... I 8 X 15 <Lf> 16 9 <Cr> 10 <Cr> 17 3 M Example Value: 50000 4 M 11 <Lf> 18 > 12 <Dly ... 2 I 8 X 15 <Dly> 16 <ACK> 9 <Cr> 10 <Cr> 17 3 M 4 M 11 <Lf> 18 12 50000 19 > 5 A 6 A ...
... of the P. Shapiro Cosmological 21-cm Background from the EOR 17:00 21cm Reionization Forecast and U-L. Pen Search at GMRT 17:20 The MWA experiment M. Morales 17:40 Prospects and challenges for EOR A. Cooray HI detection 18:00 DINNER Saturday morning 5 ...
... of the P. Shapiro Cosmological 21-cm Background from the EOR 17:00 21cm Reionization Forecast and U-L. Pen Search at GMRT 17:20 The MWA experiment M. Morales 17:40 Prospects and challenges for EOR A. Cooray HI detection 18:00 DINNER Saturday morning 5 ...
... Assuming the periastron advance is fully relativistic, the total binary mass is 2.29 0.17M ? ... This implies a total system mass of 2.17(2) M ? . From this, we can derive m p < 1.96 and m c > 0.24 M ? respectively. ...
... 1 x 10 -17 W/m 2 for frequencies from 470 to 1000 MHz; . f 2 (GHz) x 10 -17 W/m 2 for frequencies (f) above 1 GHz; . ... 1 x 10 -17 W/m 2 for frequencies from 470 to 1000 MHz; . f 2 (GHz) x 10 -17 W/m 2 for frequencies (f) above 1 GHz; . ...
... Platforms and options (K. O'Neil) Software plans of the Ultra Deep Group (W. Freudling) Software plans of the Driftscan Group (R. Giovanelli) A possible IVO/NVO portal (B. Kent) Software issues from the whitepaper (M. Haynes) M. Haynes 17:30 19:00 19:00 ...
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Ссылки http://www.naic.edu/alfa/ealfa/meeting2/misc/schedule_final.pdf -- 7.8 Кб -- 12.05.2006 Похожие документы
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