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Query : 2014A&A...570A..52S |
2014A&A...570A..52S - Astronomy and Astrophysics, volume 570A, 52-52 (2014/10-1)
Herschel observations of gamma-ray burst host galaxies: implications for the topology of the dusty interstellar medium.
SCHADY P., SAVAGLIO S., MUELLER T., KRUEHLER T., DWELLY T., PALAZZI E., HUNT L.K., GREINER J., LINZ H., MICHALOWSKI M.J., PIERINI D., PIRANOMONTE S., VERGANI S.D. and GEAR W.K.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): galaxies: high-redshift - gamma-ray burst: general - dust, extinction - infrared: galaxies - submillimeter: galaxies - galaxies: star formation
Simbad objects: 16
Number of rows : 16 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | GRB 000210 | gB | 01 59 15 | -40 40.0 | ~ | 172 | 0 | |||||
2 | [LDM2003] GRB J015915.5-403933 | G | 01 59 15.61 | -40 39 33.1 | ~ | 13 | 0 | |||||
3 | [KGS2011] GRB 090926B host G | G | 03 05 13.91 | -39 00 22.6 | 23.71 | ~ | 4 | 0 | ||||
4 | Fermi bn090926914 | gB | 03 05 14.30 | -38 59 50.9 | ~ | 131 | 1 | |||||
5 | SN 2003lw | SN* | 08 02 30.1 | -39 51 03 | 20.23 | SNIc: | 548 | 0 | ||||
6 | Anon J080230-3951 | G | 08 02 30.20 | -39 51 03.0 | 22.31 | 22.32 | 20.53 | 20.44 | 19.40 | ~ | 20 | 0 |
7 | GRB 070306 | gB | 09 52 23.220 | +10 28 55.20 | ~ | 206 | 1 | |||||
8 | SDSS J095223.31+102855.4 | G | 09 52 23.32 | +10 28 55.4 | 23.00 | ~ | 7 | 0 | ||||
9 | [BCK2003] G1 | G | 12 25 19.3 | +20 06 11 | ~ | 19 | 0 | |||||
10 | GRB 000418 | gB | 12 25 21 | +20 05.0 | ~ | 214 | 0 | |||||
11 | GRB 010222 | G | 14 52 12.5 | +43 01 06 | ~ | 355 | 1 | |||||
12 | [LDM2003] GRB J180831.6+591851 | G | 18 08 31.6 | +59 18 51 | ~ | 14 | 1 | |||||
13 | [TSC98] Host G | G | 19 34 54 | -52 49.9 | ~ | 20 | 1 | |||||
14 | [KGS2011] GRB 081109 host G | G | 22 03 09.63 | -54 42 39.9 | 23.23 | 22.85 | 21.96 | ~ | 3 | 0 | ||
15 | Fermi bn081109293 | gB | 22 03 11.50 | -54 42 40.5 | ~ | 110 | 1 | |||||
16 | Fermi bn081119184 | gB | 23 06 | +30.0 | ~ | 14 | 0 |
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