Last list for monitoring of ROSAT targets
Abstract:
The x-ray ROentgen SATellite (ROSAT) is reaching the end of its survey mode of operations at the end of January. So there are only two more weeks during which this survey mode of the satellite will continue to observe cataclysmic variables.
Justification:
Early alerts to the onset of outbursts are vital for the scheduling of simultaneous multiwavelength observations.
Requested Data Types:
Photometry
Targets
Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
---|---|---|---|---|
HT Cas | 12.60 | UGSU+E |
Cadence: Not Specified Precision: 100 |
Not Requested |
Z Cha | 11.50 | UGSU+EA |
Cadence: Not Specified Precision: 100 |
Not Requested |
OY Car | 11.20 | UGSU+E |
Cadence: Not Specified Precision: 100 |
Not Requested |
RX And | 10.30 | UGZ |
Cadence: Not Specified Precision: 100 |
Not Requested |
AR And | 11.00 | UGSS |
Cadence: Not Specified Precision: 100 |
Not Requested |
FO And | 13.10 | UGSU |
Cadence: Not Specified Precision: 100 |
Not Requested |
TT Ari | 10.20 | NL/VY |
Cadence: Not Specified Precision: 100 |
Not Requested |
KU Cas | 12.50 | UGSS |
Cadence: Not Specified Precision: 100 |
Not Requested |
TY Psc | 11.70 | UGSU |
Cadence: Not Specified Precision: 100 |
Not Requested |
KT Per | 11.50 | UGSS+ZZ |
Cadence: Not Specified Precision: 100 |
Not Requested |
NN Cen | 13.20 | UGSS |
Cadence: Not Specified Precision: 100 |
Not Requested |
BV Cen | 10.70 | UGSS |
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: N/A; Imported Campaign (Alert Notice #137)