UT May 09, 2021: Photometry of AM CVn

Michael Richmond
May 14, 2021

On the night of May 08/09, 2021, under fair conditions, I acquired images of the cataclysmic variable star AM CVn. One can find information about it at


AM CVn

Joe Patterson of the CBA requested data on this star, so I gave it a try. The star is at the faint limit for time series photometry with our equipment, but I wanted to test it.

The main setup was:

Notes from the night:

The object is located at



  RA =  12 34 54.6   Dec = +37 37 44.1   (J2000)

A chart of the field is shown below. The size of the chart is about 19 x 26 arcminutes.

I've marked the location of several comparison stars as well.



  star       AAVSO               B          V          
-----------------------------------------------------------

   A        APASS 8699612      12.226     11.639        

   B        APASS 8699621      12.952     12.290        

-----------------------------------------------------------

 

I took a photo of the finder TV's screen when pointing to this target; this could be a useful reference for the future:

The sky value shows that the sky was clear. The discontinuity is due to the change in exposure time.

The FWHM; some of the changes in direction coincide with my adjustments to the focuser's position -- but the direction of the change due to adjustment is not always towards smaller values. Strange.

Using aperture photometry with a radius of 7 pixels in a clear filter (binned 2x2, each pixel is 1.24 arcsec, so a radius of 8.7 arcsec) for all exposures, I measured the instrumental magnitudes of a number of reference stars and the target. 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.

Sigma-vs-mag plots show that the floor was about 0.008 mag for 60-second exposures.

The image-to-image zeropoint shows the period of clouds early.

Here is the light curve of the object and several field stars in the clear filter; I've shifted the instrumental magnitudes so that star "B" = APASS 8699621 has the value given by APASS as its V-band magnitude.

A periodogram -- thanks to the NASA Exoplanet Archive tool! -- shows a strong peak at the known 525-second (= 0.006076 day) period.

You can download my measurements below. A copy of the header of the file is shown to explain the format.

# Measurements of AM_CVn made at RIT Obs, UT 2021 May 9, 
#    in fair conditions, 
#    by Michael Richmond, 
#    using Meade 12-inch LX200 and ATIK 11000. 
# Exposures 60 seconds long, clear filter. 
# Tabulated times are midexposure (FITS header time - half exposure length) 
#    and accurate only to +/- 1 second (??). 
# 'mag' is a differential magnitude based on ensemble photometry 
#    using a circular aperture of radius 7 pix = 8.7 arcseconds.  
#    which has been shifted so APASS_8699621 has mag=12.29 
#    which is its V-band magnitude according to APASS.  
# 
# UT_day             JD            HJD        mag    uncert
May09.07311     2459343.57311  2459343.57556  13.891  0.020 
May09.07397     2459343.57397  2459343.57642  13.867  0.021 


Last modified 5/14/2021 by MWR.