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		题名	作者	年代	出处	被引量
	1	Assessment of the Polyphenolic Composition of the Organic Extracts of Mauritian Black Teas: A Potential Contributor to Their Antioxidant Functions 显示文摘	AMITABY L R VIDUSHI S N THEESHAN B	2006	Bio Factors2006，，27：	1
	2	Performance analysis of an improved dynamic power management model in wireless sensor node显示文摘	Anuradha Pughat Vidushi Sharma	2017	Digital Communications and Networks2017，3，1：	1
	3	Acute pancreatitis in pregnancy: A treatment paradigm based on our hospital experience显示文摘	Sunil Juneja Shweta Gupta Satpal Virk Pooja Tandon Vidushi Bindal	2013	International Journal of Applied and Basic Medical Research2013，，2：	1
	4	Effect of oral contraceptive containing ethinyl estradiol combined with drospirenone vs. desogestrel on clinical and biochemical parameters in patients with polycystic ovary syndrome显示文摘	Alka Kriplani Anurekha Janaki Periyasamy Nutan Agarwal Vidushi Kulshrestha Anand Kumar Ariachery Chinnama Ammini	2010	Contraception2010，，2：	1
	5	Serrated adenoma is a risk factor for subsequent adenomatous polyps显示文摘	Emily Glazer Vidushi Golla Robin Forman	2008	Dig Dis Sci2008，53，：	1
	6	Utilization of Platelet Count Spleen Diameter Ratio in Predicting the Presence of Esophageal Varices in Patients With Cirrhosis显示文摘	Elliot Schwarzenberger Trinh Meyer Vidushi Golla Nicole Pena Sahdala Albert D. Min	2010	Journal of Clinical Gastroenterology2010，，2：	1
	7	Magnetar giant flare originating from GRB 200415A:transient GeV emission, time-resolved E_(p)-L_(iso) correlation and implications显示文摘Giant flares(GFs)are unusual bursts from soft gamma-ray repeaters(SGRs)that release an enormous amount of energy in a fraction of a second.The afterglow emission of these SGR-GFs or GF candidates is a highly beneficial means of discerning their composition,relativistic speed and emission mechanisms.GRB 200415A is a recent GF candidate observed in a direction coincident with the nearby Sculptor galaxy at 3.5 Mpc.In this work,we searched for transient gamma-ray emission in past observations by Fermi-LAT in the direction of GRB 200415A.These observations confirm that GRB 200415A is observed as a transient GeV source only once.A pure pair-plasma fireball cannot provide the required energy for the interpretation of GeV afterglow emission and a baryonic poor outflow is additionally needed to explain the afterglow emission.A baryonic rich outflow is also viable,as it can explain the variability and observed quasi-thermal spectrum of the prompt emission if dissipation is happening below the photosphere via internal shocks.Using the peak energy(Ep)of the time-resolved prompt emission spectra and their fluxes(Fp),we found a correlation between Ep and Fp or isotropic luminosity Liso for GRB 200415A.This supports the intrinsic nature of Ep-Liso correlation found in SGRs-GFs,hence favoring a baryonic poor outflow.Our results also indicate a different mechanism at work during the initial spike,and that the evolution of the prompt emission spectral properties in this outflow would be intrinsically due to the injection process.	Vikas Chand Jagdish C.Joshi Rahul Gupta Yu-Han Yang Dimple Vidushi Sharma Jun Yang Manoneeta Chakraborty Jin-Hang Zou Lang Shao Yi-Si Yang Bin-Bin Zhang Shashi Bhushan Pandey Ankush Banerjee Eman Moneer	2021	Research in Astronomy and Astrophysics2021，21，9：	0

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