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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; 6:24 UT
Distributed as an Instant Email Notice (Request for Observations)
Password Certification: LUIS CARRASCO (carrasco@inaoep.mx)

Subjects: Infra-Red, Gamma Ray, Request for Observations, AGN, Quasars

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 Astrofísico 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.


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