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".

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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 202068010 MCG-5-23-16 146.91697 -30.94854 146.36776 -30.71597 162.6179 -41.15111 262.7437 17.23381 95.90126 60981.88616 2025-11-02 21:16:04 60985.92991 2025-11-06 22:19:04 190.196 160.000 190.196 171.734 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 183.695 171.734 0.000 0.000 11110 313430 11310 PROCESSED 2025-11-11 09:02:14 2026-11-13 00:00:00 2025-11-12 09:02:15 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000021404 MCG-5-23-16 is one of the brightest AGNs exhibiting a relativistic iron line. Unlike MCG-6-30-15, a highly significant feature of ultrafast outflow (UFO) has been reported, offering a valuable opportunity to study both the accretion disk and associated UFO. We propose a 160-ks XRISM observation of MCG-5-23-16 to resolve the Fe-K band complex, enabling a robust measurement of the inner radius. By measuring the UFO velocity (~0.1c), we will assess whether the inner radius is smaller than the launching radius of the UFO. For the first time XRISM will detect short-timescale (~20 ks) UFO variability, constraining the clumpy nature of the UFO in the sub-Eddington AGN. NON-JET-DOMINATED AGN 2 B SATOSHI YAMADA JAP 2 NOR THE LINK BETWEEN RELATIVISTIC DISK AND ULTRAFAST WIND IN MCG-5-23-16 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202068010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202068010'

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