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 201044010 IC4329A 207.33117 -30.30939 206.61702 -30.06123 216.35045 -17.77957 317.49716 30.91987 288.0001 60894.95074 2025-08-07 22:49:04 60898.33824 2025-08-11 08:07:04 146.288 130.000 146.288 99.706 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 106.650 99.706 0.000 0.000 11110 313430 11310 PROCESSED 2025-10-08 20:46:22 2026-08-26 00:00:00 2025-08-19 09:04:15 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000011234 Various structures within AGNs emit Fe K lines. IC 4329A, a prominent Seyfert 1 galaxy in X-rays with minimal absorption in its spectrum, is ideal for studying Fe K emission origins. Line width analysis suggests a radius of about 60 light-days, possibly representing an outer broad line region. We propose using a 130 ks observation with XRISM to constrain the ionization degree of this Fe K reprocessor, enabling the calculation of its number density and a deeper understanding of its properties. Anticipated log ionization parameter falls between 1 and 2, with Fe Kalpha and Kbeta lines exhibiting energy shifts of several eV within this range. XRISM is uniquely equipped to detect this energy shift within a reasonable exposure time. NON-JET-DOMINATED AGN 2 B MISAKI MIZUMOTO JAP 1 NOR ORIGIN OF THE FE K REPROCESSOR IN SEYFERT 1 GALAXY, IC 4329A processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201044010/ WINDOW2 WINDOW1 4 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201044010'

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