Index of /~michal/sed

      Name                    Last modified       Size  Description


[DIR] Parent Directory        23-Jun-2009 10:52      -  
[   ] SMG.tar                 28-May-2009 12:41   740k  
[   ] SMGz4.tar               31-Jan-2010 14:36    60k  
[   ] grb.tar                 15-Sep-2008 15:26   181k  
[TXT] grb000210.0             28-Aug-2007 15:06    14k  
[TXT] grb000210.sed           28-Aug-2007 15:12     5k  
[TXT] grb000418.0             28-Aug-2007 15:07    14k  
[TXT] grb000418.sed           28-Aug-2007 15:13     5k  
[TXT] grb010222.0             28-Aug-2007 15:07    14k  
[TXT] grb010222.sed           28-Aug-2007 15:14     5k  
[TXT] grb980425.0             15-Sep-2008 15:16    33k  
[TXT] grb980425.sed           15-Sep-2008 15:16     9k  
[TXT] grb980425WR.0           15-Sep-2008 15:16    33k  
[TXT] grb980425WR.sed         15-Sep-2008 15:16     9k  
[TXT] grb980425_low_radio.sed 15-Sep-2008 15:16    11k  
[TXT] grb980703.0             28-Aug-2007 15:06    14k  
[TXT] grb980703.sed           28-Aug-2007 15:10     5k  

SUBMM GALAXIES

SMG.tar contains the SED templates used to fit the data of submm galaxies and published in Michalowski et al. (2009, arXiv:0905.4499):
  http://arxiv.org/abs/0905.4499

The files contain SED templates scaled to the observed datapoints of SMGs in a format: rest wavelength (microns) vs. flux density (Jy)
as well as the averaged SED after normalization to the flux at 850 micron (averaged_flux.dat, rest wavelength [micron] vs. flux [Jy])
and SFR of 100 Msol/yr (averaged_sfr.dat, rest wavelength [micron] vs luminosity [Lsol]).

SMGz4.tar contains the SED templates used to fit the data of submm galaxies at z>4 and published in Michalowski et al. (2010, ApJ accepted)

The files contain SED templates scaled to the observed datapoints of SMGs in a format: rest wavelength (microns) vs. flux density (Jy).

===================================

GRB HOST GALAXIES

The SED templates are published in  Michalowski et al. (2008, ApJ, 672..817) and Michalowski et al. (2009, ApJ, 693, 347):
  http://adsabs.harvard.edu/abs/2008ApJ...672..817M
  http://adsabs.harvard.edu/abs/2009ApJ...693..347M

All of these SEDs correspond to gamma-ray burst (GRB) host galaxies, and hence
can be used to fit the observations of young, star-forming galaxies.
For GRB 980425 models for the entire galaxy (original and with supressed radio emission) and the WR region are available (see Michalowski et al. 2009 for details).

Description of the individual files:

<object>.0   : original GRASIL file with an SED in a format: rest wavelength (angstrom) vs. luminosity (1e30 erg/s/A); see the beginning of the file for more details; column 6 represent the total emission of a galaxy at different wavelengths
<object>.sed : an SED template scaled to the observed datapoints of the <object> in a format: rest wavelength (microns) vs. flux density (Jy)
grb.tar      : all files tar'ed together

===================================

SED models were produced using GRASIL model (Silva et al., 1998, ApJ, 509, 103):
  http://adlibitum.oat.ts.astro.it/silva/default.html
  http://adsabs.harvard.edu/abs/1998ApJ...509..103S
The collection of templates used to fit SMG and GRB 980425 data were compiled by Iglesias-Paramo et al. (2007, ApJ, 670, 279):
  http://adsabs.harvard.edu/abs/2007ApJ...670..279I

===================================

More models will appear soon!

If you have any question or comment, don't hesitate to contact me:
michal  -<at>- dark-cosmology.dk
Michal Michalowski