For XMM AO-6, there were no proposals submitted "on behalf of the LAT Collaboration"

There were proposals closely related to LAT work, some of which involve LAT scientists:

  • J. Ballet, RX J1713.7-3946 - two fields accepted
  • R. Romani, SEDs of High-z Blazars
  • N. Webb, Pulsar Timing - binary ms pulsars: PSR J1905+0400 PSR J1751-2857 PSR J1853+1303 PSR J1600-3053
  • S. Ciprini, OJ 287 - long-term multifrequency monitoring
  • G. Tagliaferri, Flaring Blazars - can be triggered by LAT flare
    PKS 0118-272
    B3 0133+388
    PKS 0208+512
    1ES 0219+428
    AO 0235+164
    CTA 026
    1ES 0414+009
    PKS 0446+112
    S5 0454+844
    PKS 0528+134
    PKS 0537-441
    1ES 0548-322
    1ES 0647+250
    S5 0716+714
    PKS 0735+178
    1ES 0806+524
    OJ +248
    1ES 1101-232
    Mkn 421
    RBS 0958
    Mkn 180
    PKS 1144-379
    OM 280
    1ES 1215+303
    1ES 1218+304
    W Comae
    3C 273
    3C 279
    1ES 1255+244
    PKS 1406-076
    OQ 530
    1ES 1426+428
    AP Librae
    1ES 1517+656
    OR 165
    1ES 1553+113
    PKS 1622-297
    4C +38.41
    Mkn 501
    NRAO 530
    PMN J1802-3940
    1ES 1959+650
    PKS 2005-489
    S5 2007+777
    PKS 2155-304
    BL Lac
    3C 454.3
    PKS 2254+074
    1ES 2344+514

  
XMM-Newton cycle AO-7 (deadline: Oct.5.2007 - observations period: May 2008 to May 2009)

     

XMM-Newton cycle AO-9

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