A near-infrared stellar spectral library: III. J-band spectra

dc.contributor.authorRanade, Arvind C
dc.contributor.authorAshok, N.M
dc.contributor.authorSingh, Harinder P
dc.date.accessioned2012-08-01T11:22:30Z
dc.date.available2012-08-01T11:22:30Z
dc.date.issued2007-09-03
dc.description.abstractThis paper is the third in the series of papers published on near- infrared (NIR) stellar spectral library by Ranade et al. (2004 & 2007). The observations were carried out with 1.2 meter Gurushikhar Infrared Telescope (GIRT), at Mt. Abu, India using a NICMOS3 HgCdTe 256 £ 256 NIR array based spectrometer. In paper I (Ranade et al. 2004), H-band spectra of 135 stars at a resolution of » 16 ºA & paper II (Ranade et al. 2007), K band spectra of 114 stars at a resolution of » 22 ºA were presented. The J-band library being released now consists of 126 stars covering spectral types O5{ M8 and luminosity classes I{V. The spectra have a moderate resolution of » 12:5 ºA in the J band and have been continuum shape corrected to their respective e®ective temperatures. The complete set of library in near-infrared (NIR) will serve as a good database for researchers working in the ¯eld of stellar population synthesis. The complete library in J, H & K is available online at: http://vo.iucaa.ernet.in/»voi/NIR Header.htmlen_US
dc.identifier.urihttp://hdl.handle.net/11007/1935
dc.language.isoenen_US
dc.publisherBull. Astr. Soc. Indiaen_US
dc.subjectAstronomical databasesen_US
dc.subjectatlases - techniquesen_US
dc.subjectSpectroscopic - instrumentationen_US
dc.subjectSpectrographs - methodsen_US
dc.subjectobServational- infrareden_US
dc.subjectStarsen_US
dc.titleA near-infrared stellar spectral library: III. J-band spectraen_US
dc.typeArticleen_US

Files

Original bundle

Now showing 1 - 1 of 1
No Thumbnail Available
Name:
57.pdf
Size:
384.27 KB
Format:
Adobe Portable Document Format

License bundle

Now showing 1 - 1 of 1
No Thumbnail Available
Name:
license.txt
Size:
1.71 KB
Format:
Item-specific license agreed upon to submission
Description: