A.R.A.S Spectral  Data Base
                             
 
   
  Number of spectra   25 Name Nova Car 2018       Conditions for use of data in publications  
  First Spectrum   21/03/2018 Group Eruptive Stars         Please read    
  Last Spectrum   19/05/2018 Sub Group Novae                  
            =  ASASSN-18fv         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 21/03/2018 11:45 2458198.994 PJL SPO-AU RC14+Alpy600+At 540 3800 7398 614 asdb_asassn-18fv_20180321_490.fit       v plot
  2 22/03/2018 11:00 2458199.973 BHE MEL-AU C11Lhires#22+600A 1444 3891 4618 2407 asdb_asassn-18fv_20180322_459.fit       v plot
  3 22/03/2018 11:48 2458199.999 BHE MEL-AU C11Lhires#22+600A 1795 6513 6998 1203 asdb_asassn-18fv_20180322_492.fit       v plot
  4 22/03/2018 11:55 2458200.001 PJL SPO-AU RC14+Alpy600+At 534 3700 7398 617 asdb_asassn-18fv_20180322_497.fit erg/cm^2/s/A     v plot
  5 22/03/2018 12:18 2458200.02 BHE MEL-AU C11Lhires#22+600A 1620 6038 6762 1202 asdb_asassn-18fv_20180322_513.fit       v plot
  6 23/03/2018 11:03 2458200.982 BHE MEL-AU C11Lhires#22+600A 1261 4613 5342 3612 asdb_asassn-18fv_20180323_461.fit       v plot
  7 24/03/2018 10:37 2458201.954 BHQ ARM-AU LHIRESC1135umsli 14592 6499 6669 1917 asdb_asassn-18fv_20180324_443.fit       v plot
  8 25/03/2018 10:25 2458202.945 BHQ ARM-AU LHIRESC1135umsli 15022 6498 6668 1808 asdb_asassn-18fv_20180325_434.fit       v plot
  9 26/03/2018 10:32 2458203.949 BHQ ARM-AU LHIRESC1135umsli 14335 6498 6668 1807 asdb_asassn-18fv_20180326_439.fit       v plot
  10 27/03/2018 12:05 2458205.011 PJL SPO-AU RC14+Alpy600+At 535 3700 7398 1249 asdb_asassn-18fv_20180327_504.fit erg/cm^2/s/A     v plot
  11 27/03/2018 13:42 2458205.088 PJL SPO-AU RC14+LhiresIII+ 15266 6476 6631 3020 asdb_asassn-18fv_20180327_571.fit       v plot
  12 28/03/2018 10:58 2458205.961 BHQ ARM-AU LHIRESC1135umsli 13107 6189 6373 600 asdb_asassn-18fv_20180328_458.fit       v plot
  13 28/03/2018 11:12 2458205.974 BHQ ARM-AU LHIRESC1135umsli 14719 6500 6669 1203 asdb_asassn-18fv_20180328_467.fit       v plot
  14 28/03/2018 12:11 2458206.026 PJL SPO-AU RC14+LhiresIII+ 15242 6476 6631 3046 asdb_asassn-18fv_20180328_508.fit       v plot
  15 29/03/2018 10:30 2458206.949 BHQ ARM-AU LHIRESC1135umsli 14403 6502 6669 1807 asdb_asassn-18fv_20180329_438.fit       v plot
  16 30/03/2018 10:05 2458207.931 BHQ ARM-AU LHIRESC1135umsli 14868 6500 6669 1807 asdb_asassn-18fv_20180330_421.fit       v plot
  17 30/03/2018 10:58 2458207.961 BHQ ARM-AU LISAC11Atik314L+ 1406 3800 7245 656 asdb_asassn-18fv_20180330_458.fit       v plot
  18 01/04/2018 10:58 2458209.968 BHQ ARM-AU LHIRESC1135umsli 14641 6500 6669 1807 asdb_asassn-18fv_20180401_457.fit       v plot
  19 03/04/2018 11:53 2458212.000 PJL SPO-AU RC14+Alpy600+At 536 3706 7392 667 asdb_asassn-18fv_20180403_496.fit       v plot
  20 03/04/2018 12:14 2458212.028 PJL SPO-AU RC14+LhiresIII+ 15787 6476 6631 3024 asdb_asassn-18fv_20180403_510.fit       v plot
21 09/04/2018 10:19 2458217.941 BHQ ARM-AU LHIRESC1135umsli 15387 6500 6669 1807 asdb_asassn-18fv_20180409_430.fit       v plot
  22 11/04/2018 12:00 2458220.011 BHQ ARM-AU LHIRESC1135umsli 15251 6502 6669 1807 asdb_asassn-18fv_20180411_501.fit       v plot
  23 30/04/2018 11:48 2458239.003 BHQ ARM-AU LHIRESC1135umsli 14722 6502 6669 1807 asdb_asassn-18fv_20180430_492.fit       v plot
  24 09/05/2018 12:17 2458248.019 BHQ ARM-AU LHIRESC1135umsli 17851 6500 6669 1203 asdb_asassn-18fv_20180509_512.fit       v plot
  25 19/05/2018 11:04 2458257.968 BHQ ARM-AU LHIRESC1135umsli 14736 6498 6670 1224 asdb_asassn-18fv_20180519_461.fit       v plot
                                   
       
    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