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 202074010 NGC7172 330.50722 -31.87049 329.7799 -32.11199 321.23337 -18.54945 15.1276 -53.06534 247.99433 60969.72991 2025-10-21 17:31:04 60975.25769 2025-10-27 06:11:04 215.347 180.000 215.347 186.177 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 186.177 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-11-03 13:23:17 2026-11-04 00:00:00 2025-11-04 13:23:18 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000021424 We propose to observe NGC 7172, the best-studied new type AGN (low scattering-fraction AGN) showing the brightest Fe K line, to unveil the nuclear structure. New type AGNs were recognized in 2007 as a putative population of deeply buried supermassive black holes. Despite their importance to understand the process of galaxy-black hole coevolution, their nature still remains unsolved. ALMA observations suggest that NGC 7172 is in the AGN feedback phase, where dense outflow in the innermost region of the torus obscures the nucleus. With XRISM we will measure the width and blue shifts of the Fe-K line with unprecedented accuracies. This is a crucial step to confirm the scenario that new type AGNs are in the outflow-dominant phase in a late stage of an AGN event. NON-JET-DOMINATED AGN 2 B YOSHIHIRO UEDA JAP 2 NOR UNVEILING NATURE OF NEW TYPE AGN: NGC 7172 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202074010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202074010'

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