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 201021010 3C111 64.5868 38.02637 63.75068 37.9051 69.36787 16.38982 161.67465 -8.82099 71.87593 60578.52644 2024-09-25 12:38:04 60583.40421 2024-09-30 09:42:04 224.068 200.000 224.068 178.856 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 191.313 178.856 0.000 0.000 11110 313430 11310 PROCESSED 2024-10-04 14:09:02 2025-10-05 00:00:00 2024-10-05 14:09:03 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000011132 One of the most important questions of the active galactic nucleus (AGN) is the origin of the dichotomy of radio-quiet and radio-loud AGN. This is tightly related to the formation of the relativistic jets from black holes. The key to solving it is fast accretion disk winds, so-called ultra-fast outflows (UFOs). Observational facts indicate that the UFO is launched from the vicinity of the black hole. Thus, the UFO is the best probe for the innermost region of radio-loud AGN. To tackle the radio-quiet/loud dichotomy with the UFOs, we propose a 200 ks observation of 3C 111, which most probably harbors the UFO. With high resolution of Resolve, we will detect the UFO at 6 sigma level. Resolve will also allow us to estimate the kinetic power of the UFO and magnetization of the disk and UFO. BLAZARS AND OTHER JET-DOMINATED AGN 2 B KOUICHI HAGINO JAP 1 NOR PROBING THE INNERMOST REGION OF A JETTED ACTIVE GALACTIC NUCLEUS 3C 111 archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201021010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201021010'

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