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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