AGN Research Aids
AGN Movies
Here is a movie showing variations of the Hbeta profile
in NGC 5548 between 1972 and 2001. Contaminating
narrow lines (narrow Hbeta and [O III] 4959, 5007)
have been removed. The data are mostly
photographic spectra from Crimean Astrophysical Observatory
(1972-1988) or CCD spectra from
the International AGN Watch database.
The data are described more completely in the paper
"Thirty Years of Continuum and Emission-Line Variability
in NGC 5548,'' by Sergeev, Doroshenko, Dzyuba, Peterson,
Pogge, and Pronik (in preparation).
[NGC 5548 30-Year AVI] (12.3 Mb)
The movie below shows how an isodelay surface propagates through
the broad-line region. The left panel shows the BLR as a disk.
The black-hole/accretion-disk structure is the point at the
center. The red line is an isodelay surface. The upper right
panel shows a velocity-delay map, i.e., the BLR mapped into
line-of-sight velocity/time-delay space. The horizontal red line
is the map of the isodelay surface onto the velocity-delay map.
The lower right panel is the line profile along the isodelay
surface.
[Time Delay QuickTime Movie] (7.5 Mb)
AGN Light Curves
This page contains light curves from
The Ohio State AGN Spectroscopic Monitoring Project
(1988-1996). These are supplementary tables to the paper
``Optical Continuum and Emission-Line Variability of Seyfert 1 Galaxies''
by B.M. Peterson, I. Wanders, Ray Bertram,
James F. Hunley, Richard W. Pogge,
and R. Mark Wagner, The Astrophysical Journal, 501, 82.
This work was funded by the National Science Foundation through
grant AST-9420080, and its predecessors,
AST-8702691, AST-8915258, and AST-9117086.
- The published paper (1998, ApJ, 501, 82 [July 1])
- [
Preprint ] (all files, tarred and gzipped version, 290kB)
- [
Text] (Text and Tables only, PostScript format, 361kB)
- [
Figure 1] Mean and rms spectra of 3C 120, Akn 120, and Mrk 79
(PostScript format, 64kB)
- [
Figure 2] Mean and rms spectra of Mrk 110, Mrk 335, and Mrk 509
(PostScript format, 64kB)
- [
Figure 3] Mean and rms spectra of Mrk 590, Mrk 704, and Mrk 817
(PostScript format, 64kB)
- [
Figure 4] 3C 120 light curve (PostScript format, 31kB)
- [
Figure 5] Akn 120 light curve (PostScript format, 55kB)
- [
Figure 6] Mrk 79 light curve (PostScript format, 55kB)
- [
Figure 7] Mrk 110 light curve (PostScript format, 40kB)
- [
Figure 8] Mrk 335 light curve (PostScript format, 49kB)
- [
Figure 9] Mrk 509 light curve (PostScript format, 69kB)
- [
Figure 10] Mrk 590 light curve (PostScript format, 44kB)
- [
Figure 11] Mrk 704 light curve (PostScript format, 23kB)
- [
Figure 12] Mrk 817 light curve (PostScript format, 37kB)
- [
Figure 13] Cross-correlations (ICCF and DCF) for
all objects (PostScript format, 154kB)
- [
Figure 14] Cross-correlations (ICCF and DCF) for best subsets
(PostScript format, 34kB)
- [
Figure 15] Combined light curves for Akn 120, 1979-1996
(PostScript format, 75kB)
- [
Figure 16] Akn 120 cross-correlations of old data (ICCF and DCF)
(PostScript format, 30kB)
- Detailed Observational Logs (PostScript format)
- Light curves (tabular form)
- [
3C 120 (Postscript, 43kB)]
[
3C 120 (ASCII table, 2.7kB)]
- [
Akn 120 (Postscript, 57kB)]
[
Akn 120 (ASCII table, 7.2kB)]
- [
Mrk 79 (Postscript, 59kB)]
[
Mrk 79 (ASCII table, 7.3kB)]
- [
Mrk 110 (Postscript, 51kB)]
[
Mrk 110 (ASCII table, 4.8kB)]
- [
Mrk 335 (Postscript, 55kB)]
[
Mrk 335 (ASCII table, 6.3kB)]
- [
Mrk 509 (Postscript, 44kB)]
[
Mrk 509 (ASCII table, 9.9kB)]
- [
Mrk 590 (Postscript, 52kB)]
[
Mrk 590 (ASCII table, 5.2kB)]
- [
Mrk 704 (Postscript, 39kB)]
[
Mrk 704 (ASCII table, 1.5kB)]
- [
Mrk 817 (Postscript, 49kB)]
[
Mrk 817 (ASCII table, 4.1kB)]
- Format of Data:
- Column 1: JD - 2400000
- Column 2: Continuum flux (at approximately 5100 Å
in the rest frame of the object) in units of
10-15 ergs s-1 cm-2 Å-1.
- Column 3: Uncertainty in continuum flux, same units.
- Column 4: Hbeta flux in units of
10-13 ergs s-1 cm-2.
- Column 5: Uncertainty in Hbeta flux, same units.
Here is a finder chart for the comparison star sequence around
NGC 5548, from Penston, Penston, and Sandage (1972, PASP, 83, 783),
from the Palomar Sky Survey (© National Geographic Society -
Palomar Observatory Sky Survey). North is up, east is to
the left. The size of the field shown is approximately
24 arcminutes N-S and 20 arcminutes E-W.
[OSU Astronomy Home Page]
[Brad Peterson's Home Page]
Updated 3 July 2006
peterson@astronomy.ohio-state.edu