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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