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 902001060 C2025_N1 183.30718 -0.55183 182.66642 -0.27381 183.25403 0.80847 283.02423 60.8345 109.48287 61006.65977 2025-11-27 15:50:04 61006.79171 2025-11-27 19:00:04 5.892 60.000 5.892 6.344 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 6.344 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-12-03 09:34:14 2023-09-06 00:00:00 2025-12-04 09:34:14 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000029002 C/2025 N1 represents the first credible opportunity to detect soft X-ray emission from solar wind charge exchange (SWCX) in an interstellar comet. Interstellar comets are important because they provide direct samples of volatile substances from other planetary systems, preserving the chemical composition of exsolar protoplanetary discs and enabling comparisons between extrasolar planet-formation environments and our own. When active near perihelion, their neutral comae can attain scales of 10^5--10^6 km. SWCX emissions from this extensive "halo" identify the content and spatial distribution of neutral gas and volatile material, a capability beyond that of optical and infrared studies. SOLAR SYSTEM 9 A XRISM Collaboration DDT 2 DDT-TOO DDT TOO REQUEST OF THE INTERLOPER archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/9/902001060/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '902001060'

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