Luminosity-time correlations for GRBs afterglows Maria Giovanna Dainotti Department of Astronomy, Stanford University, Stanford, California In collaboration.
RXJ0146.9 +6121 a soft X-ray excess in a low luminosity accreting pulsar La Palombara & Mereghetti astro-ph/0604193.
Broad iron lines from accretion disks
Star and Planet Formation
5 th RHESSI workshop, Locarno. WG 4 Report Participants: Steven ChristeSäm Krucker Brian DennisMonique Pick Lyndsay FletcherEd Schmahl Peter GallagherManuela.
Luminosity-time correlations for GRBs afterglows
Unlocking the nature of ULXs using their X-ray spectra
GRB CORRELATIONS AND THEIR COSMOLOGICAL APPLICATIONS Maria Giovanna Dainotti JSPS Fellow at Riken, Tokyo, Japan 1 RIKEN(ITHES/RNC)-IPMU-RESCEU, 7TH OF.
5 th RHESSI workshop, Locarno. WG 4 Report
Is the plateau emission also a feature of high energy GRBs?
GRB correlations and their cosmological applications
Latest Results from the Milagro Observatory
