DARTS/Astro Query System - SQL Search -

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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 201083010 MRK279 208.2657 69.30836 207.97464 69.55382 144.91488 67.64716 115.04092 46.86442 210.81787 60572.83199 2024-09-19 19:58:04 60576.38130 2024-09-23 09:09:04 181.110 150.000 181.110 154.689 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 165.463 154.689 0.000 0.000 11110 313430 11310 PROCESSED 2024-09-28 11:50:06 2025-10-03 00:00:00 2024-09-29 11:50:07 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000012098 Observations of extreme variability in the narrow Fe K-alpha emission line - independent of a moderately broad line component - demonstrate that multiple geometries can be explored in the Sy-1.5 AGN Mrk 279. This makes it an optimal target for XRISM Cycle 1. Variability in the narrow line component suggests a modest radius and extent, consistent with the optical broad line region. The "broad" Fe Ka component is not extreme and suggests a truncated inner disk and/or one with a warp. We request a 150 ks obs. of Mrk 279 in XRISM Cycle 1 to (1) precisely locate the Fe Ka emission components within the accretion flow, (2) compare the radii and geometries to optical line constraints, (3) test models of warped and/or truncated disks, (4) study ionized winds in emission. NON-JET-DOMINATED AGN 2 A JON MILLER USA 1 NOR IRONING-OUT THE ACCRETION FLOW IN SEYFERT AGN WITH MRK 279 archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201083010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201083010'

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