LQ Peg being observed with Chandra
Abstract:
Further to AAVSO Alert Notice 652, Dr. Koji Mukai (NASA-Greenbelt Space Flight Center) informs us that LQ Peg, one of the novalike variables in his target list, will be observed with Chandra on 2019 July 19 13:09 UT - 17:30 UT. Knowing the status of the target is essential for interpreting the X-ray data.
Justification:
We think we know how dwarf novae behave in X-rays, through various campaigns: they are X-ray bright in optical quiescence, and fainter and softer in X-rays during outburst. In the optical, we think of nova-likes as systems in permanent outburst — but in X-rays, they don’t quite resemble dwarf novae in outburst. This Chandra program is part of an effort to look for patterns and to understand their X-ray emission.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| LQ Peg | 14.30 | NL/VY |
Cadence: Not Specified Precision: 100 |
Not Requested |
Spectroscopy Lines:
No spectroscopy lines provided
Photometry Filters:
No photometry filters provided
Comparison Stars:
No comparison stars provided
Co-Authorship
Observers are not eligible for co-authorship.
Additional Observer Input:
Not provided
Additional Submission Location:
Not provided
Forum URL
N/A
Notes:
Principal Investigator: Dr. Koji Mukai; Imported Campaign (Alert Notice #671)