The XinJiang astronomical observatory NSRT pulsar data archive

The sensitivity of our pulsar observation system with typical integration time of 16 minutes has reached 0.4 mJy after we have upgraded the receiver cooling system of NanShan 25-m radio telescope (NSRT) at Xinjiang Astronomical Observatory (XAO) in 2002. About 280 pulsars were observed after the upg...

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Bibliographic Details
Main Authors: Zhang, Hailong (Author) , Demleitner, Markus (Author)
Format: Article (Journal)
Language:English
Published: 23 January 2019
In: Advances in astronomy

ISSN:1687-7977
DOI:10.1155/2019/5712682
Online Access:Verlag, Volltext: http://dx.doi.org/10.1155/2019/5712682
Verlag: https://www.hindawi.com/journals/aa/2019/5712682/
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Author Notes:Hailong Zhang, Markus Demleitner, Jie Wang, Na Wang, Jun Nie, and Jianping Yuan

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520 |a The sensitivity of our pulsar observation system with typical integration time of 16 minutes has reached 0.4 mJy after we have upgraded the receiver cooling system of NanShan 25-m radio telescope (NSRT) at Xinjiang Astronomical Observatory (XAO) in 2002. About 280 pulsars were observed after the upgrade. The NanShan station pulsar data is transmitted to the data center at XAO headquarters via a 300Mb/s dedicated data link for long-term storage, and the remote backup is realized by synchronous data transmission between NanShan station and XAO headquarters. Metadata extraction, archiving, and releasing are completed by the data release servers which are located in XAO headquarters. At present, more than 84000 pulsar observation data files in the PSRFITS format have been released with a maximum file size of 1GB. XAO pulsar data online service provides cone search and multiobject constraint query. We have published our data based on Virtual Observatory (VO) standards. The online pulsar data service is registered in the International Virtual Observatory Alliance’s Registry. Users can access the data through common VO tools. 
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