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 203076010 PDS456 262.08307 -14.26572 261.37236 -14.22566 262.23333 8.96038 10.3923 11.16296 272.97027 61304.58407 2026-09-21 14:01:04 61308.13963 2026-09-25 03:21:04 146.425 250.000 146.425 138.863 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 138.863 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2026-10-09 11:13:42 2099-12-31 00:00:00 2026-10-10 11:13:43 03.03.015.013 gen20241115_xtd20260315_rsl20260315 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000032009 The luminous nearby quasar, PDS 456, hosts the archetypical UFO, with a typical outflow velocity of 0.3c. In 2024, XRISM revealed a highly clumpy wind in PDS 456, requiring a super-Eddington outflow rate of at least 60 solar masses per year. Now the goal is to understand the variability of the massive outflow in PDS 456, through a new, simultaneous, XRISM, XMM and NuSTAR campaign. Here, a 250ks XRISM exposure is requested, to understand the variability of the clumpy Fe K wind at high spectral resolution. The 2024 PV observation captured a rare obscured state and the new observations may probe very different wind properties, through the variations of the absorption troughs. This will reveal whether the clumpy, super-Eddington wind phase remains persistent and how its kinetic power responds. NON-JET-DOMINATED AGN 2 A JAMES REEVES USA 3 NOR VARIABILITY OF THE CLUMPY, SUPER EDDINGTON WIND IN PDS 456 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/203076010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '203076010'

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