Index of /~bessell/FTP/Cohen

 Name                    Last modified      Size  Description
 Parent Directory                             -   
 2007NovDBS.log          18-Dec-2007 15:56  6.0K  
 sp115bf.fits            18-Dec-2007 16:10   17K  
 sp116bf.fits            18-Dec-2007 16:10   17K  
 sp117bf.fits            18-Dec-2007 16:10   17K  
 sp118bf.fits            18-Dec-2007 16:10   17K  
 sp119bf.fits            18-Dec-2007 16:10   17K  
 sp119rf.fits            19-Dec-2007 07:56   17K  
 sp120bf.fits            18-Dec-2007 16:10   17K  
 sp121_6bf.fits          18-Dec-2007 16:10   17K  
 sp121rf.fits            19-Dec-2007 07:56   17K  
 sp123bf.fits            18-Dec-2007 16:10   17K  
 sp123rf.fits            19-Dec-2007 07:56   17K  
 sp124bf.fits            18-Dec-2007 16:10   17K  
 sp125bf.fits            18-Dec-2007 16:10   17K  
 sp125rf.fits            19-Dec-2007 07:56   17K  
 sp127rf.fits            19-Dec-2007 07:56   17K  
 sp129rf.fits            19-Dec-2007 07:56   17K  
 sp131_2rf.fits          19-Dec-2007 07:56   17K  
 sp134rf.fits            19-Dec-2007 07:56   17K  
 sp136rf.fits            19-Dec-2007 07:56   17K  
 spectra.tar.gz          19-Dec-2007 08:09  141K  

The filenames are referenced in the logfile. As the red and blue were 
done on separate nights instead of simultaneously (only one controller
was working), the file numbers are independent. 

Got the spectra in November between cloud and rain. They fluxed out well 
using the Gregg STIS stars as spectrophotometric standards. I compared the 
blue spectra with the MILES http://www.ucm.es/info/Astrof/miles/miles.html
spectra and got good fits to most of the stars. My relative absolute fluxes 
are OK but the clouds means the absolute fluxes are arbitrary.

----------------------------------------------------------------------------
2MASS NAME: 2MJ      RA   J2000   DEC     NAME        V   SpT    Ref  Notes
----------------------------------------------------------------------------
05592094-6631558 05 59 20.94 -66 31 55.8  WOH G642   11.7  MIII? lit    *
06013747-6635200 06 01 37.47 -66 35 20.0  HD271776   10.2  A3    lit
06005105-6644395 06 00 51.05 -66 44 39.5  -------    11.2  M0    lit
05581222-6620235 05 58 12.22 -66 20 23.5  HD270467   10.1  F8V   lit    %
05581475-6619273 05 58 14.75 -66 19 27.3  -------    12.4  (A0V) 2Mcol  %**
05564771-6639054 05 56 47.71 -66 39 05.4  HD270422   10.0  G0    lit
06022786-6647286 06 02 27.86 -66 47 28.6  HD271791   12.3  B2III 2Mcol  %%
06001860-6613273 06 00 18.60 -66 13 27.3  HD41466     9.5  F3V   lit
06005313-6655481 06 00 53.13 -66 55 48.1  HD270485   10.4   ?     -
----------------------------------------------------------------------------

Following are the MILES spectra and MILES information on the MILES stars that 
resemble the spectra.
0556-6639 is not quite as weak as 00493(=HD122563) but prob -2.
0558-6619 is high velocity star. It has really weak metal lines which 
confused me. It probably has [Fe/H]=-1.2 or thereabouts and a temperature 
about 9700K. Its continuum looks quite similar to MILES 0288 HD65900 but 
its lines look more like MILES 0519 HD128801.

----------------------------------------------------------------------------
2MASS NAME: 2MJ        MILES    HD    Sp    Te    logg    [M/H]
----------------------------------------------------------------------------
05592094-6631558    00116    021017    K4III    4400    2.2
06013747-6635200    00126    023194    A5V      8542    4.0
06005105-6644395    00264    060522    M0III    3884    1.2
05581222-6620235    00436    106516    F5V      6200    4.4    -0.7
05581475-6619273    0288     065900             9700K   4.2    -1.2 
                    0519     128801    
05564771-6639054    00493    122563    halo K   4550    1.5    -2.5
06022786-6647286    00817    207330    B3III   18350    2.5
06001860-6613273    00666    166285    F5V      6348    4.13   -0.2
06005313-6655481    06198    159307    F8V      6198    3.9    -1.1   
----------------------------------------------------------------------------