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J/AcA/65/313 One thousand new dwarf novae from the OGLE Survey (Mroz+, 2015)
The following files can be converted to FITS (extension .fit or fit.gz)
table1.dat table2.dat orb_per.dat sh_per.dat cv_xrays.dat cv_vsx.dat
cv_k2c9.dat
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-r--r--r-- 1 cats archive 2210 May 10 2016 cv_k2c9.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 4328 May 15 2016 cv_vsx.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 2067 May 15 2016 cv_xrays.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 1014 May 15 2016 orb_per.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 490 May 15 2016 sh_per.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 126556 Jun 17 2016 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 5508 May 15 2016 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/AcA/65/313 One thousand new dwarf novae from the OGLE Survey (Mroz+, 2015)
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One thousand new dwarf novae from the OGLE Survey.
Mroz P., Udalski A., Poleski R., Pietrukowicz P., Szymanski M.K.,
Soszynski I., Wyrzykowski L., Ulaczyk K., Kozlowski S., Skowron J.
<Acta Astron., 65, 313 (2015)>
=2015AcA....65..313M (SIMBAD/NED BibCode)
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ADC_Keywords: Novae ; Photometry
Keywords: novae, cataclysmic variables - stars: dwarf novae
Abstract:
We present one of the largest collections of dwarf novae (DNe)
containing 1091 objects that have been discovered in the long-term
photometric data from the Optical Gravitational Lensing Experiment
(OGLE) survey. They were found in the OGLE fields toward the Galactic
bulge and the Magellanic Clouds. We analyze basic photometric
properties of all systems and tentatively find a population of DNe
from the Galactic bulge. We identify several dozen of WZ Sge-type DN
candidates, including two with superhump periods longer than 0.09d.
Other interesting objects include SU UMa-type stars with "early"
precursor outbursts or a Z Cam-type star showing outbursts during
standstills. We also provide a list of DNe which will be observed
during the K2 Campaign 9 microlensing experiment in 2016. Finally, we
present the new OGLE-IV real-time data analysis system: CVOM, which
has been designed to provide continuous real time photometric
monitoring of selected CVs.
Description:
Photometric data that were analyzed in this paper were collected in
the course of two phases of the OGLE survey: OGLE-III (2001-2009,
Udalski et al. 2008) and OGLE-IV (since 2010, Udalski et al. 2015).
Additionally, light curves of several dozens of objects are
supplemented by photometry from the OGLE-I (1992-1995, Udalski et al.
1992) and OGLE-II (1997-2000, Udalski et al. 1997). For thirty objects
our photometry spans over twenty years.