A.R.A.S Spectral  Data Base
                             
 
   
  Number of spectra   8 Name Nova Sgr 2016d       Conditions for use of data in publications  
  First Spectrum   27/10/2016 Group Eruptive Stars         Please read    
  Last Spectrum   18/11/2016 Sub Group Novae                  
            = ASASSN-16ma         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 27/10/2016 11:18 2457688.992 PJL SPO-AU RC14+Alpy600+At 525 3800 7200 3618 asdb_novasgr2016d_20161027_471.fit       v plot
  2 28/10/2016 11:09 2457689.989 PJL SPO-AU RC14+Alpy600+At 529 3750 7399 4221 asdb_novasgr2016d_20161028_465.fit       v plot
  3 30/10/2016 11:26 2457691.998 PJL SPO-AU RC14+Alpy600+At 533 3750 7399 3618 asdb_novasgr2016d_20161030_477.fit       v plot
  4 01/11/2016 12:08 2457694.02 PJL SPO-AU RC14+Alpy600+At 522 3750 7399 2481 asdb_novasgr2016d_20161101_506.fit       v plot
  5 09/11/2016 11:51 2457701.997 PJL SPO-AU RC14+Alpy600+At 536 3750 7399 482 asdb_novasgr2016d_20161109_494.fit       v plot
  6 09/11/2016 12:14 2457702.017 PJL SPO-AU RC14 + LhiresIII + Atik314 8867 4804 4952 1202 asdb_novasgr2016d_20161109_510.fit       v plot
  7 12/11/2016 11:34 2457704.985 PJL SPO-AU RC14+Alpy600+At 541 3700 7400 482 asdb_novasgr2016d_20161112_482.fit       v plot
  8 18/11/2016 11:48 2457710.996 PJL SPO-AU RC14+Alpy600+At 530 3750 7380 634 asdb_novasgr2016d_20161118_492.fit       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