Search Results - "Antony, Susmitha"

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  1. 1

    Mining the GALAH Data. I. Study of Five Super Lithium-rich Metal-poor Giants by Susmitha, Antony, Mallick, Anohita, Reddy, Bacham E.

    Published in The Astrophysical journal (01-05-2024)
    “…Abstract The presence of a large amount of Li in giants is still a mystery. Most of the super Li-rich (SLR) giants reported in recent studies are in the solar…”
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    Journal Article
  2. 2

    Chemical Composition of Two Bright, Extremely Metal-poor Stars from the SDSS MARVELS Pre-survey by Bandyopadhyay, Avrajit, Sivarani, Thirupathi, Susmitha, Antony, Beers, Timothy C., Giridhar, Sunetra, Surya, Arun, Masseron, Thomas

    Published in The Astrophysical journal (01-06-2018)
    “…SDSS J082625.70+612515.10 (V = 11.4; [Fe/H] = −3.1) and SDSS J134144.60+474128.90 (V = 12.4; [Fe/H] = −3.2) were observed with the SDSS 2.5m telescope as part…”
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  6. 6

    Mining the GALAH data I: Study of five Super lithium-rich metal-poor giants by Susmitha, Antony, Mallick, Anohita, Reddy, Bacham E

    Published 22-03-2024
    “…The presence of a large amount of Li in giants is still a mystery. Most of the super Li-rich giants reported in recent studies are in the solar metallicity…”
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    Journal Article
  7. 7

    A chemodynamical analysis of bright metal-poor stars from the HESP-GOMPA survey -- Indications of a non-prevailing site for light r-process elements by Bandyopadhyay, Avrajit, Beers, Timothy C, Ezzeddine, Rana, Sivarani, Thirupathi, Nayak, Prasanta K, Pandey, Jeewan C, Saraf, Pallavi, Susmitha, Antony

    Published 27-02-2024
    “…Monthly Notices of the Royal Astronomical Society, Volume 529, Issue 3, pp.2191-2207, 2024 We present a comprehensive analysis of the detailed chemical…”
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  8. 8

    Chemical composition of two bright extremely metal-poor stars from the SDSS MARVELS pre-survey by Bandyopadhyay, Avrajit, Thirupathi, Sivarani, Susmitha, Antony, Beers, Timothy C, Giridhar, Sunetra, Surya, Arun, Masseron, Thomas

    Published 06-05-2018
    “…The Adtrophysical Journal(1996-present) \sdsszeroeight\ (V = 11.4; [Fe/H] = $-$3.1) and \sdssonethree\ (V = 12.4; [Fe/H] = $-$3.2) were observed with the SDSS…”
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