B1  UBVRc,i photometry, EE Cep eclipse 1997, Piwnice Obs., 0.6m Cassegrain tel.
B1   Photometry in standard UBVR_C filters and a non-standard 'i'
B1   (lambda_i_~7420{AA}) filter obtained at Piwnice Observatory (Poland) during
B1   and near the 1997 eclipse (E=8). A one-channel photometer with an uncooled
B1   EMI 9558B photomultiplier on the 0.6m Cassegrain telescope was used. The
B1   differential magnitudes are given with respect to standard star BD+55 2690,
B1   together with the corresponding standard deviations.
B1   Observers: D. Graczyk, J. Janowski, M. Mikolajewski.
B2  BV(RI)c photometry, EE Cep eclipse 2003, Athens Obs., 0.4m Cassegrain tel.
B2   Photometry obtained at Athens Observatory (Greece) with standard BV(RI)_C
B2   (Bessell) filters during and near the 2003 eclipse (E=9). The 0.4m
B2   Cassegrain telescope with an SBIG ST8 CCD camera was used. Differential
B2   magnitudes are given with respect to BD+55 2690. Each point is the mean
B2   value obtained from several to tens of frames. The columns labelled 'HJD+'
B2   denote the fraction of the day.
B2   Observers: K. Gazeas, P. Niarchos.
B3  BIc H-alpha photometry, EE Cep eclipse 2003, Bialkow Obs., 0.6m Cassegrain
B3   telescope.
B3   Photometry in standard VI_C filters and wide H-alpha(wide) and narrow
B3   H-alpha(narrow) filters (FWHM~200 and ~30{AA}, respectively)
B3   obtained at Bialkow Observatory (Poland) during and near the 2003 eclipse
B3   (E=9). The 0.6m Cassegrain telescope with a Photometrics Star I CCD
B3   camera was used.
B3   Observers: Z. Kolaczkowski, G. Michalska, A. Pigulski
B4  UBV(RI)c photometry, EE Cep eclipse 2003, Krakow Obs., 0.5m Cassegrain tel.
B4   UBV(RI)_C photometry obtained at Krakow Observatory (Poland) during and
B4   near the 2003 eclipse (E=9). The 0.5m Cassegrain telescope with a
B4   Photometrics CH350 CCD camera was used.
B4   Each point is the mean value obtained from several to tens of frames.
B4   Observers: M. Drahus, M. Kurpinska-Winiarska, A. Majewska, M. Siwak,
B4   W. Waniak, M. Winiarski, S. Zola.
B5  UBV(RI)c photometry, EE Cep eclipse 2003, Kryoneri Obs., 1.2m Cassegrain
B5   telescope.
B5   UBV(RI)_C} photometry obtained at Kryoneri Observatory (Greece) during the
B5   2003 eclipse (E=9). The 1.2m Cassegrain telescope with a CCD camera was
B5   used. Each point is the mean value obtained from several to tens of frames.
B5   Observers: I. Bellas-Velidis, A. Dapergolas.
B6  UBV(RI)c,c,H-beta photometry, EE Cep eclipse 2003, Piwnice Obs., 0.6m
B6   Cassegrain telescope.
B6   Photometry in standard UBV(RI)_C and narrow (FWHM ~100{AA}) 'c'
B6   (continuum at lambda=4804{AA}) and H-beta filters obtained at
B6   Piwnice Observatory (Poland) during and near the 2003 eclipse (E=9). A
B6   one-channel photometer with a cooled Burle C31034 photomultiplier on the
B6   0.6m Cassegrain telescope was used. Differential magnitudes are given with
B6   respect to BD+55 2690, together with the corresponding standard deviations.
B6   Observers: C. Galan, A. Majcher, M. Mikolajewski.
B7  UBV(RI)c photometry, EE Cep eclipse 2003, Rozhen Obs., 2m Ritchey-Chretien
B7   telescope.
B7   UBV(RI)_C photometry obtained at Rozhen Observatory (Bulgaria) during the
B7   2003 eclipse (E=9). The 2m Ritchey-Chretien telescope with a CCD camera
B7   was used.
B7   Observers: M. Gromadzki, D. Kolev.
B8  V photometry, EE Cep eclipse 2003, Rozhen Obs., 0.5/0.7m Schmidt telescope.
B8   Photometry in the V filter obtained at Rozhen Observatory (Bulgaria) during
B8   the 2003 eclipse (E=9). The 0.5/0.7m Schmidt telescope with a CCD
B8   camera was used.
B8   Observers: G. Apostolovska, B. Bilkina, M. Gromadzki, D. Kolev.
B9  UBV photometry, EE Cep eclipse 2003, Rozhen Obs., 0.6m Cassegrain telescope.
