Optical photometry of SWIFT J1753.5-0127 following its X-ray brightening

Details Optical photometry of SWIFT J1753.5-0127 following its X-ray brightening Optical photometry of SWIFT J1753.5-0127 following its X-ray brightening

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1608....1d&link_type=abstract

The Astronomer's Telegram, #1608

Astronomy and Astrophysics

Astronomy

Optical, Black Holes

Scientific paper

In ATel #1599; Krimm et al. report a gradual brightening and softening of SWIFT J1753.5-0127's X-ray emission, using the SWIFT satellite on June 30, 2008. We performed contemporaneous BVRI imaging of the system with the IAC80 telescope at the Observatorio del Teide, Tenerife around T2300, 29 June and 02 July, 2008. We find average magnitudes: B=17.07, V=16.64, R=16.41 and I=15.97.

Affiliated with

Also associated with

No associations

Rating

Optical photometry of SWIFT J1753.5-0127 following its X-ray brightening does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Optical photometry of SWIFT J1753.5-0127 following its X-ray brightening, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical photometry of SWIFT J1753.5-0127 following its X-ray brightening will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1360187