Assassin Picture of the Week

2013 November 11


Active (Some Less, Some More) Galactic Nuclei with ASAS-SN

There are many kinds of objects that vary on the sky, and we already had an APOW about an extreme M-dwarf flare, several about ASAS-SN supernovae, and we also talked about dramatic AGN outburst in NGC 2617. Active Galactic Nuclei represent some of the most exotic conditions in the universe, and are one of the few observational signatures of the supermassive black holes (SMBHs) at the centers of all massive galaxies. Furthermore, there are observed correlations between SMBHs and their host galaxies, indicating that they influence each others' evolution with time. Yet, AGN are largely ignored in most current transient surveys, even though it is well known that both the broad line and continuum components of active galactic nuclei are time variable at all wavelengths. This variability enables, for example, the reverberation mapping (RM) technique for studying black hole masses and the structure of the broad line region. However, despite decades of research, the structure of AGN and the drivers of their variability are still poorly understood.

As we have already discussed, ASAS-SN has already proven capable of finding rare outbursts and constraining the source of AGN variability. In case of NGC 2617 we (Shappee et al. 2013) have unambiguously showed that the X-ray variability preceded the UV-optical-IR changes, almost certainly due to irradiation and heating of the disk. This was the first case of a clear and convincing determination as to whether X-ray variability drives UV to NIR variability or the reverse.

Encouraged by the reception of this discovery by the AGN community, in 2014, with six cameras deployed, we are planning to implement the ``ASAS-SN AGN Patrol.'' ASAS-SN will monitor all bright (V<17) AGN, quasars, and blazars, and produce publicly available light curves for these objects in real time. Here we show ASAS-SN light curves of several known AGN to illustrate our cadence and photometric precision with only two cameras. Stay tuned!

Back to ASAS-SN page.

See previous APOWs:

Brutus is EXPANDING!

Swift Ultraviolet and Optical Follow-Up of ASASSN-13dl, Our Latest Supernova

Dramatic AGN Outburst in NGC 2617

M81 and Friends

Two ASAS-SN Views of Orion Nebula

AAVSO Observations of Cataclysmic Variable ASASSN-13ck

Two ASAS-SN Supernovae in One Day!

It is Good to be Lucky!

Extreme M-dwarf Flare Observed by ASAS-SN;

Neptune Discovered!

Multiband photometric follow-up of ASASSN-13aw (SN 2013dr);

"Assassin" Unit 1: Brutus;

How ASAS-SN Discovers Supernovae: Case of Supernova ASASSN-13bb;

NGC 2617: Dramatic Seyfert Type Change;

ASASSN-13/SN 2013da: Our First Supernova Three Weeks Later;

M31 and Companions;

This homepage is maintained by Ben Shappee, Tom Holoien and Kris Stanek. Updated Mon Nov 11 13:45:54 EST 2013

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