From: garcia@cfa219.harvard.edu (Mike Garcia) Message-ID: <vsnet-alert1834@hoge.baba.hajime.jp> To: BAILYN@astro.yale.edu, ajct@laeff.esa.es, chaswell@star.maps.susx.ac.uk, e.kuulkers1@physics.oxford.ac.uk, fghigo@nrao.edu, garcia@head-cfa.harvard.edu, guy@mrao.cam.ac.uk, ewaltman@rsd.nrl.navy.mil, jem@head-cfa.harvard.edu, lewin@space.mit.edu, marshall@milkyway.gsfc.nasa.gov, pac@astro.ox.ac.uk, rhjellmi@aoc.nrao.edu, rmw@lowell.Lowell.Edu, rpf@astro.uva.nl, rr@space.mit.edu, shrader@grossc.gsfc.nasa.gov, starrfie@hydro.la.asu.edu, stroh@pcasun1.gsfc.nasa.gov, swank@pcasun1.gsfc.nasa.gov, takeshim@ginpo.gsfc.nasa.gov, tavani@astro.columbia.edu, narayan@cfa.harvard.edu, vsnet-alert@kusastro.kyoto-u.ac.jp Cc: garcia@cfa219.harvard.edu Precedence: list X-Distribute: distribute [version 2.1 (Alpha) patchlevel=24] X-Sequence: vsnet-alert 0 Subject: [vsnet-alert 0] XTE J2012+381 optical photometry and spectra Errors-To: owner-vsnet-alert@kusastro.kyoto-u.ac.jp Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp Dear Colleauges: Attached is an item on XTE J2012+381 which we have submitted to the IAUC. -Mike Garcia --------------- XTE J2012+381 M.R. Garcia, J.E. McClintock, P. Berlind, and E. Barton report: Spectra and photometry of the proposed counterpart to XTE J2012+381 (Wagner etal, IAUC 6920) with the Mt. Hopkins 1.5m and 1.2m show that this star is a heavily reddened M-giant. Photometry on the night of 28~May (7:30 UT - 11:16 UT), finds V=19.7 +/- 0.2, R=16.3 +/- 0.1, and I=12.2 +/= 0.1, with no detected variability. The apparent brightening described in IAUC 6920 is most probably an artifact of the extreme red colors and the miss-match in the bandpasses of the LONEOS images (which used an unfiltered CCD) and the DSS images. Neither our photometry nor that in IAUC 6920 provide any evidence that this star is the counterpart to XTE J2012+381.