C H A N D R A   S C I E N C E   C E N T E R
O B S E R V A T I O N   C A T A L O G

OBSID:
26163
Title:
Re-visiting an Old Friend: Monitoring X-ray Sources in the Bulge of M31  
Investigator:
Irwin
Observer:
Irwin, Jimmy
Phone:
205-348-3791
Email:
jairwin@ua.edu
Target Name:
m31
Sequence Number:
601540
Instrument:
HRC-I
Grating:
NONE
SI Mode:
OBS20743
Raster Scan:
N
Annotated DOT:
OCT1821a

Proposal Number:
22620093
Right Ascension:
10.6847
Declination:
41.2687
Status:
archived
Start Date:
2021-10-20 23:18:17
Category:
NORMAL GALAXIES
Type:
GO
AO Cycle:
22
Dither Flag:
Y
Y Offset:

Z Offset:

Est. Count Rate:
0.1
Order-1 Count Rate:

Exposure Time:
24.00
Time Remaining:

Reqd Start Time:

Reqd Stop Time:

Period:

Epoch:

Start of Period:

End of Period:

PS Margin:

PE Margin:

Max Segments:
0

Trigger Level:
DEF
Range Switch Lvl:
DEF
Spect Mode:
DEF
Antico Enab:
DEF
Width Enab:
DEF
Width Thold:
DEF
Uld Enab:
DEF
Upper Lvl Disc:
DEF
Blank Enab:
EDGE
U Blank Hi:
119
V Blank Hi:
119
U Blank Lo:
69
V Blank Lo:
69
Py Shutter Pos:
DEF
My Shutter Pos:
DEF
Timing Mode:
N

Abstract:
After 16 years of near-monthly monitoring, Chandra has not observed the bulge of M31 since 2015. We propose a 3-year program to image M31 with the HRC-I once per year to continue monitoring campaigns such as searching for flares from the supermassive black hole in the nucleus M31*, determining turn-off times of post-nova supersoft emission, and investigate the variability of X-ray sources near [O III] nebula, possibly induced by microquasar-powered jets of the variable X-ray source. Continued 20+ year monitoring of over a hundred X-ray sources to a limiting luminosity of 2e35 ergs/s will also be performed.

Remarks:
Multi-cycle - 50 ksec per cycle

OBSID 26163 not found in Q/L Processing Logs dated Sun Mar 30 22:53:58 EST 2025


pgf@space.mit.edu Mon Mar 31 10:36:39 EST 2025