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 000162000 Circinus_Galaxy 213.29011 -65.33927 212.32257 -65.10519 238.61027 -47.96236 311.32543 -3.80794 114.47734 60348.47088 2024-02-08 11:18:04 60352.99727 2024-02-12 23:56:04 328.030 100.000 328.030 286.818 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 32000010 306.795 286.818 0.000 0.000 11110 313430 11310 PROCESSED 2024-09-22 00:16:21 2025-08-31 00:00:00 2024-03-04 02:22:31 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000000058 We propose to observe the Circinus galaxy with XRISM, the most nearby (4.2 Mpc) Compton-thick AGN showing the brightest narrow Fe-Ka line among all known AGNs. The bright fluorescence lines and Compton-thick nature make it the best target for studying the torus itself through high resolution spectroscopy. We use the Compton shoulder structure of Fe-Ka and the properties of other fluorescence lines to unveil the torus structure. The Resolve spectrum will also reveal the origins and kinematics of the extended soft X-ray emission. NON-JET-DOMINATED AGN 0 A XRISM Collaboration JAP 0 NOR UNVEILING NATURE OF COMPTON-THICK TORUS IN CIRCINUS GALAXY archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/0/000162000/ WINDOW2 WINDOW1 4 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '000162000'

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