1SWASP J022916.91-395901.4 being observed with Chandra
Abstract:
1SWASP J022916.91-395901.4, one of the novalike variables, will be observed with Chandra to understand their X-ray emission.
Justification:
Knowing the status of the target is essential for interpreting the X-ray data. This Chandra program is part of an effort to look for patterns and understand X-ray emission of nova-like systems.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| V0410 Peg | 11.00 | E: |
Cadence: Not Specified Precision: 100 |
Not Requested |
| 1SWASP J022916.91-395901.4 | 12.80 | UGZ/IW+VY |
Cadence: Not Specified Precision: 100 |
Not Requested |
| KQ Mon | 12.10 | NL |
Cadence: Not Specified Precision: 100 |
Not Requested |
| EC 21178-5417 | 13.40 | NL+E |
Cadence: Not Specified Precision: 100 |
Not Requested |
| LQ Peg | 14.30 | NL/VY |
Cadence: Not Specified Precision: 100 |
Not Requested |
| UU Aqr | 12.85 | NL/VY+E |
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 #663)