September at 20:30 UT

Swift provides an opportunity for simultaneous optical to hard X-ray observations of targets, allowing broad-band analysis. The X-ray Telescope is specifically designed to choose the best operating mode for the X-ray flux of the object in question.

As started in Cycle 12, there is a Key Projects category. Such projects are intended to provide significant advances in Swift science, and require a very strong justification. In these cases, 6 pages are allowed for the scientific justification (4 pages only are allowed for all other proposals), with an additional 1 page narrative required if funding is being requested.

Cycle 15 again includes the option to submit a single proposal for combined observing programs between Swift and XMM-Newton, Chandra, INTEGRAL, NRAO (VLA, GBT and VLBA) and NuSTAR. More details are available on the main GI page.

In this cycle, there will be up to 2 Ms available for non-ToO targets, 1 Ms for ToOs, 1 Ms for large programs and 1 Ms for fill-in targets. ToOs for GRBs detected with instruments other than Swift (e.g., MAXI, Fermi, IPN) are included in this time.

Requests for fill-in observations cannot be time-constrained (e.g. coordinated with ground- or space-based facilities), although both ToOs and non-ToOs may be, provided the window for the observation exceeds 3 hours. There is no restriction on the maximum number of time-constrained observations permitted.

The duration of an observation (ie a single visit to a target) is limited to between 1 and 40 ks, although several observations may be requested.

See the NASA page for more details (FAQs), or contact the Leicester Swift help-desk.

List of Cycle 14 (2018-2019) accepted targets

Previous Cycles

Cycle 14 (2018-2019)
Cycle 13 (2017-2018)
Cycle 12 (2016-2017)
Cycle 11 (2015-2016)
Cycle 10 (2014-2015)
Cycle 9 (2013-2014)
Cycle 8 (2012-2013)