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