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 201030010 H1821+643 275.48893 64.34386 275.4247 64.31737 318.33027 86.82175 94.00305 27.41687 289.99964 60557.10074 2024-09-04 02:25:04 60563.06602 2024-09-10 01:35:04 283.716 250.000 283.716 278.888 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 278.888 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-07-16 21:23:52 2025-09-19 00:00:00 2024-09-17 21:33:04 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000011159 We propose a 250 ks XRISM observation of H1821+643, a recoiling and extremely accreting supermassive black hole (SMBH) in a cooling flow cluster. Cooling flows are expected to have a huge impact on the active galactic nuclei (AGNs), yet they are scarcely observed in the local Universe, known as the cooling flow problem. H1821+643 is an irreplaceable target hosting cooling flows and a radio-quiet quasar. We will measure the turbulent motions within the cooling core to understand quasar-mode feedback. To comprehend how the SMBH acquires its large mass, we will also examine the AGN structure (torus, broad-line region, and accretion disk) by resolving the complex Fe lines. This observation will reveal new frontiers on the long-standing cooling flow problem and SMBH formation in cooling cores. NON-JET-DOMINATED AGN 2 B SATOSHI YAMADA JAP 1 NOR A RECOILING AND EXTREMELY ACCRETING SUPERMASSIVE BLACK HOLE IN A COOLING FLOW CLUSTER archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201030010/ WINDOW1 3 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201030010'

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