Figure 8.
The SED of the host galaxy of sGRB 130603B fitted by the lephare with fixed redshift z = 0.356. Filled red circles depict, respectively, the data points in the filters uvw2, uvm2, uvw1, U, taken from de Ugarte Postigo et al. (2014, Table 4), and B, g, r, RC, i, z, J, H, Ks from original observations (see Section 2.2). Data points in B and RC pass-bands were obtained using the 4K × 4K CCD Imager (Pandey et al. 2018) mounted at the axial port of the recently commissioned 3.6m DOT at Nainital, India (Kumar et al. 2018). Open circles represent model magnitudes for each filter. All magnitudes are in AB system.

The SED of the host galaxy of sGRB 130603B fitted by the lephare with fixed redshift z = 0.356. Filled red circles depict, respectively, the data points in the filters uvw2, uvm2, uvw1, U, taken from de Ugarte Postigo et al. (2014, Table 4), and B, g, r, RC, i, z, J, H, Ks from original observations (see Section 2.2). Data points in B and RC pass-bands were obtained using the 4K × 4K CCD Imager (Pandey et al. 2018) mounted at the axial port of the recently commissioned 3.6m DOT at Nainital, India (Kumar et al. 2018). Open circles represent model magnitudes for each filter. All magnitudes are in AB system.

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close