followup observations in the swift era s. r. kulkarni california institute of technology

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Followup Observations in the Swift Era S. R. Kulkarni California Institute of Technology

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Page 1: Followup Observations in the Swift Era S. R. Kulkarni California Institute of Technology

Followup Observations in the Swift Era

S. R. Kulkarni

California Institute of Technology

Page 2: Followup Observations in the Swift Era S. R. Kulkarni California Institute of Technology

New at Palomar

• Palomar 60-inch now automated Goal: Produce uniform set of light curves Fox (Project Scientist), Harrison & Kulkarni (PI) CCD + filter wheel (focus on I, z bands) 20% Caltech Community (only Q scheduled) 10% IPAC (Q scheduled; Data Pipeline and Archive) 70% GRB Team (all TOO)

• Palomar 24-inch robotic telescope Brown (PI); First light April 2004

20% SRK CCD + filter wheel

Page 3: Followup Observations in the Swift Era S. R. Kulkarni California Institute of Technology

Radio Followup• Will there be sufficient resources? Need radio light curves for many bursts (ordinary and

otherwise) But, few radio facilities (cf optical facilities) Our large VLA/BeppoSAX Large program: 1hr/day >> Suggest aggressive WSRT & ATCA program

• Radio monitoring would be useful (especially for supernovae and other transients) refurbish old facilities? e.g. 40-m OVRO telescope linkup with JPL DSN upgrade project?

Page 4: Followup Observations in the Swift Era S. R. Kulkarni California Institute of Technology

First few months: Shared Risk

• Maintain transparency

• View community at large as volunteers to help out the project

• Astronomers understand error radii, stochastic and systematic errors

• Rough fluences and fluxes should be a part and parcel of every event

Page 5: Followup Observations in the Swift Era S. R. Kulkarni California Institute of Technology

Routine Operations

• An impressive number of followup facilities have been organized in response to Swift.

- Robotic Telescopes

- Large Telescope Key projects

- Existing Networks are ready to go

• Host galaxy studies will lag other studies.

This is not a major issue.

Page 6: Followup Observations in the Swift Era S. R. Kulkarni California Institute of Technology

Followup Architecture

• Plan A: Swift project spearheads followup.

Organization of such a large followup program is logistically hard.

• Plan B: GCN as the central clearing house.

Assumes organic growth of community based efforts.

Swift sold as community mission.

>> Suggest a workshop in Spring.

Page 7: Followup Observations in the Swift Era S. R. Kulkarni California Institute of Technology

Swift Response: My view

• Have a default X-ray/UVOT observing sequence

Helps the community plan followup

Uniform data sets will be one of the legacies of Swift

• Exceptions to be made for exceptional bursts

Announce these via GCN.

Page 8: Followup Observations in the Swift Era S. R. Kulkarni California Institute of Technology

Advice to Team

• Please publish Swift-specific papers rapidly

Obviously morale booster for team

Energizes community to respond with

followup papers

• Publish Swift catalog every six months

This will drive synthesis studies