Main Search Form Search of IXPE Catalog(s) Tips Archive Hera Data Analysis Help

Description Catalog Data Default Radius (arcmin) Mission Table Type
IXPE Master Catalog ixmasterY
10
 IXPE Observation

1. Enter any constraints on the query below. [ Help on constraint syntax ]

(What about wildcards, spaces, and case sensitivity?)

2. To change the fields that are returned, select the box in the "View" column beside each field desired.

3. To sort the results by any field, select one box in the "Sort" column beside the field to sort on.


 Parameter (Unit) Min Value Max Value Value Type
obsid 01001099 03250201 string
name 1E 2259+586 XTE J1701-462 string
ra 00 25 18.0 23 23 28.0 position
dec -73 26 36 +84 35 30 position
lii (degree) 0.0873 359.0941 float
bii (degree) -52.2458 82.7345 float
roll_angle_req (degree) float
time 2022-01-11 11:23:47.184 UTC 2024-04-28 05:34:29.390 UTC date
end_time 2022-01-29 12:39:44.205 UTC 2024-05-03 12:40:29.680 UTC date
fcw_1 gray open string
fcw_2 gray open string
fcw_3 gray open string
exposure_1 (s) 5768.2326 1152149.8802 float
exposure_2 (s) 5765.5959 1152711.7041 float
exposure_3 (s) 5766.4362 1152999.8023 float
ontime_1 (s) 5771.9830 1152726.8460 float
ontime_2 (s) 5772.0730 1153548.6537 float
ontime_3 (s) 5772.0140 1153917.6606 float
processing_date 2022-04-04 14:05:39.412 UTC 2024-04-30 22:10:36.777 UTC date
public_date 2022-01-03 2024-10-30 date
software_version Hea_10Mar2022_V6.30_IXPE_16MAY2022_1.4 Hea_17Jul2023_V6.32_IXPE_12JUN2023_1.7 string
obs_type ddt too string
coordinated After the IXPE observations are scheduled; the PI will notify the NuSTAR and Swift staff to arrange XRSIM will observed in the Performance verification phase. I propose simultaneous observation. NuSTA string
issue_flag 0 0 integer
status accepted processed string
caldb_version 20211118 20211118 string
comments string
prnb 1009 1236 integer
title A NOVEL VIEW OF DISK WINDS IN TRANSIENT BLACK HOLE LOW-MASS X-RAY BINARIES WITH X-RAY SPECTRO-POLARIMETRY X-RAY POLARIZATION OF A TEV BINARY string
pi_names Ajay Ratheesh WONG; JOSEPHINE string
      abstract 3C58 (G130.7+3.1) is a young Pulsar Wind Nebula. It shows clear evidence of energy injection from the central pulsar PSR J0205+6449 in the form of a jet torus structure, observed edge-on. Polarization has been measured in Radio, with a typical average value of the PD for the entire nebula of 6%, with an average B-field roughly aligned with the nebular axis. Local highly polarised patches with PD up to 25% and sizes comparable to 1/10 of the nebula have also been reported. This is the only PWN, left out, tha Z sources are some of the most enigmatic persistent sources in the X-ray sky. We propose observations of the Z source GX 340+0 with IXPE and NICER for total exposures of 300 ks and 12 ks, respectively. The main goal of this program is to constrain the accretion geometry, in particular, that of the thermal component and the corona, by measuring the energy dependent polarization. By comparing our results with spectro-polarimetric modeling of other Z sources, we aim to develop a more robust picture of the comp string
subject_category Accreting Black Hole mag string
category_code 1 7 integer
priority 0 L string
cycle 1 1 integer

4. Do you want to change your current query settings?


(e.g. 'Cyg X-1' or '12 00 00, 4 12 6')
Use semicolons (;) to separate multiple object names or coordinate pairs (e.g. 'Cyg X-2; 12.235, 15.345').
Default uses the optimum radius for each catalog searched.

Not all tables have observation dates/times. For those that do, the time portion of the date is optional.
Times are always in UTC. Separate multiple dates/ranges with semicolons (;). Range operator is '..'
(e.g. '1992-12-31; 48980.5; 1995-01-15 12:00:00; 1997-03-20 .. 2000-10-18').
rows
Select to display all catalog parameters instead of only defaults.

5.


Browse Feedback