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 203041010 MCG+8-11-11 88.72316 46.43986 87.79005 46.4314 89.04413 23.0048 165.73062 10.40716 90.00003 61292.10907 2026-09-09 02:37:04 61297.62366 2026-09-14 14:58:04 177.987 200.000 177.987 258.573 PX_NORMAL N N N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 276.583 258.573 0.000 0.000 11110 313430 11310 PROCESSED 2026-09-23 10:24:58 2099-12-31 00:00:00 2026-09-24 10:24:58 03.03.015.013 gen20241115_xtd20260315_rsl20260315 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000031243 We propose to observe MCG+8-11-11, the Fe-K brightest Seyfert galaxy that is free from neutral or ionized absorption. This clean AGN spectrum provides us with the best opportunity to study the detailed line profile of the Fe K emission lines de-coupled from complex absorption features commonly observed in AGNs. The primary goals are (1) to identify the physical origin of the X-ray broad line region by comparison with extinction-free optical broad line spectra simultaneously observed, and (2) to test the hypothesis that the torus is predominantly made of radiation-driven outflow by detecting an expected blue shift when viewed face-on. As a secondly goal, we aim to reveal the velocity field of highly ionized gas using the Fe Lya line. NON-JET-DOMINATED AGN 2 A YOSHIHIRO UEDA JAP 3 NOR X-RAY BROAD LINE REGION AND TORUS STRUCTURES IN MCG+8-11-11 preprocessed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/203041010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '203041010'

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