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 201076090 NGC4151 182.63393 39.40703 182.00258 39.68514 164.09467 36.62426 155.07852 75.06128 109.5996 60674.00838 2024-12-30 00:12:04 60674.96463 2024-12-30 23:09:04 43.618 40.000 43.618 35.097 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 37.542 35.097 0.000 0.000 11110 313430 11310 PROCESSED 2025-01-04 10:35:13 2026-01-09 00:00:00 2025-01-05 10:35:13 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000012061 Optical broad line reverberation mapping of Seyferts has helped the field to understand the geometry of accretion onto massive black holes, and to measure black hole masses. Now, XRISM observations of NGC 4151 during the PV phase have resolved specific line components that may reveal even more. We request a total of 360 ks in 9 exposures in XRISM Cycle 1 to undertake a pioneering simultaneous X-ray and optical reverberation lag study of NGC 4151. Building on key prior results, we demonstrate that modest observations will achieve the sensitivity needed to detect a reverberation lag in X-rays. This is the first step to understanding the relative geometry of the X-ray and optical components of the broad line region, and weighing massive black holes in X-rays. NON-JET-DOMINATED AGN 2 A JON MILLER USA 1 NOR REVERBERATION IN NGC 4151 WITH XRISM processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201076090/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201076090'

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