ARIES Insitutional Digital Repositary (ARIES-IDR): Recent submissions

  • Pandey, S. B., ... et al. (2003)
    The CCD magnitudes in Hohnson B, V and Cousins R and I photometric passbands are determined for the bright long duration GRB 021004 afterglow from 2002 October 4 to 16 starting ~ 3 hours after the γ-ray burst. Light curves ...
  • Singh, M.; Sanwal, B. B.; Stalin, C. S. (2000)
    We present here the results from B and V photometric observations of the Wolf Rayet galaxy Mink which was observed through the 104 cm telescope of U. P. State Observatory using 1K × 1K CCD. The surface brightness profiles ...
  • Masetti, N,. ...et al. (including Pandey, S. B. & Sagar, R.) (2003)
    We report on photometric, spectroscopic and polarimetric monitoring of the optical and near-infrared (NIR) afterglow of GRB020405. Ground-based optical observations, performed with 8 different telescopes, started about 1 ...
  • Yadav, R. K. S.; Sagar, R. (2003)
    We report the first deep UBVRI CCD photometry of 2460 stars in the field of two poorly studied OB associations Bochum 1 and Bochum 6. We selected 15 and 14 probable members in Bochum 1 and Bochum 6 respectively using ...
  • Gopal-Krishna; Gupta, A. C.; Sagar, R.; Wiita, P. J.; Chaubey, U. S.; Stalin, C. S. (2000)
    We report results of the observations at the Vainu Bappu Observatory and the Uttar Pradesh State Observatory of eight radio-quiet quasi-stellar objects (RQQSOs) during 1996-99. This is a part of our ongoing programme to ...
  • Stalin, C. S. (2003)
    This thesis explores mainly the problem of the radio loudness dichotomy in quasars. This is addressed by carrying out an extensive search for intra-night optical variability (INOV) in seven sets of optically luminous ...
  • Rautela, B. S.; Joshi, G. C.; Srivastava, J. B. (2000)
    Haser Model production rates of CN and C₂ in the coma of the comet Hale-Bopp (C/1995 O1) have been obtained. Molecular production rate, size of the nucleus and continuum flux at 484.0 nm have further been analyzed to get ...
  • Uddin, W.; Joshi, B.; Chandra, R.; Joshi, A. (2003)
    In this paper we present the analysis of M 1.8 class (GOES SXR) limb flare and associated post flare loops of 2 May, 2001 which erupted on the west limb in NOAA 9433 (N15, W88). The flare started at around 00:32 UT from a ...
  • Yadav, R. K. S. (2003)
    We present a detailed study of four young open star clusters and two OB associations using deep CCD UBVRI and 2MASS JHK measurements. Physical parameters of the clusters have been estimated using optical as well as near ...
  • Pandey, J. C. (2003)
    Optical photometric and spectroscopic studies of the star FR Cnc = BD + 16 1753 have been carried out during the years 2001-2002. The rapid changes in the shape of light curve can be attributed to the formation and ...
  • Pandey, A. K. (2003)
    Observational evidences indicate that the formation of open star clusters has been efficient throughout the life of our Galaxy. As a consequence, we find open clusters with ages ranging from a few Myr to few Gyr. This makes ...
  • Pandey, S. B.; Sahu, D. K.; Anupama, G. C.; Bhattacharya, D.; Sagar, R. (2003)
    The supernova SN2002ap was discovered in the outer regions of the nearby spiral M74 on January 29.4 UT. Early photometric and spectroscopic observations indicate the supernova belongs to the class of Ic hypernovae SN 1997ef ...
  • Lachowicz, P.; Gupta, A. C.; Gaur, H.; Wiita, P. J. (2009)
    We report a possible detection of an ̴4.6-h quasi-periodic oscillation (QPO) in the 0.3–10 keV emission of the high-energy peaked blazar PKS 2155−304 from a 64 ks observation by the XMM-Newton EPIC/pn detector. We identify ...
  • Verma, V. K.; Vats, H. O. (2003)
    In the paper, we present a study of three homologous Hα flares observed on 12th June 2000 in active region (AR) NOAA 9033. During the observation of AR NOAA 9033 on 12th June 2000, we observed 1st solar flare between ...
  • Pandey, A. K.; Upadhyay, K.; Ogura, K.; Sagar, R. (2003)
    A deep and wide field CCD photometry of the young open cluster NGC 663 has been carried out. We report preliminary results of our investigations, specifically the determination of the cluster mass function which is found ...
  • Joshi, Y. C.; Pandey, A. K.; Narasimha, D.; Sagar, R. (2003)
    M 31 has been a promising target to search for microlensing events. Consequently a number of groups have started observations towards this galaxy, however, analyzing the observations in the large background of unresolved ...
  • Lata, S.; Mohan, V.; Pandey, A. K.; Sagar, R. (2004-07)
    We present the broad band Johnson UBV and Cousins RI CCD photometric observations for open clusters Be 10, Be 67 and To 5. So far no photometric study of these clusters in published. The colour-magnitude diagrams indicate ...
  • Sanwal, B. B.; Kumar, B.; Singh, M. (2004-03)
    The 1.2-m Schmidt telescope at IIalcakala found a comet on November 6, 2002 during the Near Earth Asteroid Tracking (NEAT)and it was reported by S.II.Pravdo. At the time of discovery its magnitude was around 17.3. Several ...
  • Rautela, B. S.; Joshi, G. C.; Pandey, J. C. (2004-09)
    An Imaging Polarimeter has been fabricated for use with liquid- N2 cooled CCD camera and is designed to suit 104-cm Sampurnanand telescope with an f/13 focus at Aryabhatta Research Institute of Observational ...
  • Lata, S. (2005-06)
    In the Present study, we have used the CCD data to determine the luminosity and mass function of six open clusters. Members of clusters are identified using photometric and statistical criteria. From these members, er have ...

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