B9   UBV photometry obtained at Rozhen Observatory (Bulgaria) during the 2003
B9   eclipse (E=9). The 0.6m Cassegrain telescope with a one-channel
B9   photomultiplier was used.
B9   Observer: D. Dimitrov.
B10 UBV(RI)c photometry, EE Cep eclipse 2003, Skinakas Obs., 1.3m
B10  Ritchey-Chretien telescope
B10  UBV(RI)_C photometry obtained at Skinakas Observatory (Crete, Greece)
B10  during the 2003 eclipse (E=9). The 1.3m Ritchey-Chretien telescope with
B10  a CCD camera was used.
B10  Observer: E. Semkov.
B11 BV(RI)c photometry, EE Cep eclipse 2003, Piszkesteto Obs., 0.6/0.9m Schmidt
B11  telescope.
B11  BV(RI)_C photometry obtained at Piszkesteto Observatory (Hungary) during
B11  the 2003 eclipse (E=9). The 0.6/0.9m Schmidt telescope with an AT200
B11  CCD camera was used. The differential magnitudes are given with respect to
B11  BD+55$ 2690.
B11  Observers: B. Csak, B. Gere, P. Nemeth.
B11  HJD dBmag dVmag dRcmag dIcmag
B12 BV(RI)c photometry, EE Cep eclipse 2008/9, Altan Obs., 0.2m RL Vixen VMC200L
B12  telescope.
B12  BV(RI)_C photometric data obtained at Altan Observatory (Czech Republic)
B12  during the 2008/9 eclipse (E=10). The 0.2 meter RL Vixen VMC200L
B12  telescope with a G2-0402 CCD camera was used. Differential magnitudes are
B12  given with respect to BD+55 2690 together, with the corresponding standard
B12  deviations.
B12  Observer: L. Brat.
B13 BV(RI)c photometry, EE Cep eclipse 2008/9, Bialkow Obs., 0.6m Cassegrain
B13  telescope.
B13  BV(RI)_C photometric data obtained at Bialkow Observatory (Poland) during
B13  the 2008/9 eclipse (E=10). The 0.6m Cassegrain telescope with a CCD
B13  camera was used.
B13  Observers: G. Kopacki, A. Majewska, A. Narwid, E. Niemczura, A. Pigulski,
B13  M. Steslicki
B13  HJD HJD+ dBmag HJD+ dVmag HJD+ dRcmag HJD+ dIcmag
B14 BV(RI)c photometry, EE Cep eclipse 2008/9, Green Island Obs., 0.35m
B14  Ritchey-Chretien telescope.
B14  BV(RI)_C photometric data obtained at Green Island Observatory (North
B14  Cyprus) during the 2008/9 eclipse (E=10). The 0.35m telescope (Meade
B14  14"LX200R ) with a Meade DSI II Pro CCD camera was used. Differential
B14  magnitudes are given with respect to BD+55 2690 together with the
B14  corresponding standard deviations.
B14  Observer: Y. Ougmen.
B15 BV(RI)c photometry, EE Cep eclipse 2008/9, Furzehill House Obs., 0.35m
B15  Schmidt-Cassegrain telescope.
B15  BV(RI)_C photometric data obtained at Furzehill House Observatory (Ilston,
B15  Swansea, United Kingdom) during the 2008/9 eclipse (E 10). The 0.35m
B15  Schmidt-Cassegrain telescope with an SXVF-H16 CCD camera was used.
B15  Differential magnitudes are given with respect to BD+55 2690, together with
B15  the corresponding standard deviations.
B15  Observer: I. Miller.
B16 V photometry, EE Cep eclipse 2008/9, Navas de Oro, Obs., Reflector 0.35m
B16  telescope.
B16  Photometry in the V filter obtained at Observatorio Astronomico "Las
B16  Pegueras" (Navas de Oro, Segovia, Spain) during the 2008/9 eclipse (E=10).
B16  The 0.35m Reflector with a CCD camera was used. Differential
B16  magnitudes are given with respect to GSC 3973-2150 comparison star.
B16  Observer: T. Arranz Heras.
B17 BV(RI)c photometry, EE Cep eclipse 2008/9, Ostrava Obs., 0.3m
B17  Schmidt-Cassegrain telescope.
B17  Photometry obtained at Ostrava Observatory (Czech Republic) with standard
B17  BV(RI)_C filters during the 2008/9 eclipse (E=10). The 0.3m
B17  Schmidt-Cassegrain telescope with a CCD camera has been used.
B17  Observer: R. Kocian.
B18 BV(RI)c photometry, EE Cep eclipse 2008/9, Rozhen Obs., 2m Ritchey-Chretien
B18  telescope.
