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OBSID:
27597
Title:
DISCOVERING AXIONS WITH X-RAY SEARCHES TOWARDS MAGNETIC WHITE DWARFS  
Investigator:
Safdi
Observer:
Safdi, Benjamin R.
Phone:
5136042373
Email:
brsafdi@berkeley.edu
Target Name:
WD 1859+148
Sequence Number:
201558
Instrument:
ACIS-I
Grating:
NONE
SI Mode:
TE_00D4EB
Raster Scan:
N
Annotated DOT:
DEC0522a

Proposal Number:
24200244
Right Ascension:
285.386
Declination:
14.9687
Status:
archived
Start Date:
2022-12-10 10:33:10
Category:
STARS AND WD
Type:
GO
AO Cycle:
24
Dither Flag:
Y
Y Offset:
0
Z Offset:
0
Est. Count Rate:
0.0001134
Order-1 Count Rate:

Exposure Time:
10
Time Remaining:
10.115
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:
Axions, which are hypothetical ultra-light particles, are a well-motivated extension to the Standard Model of particle physics. White dwarf (WD) stars may radiate keV-energy axions produced in their stellar cores. This has been studied as a channel by which WDs may cool, with some analyses suggesting that axions can help explain the WD luminosity function. The radiated axions may convert into X-rays in the magnetic fields surrounding magnetic WDs (MWDs). We propose two 40 ks observations of the MWDs WD 1859+148 and PG 0945+246. In the absence of axions we will set the strongest limits to-date on the axion coupling strength and disfavor nearly all of the parameter space for axions predicted by string theory.

psci Run:
255
Processing Date:
Dec 14 2022
psci Directory:
/nfs/maaxnew/r3/fh/acis122d/acis122.log
OBSID:
27597
SIM Mode:
ACIS-I
OTG Mode:
NONE
Seq Number:
201558
Target Name:
WD_1859+148
AO:
24
Start VCDU:
128401:008
Start Time (UTC):
344:39278.887
Stop Time (UTC):
344:49405.479
Kilosecs:
10.1
% Frames:
100.0
# CCDs:
I1
# Frames:
3330
# Events:
60608
Events/sec:
5
PSCI errors:
0
% drops:
0.0
Bias Errs:
0
FP Temp:
-112.0
Parameter Block:
0x00d4e014
Window Block:
-
# Windows:
0
FEP Mode:
Te5x5
BEP Mode:
F
Start Row:
0
# Rows:
1024
Primary Exposure:
30
Secondary Exposure:
0
Duty Cycle:
0
Summing?:
No
Bias?:
Yes
Trickle?:
Yes
Bias Run:
255


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