XMM-Newton Large Programme Details



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
Authors marked in red are (co-)investigators in the proposal

Classification of papers are:
- 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


There are no papers associated to this proposal