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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