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 201116010 NGC1068 40.66964 -0.01351 40.02939 -0.2257 38.24482 -15.03722 172.10397 -51.93394 255.08992 60714.04241 2025-02-08 01:01:04 60716.49032 2025-02-10 11:46:04 114.990 100.000 114.990 112.816 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 112.816 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-02-17 07:57:01 2026-02-19 00:00:00 2025-02-18 07:57:02 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000014019 We propose a 100 ks XRISM observation of the Compton-thick AGN NGC1068, to serve as a benchmark for advancing the study of circumnuclear matter via high-resolution X-ray spectroscopy. The combination of XRISM and the already available broad-band (spectro-polarimetric) X-ray dataset, along with the possibility to extend the self-consistent modelling down to the sub-mm band, will offer an unprecedented view of the geometrical and physical properties of the torus. Moreover, the XRISM spectrum will allow us to measure the properties of the ionized gas and, together with existing soft X-ray high-resolution spectra, understand its origin. State-of-the-art models, developed or specifically adapted by members of the proposing team, will be crucial to leverage the potential of the XRISM spectrum. NON-JET-DOMINATED AGN 2 A STEFANO BIANCHI EUR 1 NOR NGC 1068: A XRISM BENCHMARK FOR COMPTON-THICK SEYFERT 2S processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201116010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201116010'

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