Please use this identifier to cite or link to this item: http://hdl.handle.net/2080/3509
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dc.contributor.authorPandey, Divya-
dc.contributor.authorSaha, Kanak-
dc.contributor.authorPradhan, Ananta C.-
dc.date.accessioned2020-03-03T12:38:49Z-
dc.date.available2020-03-03T12:38:49Z-
dc.date.issued2020-02-
dc.identifier.citation38th Annual Meeting of Astronomical Society of India, IISER, Tirupati, 13 - 17, February 2020en_US
dc.identifier.urihttp://hdl.handle.net/2080/3509-
dc.descriptionCopyright belongs to proceedings publisheren_US
dc.description.abstractBootes void appears to be one of the largest void in the universe $\sim$ 60 Mpc across with mean redshift $\sim$ 0.05. Previous studies suggests that galaxies in voids are star forming, bluer and slowly evolving as compared to field galaxies. We have done multi-wavelength analysis of the galaxies present in Bootes void region using proposed ASTROSAT/UVIT observation aided with SDSS and 2MASS archival imaging data. Analysis based on ultra-violet (UV), optical and infrared colors reveal that most of the galaxies present in Bootes void region are blue and highly star forming. On further investigation, two galaxies were found to be present inside the void along our field of view ($\sim$ 28’).en_US
dc.subjectMultiwavelength Analysisen_US
dc.subjectGalaxiesen_US
dc.subjectBootes Voiden_US
dc.titleMultiwavelength Analysis of Galaxies in Bootes Voiden_US
dc.typeArticleen_US
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