Discovering a celestial object using a non-parametric algorithm

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7886

Full metadata record

DC Field	Value	Language
dc.contributor.author	Vyasanakere, Jayanth P	-
dc.contributor.author	Bhatnagar, Siddharth	-
dc.contributor.author	Murthy, J	-
dc.date.accessioned	2021-12-16T04:06:15Z	-
dc.date.available	2021-12-16T04:06:15Z	-
dc.date.issued	2021-12	-
dc.identifier.citation	Pramana Journal of Physics, Vol. 95, No. 4, 192	en_US
dc.identifier.issn	0304-4289	-
dc.identifier.uri	http://hdl.handle.net/2248/7886	-
dc.description	Restricted Access	en_US
dc.description	The original publication is available at springerlink.com	-
dc.description.abstract	We describe a method that does not use any orbital parameters, to arrive at the position and mass of a new celestial object, using high-precision orbital state vector data of the rest of the objects in the system. As an illustration of this approach, we rediscover Neptune with remarkable accuracy.	en_US
dc.language.iso	en	en_US
dc.publisher	Springer	en_US
dc.relation.uri	https://doi.org/10.1007/s12043-021-02238-2	-
dc.rights	© Indian Academy of Sciences	-
dc.subject	Non-parametric algorith	en_US
dc.subject	Neptune	en_US
dc.subject	iteration method	en_US
dc.title	Discovering a celestial object using a non-parametric algorithm	en_US
dc.type	Article	en_US
Appears in Collections:	IIAP Publications

Files in This Item:

File	Description	Size	Format
Discovering a celestial object using a non-parametric algorithm.pdf Restricted Access		549.21 kB	Adobe PDF	View/Open Request a copy

DSpace JSPUI