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: It is expected that the ultra-dense core of a neutron star is superfluid. While being a key ingredient for understanding many observable properties of neutron stars, including the long-term evolution of their temperature, spin, and magnetic field, we have no detailed information about the core superfluid. We propose a 500 ks Chandra observation of the transient low-mass X-ray binary HETE J1900.1-2455 to obtain such important constraints. Our 2018 Chandra observation revealed that this neutron star is exceptionally cold, despite actively accreting from 2005 to 2015. With a new deep exposure we will accurately measure its temperature and constrain its heat capacity. This, in turn, determines what fraction of the core is superfluid. We will also directly test equation of state models. |
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: |