A.R.A.S Spectral  Data Base
                       
  Number of spectra   8 Name Nova Aql 2015       Conditions for use of data in publications  
  First Spectrum   08/10/2015 Group Eruptive Stars       Please read   ARAS Data Base
  Last Spectrum   17/11/2015 Sub Group Novae               Novae
                        List of Observers        
                  send spectra to : francoismathieu.teyssier [at] bbox.fr    
  Start Mid Download : Right click on file and Choose "Save As"
  # Date Time (UT) J.D. Observer Site Instrument Resolution l_min l_max Exposure (s) File Flux Zip Serie Validation
 
    07/10/2015 21:46 2457303.409 HBO SAT-FR SC11+LISA 586 3880 7900 360 asdb_v1831aql_20151007_907.fit        
  1 08/10/2015 22:00 2457304.424 HBO SAT-FR SC11+LISA 560 3882 7900 1203 asdb_v1831aql_20151008_917.fit       v
  2 09/10/2015 18:37 2457305.301 HBO SAT-FR SC11+LISA 574 4000 7897 4232 asdb_v1831aql_20151009_776.fit       v
  3 11/10/2015 18:41 2457307.323 SOL AQL-IT Slit_specC8ST-830   4000 8100 7631 asdb_novaaql2015_20151011_779.fit       v
  4 11/10/2015 18:53 2457307.334 BER BVO-IT SC9+LIRESIII600 3271 7852 8859 8081 asdb_v1831aql_20151011_787.fit       v
  5 11/10/2015 19:58 2457307.333 HBO SAT-FR SC11+LISA 532 3900 7901 3600 asdb_v1831aql_20151011_833.fit       v
  6 15/10/2015 21:02 2457311.391 HBO SAT-FR SC11+LISA 496 4000 7901 2413 asdb_novasgr2_20151015_877.fit       v
  7                             v
  9 17/11/2015 16:59 2457344.216 SOL AQL-IT Alpy600C8ST-8300 3000 3730 7900 1456 asdb_v1831aql_20151017_777.fit       v
                                 
 
 
 
       
 
 
 
 
 
       
  Conditions for use of data in publications    
  Note there is a first level validation check prior to adding spectra to this table. Users should verify the quality of the spectra with the observers concerned.    
  Use of these data in research publications is encouraged subject to the following conditions:    
  * The observers concerned should be contacted to confirm the particular acquisition and data reduction procedures used.    
  * Observers contributing  should be aknowledged    
  * Observers contributing a significant amount of data or whose data are pivotal to the findings of the paper should be included as co-authors.    
  Please contact François Teyssier    
  francoismathieu.teyssier [at] bbox.fr    
  before submitting the publication