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              <text>AstroSat's view of 4U 1735-44: spectral, temporal, and type I X-ray burst studies</text>
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              <text>accretion, accretion discs; stars: neutron; X-rays: binaries; X-rays: bursts; X-rays: individual: 4U 1735-44</text>
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              <text>This study utilizes the simultaneous broad-band observations of 4U 1735-44 from AstroSat, offering enhanced spectral and temporal resolution, to investigate its spectral properties, temporal behaviour, and burst characteristics. Spectral, type I X-ray burst, and temporal analyses on 4U 1735-44 were performed using AstroSat/Soft X-ray Telescope and Large Area X-ray Proportional Counter (LAXPC) observations. The hardness-intensity diagram from LAXPC-20 showed a positive correlation between hardness and intensity, with a pattern resembling the banana branch typical of atoll sources. Spectral analysis carried out in the 0.7-20.0 keV energy range, using the model combination - (), suggested a cool accretion disc truncated at a large distance from the neutron star in the system. Time-resolved spectral studies of two type I X-ray bursts detected from the source revealed evidence of photospheric radius expansion, allowing for an estimation of the source distance. Temporal analysis showed the presence of low-frequency quasi-periodic oscillation at 69 Hz (3.3 significance with more than 99 per cent confidence) and prominent noise features below 30 Hz.   2024 The Author(s).</text>
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              <text>Lavanya S.; Thomas N.T.; Gudennavar S.B.; Bubbly S.G.</text>
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              <text>Monthly Notices of the Royal Astronomical Society, Vol-534, No. 3, pp. 2783-2794.</text>
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              <text>Oxford University Press</text>
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              <text>2024-01-01</text>
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              <text>&lt;a href="https://doi.org/10.1093/mnras/stae2269" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1093/mnras/stae2269&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85207091974&amp;amp;doi=10.1093%2Fmnras%2Fstae2269&amp;amp;partnerID=40&amp;amp;md5=e95d2aa2421850fb675754c0f63cbc93" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85207091974&amp;amp;doi=10.1093%2fmnras%2fstae2269&amp;amp;partnerID=40&amp;amp;md5=e95d2aa2421850fb675754c0f63cbc93&lt;/a&gt;</text>
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              <text>All Open Access; Gold Open Access</text>
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              <text>ISSN: 358711; CODEN: MNRAA</text>
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              <text>Lavanya S., Department of Physics and Electronics, CHRIST University, Karnataka, Bangalore, 560029, India; Thomas N.T., Department of Physics and Electronics, CHRIST University, Karnataka, Bangalore, 560029, India; Gudennavar S.B., Department of Physics and Electronics, CHRIST University, Karnataka, Bangalore, 560029, India; Bubbly S.G., Department of Physics and Electronics, CHRIST University, Karnataka, Bangalore, 560029, India</text>
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