A.R.A.S Spectral  Data Base
                             
 
   
  Number of spectra   7 Name Nova Lup 2018       Conditions for use of data in publications  
  First Spectrum   29/06/2018 Group Eruptive Stars         Please read    
  Last Spectrum   06/09/2018 Sub Group 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 Plot
                                 
  1 29/06/2018 13:06 2458299.053 PJL SPO-AU RC14+Alpy600+At 531 3790 7390 1229 asdb_novalup2018_20180629_546.fit       v plot
  2 06/07/2018 12:08 2458306.02 PJL SPO-AU RC14+Alpy600+At 524 3800 7300 2411 asdb_novalup2018_20180706_506.fit       v plot
  3 17/07/2018 11:34 2458316.987 BHQ ARM-AU LISAC11ASI183MM2 1618 3800 7380 917 asdb_novalup2018_20180717_482.fit       v plot
  4 19/07/2018 12:18 2458319.027 PJL SPO-AU RC14+Alpy600+At 524 3800 7300 2418 asdb_novalup2018_20180719_513.fit       v plot
  5 20/08/2018 11:06 2458350.97 BHQ ARM-AU LISAC11ASI183MM2 1681 3800 7340 1226 asdb_novalup2018_20180820_463.fit erg/cm^2/s/A     v plot
  6 27/08/2018 11:40 2458357.992 BHQ ARM-AU LOWRESC11Atik314L 5653 5950 6859 904 asdb_novalup2018_20180827_487.fit       v plot
  7 06/09/2018 10:21 2458367.938 BHQ ARM-AU LISAC11ASI183MM2 1331 3800 7301 993 asdb_novalup2018_20180906_432.fit erg/cm^2/s/A     v plot
                                   
                                   
  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.      
  *ARAS group should be aknowledege with a reference to the database      
  Please contact François Teyssier      
  francoismathieu.teyssier [at] bbox.fr      
  before submitting the publication