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Faulkes Telescope Project Privacy Policy
content-views-query-and-display-post-page domain was triggered too early. This is usually an indicator for some code in the plugin or theme running too early. Translations should be loaded at the init action or later. Please see Debugging in WordPress for more information. (This message was added in version 6.7.0.) in /home1/downear3/public_html/drupal-5/wp-includes/functions.php on line 6131blank-slate domain was triggered too early. This is usually an indicator for some code in the plugin or theme running too early. Translations should be loaded at the init action or later. Please see Debugging in WordPress for more information. (This message was added in version 6.7.0.) in /home1/downear3/public_html/drupal-5/wp-includes/functions.php on line 6131The 2009 – 2010 outburst (data from the Faulkes Telescopes, Swift BAT, RXTE ASM and WHT. These data have appeared in ATel #2775 and in the MNRAS paper, “A late jet rebrightening revealed from multi-wavelength monitoring of the black hole candidate XTE J1752-223” by Russell et al. here.

Finding charts (all north = top, east = left):
Faulkes i’-band on 2010-07-15 (260 sec, seeing = 0.9″):
40 x 60 arcsec FOV; red circle = 0.31″ UVOT error circle from Curran et al. 2010.
The faint star 0.8″ to the north has magnitudes V > 20.3; R = 19.7 +- 0.1; i’ = 18.4 +- 0.2

2MASS H-band
40 x 60 arcsec FOV; red circle = 0.31″ UVOT error circle from Curran et al. 2010.

WHT LIRIS images: H-band (left; 240 sec) and Ks-band (right; 360 sec) on 2010-07-01 (seeing = 0.6″ – 0.8″):
20 x 20 arcsec FOV; counterpart marked
XTE J1752-223 had magnitudes H = 15.6 +- 0.1; Ks = 15.2 +- 0.1 on this date (fade towards quiescence).
The faint star 0.8″ to the north has magnitudes H = 15.5 +- 0.1; Ks = 15.2 +- 0.1

Click here to return to the main XRB page
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