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OBSID:
29506
Title:
Electron heating mechanism behind the equatorial shock     
Investigator:
Sarkar
Observer:
Sarkar, Arnab
Phone:
6462553017
Email:
arnabsar@mit.edu
Target Name:
1E 2215.7-0404 / 1E 2216.0-0401
Sequence Number:
802152
Instrument:
ACIS-I
Grating:
NONE
SI Mode:
TE_006E6B
Raster Scan:
N
Annotated DOT:
AUG1224a

Proposal Number:
25800327
Right Ascension:
334.612
Declination:
-3.77474
Status:
observed
Start Date:
2024-08-13 06:27:09
Category:
CLUSTERS OF GALAXIES
Type:
GO
AO Cycle:
25
Dither Flag:
Y
Y Offset:
0
Z Offset:
0
Est. Count Rate:
0.1
Order-1 Count Rate:

Exposure Time:
31
Time Remaining:
31.093
Reqd Start Time:

Reqd Stop Time:

Period:

Epoch:

Start of Period:

End of Period:

PS Margin:

PE Margin:

Max Segments:
0

ACIS Mode:
TE
Standard?:
No
BEP Mode:
VF
Dropped Chip Count:
1
Optional Chips:
S2
On-Chip Summing?:
No
Row Sum:

Column Sum:

Frame Time:

Subarray Mode:
NONE
Starting Row:
0
Row Count:
1023
Subarray Frame Time:


Duty Cycle?:
No
Cycle Count:
0
Primary Exp Time:

Secondary Exp Time:

Event Filter?:
No
Filter Threshold:

Filter Range:

Bias Requested?:
No
Bias Frequency:

Bias After?:
No
Spatial Window?:
No

Abstract:
Electron heating mechanism behind a shock front is still up for debate. With this 740 ks Chandra observation of 1E2215/16, we will primarily investigate the electron heating mode behind the only known equatorial merger shock. Though axial merger shocks have been studied extensively using Chandra and XMM-Newton (Abell 2146 for example), the driving mechanism and properties of equatorial shocks are largely unknown.

psci Run:
84
Processing Date:
Sep 4 2024
psci Directory:
/nfs/maaxnew/r3/fn/acis128b/acis128.log
OBSID:
29506
SIM Mode:
ACIS-I
OTG Mode:
NONE
Seq Number:
802152
Target Name:
1E_2215.7-0404_
AO:
25
Start VCDU:
119963:064
Start Time (UTC):
226:24185.277
Stop Time (UTC):
226:55287.948
Kilosecs:
31.1
% Frames:
100.0
# CCDs:
I4
# Frames:
9902
# Events:
442310
Events/sec:
14
PSCI errors:
0
% drops:
0.0
Bias Errs:
0
FP Temp:
-110.4
Parameter Block:
0x006e6034
Window Block:
-
# Windows:
0
FEP Mode:
Te5x5
BEP Mode:
F
Start Row:
0
# Rows:
1024
Primary Exposure:
31
Secondary Exposure:
0
Duty Cycle:
0
Summing?:
No
Bias?:
Yes
Trickle?:
Yes
Bias Run:
84


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