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4 catalogs found
  
J/ApJS/248/21
(density 7)
  Swift long gamma-ray bursts (Hao+, 2020)
img(gal)
    J/ApJS/248/21/table1(c)The list of 371 Swift long gamma-ray bursts (LGRBs) (371 rows)
    J/ApJS/248/21/table2(c)Table of LGRB hosts (42 rows)
  
J/A+A/659/A39
(density 7)
  GRB190114C spectra and light curves (Melandri+, 2022)
spectrum
timeSerie
  
    J/A+A/659/A39/table2Summary of spectroscopic observations[spectrum] (5 rows)
    J/A+A/659/A39/rbandr-band Photometry table of GRB190114C (Fig. 2) compiled by A. Melandri (data are all dereddened for Galactic extinction) [timeSerie](light curve)
timeSerie
(34 rows)
    J/A+A/659/A39/ibandi-band Photometry table of GRB190114C (Fig. 2) compiled by A. Melandri (data are all dereddened for Galactic extinction) [timeSerie](light curve)
timeSerie
(23 rows)
    J/A+A/659/A39/zbandz-band Photometry table of GRB190114C (Fig. 2) compiled by A. Melandri (data are all dereddened for Galactic extinction) [timeSerie](light curve)
timeSerie
(20 rows)
  
J/MNRAS/482/2731
(density 7)
  Metals, depletion, and dimming: decrypting dust (Zafar+, 2019)
img(gal)
    J/MNRAS/482/2731/table1(c)GRBs data used to estimate dust-to-metals ratios and N(Fe,Si)dust (48 rows)
    J/MNRAS/482/2731/refs1References for table1 (47 rows)
    J/MNRAS/482/2731/table2(c)QSO DLAs and sub-DLAs data used to estimate dust-to-metals ratios and N(Fe,Si)dust (47 rows)
    J/MNRAS/482/2731/refs2References for table2 (32 rows)
  
J/MNRAS/469/3125
  Abundance ratio in gamma-ray burst (Contini, 2017)
img(gal)
    J/MNRAS/469/3125/table1(c)Modelling line ratios to Hβ=1 from the CALIFA HII regions (Marino et al., 2013, Cat. J/A+A/559/A114) (32 rows)
    J/MNRAS/469/3125/table2Models used to reproduce the spectra presented in Table 1 (16 rows)
    J/MNRAS/469/3125/table3(c)Modelling line ratios to Hβ=1 from the HII regions sample of Berg et al. (2012ApJ...754...98B) (102 rows)
    J/MNRAS/469/3125/table4Models used to reproduce the spectra presented in Table 3 (51 rows)
    J/MNRAS/469/3125/table5(c)Modelling line ratios to Hβ=1 of AGN spectra at z≤0.1 (Dors et al. 2017MNRAS.468L.113D) (56 rows)
    J/MNRAS/469/3125/table6Models used to reproduce the spectra presented in Table 5 (28 rows)
    J/MNRAS/469/3125/table7(c)Modelling line ratios to Hβ=1 of Type I SN host spectra at z≤0.03 (Gallagher et al., 2005ApJ...634..210G) (54 rows)
    J/MNRAS/469/3125/table8Models used to reproduce the spectra presented in Table 7 (27 rows)

ALL
     
       (c)  indicates tables which contain celestial coordinates 
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