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Charlot, P. |
Volume |
Paper Title |
Page Number |
Authors |
19 |
Are the Band Width Synthesis delay and delay rate observables useful for VLBI imaging? |
302 |
Charlot, P. |
144 |
EVN Observations of BL Lac Objects with Distorted Structures |
161 |
Charlot, P.; Sol, H.; Vicente, L. |
144 |
VLBA Observations of Radio Reference Frame Sources. II. Astrometric Suitability Based on Observed Structure |
387 |
Fey, A. L.; Charlot, P. |
266 |
Phase Retrieval in Very-Long-Baseline Interferometry |
254 |
Mezaoui, A.; Baudry, A.; Charlot, P. |
290 |
Simulations of the long-term evolution of cooling flow clusters containing radio sources |
329 |
Charlot, P.; Gabuzda, D. C.; Sol, H.; Degrange, B.; Piron, F. |
290 |
Simultaneous VLBI and high-energy TeV observations of the γray blazar Mkn 421 |
329 |
Charlot, P.; Gabuzda, D. C.; Sol, H.; Degrange, B.; Piron, F. |
340 |
Multi-Frequency, Multi-Epoch VLBA Polarization Observations of Mrk501 |
177 |
Croke, S.; Charlot, P.; Gabuzda, D.; Sol, H. |
340 |
Phase-Referenced VLBI Astrometry of Compact Symmetric Objects |
511 |
Charlot, P.; Pradel, N.; Lestrade, J.-F. |
340 |
Extending the ICRF to Higher Radio Frequencies: First Imaging Results |
514 |
Fey, A.L.; Boboltz, D.A.; Charlot, P.; Fomalont, E.B.; Lanyi, G.E.; Zhang, L.D. |
340 |
Extending the ICRF to Higher Radio Frequencies: Astrometry at 24 and 42 GHz |
523 |
Jacobs, C.S.; Lanyi, G.E.; Naudet, C.J.; Sovers, O.J.; Zhang, L.D.; Charlot, P.; Gordon, D.; Ma, C. |
340 |
Simulation of Systematic Errors in Phase-Referenced VLBI Astrometry |
538 |
Pradel, N.; Charlot, P.; Lestrade, J.-F. |
402 |
Space VLBI and the Radio Reference Frame |
480 |
Charlot, P. |
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