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 201048010 NGC4395 186.45451 33.54741 185.83371 33.82416 170.81796 32.97634 162.08845 81.533 137.52587 60621.16949 2024-11-07 04:04:04 60626.29241 2024-11-12 07:01:04 237.325 200.000 237.325 166.519 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 166.573 0.050 0.000 0.000 11110 313430 11310 PROCESSED 2024-11-21 18:23:08 2025-12-11 00:00:00 2024-11-22 18:23:08 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000011251 In understanding the mass accretion onto the BH in all mass range from stellar-mass to supermassive BHs, obscuring structures are crucial, but particularly those of low-mass AGNs are poorly understood. Thus, this proposal aims to study obscuring matter of the nearby low-mass AGN NGC 4395 by 200-ks observation. Our objectives are as follows. (1) Assess the geometrical thickness of the torus by focusing on iron emission originating at radii larger than a dust-sublimation radius. (2) Constrain the inner radius of an iron broad-line region (BLR) by reverberation mapping between the iron-line and continuum emission, and derive a virial factor. Then, assuming a disk model, we will constrain the geometric structure of the BLR, and will conclude the main obscuring structure of the low-mass AGN. NON-JET-DOMINATED AGN 2 A TAIKI KAWAMURO JAP 1 NOR REVEALING THE NUCLEAR OBSCURING STRUCTURES IN LOW-MASS AGN processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201048010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201048010'

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