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OBSID:
27935
Title:
Milky Way HEPCATs           
Investigator:
Povich
Observer:
Povich, Matthew
Phone:
(909) 869-3608
Email:
mspovich@csupomona.edu
Target Name:
HEP G011.675-01.822
Sequence Number:
201633
Instrument:
ACIS-I
Grating:
NONE
SI Mode:
TE_006E6B
Raster Scan:
N
Annotated DOT:
JUL0323a

Proposal Number:
20201073
Right Ascension:
274.497
Declination:
-19.6947
Status:
archived
Start Date:
2023-07-09 19:02:42
Category:
STARS AND WD
Type:
CCT
AO Cycle:
20
Dither Flag:
Y
Y Offset:
0
Z Offset:
0
Est. Count Rate:
0.1
Order-1 Count Rate:

Exposure Time:
10
Time Remaining:
11.091
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
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:
With this white paper we recommend Milky Way HEPCATs (High Energy Panoramas of Cool Attitude Targets), a comprehensive Chandra/ACIS-I program to survey massive star-forming regions (MSFRs) in the Galactic Plane. HEPCATs will transform Chandra's operational necessity for cool attitude targets into a rich scientific legacy by X-raying the Galaxy's spiral arms. Its primary goal is to obtain ~2500 sharp X-ray snapshots of WISE and Spitzer bubbles, to reveal the massive stars driving these iconic structures and the wind-generated hot plasma that fills them. Over time, HEPCATs will build up wide-field X-ray mosaics of the vast giant molecular clouds that fuel the great MSFR complexes in the Milky Way, blazing a trail for future high-resolution X-ray missions.

Remarks:
N/A

psci Run:
402
Processing Date:
Jul 25 2023
psci Directory:
/nfs/maaxnew/r3/fj/acis124e/acis124.log
OBSID:
27935
SIM Mode:
ACIS-I
OTG Mode:
NONE
Seq Number:
201633
Target Name:
HEP_G011.675-01
AO:
20
Start VCDU:
113629:120
Start Time (UTC):
190:69549.289
Stop Time (UTC):
190:80652.812
Kilosecs:
11.1
% Frames:
100.0
# CCDs:
I4
# Frames:
3535
# Events:
187667
Events/sec:
16
PSCI errors:
0
% drops:
0.0
Bias Errs:
0
FP Temp:
-119.0
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:
402


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