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 300019010 CENTAURUS_A 201.36512 -43.019 200.63176 -42.75903 217.14334 -31.33179 309.51595 19.41737 299.9728 60526.80352 2024-08-04 19:17:04 60531.68338 2024-08-09 16:24:04 227.986 100.000 227.986 182.753 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 195.482 182.753 0.000 0.000 11110 313430 11310 PROCESSED 2024-09-26 01:27:32 2025-08-31 00:00:00 2024-08-17 13:31:24 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000000037 A full understanding of the AGN that drive the most powerful jets - those that reshape clusters and galaxies - requires that we study the accretion disk in such systems. However, in most cases, the accretion inflow is obscured, hidden, or otherwise inaccessible. Cen A is a nearby radio galaxy (d=3.8 Mpc) with dramatic bipolar jets; it is the brightest such galaxy in the 4-10~keV band, and its spectra show the strongest narrow Fe~Ka emission line among radio-loud AGN. It is possible to associate the narrow Fe line with the elusive optical BLR, and some spectra hint at ultra-fast, v~0.1c winds. Resolve spectroscopy of Cen A will reveal the inner and intermediate disk in the jet mode, and reveal the properties of slow and ultra-fast disk winds. BLAZARS AND OTHER JET-DOMINATED AGN 3 A XRISM Collaboration JAP 0 NOR THE JET-LAUNCHING DISK AND ACCRETION FLOW IN CENTAURUS A archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/3/300019010/ WINDOW2 WINDOW1 2 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '300019010'

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