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Äàòà èçìåíåíèÿ: Thu Oct 13 17:32:21 2011
Äàòà èíäåêñèðîâàíèÿ: Mon Feb 4 21:19:32 2013
Êîäèðîâêà:

Ïîèñêîâûå ñëîâà: jet
Proposal Identification No.: V2691 Date Received: 2011­Oct­03 19:21:25
Technical Page
Proposal Type: Regular
General Category: VLBI
Observation Category: Extragalactic
Total Time Requested: 40 Hours
Minimum Useful Time: 1 hour
Proposal Title: Radioastron­Arecibo Space VLBI survey of AGN at extreme angular resolution
ABSTRACT:
We request 40 hours of Arecibo time in February­May 2012 for a non­imaging Space VLBI survey for the brightest
and most compact AGN jet cores with Radioastron and Arecibo at L and C bands. The main goal of this project is
to determine the correlated flux density, angular size, and brightness temperature of the most compact structure(s)
in the AGN radio core located in the jet base. We will probe the inverse­Compton limit and Doppler boosting of
AGN cores testing the current widely accepted jet model of synchrotron emitting relativistic electrons,
inverse­Compton cooling, and relativistic beaming. This proposal is submitted as part of the Radioastron early
science program.
Name Institution E­mail Phone Student
Yuri Y. Kovalev Astro Space Center
of Lebedev Physical
Institute
yyk@asc.rssi.ru +7 495
3332167
no
Remote Observing Request
Observer will travel to AO
Remote Observing
X In Absentia (instructions to oper­
ator)
Instrument Setup
L­wide C
Atmospheric Observation Instruments:
Special Equipment or setup: MK5A VLBI disk recording
RFI Considerations
1

Frequency Ranges Planned
2