Oct 30, 2011 UT: Photometry of SN 2011fe in the morning

Michael Richmond
Oct 30, 2011

On the night of Oct 29/30, 2011, I observed the newly discovered supernova known as PTF 11kly = SN 2011fe in the galaxy M101.

The setup was:

Notes from the night

This is a chart of the field of SN 2011fe, based on a stack of five R-band images. The field of view is about 10 by 8 arcminutes.

The marked objects appear in a list of comparison stars with magnitudes in BVRI, created by the AAVSO. You can find the original at the AAVSO web site; go to the Variable Star Plotter (VSP) area. I've made a simplified ASCII version of the catalog below, or you can look at the AAVSO's original version in a local copy.


#AUID   RA.   Dec.   Label   U   B   V   Rc   Ic   J   H   K   Comments
# Label            RA         Ra(deg)       Dec        Dec(deg)  ID       U    B                 V                  R                 I
000-BKD-527   14:03:49.86 [210.95775d]   54:09:05.8 [54.15161d]   117 x   -   12.268 (0.057)29  11.735 (0.040)29  11.359 (0.048)29  11.006 (0.054)29  -   -   -    
000-BKD-528   14:04:21.68 [211.09033d]   54:19:22.4 [54.32289d]   119 x   -   12.572 (0.068)29  11.948 (0.047)29  11.528 (0.056)29  11.134 (0.063)29  -   -   -    
000-BKD-529   14:02:00.79 [210.50330d]   54:23:15.8 [54.38772d]   128 x   -   13.553 (0.062)29  12.751 (0.031)29  12.253 (0.045)29  11.788 (0.056)29  -   -   -    
000-BKD-530   14:01:55.32 [210.48050d]   54:16:21   [54.27250d]   131 x   -   13.540 (0.064)29  13.094 (0.044)29  12.716 (0.051)29  12.361 (0.056)29  -   -   -    
000-BKD-531   14:02:02.00 [210.50833d]   54:20:43.9 [54.34553d]   133 x   -   14.188 (0.094)29  13.291 (0.057)29  12.772 (0.074)29  12.287 (0.088)29  -   -   -    
000-BKD-532   14:01:49.79 [210.45746d]   54:23:02.7 [54.38408d]   134 x   -   14.187 (0.047)29  13.436 (0.033)29  12.970 (0.049)29  12.534 (0.061)29  -   -   -    
000-BKD-533   14:03:13.67 [210.80696d]   54:15:43.4 [54.26205d]   138 A  -   14.699 (0.091)29  13.801 (0.046)29  13.230 (0.062)29  12.698 (0.074)29  -   -   -    
000-BKD-534   14:02:54.17 [210.72571d]   54:16:29.5 [54.27486d]   140 B   -   14.557 (0.107)29  13.991 (0.074)29  13.581 (0.078)29  13.197 (0.083)29  -   -   -    
000-BKD-535   14:02:29.54 [210.62308d]   54:16:55.2 [54.28200d]   141 C   -   14.959 (0.102)29  14.100 (0.045)29  13.598 (0.063)29  13.130 (0.077)29  -   -   -    
000-BKD-536   14:02:31.15 [210.62979d]   54:14:03.9 [54.23442d]   146 G   -   15.158 (0.078)29  14.605 (0.029)29  14.204 (0.061)29  13.828 (0.082)29  -   -   -    
000-BKD-540   14:01:50.86 [210.46191d]   54:16:08.1 [54.26892d]   149 x   -   15.373 (0.010)29  14.925 (0.000)29  14.635 (0.006)29  14.361 (0.008)29  -   -   -    
000-BKD-538   14:03:23.74 [210.84892d]   54:14:32.6 [54.24239d]   155 H   -   16.015 (0.042)29  15.475 (0.000)29  15.133 (0.046)29  14.811 (0.065)29  -   -   -    
000-BKD-539   14:03:05.64 [210.77350d]   54:17:26.2 [54.29061d]   162 x   -   16.776 (0.091)29  16.177 (0.000)29  15.640 (0.079)29  15.140 (0.112)29  -   -   -    
#Report this sequence as: 5249bgj in the chart field of your observation report. This table is for a 0.25000° fov around PTF11KLY, RA: 14:03:05.81 (210.77421) & Decl.: 54:16:25.40 (54.27372). 

I measured the instrumental magnitude of each star with aperture photometry, using a radius of 3 pixels = 5.6 arcseconds in B, and a radius of 4 pixels = 7.4 arcseconds in VRI, and sky defined by an annulus around each star. Following the procedures outlined by Kent Honeycutt's article on inhomogeneous ensemble photometry, I used all stars available in each image to define a reference frame, and measured each star against this frame.

Below is a graph of the scatter in differential magnitude versus magnitude in the ensemble solution for the R-band.

Tests over the past week have indicated that, although stars A, B, C, G and H have photometry from the AAVSO, the best results occur when I discard H. It is significantly fainter than the others, and almost always is an outlier from the photometric solution.

Applying the color corrections determined on UT Aug 27 to the ensemble photometry of SN 2011fe and the comparison stars in its field, I find the magnitude of SN 2011fe on this night was

                   
Passband       JD-2,455,000        Mag     +/-   
-------------------------------------------------
   B             864.883          13.31    0.11  
   V             864.895          12.30    0.07  
   R             864.907          12.03    0.06  
   I             864.924          11.83    0.07  
-------------------------------------------------

The uncertainties here are dominated by the photometry of the reference stars; however, the measurements in B-band have low signal-to-noise, and the uncertainties from the measurements are not much less than those due to the calibration.

I have reported these measurements to the AAVSO via their WebObs tool ....

You can find a complete set of the RIT Obs measurements by grabbing the file sn2011fe_mags.out. I've plotted our measurements in two graphs. First, the measurements of SN 2011fe so far:

Second, the new SN compared to another Type Ia SN, SN 1994D in NGC4526. I've shifted the SN 1994D measurements in time and in magnitude so that they sort of match the early observations of SN 2011fe.

These measurements provide additional evidence that the B-band value from UT Oct 24 was a little bit low.


Last modified 10/30/2011 by MWR.