B18  BV(RI)_C photometry obtained at Rozhen Observatory (Bulgaria) during the
B18  2008/9 eclipse (E=10). The 2m Ritchey-Chretien telescope with a CCD
B18  camera was used.
B18  Observers: S. Peneva, E. Semkov.
B19 UBV(RI)c photometry, EE Cep eclipse 2008/9, Rozhen Obs., 0.5/0.7m Schmidt
B19  telescope.
B19  UBV(RI)_C photometry obtained at Rozhen Observatory (Bulgaria) during and
B19  near the 2008/9 eclipse (E=10). The 0.5/0.7m Schmidt telescope with a
B19  CCD camera was used.
B19  Observers: S. Peneva, E. Semkov.
B20 UBV(RI)c photometry, EE Cep eclipse 2008/9, Rozhen Obs., 0.6m Cassegrain
B20  telescope.
B20  Photometry obtained at Rozhen Observatory (Bulgaria) during the 2008/9
B20  eclipse (E=10) with standard UBV(RI)_C (Bessell) filters. The 0.6m
B20  Cassegrain telescope with a FLI PL09000 CCD camera was used.
B20  Each point is the mean B20 value obtained from several frames.
B20  Observers: D. Dimitrov, V. Popov.
B21 BV(RI)c photometry, EE Cep eclipse 2008/9, Kryoneri Obs., 1.2m Cassegrain
B21  telescope.
B21  BV(RI)_C photometry obtained at Kryoneri Observatory (Greece) at the
B21  beginning of the 2008/9 eclipse (E=10). The 1.2m Cassegrain telescope
B21  with a CCD camera was used.
B21  Observers: I. Bellas-Velidis, A. Dapergolas.
B22 BV(RI)c photometry, EE Cep eclipse 2008/9, Sonoita Res. Obs., 0.5m
B22  Cassegrain telescope.
B22  BV(RI)_C photometry obtained at Sonoita Research Observatory (Arizona, USA)
B22  during and near the 2008/9 eclipse (E=10). The 0.5m Cassegrain
B22  telescope with an SBIG STL 6303 CCD camera was used. Comparisons were made
B22  against two stars designated with the AAVSO Unique Identifiers as:
B22  000-BCQ-040, 000-BJJ-300. The former is a 'd' object from Meinunger's
B22  comparison star sequence (Meinunger 1975). The apparent magnitudes are
B22  also given with respect to BD+55 2690 (calculated with the adoption of
B22  BV(RI)_C magnitudes of BD+55 2690 given in Mikolajewski et al,
B22  2003IBVS.5412....1M.
B22  Observer: B. Staels.
B23 BV(RI)c photometry, EE Cep eclipse 2008/9, Sonoita Res. Obs., 0.5m
B23  Cassegrain telescope.
B23  BV(RI)_C photometry obtained at Sonoita Research Observatory (Arizona, USA)
B23  during and near the 2008/9 eclipse (E=10). The 0.5m Cassegrain
B23  telescope with an SBIG STL 6303 CCD camera was used. The apparent
B23  magnitudes are also given with respect to BD+55 2690 (calculated by
B23  adopting BV(RI)_C magnitudes of BD+55 2690 from Mikolajewski et al.
B23  2003IBVS.5412....1M.
B23  Observers: L. Elder, J. Hopkins, J. Pye.
B24 BV(RI)c photometry, EE Cep eclipse 2008/9, Athens Obs., 0.4m Cassegrain
B24  telescope.
B24  Photometry obtained at Athens Observatory (Greece) with standard BV(RI)_C
B24  (Bessell) filters during and near the 2008/9 eclipse (E=10). The 0.4m
B24  Cassegrain telescope with an SBIG ST-8XMEI CCD camera was used.
B24  Differential magnitudes are given with respect to three comparison stars:
B24  a=BD+55 2690, b=GSC 3973-2150, and c=BD+55 2691. Each point is the
B24  mean value obtained from several frames.
B24  Observers: K. Gazeas, A. Liakos, P. Niarchos.
B25  Photometry obtained at Hankasalmi Observatory (Finland) with standard
B25 BV(RI)c photometry, EE Cep eclipse 2008/9, Hankasalmi Obs., 0.4m RCOS tel.
B25  BV(RI)_C (Bessell) filters during the 2008/9 eclipse (E=10). The 0.4m
B25  RCOS telescope with an SBIG STL-1001 CCD camera was used. Differential
B25  magnitudes are given with respect to three comparison stars:
B25  a=BD+55 B25 2690, b=GSC 3973-2150, and c=BD+55 2691. Each point is the
B25  mean value obtained from several frames.
B25  Observer: A. Oksanen.
