Project | Band(s) | Test Code | Test Status | Allocation Status (D) | Notes | JIRA |
---|---|---|---|---|---|---|
RSRO | ||||||
ECSO | ||||||
AB1346 | K | TRSR0005 TSPE0001 |
23Jun10 | 39/40 | 2 hour makeup pending for DnC | RSRO-3 |
AM1014 | C | TRSR0009 | 22Jun10 | 0/0 | C config | RSRO-9 |
AT374 | C | TRSR0011 | 25Jul10 | 0/0 | C config | RSRO-12 |
AC982 | CKKaQ | TRSR0002 | 28Jul10 | 30/30 | Complete | RSRO-4 |
AK726 | Ka | TRSR0007 | - | 29.5/29.5 | Complete | RSRO-6 |
AL746 | CKa | TRSR0008 | 05Jul10 | 11/11 | Complete | RSRO-7 |
AS1015 | C | TRSR0010 | 21May10 | 4/4 | Complete | RSRO-11 |
AM1038 | Q | TRSR0019 | 21May10 | 10/10 | Complete | - |
AM1040 | Ka | TRSR0019 | 21May10 | 10/10 | Complete | - |
AC992 | L | TRSR0018 | 26Jun10 | 4/4 | Complete | - |
AO255 | Ka | TRSR0016 | - | 36/40 | Complete | - |
AV318 | L | TRSR0012 | - | 12/12 | Complete; PI converted to OSRO | RSRO-13 |
AB1353 | Ka | TRSR0013 | - | 0/51 | Moved to C config | - |
AM1018 | Ka | TRSR0015 | - | 0/48 | Needs test for DnC | - |
AA30 | Q | TRSR0003 | - | 0/51 | Not started | RSRO-1 |
AH1006 | LCXKa | TRSR0006 | - | 30/36 | Partial | RSRO-5 |
AW775 | L | TRSR0017 | 05Jul10 | 56/72 | Partial | - |
AM1005 | KKaQ | TRSR0014 | - | 3/20 | Partial (carry to C config) | - |
AB1345 | L | TRSR0004 | 21May10 | 23/40 | Partial; adequate for D | RSRO-2 |
Project | Status | Time | Comments | SB |
---|---|---|---|---|
Crab nebula | Complete | 10/10 | Complete; L-band OSRO1/OSRO2 | |
IRC+10216 | Ready (HF) | 11/33 | Partial; revisit in DnC/C | |
M87 | Ready (HF) | 0/6 | Ka | Not done |
M51 | Ready (MR) | 8/8 | Complete | |
Cygnus A | Ready | 3x6 | 1x10 possible; 12 OSRO hours obtained | Withdrawn |
M82 | Complete | 2/2 | L band | Complete |
Herc A | Ready | 3/5 | CX bands | Partial |
At the Cal-Im meeting in Dwingeloo 2 weeks ago, the ASTRON folks advertised this image as a 'surprise' for NRAO attendees - and were very pleased that Rick had given them these data. Rick had told them that the best that could be done with these data was a dynamic-range of a few thousand to one. Sarod-Yatawatta (ASTRON) ran it through a multiscale-type imaging algorithm of his own, and produced a dynamic range of 13000:1. This was used to claim a superior algorithm compared to those in any NRAO software. Note however that it was not known if anyone other than Rick/Bill at NRAO had imaged these data or tried multi-scale/mem methods from either CASA or AIPS.
I | Attachment | Action | Size | Date | Who | Comment |
---|---|---|---|---|---|---|
ps | 2GHZ-15X22-CAL.ps | manage | 160 K | 2010-09-14 - 16:35 | UnknownUser | |
ps | 2GHZ-15X22-RAW.ps | manage | 159 K | 2010-09-16 - 11:36 | UnknownUser | |
ps | 3B-LCP.ps | manage | 7 K | 2010-09-16 - 11:35 | UnknownUser | |
ps | 8B-LCP.ps | manage | 7 K | 2010-09-16 - 11:35 | UnknownUser |