NIR flaring of the Gamma ray source [HB89] 0754+100
ATel #2516; Carrasco, L., Mayya, Y. D., Carramiñana, A., Recillas, E., Porras, A.
on 27 Mar 2010; 06:24 UT
Distributed as an Instant Email Notice Request For Observations
Credential Certification: LUIS CARRASCO (carrasco@inaoep.mx)
Subjects: Infra-Red, Gamma Ray, Request for Observations, AGN, Quasar
We call attention on our recent observation of the Gamma Ray source [HB89] 0754+100 with the CANICA NIR camera on the 2.1m telescope at the Observatorio AstrofÃsico Guillermo Haro, located in Cananea, Mexico. We found this BLLac type object, to show fluxes about 2 magnitudes brighter than our previous observation 30 days earlier. Below, we list our photometric results in the H Band for this period.
JD2455241.868948, H=14.542 +/- 0.04
JD2455259.830452, H=13.543 +/- 0.05
JD2455272.784343, H=12.638 +/- 0.01
Multiwavelength follow up observations would be desirable.
