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Name
  TCP J05074264+2447555  
AAVSO UID
000-BML-703 (4114 observations)  
Constellation
Taurus Sequence
J2000.0
05 07 42.73 +24 47 56.5  (76.92804 +24.79903) Search nearby
B1950.0 05 04 39.02 +24 44 03.3
Galactic coord. 178.756 -9.325
Other names

(Internal only)
2MASS J05074272+2447564 AllWISE J050742.72+244756.3 CMC15 J050742.7+244756
GALEX J050742.7+244756 GSC 01849-01566 GSC2.3 N9TS000630
SDSS J050742.71+244756.2 UCAC2 40474298 UCAC4 574-013830
USNO-A2.0 1125-02093329 USNO-B1.0 1147-0066243 WISE J050742.71+244756.4
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Variability type
Microlens
Spectral type F5V
Mag. range
11.5 - 14.1 V
Discoverer Tadashi Kojima
Epoch
--
Outburst --
Period --
Rise/eclipse dur. --
Remarks
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References
Click reference title/citation to view in new window. Roll over index number to view submission details.
1 Kochanek, C. S.; et al., 2017, The All-Sky Automated Survey for Supernovae
(ASAS-SN) Light Curve Server v1.0 (online data)
2017PASP..129j4502K
2 Kochanek, C. S.; et al., 2017, The All-Sky Automated Survey for Supernovae
(ASAS-SN) Light Curve Server v1.0
2017PASP..129j4502K
3 A. A. Nucita; et al., 2017, ATel #10934 2017ATel10934....1N
4 T. Jayasinghe; et al., 2017, ATel #10923 2017ATel10923....1J
5 R. Leadbeater, 2017, vsnet-alert #21563 --
6 CBAT "Transient Object Followup Reports" --
External Links
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Catalog Data
Information from selected catalogs obtained by cross-matching to 2 arc seconds using the CDS X-Match Service. These data may not be complete.
2MASS J = 12.25H = 11.85K = 11.68J - K = 0.57
AllWISE W1 = 11.62W2 = 11.62W3 = 11.36W1 - W2 = -0.00
APASS-DR9 B = 14.99V = 14.09g' = 14.52r' = 13.80i' = 13.66B - V = 0.91
GALEX-DR5 NUV = 20.03
SDSS-DR12 u = 16.32g = 14.81r = 13.92i = 16.39z = 13.48u - g = 1.51r - i = -2.47
Images
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Supporting Documents
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Revision History
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3 Otero, Sebastian Alberto 2017-11-03 01:37 UTC Range from ATel #10923. Spectral type from vsnet-alert 21563.
2 Otero, Sebastian Alberto 2017-11-02 12:47 UTC Maximum magnitude from ASAS-SN data.
1 Schmeer, Patrick 2017-11-01 16:28 UTC Minimum magnitude from APASS. PPMXL position. The ASAS-SN light curve shows a typical microlens profile (S. Otero).