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ASAS-SN Prediscovery Limits for SPIRITS16tn

ATel #9446; B. J. Shappee (Hubble Fellow, Carnegie Observatories), K. Z. Stanek, C. S. Kochanek, T .W.-S. Holoien (Ohio State), J. L. Prieto (Diego Portales; MAS)
on 1 Sep 2016; 19:46 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Benjamin Shappee (bshappee@obs.carnegiescience.edu)

Subjects: Optical, Supernovae

Following the discovery of SPIRITS16tn (ATel #9434), a possible supernova discovered with Spitzer in Messier 108 (NGC 3556), we analyzed prediscovery ASAS-SN data at its reported location. SPIRITS16tn was not detected in images obtained on UT 2016-06-10.262 and before. Our prediscovery limits are as follows:

 
JD           UT Date         V-Band Limit                                               
2457524.797  2016-05-16.297  >17.59                                                                                                                  
2457528.782  2016-05-20.282  >17.22                                                                                                                  
2457532.810  2016-05-24.311  >17.48                                                                                                                  
2457537.789  2016-05-29.289  >17.93                                                                                                                  
2457542.779  2016-06-03.279  >17.76                                                                                                                  
2457545.792  2016-06-06.292  >17.80                                                                                                                  
2457547.758  2016-06-08.258  >17.85                                                                                                                  
2457549.762  2016-06-10.262  >17.81                                                                                                                  

It is currently not clear if these limits constrain the explosion date because SPIRITS16tn is likely heavily extinguished (ATel #9441).

We thank LCOGT and its staff for their continued support of ASAS-SN. ASAS-SN is supported by NSF grant AST-1515927, the Center for Cosmology and AstroParticle Physics (CCAPP) at OSU, the Mt. Cuba Astronomical Foundation, George Skestos, and the Robert Martin Ayers Sciences Fund. For more information about the ASAS-SN project, see the ASAS-SN Homepage and the list of all ASAS-SN transients.