Index of /ogle/ogle4/NOVAE

[ICO]NameLast modifiedSizeDescription
[PARENTDIR]Parent Directory  -  
[DIR]BLG/2015-05-01 10:31 -  
[DIR]MC/2015-11-19 21:56 -  
[ ]V3890_Sgr_V.dat2014-06-30 12:08 48  
[ ]V5590_Sgr_V.dat2014-06-30 12:08 528  
[TXT]README2014-07-18 21:06 1.8K 
[ ]OGLE-2011-BLG-1444_V.dat2014-06-30 12:08 1.8K 
[ ]V745_Sco_V.dat2014-06-30 12:08 1.9K 
[ ]V3890_Sgr_I.dat2014-06-30 12:08 2.3K 
[ ]LMC1990b_V.dat2014-06-30 12:08 2.7K 
[ ]LMC1990b_I.dat2014-06-30 12:08 14K 
[ ]V5590_Sgr_I.dat2014-06-30 12:08 16K 
[ ]OGLE-2011-BLG-1444_I.dat2014-06-30 12:08 33K 
[ ]V745_Sco_I.dat2014-06-30 12:08 37K 
========================================================================
             The Optical Gravitational Lensing Experiment.
            Recurrent and symbiotic novae in the OGLE data

     P. Mroz, R. Poleski, A. Udalski, I. Soszynski, M.K. Szymanski, 
  M. Kubiak, G. Pietrzynski, L. Wyrzykowski, K. Ulaczyk, S. Kozlowski,  
                    P. Pietrukowicz, and J. Skowron

========================================================================
pmroz@astrouw.edu.pl


This directory contains the time series I- and V-band photometry
of recurrent and symbiotic novae observed in the OGLE sky survey.

The directory structure is as follows:

README                   - this file

LMC1990b_I.dat           - I-band photometry of Nova LMC 1990b
LMC1990b_V.dat           - V-band photometry of Nova LMC 1990b
OGLE-2011-BLG-1444_I.dat - I-band photometry of OGLE-2011-BLG-1444
OGLE-2011-BLG-1444_V.dat - V-band photometry of OGLE-2011-BLG-1444
V745_Sco_I.dat           - I-band photometry of V745 Sco
V745_Sco_V.dat           - V-band photometry of V745 Sco
V5590_Sgr_I.dat          - I-band photometry of V5590 Sgr
V5590_Sgr_V.dat          - V-band photometry of V5590 Sgr
V3890_Sgr_I.dat          - I-band photometry of V3890 Sgr
V3890_Sgr_V.dat          - V-band photometry of V3890 Sgr


Format of the photometry files:
------------------------------------------------------------------------
 Bytes  Format Units   Description
------------------------------------------------------------------------
  1- 10  F10.5 d       HJD-2450000.0
 12- 17  F6.3  mag     Brightness
 19- 23  F5.3  mag     Photometric uncertainty
------------------------------------------------------------------------

PLEASE cite the following paper when using the data or referring 
to these OGLE results:

Mroz et al. 2014, MNRAS 443, 784