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| Query : 2009CBET.1861....1D |
2009CBET.1861....1D - Central Bureau Electronic Telegrams, 1861, 1 (2009/June-0)
Supernovae 2009gm-2009gs and possible supernovae K0905-10, K0905-11, K0905-12.
DRAKE A.J., DJORGOVSKI S.G., MAHABAL A., GRAHAM M.J., WILLIAMS R., CATELAN M., BESHORE E.C., LARSON S.M., HILL R., KOWALSKI R., BOATTINI A., GIBBS A. and CHRISTENSEN E.
Abstract (from CDS):
---------------------------------------------------------------------------— SN 2009 UT R.A. (2000.0) Decl. Mag. Offset ---------------------------------------------------------------------------— 2009gm May 23.16 14 27 58.10 +11 24 33.9 18.2 8".7 E, 8".9 S 2009gn May 26.30 16 05 23.53 -16 08 34.2 18.0 2".2 W, 5".6 N 2009go May 29.36 16 38 54.17 +21 49 06.0 18.3 2".0 W, 2".0 N 2009gp May 30.25 14 19 33.93 + 2 44 45.5 19.0 0".2 W, 2".0 N 2009gq June 2.40 22 14 52.81 +17 30 47.2 18.3 5".5 W, 14".7 N 2009gr June 14.42 17 25 38.28 +19 07 05.8 18.8 3".5 E, 3".0 N 2009gs June 15.44 21 18 49.42 - 5 57 10.8 16.6 1".1 E, 0".4 N ---------------------------------------------------------------------------— PSN 2009 UT R.A. (2000.0) Decl. Mag. Offset ---------------------------------------------------------------------------— K0905-10 May 23.16 14 26 47.44 +12 35 29.1 18.5 0".4 E, 0".8 N K0905-11 May 26.27 13 51 43.30 + 9 06 53.2 19.4 0".2 W, 0".1 N K0905-12 May 30.35 14 20 21.31 +29 11 59.4 19.1 1".1 W, 0".2 N ---------------------------------------------------------------------------—
Discoveries were compared with reference images from deeper Sloan Digital Sky Survey, Canada-France-Hawaii Telescope, and Digitized Sky Survey images, as well as CSS and "Palomar Quest" co-added images and CSS lightcurves. The objects were followed with the Palomar 1.5-m telescope using Gunn filters.
Further magnitudes for 2009gm: Apr. 28.38, [20.7 (CSS); May 27.22, g = 18.9, r = 18.0, i = 18.1 (Palomar); June 1.25, 18.4 (CSS); 16.24, 19.2 (CSS).
Further magnitudes for 2009gn: Apr. 19.43, [20.2 (CSS); 30.39, 18.5 (CSS); May 27.23, g = 18.6, r = 18.3, i = 18.5 (Palomar); June 14.26, 18.6 (CSS).
Further magnitudes for 2009go: May 4.37, [20.4 (CSS); 16.33, 18.7 (CSS); June 2.22, g = 18.4, r = 18.4, i = 18.6 (Palomar); 4.20, g = 18.8, r = 18.8, i = 18.6 (Palomar); 16.42, g = 19.7, r = 19.5, i = 19.8 (Palomar); 21.33, 19.6 (CSS).
Further magnitudes for 2009gp: Apr. 27.35, [20.2 (CSS); May 24.27, 18.9 (CSS); June 2.21, g = 19.2, r = 18.9, i = 19.2 (Palomar); 15.25, 19.8 (CSS).
Further magnitudes for 2009gq: Apr. 29.48, [20.2 (CSS); June 11.44, 18.7 (CSS); 16.41, g = 19.2, r = 18.9 (Palomar); 22.40, 19.2 (CSS).
Further magnitudes for 2009gr: Feb. 5.53, [20.0 (CSS); May 27.37, 18.1 (CSS); June 22.37, 19.3 (CSS).
Further magnitudes for 2009gs: May 27.44, [20.1 (CSS); June 16.44, g = 16.4, r = 16.5, i = 16.6 (Palomar).
Further magnitudes for K0905-10: Apr. 18.44 UT, [20.0 (CSS); 28.38, 19.5 (CSS); May 27.22, g = 18.6, r = 18.6, i = 18.7 (Palomar); June 1.25, 18.6 (CSS); 16.24, 19.3 (CSS).
Further magnitudes for K0905-11: Apr. 28.35, [20.5 (CSS); May 27.22, g = 19.4, r = 19.4, i = 19.4 (Palomar); June 11.26, 19.9 (CSS).
Abstract Copyright: ∼
Journal keyword(s):
Simbad objects: 10
| Number of rows : 10 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | PSN K0905-011 | SN* | 13 51 43.30 | +09 06 53.2 | ~ | 3 | 0 | |||||
| 2 | SN 2009gp | SN* | 14 19 33.93 | +02 44 45.5 | ~ | 5 | 1 | |||||
| 3 | PSN K0905-012 | SN* | 14 20 21.31 | +29 11 59.4 | ~ | 3 | 0 | |||||
| 4 | PSN K0905-010 | SN* | 14 26 47.44 | +12 35 29.1 | ~ | 3 | 0 | |||||
| 5 | SN 2009gm | SN* | 14 27 58.10 | +11 24 33.9 | ~ | 4 | 1 | |||||
| 6 | SN 2009gn | SN* | 16 05 23.53 | -16 08 34.2 | ~ | 5 | 1 | |||||
| 7 | SN 2009go | SN* | 16 38 54.17 | +21 49 06.0 | ~ | 5 | 1 | |||||
| 8 | SN 2009gr | SN* | 17 25 38.28 | +19 07 05.8 | ~ | 3 | 1 | |||||
| 9 | SN 2009gs | SN* | 21 18 49.4 | -05 57 11 | SNIa-norm | 8 | 1 | |||||
| 10 | SN 2009gq | SN* | 22 14 52.8 | +17 30 47 | SNIa-norm | 8 | 1 |
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