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 300041010 SS433 287.95612 4.98315 287.33829 4.89874 290.19541 27.17226 39.69429 -2.24405 80.53479 60410.57019 2024-04-10 13:41:04 60415.43894 2024-04-15 10:32:04 206.351 80.000 206.351 184.118 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 184.118 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2024-09-23 20:37:55 2025-08-31 00:00:00 2024-04-24 19:27:28 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000000066 We propose an 80 ks observation of the Galactic microquasar SS 433 around an eclipse phase, consisting of a 50 ks exposure in eclipse and 30 ks out of eclipse, to investigate the jet structure by measuring the line widths of ionized metal lines emitted from different regions in the jets. High resolution X-ray spectroscopy of SS 433 with Resolve gives unique opportunity to understand the jet structure at supercritical accretion rates. The jet collimation of SS 433 can be resolved by comparing the velocity dispersions of Fe XXVI and Si XIV Ly alpha lines, and more direct evidence can be obtained from a comparison between the line structures in eclipse and and non-eclipse phases. BH AND NS BINARIES 3 A XRISM Collaboration JAP 0 NOR INVESTIGATING JET STRUCTURE OF SS 433 archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/3/300041010/ WINDOW1 2 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '300041010'

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