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: |
Title: |
Investigator: |
Observer: |
Phone: |
Email: |
Target Name: |
Sequence Number: |
Instrument: |
Grating: |
SI Mode: |
Raster Scan: |
Annotated DOT: |
Proposal Number: |
Right Ascension: |
Declination: |
Status: |
Start Date: |
Category: |
Type: |
AO Cycle: |
Dither Flag: |
Y Offset: |
Z Offset: |
Est. Count Rate: |
Order-1 Count Rate: |
Exposure Time: |
Time Remaining: |
Reqd Start Time: |
Reqd Stop Time: |
Period: |
Epoch: |
Start of Period: |
End of Period: |
PS Margin: |
PE Margin: |
Max Segments: |
Duty Cycle?: |
Cycle Count: |
Primary Exp Time: |
Secondary Exp Time: |
Event Filter?: |
Filter Threshold: |
Filter Range: |
Bias Requested?: |
Bias Frequency: |
Bias After?: |
Spatial Window?: |
Abstract: The rare misaligned pulsar filaments (e.g. the Guitar nebula filament) represent an important channel for the escape of multi-TeV e+/e- to the ISM, likely enabled by a small bow shock stand-off distance. From the ATNF catalog, we select pulsars expected to have small stand-off and find that almost none have had sensitive X-ray observations. From the best such candidates, we identify a set with small CXO resource cost. We also develop a new statistic capable of identifying filaments comparable to the faintest long filament known, using modest ACIS exposures. Our survey could double the number of known pulsar filaments, helping test their physical nature and importance for the Galactic cosmic ray positrons. |
psci Run: |
Processing Date: |
psci Directory: |
OBSID: |
SIM Mode: |
OTG Mode: |
Seq Number: |
Target Name: |
AO: |
Start VCDU: |
Start Time (UTC): |
Stop Time (UTC): |
Kilosecs: |
% Frames: |
# CCDs: |
# Frames: |
# Events: |
Events/sec: |
PSCI errors: |
% drops: |
Bias Errs: |
FP Temp: |
Parameter Block: |
Window Block: |
# Windows: |
FEP Mode: |
BEP Mode: |
Start Row: |
# Rows: |
Primary Exposure: |
Secondary Exposure: |
Duty Cycle: |
Summing?: |
Bias?: |
Trickle?: |
Bias Run: |