DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
| No. |
observation_id
|
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
exposure
|
awarded_exposure
|
resolve_exposure
|
xtend_exposure
|
resolve_data_mode
|
resolve_with_filter_be
|
resolve_with_filter_fe55
|
resolve_with_filter_nd
|
resolve_with_filter_poly
|
resolve_with_filter_open
|
resolve_with_filter_undef
|
is_resolve_gatevalve_closed
|
is_resolve_mxs1
|
is_resolve_mxs2
|
is_resolve_mxs3
|
is_resolve_mxs4
|
xtend_number_modes
|
xtend_dataclass_file1
|
xtend_dataclass_file2
|
xtend_window1_exposure
|
xtend_window2_exposure
|
xtend_window1_burst_exposure
|
xtend_window2_burst_exposure
|
xtend_code
|
resolve_code
|
gen_code
|
processing_status
|
processing_date
|
public_date
|
distribution_date
|
processing_version
|
caldb_version
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
proposal_type
|
proposal_title
|
observation_status
|
data_access_url
|
xtend_data_mode1
|
xtend_data_mode2
|
processing_count
|
remarks
|
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | 202081010 | 4U1627-67 | 248.0683 | -67.46055 | 246.80956 | -67.35369 | 258.33753 | -44.90715 | 321.7882 | -13.09099 | 123.75675 | 61136.94866 | 2026-04-06 22:46:04 | 61138.04241 | 2026-04-08 01:01:04 | 49.191 | 40.000 | 49.191 | 43.084 | PX_NORMAL | N | Y | N | N | Y | Y | Y | OFF | OFF | OFF | OFF | 2 | 31100010 | 320000A0 | 46.085 | 43.084 | 0.000 | 0.000 | 11110 | 313430 | 11310 | PROCESSED | 2026-04-14 09:22:36 | 2027-04-30 00:00:00 | 2026-04-15 09:22:38 | 03.03.015.012 | gen20241115_xtd20250915_rsl20250915 | Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 | 000021457 | 4U 1626-67 is a low-mass X-ray binary pulsar (LMXBP) with a rotation period of P_spin = 7.7 s. Since its discovery, many X-ray instruments have observed 4U 1626-67, and the detection of the Fe emission line has been reported. However, the origin of the Fe line is still uncertain. For the emission region, two possibilities will be suggested: the inner edge of the accretion disk at the Alfven radius and further inner accretion flow onto the magnetic pole of the neutron star (NS). We aim to resolve the emission region of the Fe line with XRISM. Furthermore, we perform a phase-resolved spectroscopy for the Fe line. Due to the short spin period, the high-resolution phase-resolved spectroscopy can be carried out only with XRISM. | BH AND NS BINARIES | 2 | C | TOMOKAGE YONEYAMA | JAP | 2 | NOR | FE EMISSION REGION AND THE ACCRETION GEOMETRY OF THE LMXB PULSAR 4U1626-67 | processed | https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202081010/ | WINDOW2 | WINDOW1 | 1 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '202081010'
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