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 201019010 3C120 68.29696 5.35417 67.63242 5.24971 67.43077 -16.40083 190.37349 -27.39635 268.4925 60753.74032 2025-03-19 17:46:04 60758.65699 2025-03-24 15:46:04 221.970 200.000 221.970 195.932 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 209.578 195.932 0.000 0.000 11110 313430 11310 PROCESSED 2025-03-28 21:45:28 2026-04-05 00:00:00 2025-03-29 21:45:28 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000011124 The jet production mechanism remains one of the most important questions in astrophysics, and a key is how mass accretion and disk wind are related to a jet. Therefore, we propose a 200 ksec observation on an X-ray bright radio galaxy 3C120 with XRISM, combining observations by mm-VLBIs: EAVN, GMVA, and EHT. With Resolve, we can constrain the disk wind properties, the mass accretion structure, and the disk truncation radius by resolving Fe XXV/XXVI lines, and narrow and broad Fe-K lines, respectively. Xtend can determine the jet synchrotron in soft X-ray. These can be directly compared to the jet activity and structure, spatially resolved by mm-VLBIs. By this powerful method, we constrain the relation of the jet production to mass accretion/disk wind most strongly so far. BLAZARS AND OTHER JET-DOMINATED AGN 2 A HIROFUMI NODA JAP 1 NOR RESOLVING THE MASS ACCRETION AND JET EJECTION IN 3C120 WITH XRISM & MM-VLBIS (EAVN, GMVA, AND EHT) processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201019010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201019010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