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 202035010 ESP39607 11.58624 -40.09706 10.99168 -40.37015 351.25705 -40.69624 307.26157 -76.98834 256.37097 61045.96741 2026-01-05 23:13:04 61048.18755 2026-01-08 04:30:04 112.123 90.000 112.123 102.357 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 102.357 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2026-01-14 06:40:05 2027-01-17 00:00:00 2026-01-15 06:40:06 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000022171 We propose to investigate a 4.8 keV absorption feature in the z=0.201 AGN ESP39607, recently detected in two NuSTAR observations (>4sigma combined significance) and identified as a potential sustained ultra-fast inflow (UFI). The feature, likely arising from Fe XXV and/or Fe XXVI Ka transitions, suggests inflow velocities of 0.15-0.20c and has persisted across two epochs (2023 and 2024). With XRISM, we aim to: 1) confirm the feature at >6sigma, and 2) conduct detailed spectroscopy to determine its origin and physical properties. This would provide the clearest evidence of a UFI to date, as previous detections never exceeded 3-3.5sigma. The year-long persistence of the feature offers a rare and time-sensitive opportunity to capture this phenomenon before it potentially fades. NON-JET-DOMINATED AGN 2 A ALESSANDRO PECA USA 2 NOR PROBING A SUSTAINED ULTRA-FAST INFLOW WITH XRISM processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202035010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202035010'

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