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:
29179
Title:
Simultaneous Chandra and XRISM Spectroscopy of NGC 4151     
Investigator:
Miller
Observer:
Miller, Jon
Phone:
617 529 5725
Email:
jonmm@umich.edu
Target Name:
NGC 4151
Sequence Number:
705150
Instrument:
ACIS-S
Grating:
HETG
SI Mode:
TE_0088EB
Raster Scan:
N
Annotated DOT:
DEC2523b

Proposal Number:
24708948
Right Ascension:
182.636
Declination:
39.4059
Status:
archived
Start Date:
2023-12-26 12:10:13
Category:
ACTIVE GALAXIES AND QUASARS
Type:
DDT
AO Cycle:
24
Dither Flag:
Y
Y Offset:
0
Z Offset:
0
Est. Count Rate:
1.2
Order-1 Count Rate:
1.2
Exposure Time:
18
Time Remaining:
17.612
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:
F
Dropped Chip Count:
0
Optional Chips:
S0 S5
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:
XRISM is currently scheduled to observe NGC 4151 on Dec 27, 2023, for 45 ks. This is the first of four planned XRISM exposures; the rest will likely be taken in late April 2024. Below 4 keV, the HETGS offers superior resolution to the Resolve calorimeter. Simultaneous - or at least contemporaneous observations - will provide the best opportunity to study the variable absorption and winds in NGC 4151, the nature and origin of the narrow Fe K line, and to search for relativistic disk reflection. NuSTAR will also observe NGC 4151 providing coverage of the ionizing continuum out to 79 keV, but no coverage below 3 keV. Chandra spectroscopy is essential for characterizing the lines and absorption edges at low energy that ultimately shape the continuum through the Fe K band, where the strongest outflows and relativistic disk reflection are evident. [Submitted on behalf of the XRISM team; additional communication with the Director includes some privileged information.]

psci Run:
191
Processing Date:
Jan 3 2024
psci Directory:
/nfs/maaxnew/r3/fl/acis126b/acis126.log
OBSID:
29179
SIM Mode:
ACIS-S
OTG Mode:
HETG
Seq Number:
705150
Target Name:
NGC_4151
AO:
24
Start VCDU:
36392:104
Start Time (UTC):
360:45113.710
Stop Time (UTC):
360:62738.463
Kilosecs:
17.6
% Frames:
100.0
# CCDs:
S6
# Frames:
5438
# Events:
588219
Events/sec:
33
PSCI errors:
0
% drops:
0.0
Bias Errs:
1
FP Temp:
-115.2
Parameter Block:
0x0088e024
Window Block:
-
# Windows:
0
FEP Mode:
Te3x3
BEP Mode:
F
Start Row:
0
# Rows:
1024
Primary Exposure:
32
Secondary Exposure:
0
Duty Cycle:
0
Summing?:
No
Bias?:
Yes
Trickle?:
Yes
Bias Run:
191


pgf@space.mit.edu Thu Apr 3 20:00:53 EST 2025