B26 BV(RI)c photometry, EE Cep eclipse 2008/9, Ostrava Obs., 0.2m Newton tel.
B26  Photometry obtained at Ostrava Observatory (Czech Republic) with standard
B26  BV(RI)_C filters during the 2008/9 eclipse (E=10). The 0.2m Newton
B26  telescope with an SBIG ST8-XME CCD camera has been used. Differential
B26  magnitudes are given with respect to three comparison stars:
B26  a=BD+55 2690, b=GSC 3973-2150, and c=BD+55 2691. Each point is the mean
B26  value B26 obtained from several frames.
B26  Observer: H. Kucakova.
B27 UBV(RI)c photometry, EE Cep eclipse 2008/9, Krakow Obs., 0.5m Cassegrain
B27  telescope.
B27  UBV(RI)_C photometry obtained at Krakow Observatory (Poland) during and
B27  near the 2008/9 eclipse (E=10). The 0.5m Cassegrain telescope with a
B27  CCD camera was used. The differential magnitudes are given with respect to
B27  three comparison stars: a=BD+55 2690, b=GSC 3973-2150, and c=BD+55 2691.
B27  Each point is the mean value obtained from several to tens of frames.
B27  Observers: E. Kuligowska, T. Kundera, M. Kurpinska-Winiarska, A. Kuzmicz,
B27  T. Szymanski, M. Winiarski, S. Zola.
B28 UBV(RI)c photometry, EE Cep eclipse 2008/9, Tenagra-II Obs., 0.81m
B28  Ritchey-Chretien telescope.
B28  CCD photometry obtained in UBV(RI)_C (Bessel) filters with 0.81m
B28  Tenagra-II telescope in Southern Arizona (USA) during and near the 2008/9
B28  eclipse (E=10). Differential magnitudes are given with respect to three
B28  comparison stars: a=BD+55 2690, b=GSC 3973-2150, and c=BD+55 2691.
B28  Each point is the mean value obtained from several frames.
B28  Observer: T. Lister.
B29 UBV(RI)c photometry, EE Cep eclipse 2008/9, Piwnice Obs., 0.6m Cassegrain
B29  telescope.
B29  UBV(RI)_C photometry obtained at Piwnice Observatory (Poland) during and
B29  near the 2008/9 eclipse (E=10). The 0.6m Cassegrain telescope with SBIG
B29  STL-1001 CCD camera was used. Differential magnitudes are given with
B29  respect to three comparison stars: a=BD+55 2690, b=GSC 3973-2150, and
B29  c=BD+55 2691. Each point is the mean value obtained from several to tens
B29  of frames.
B29  Observers: P. Dobierski, S. Frackowiak, C. Galan, G. Maciejewski,
B29  P. Rozanski, E. Swierczynski, M. Wiecek, P. Wychudzki.
B30 UBV(RI)c photometry, EE Cep eclipse 2008/9, Suhora Obs., 0.6m Cassegrain
B30  telescope.
B30  UBV(RI)_C photometry obtained at Suhora Observatory (Poland) during and
B30  near the 2008/9 eclipse (E=10). The 0.6m Cassegrain telescope with a
B30  CCD camera was used. The differential magnitudes are given with respect to
B30  three comparison stars: a=BD+55 2690, b=GSC 3973-2150, and c=BD+55 2691.
B30  Each point is the mean value obtained from several to tens of frames.
B30  Observers: M. Drozdz, J. Krzesinski, W. Ogloza, M. Siwak, M. Winiarski,
B30  S. Zola.
B31 BVIc photometry, EE Cep eclipse 2008/9, GRAS, Mayhill Obs., 0.3m GRAS-001
B31  telescope.
B31  BVI_C photometry obtained at GRAS Observatory (Mayhill, New Mexico, USA)
B31  during the 2008/9 eclipse (E=10). The 0.3m GRAS-001 Telescope with an
B31  FLI IMG 1024 DM CCD camera was used. Differential magnitudes are given
B31  with respect to three comparison stars: a=BD+55 2690, b=GSC 3973-2150,
B31  and c=BD+55 2691.
B31  Observer: G. Myers.
B32 BV photometry, EE Cep eclipse 2008/9, Rolling Hills Obs., 0.25m (10")
B32  LX200 telescope.
B32  BV photometry obtained at Rolling Hills Observatory (Florida, USA) during
B32  the 2008/9 eclipse (E=10). The 0.25m (10") LX 200 telescope with an
B32  SBIG ST-9XE CCD camera was used. Differential magnitudes are given with
B32  respect to three comparison stars: a=BD+55 2690, b=GSC 3973-2150, and
B32  c=BD+55 2691.
B32  Observer: S. Dvorak.