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 202044010 AT2019WEY 68.84779 55.37605 67.83323 55.27333 75.85435 32.97073 151.16154 5.29998 251.73602 61120.30630 2026-03-21 07:21:04 61121.07088 2026-03-22 01:42:04 34.095 30.000 34.095 34.020 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 36.390 34.020 0.000 0.000 11110 313430 11310 PROCESSED 2026-03-28 03:25:38 2027-04-10 00:00:00 2026-03-29 03:25:39 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000022224 One of the most important, unresolved systematic uncertainty in the field of relativistic reflection studies of accreting stellar-mass black holes (BH) is the effect of unresolved, unaccounted-for narrow spectral features on the ability to measure system parameters, including BH spin and viewing inclination. The sensitivity and energy resolution of Resolve guarantee an immediate and definitive resolution to this issue. Owing to its low inclination, the ideal source for this study is the galactic BH low-mass X-ray binary AT2019wey. We propose obtaining a 30ks XRISM observation of this source with the goals of identifying narrow absorption features in the Fe band, breaking parameter degeneracies, and quantifying the impact of narrow features on BH spin and inclination measurements. BH AND NS BINARIES 2 A PAUL DRAGHIS USA 2 NOR THE SPIN AND INCLINATION OF BH LMXB AT2019WEY processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202044010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202044010'

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