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)

•  S. Ciprini, [3 blazars, GO-type proposal]  (confluence log-in & passwd needed).