PROPOSAL OVERVIEW | |
Proposal Title | XMM-Newton follow-up of electromagnetic counterparts to GW triggers during LVKC- |
Proposal Category | Isolated and Binary Compact Objects & their Evolution |
Proposal Type | LARGE PROGRAM |
Proposal Id | 090357 |
Number of Observations | 8 |
Total exposure time (ks) | 586 |
PI DETAILS | |
PI | Dr. Sergio Campana |
Institute | INAF - Osservatorio Astronomic |
Country | ITALY |
CO-INVESTIGATORS | ||
Name | Country | |
P. D'Avanzo | ITALY | |
M. Bernardini | ITALY | |
G. Ghirlanda | ITALY | |
O. Salafia | ITALY | |
A. Bulgarelli | ITALY | |
N. Tanvir | UNITED KINGDOM | |
P. Jonker | NETHERLANDS | |
A. Melandri | ITALY | |
W. Fong | UNITED STATES | |
A. Levan | NETHERLANDS | |
E. Berger | UNITED STATES | |
A. Hajela | UNITED STATES | |
K. Alexander | UNITED STATES | |
A. Ruoco Escorial | UNITED STATES | |
J. Rastinejad | UNITED STATES | |
R. Chornock | UNITED STATES | |
J. Bright | UNITED STATES | |
D. Brethauer | UNITED STATES |
ABSTRACT | |
The joint detection of GWs and light from the NS merger GW170817 ushered us into a new era. Deep X-ray observations of GW170817 over 4 yr constrained the structural properties of a relativistic outflow launched by an NS merger and possibly detected the first evidence for the emerging kilonova afterglow. After this landmark discovery, the frontier is now to map the properties of a population of GW sources. We propose to exploit the unique capabilities of XMM-Newton to constrain the broad-band properties of 2 GW sources detected during LVKC-O4. Our immediate goals are: (i) map the diversity of emission from NS mergers, (ii) test the nature of the remnant object, (iii) determine if all mergers launch a jet, (iv) enable the first X-ray detections of NS-BH mergers or unclassified GW sources. |
PAPERS |
- CLASS 1: | papers that present specific XMM-Newton observations |
- CLASS 2: | papers that refer to published XMM-Newton results with complementary observations, follow-up analysis, or theoretical analysis |
- CLASS 3: | further deliveries which resulted from the program and which are made available to the community (e.g. source catalogues, processed images or spectra in public data base) |
- CLASS 4: | comments and suggestions from PI |