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 201063010 NGC4388 186.44428 12.6629 185.81037 12.93968 180.7843 14.1632 279.11812 74.336 103.00075 60648.78477 2024-12-04 18:50:04 60653.09866 2024-12-09 02:22:04 182.548 160.000 182.548 168.404 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 180.133 168.404 0.000 0.000 11110 313430 11310 PROCESSED 2024-12-16 07:29:18 2025-12-24 00:00:00 2024-12-17 07:29:19 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000011336 High resolution spectroscopy with Resolve will enable us to perform unprecedented studies of the circumnuclear structure of AGN using the detailed velocity structure of the narrow Fe-Ka fluorescence line. Here we propose to observe NGC 4388, which exhibits the brightest narrow Fe-Ka emission line among Compton-thin Seyfert 2 galaxies. The bright narrow Fe-K line, Compton-thin absorption, and high inclination make it the best target for studying the ``torus'' and inner region. With Resolve, we can for the first time measure the detailed line profile itself, leading to unbiased determination of matter distribution profile around the nucleus. NON-JET-DOMINATED AGN 2 A YOSHIHIRO UEDA JAP 1 NOR RESOLVING CIRCUMNUCLEAR STRUCTURE IN SEYFERT 2 GALAXY NGC 4388 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201063010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201063010'

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