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".

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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 202009020 1ES1927+654 291.8332 65.56517 291.7599 65.46181 3.66292 81.13211 96.98442 20.9601 224.05952 61007.86046 2025-11-28 20:39:04 61010.67435 2025-12-01 16:11:04 129.106 130.000 129.106 131.230 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 131.230 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-12-05 10:50:13 2099-12-31 00:00:00 2025-12-06 10:50:13 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000022103 1ES~1927+654 is an enigmatic post-changing-look active galaxy (CL-AGN) which has shown a recent rise in the soft X-ray flux (by 10 times) and radio flux (by 60 times) in a few months, followed by detection of radio outflows (v=0.2c) with VLBA. In December 2024 for the first time a 2% linear polarization (in VLA X-band radio) was detected (priv comm.), revealing a real-time magnetic field alignment at the core of the AGN as the jet/UFO forms and evolves. Here we propose to observe the source with XRISM for a 200 ks snapshot to detect and characterize the emerging Fe K emission line and the UFOs in the 7-9 keV energy band. An affirmative detection of UFOs with XRISM will be the first ever `direct' (real-time) evidence of involvement of magnetic fields in the launching of UFOs. NON-JET-DOMINATED AGN 2 A SIBASISH LAHA USA 2 NOR AN ONGOING MAGNETIC FIELD ALIGNMENT CONTEMPORANEOUS WITH A JET/UFO LAUNCH IN THE POST-CHANGING-LOOK AGN 1ES~1927+654. preprocessed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202009020/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202009020'

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